Browse All : Images of Texas from 2007

Two Moons Meet over Jupiter

title	Two Moons Meet over Jupiter
date	03.02.2007
description	This beautiful image of the crescents of volcanic Io and more sedate Europa was snapped by New Horizons' color Multispectral Visual Imaging Camera (MVIC) at 10:34 UT on March 2, 2007, about two days after New Horizons made its closest approach to Jupiter. The picture was one of a handful of the Jupiter system that New Horizons took primarily for their artistic, rather than scientific value. This particular scene was suggested by space enthusiast Richard Hendricks of Austin, Texas, in response to an Internet request by New Horizons scientists for evocative, artistic imaging opportunities at Jupiter. This image was taken from a range of 4.6 million kilometers (2.8 million miles) from Io and 3.8 million kilometers (2.4 million miles) from Europa. Although the moons appear close in this view, a gulf of 790,000 kilometers (490,000 miles) separates them. The night side of Io is illuminated here by light reflected from Jupiter, which is out of the frame to the right. Europa's night side is completely dark, in contrast to Io, because that side of Europa faces away from Jupiter. Here, Io steals the show with its beautiful display of volcanic activity. Three volcanic plumes are visible. Most conspicuous is the enormous 300-kilometer (190-mile) -high plume from the Tvashtar volcano at the 11 o'clock position on Io's disk. Two much smaller plumes are barely visible: one from the volcano Prometheus, at the 9 o'clock position on the edge of Io's disk, and one from the volcano Amirani, seen between Prometheus and Tvashtar along Io's terminator (the line dividing day and night). The plumes appear blue because of the scattering of light by tiny dust particles ejected by the volcanoes, similar to the blue appearance of smoke. In addition, the contrasting red glow of hot lava can be seen at the source of the Tvashtar plume. The images are centered at 1 degree north, 60 degrees west on Io, and 0 degrees north, 149 degrees west on Europa. The color in this image was generated using individual MVIC images at wavelengths of 480, 620 and 850 nanometers. The human eye is sensitive to slightly shorter wavelengths, from 400 to 700 nanometers, and thus would see the scene slightly differently. For instance, while the eye would notice the difference between the yellow and reddish brown colors of Io's surface and the paler color of Europa, the two worlds appear very similar in color to MVIC's longer-wavelength vision. The night side of Io appears greenish compared to the day side, because methane in Jupiter's atmosphere absorbs 850-nanometer light and makes Jupiter-light green to MVIC's "eyes." MVIC is a component of the Ralph imaging instrument. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute

An Eruption on Io

title	An Eruption on Io
date	02.26.2007
description	The first images returned to Earth by New Horizons during its close encounter with Jupiter feature the Galilean moon Io, snapped with the Long Range Reconnaissance Imager (LORRI) at 0840 UTC on February 26, while the moon was 2.5 million miles (4 million kilometers) from the spacecraft. Io is intensely heated by its tidal interaction with Jupiter and is thus extremely volcanically active. That activity is evident in these images, which reveal an enormous dust plume, more than 150 miles high, erupting from the volcano Tvashtar. The plume appears as an umbrella-shaped feature of the edge of Io's disk in the 11 o'clock position in the right image, which is a long-exposure (20-millisecond) frame designed specifically to look for plumes like this. The bright spots at 2 o'clock are high mountains catching the setting sun, beyond them the night side of Io can be seen, faintly illuminated by light reflected from Jupiter itself. The left image is a shorter exposure -- 3 milliseconds -- designed to look at surface features. In this frame, the Tvashtar volcano shows as a dark spot, also at 11 o'clock, surrounded by a large dark ring, where an area larger than Texas has been covered by fallout from the giant eruption. This is the clearest view yet of a plume from Tvashtar, one of Io's most active volcanoes. Ground-based telescopes and the Galileo Jupiter orbiter first spotted volcanic heat radiation from Tvashtar in November 1999, and the Cassini spacecraft saw a large plume when it flew past Jupiter in December 2000. The Keck telescope in Hawaii picked up renewed heat radiation from Tvashtar in spring 2006, and just two weeks ago the Hubble Space Telescope saw the Tvashtar plume in ultraviolet images designed to support the New Horizons flyby. Most of those images will be stored onboard the spacecraft for downlink to Earth in March and April. Image Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute

Hubble Images of Asteroids Help Astronomers Prepare for Spacecraft Visit

Hubble Images of Asteroids H …

Title	Hubble Images of Asteroids Help Astronomers Prepare for Spacecraft Visit

The German-built 100-inch telescope that is the heart of NASA's Stratospheric Observatory for Infrared Astronomy is nestled in the SOFIA 747's rear fuselage.

Photo Description	The German-built 100-inch telescope that is the heart of NASA's Stratospheric Observatory for Infrared Astronomy is nestled in the SOFIA 747's rear fuselage.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 100-inch (2.5 meter) diameter infrared telescope weighing 20 tons mounted in a highly-modified Boeing 747SP aircraft, is approaching the flight test phase as part of a joint program by NASA and DLR Deutsches Zentrum fuer Luft- und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope has been carried out at L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations will be conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif, beginning in 2007. SOFIA's science and mission operations are being planned jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are currently based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	February 2, 2006

A rotating external door (white) was installed over the telescope cavity in the rear fuselage of NASA's SOFIA Boeing 747SP during modifications in Waco, Texas.

Photo Description	A rotating external door (white) was installed over the telescope cavity in the rear fuselage of NASA's SOFIA Boeing 747SP during modifications in Waco, Texas.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 100-inch (2.5 meter) diameter infrared telescope weighing 20 tons mounted in a highly-modified Boeing 747SP aircraft, is approaching the flight test phase as part of a joint program by NASA and DLR Deutsches Zentrum fuer Luft- und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope has been carried out at L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations will be conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif, beginning in 2007. SOFIA's science and mission operations are being planned jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are currently based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	February 2, 2006

Kelly Latimer is a research pilot in the Flight Crew Branch of NASA's Dryden Flight Research Center, Edwards, Calif. Latimer joined NASA in March 2007 and will fly the T38, T-34, G-III, C-17 and the "Ikhana" Predator B. Latimer is Dryden's first female research test pilot. Prior to joining NASA, Latimer was on active duty with the U.S. Air Force. She has accumulated more than 5,000 hours of military and civilian flight experience in 30 aircraft. Latimer's first association with NASA was while attending graduate school at George Washington University, Washington, D.C. Her studies included work with the Joint Institute for the Advancement of Flight Sciences at NASA's Langley Research Center, Hampton, Va. She flew an Air Force C-17 during a 2005 NASA study to reduce aircraft noise. A team of California Polytechnic State University students and Northrop Grumman personnel were stationed on Rogers Dry Lake located at Edwards Air Force Base, Calif., to record the noise footprint of the aircraft as it made various landing approaches to Edwards' runway. Latimer completed undergraduate pilot training at Reese Air Force Base, Texas, in 1990. She remained at Reese as a T-38 instructor pilot until 1993. She was assigned as a C-141 aircraft commander at McCord Air Force Base, Tacoma, Wash., until 1996. Latimer graduated from the U.S. Air Force Test Pilot School at Edwards in Class 96B. She served as a C-17 and C-141 experimental test pilot at Edwards until 2000. She then became the chief of the Performance Branch and a T-38 instructor pilot at The Air Force Test Pilot School. She returned to McCord in 2002, where she was a C-17 aircraft commander and the operations officer for the 62nd Operations Support Squadron. In 2004, Latimer became the commander of Edwards' 418th Flight Test Squadron and director of the Global Reach Combined Test Force. Following that assignment, she deployed to Iraq as an advisor to the Iraqi Air Force. Her last active duty tour was as an instructor at the Air Force Test Pilot School. She retired from active duty in 2007 with the rank of lieutenant colonel. She received her commission from the U.S. Air Force Academy in 1987 with a Bachelor of Science in astronautical engineering. Latimer earned a Master of Science in astronautics from George Washington University.

Photo Description	Kelly Latimer is a research pilot in the Flight Crew Branch of NASA's Dryden Flight Research Center, Edwards, Calif. Latimer joined NASA in March 2007 and will fly the T38, T-34, G-III, C-17 and the "Ikhana" Predator B. Latimer is Dryden's first female research test pilot. Prior to joining NASA, Latimer was on active duty with the U.S. Air Force. She has accumulated more than 5,000 hours of military and civilian flight experience in 30 aircraft. Latimer's first association with NASA was while attending graduate school at George Washington University, Washington, D.C. Her studies included work with the Joint Institute for the Advancement of Flight Sciences at NASA's Langley Research Center, Hampton, Va. She flew an Air Force C-17 during a 2005 NASA study to reduce aircraft noise. A team of California Polytechnic State University students and Northrop Grumman personnel were stationed on Rogers Dry Lake located at Edwards Air Force Base, Calif., to record the noise footprint of the aircraft as it made various landing approaches to Edwards' runway. Latimer completed undergraduate pilot training at Reese Air Force Base, Texas, in 1990. She remained at Reese as a T-38 instructor pilot until 1993. She was assigned as a C-141 aircraft commander at McCord Air Force Base, Tacoma, Wash., until 1996. Latimer graduated from the U.S. Air Force Test Pilot School at Edwards in Class 96B. She served as a C-17 and C-141 experimental test pilot at Edwards until 2000. She then became the chief of the Performance Branch and a T-38 instructor pilot at The Air Force Test Pilot School. She returned to McCord in 2002, where she was a C-17 aircraft commander and the operations officer for the 62nd Operations Support Squadron. In 2004, Latimer became the commander of Edwards' 418th Flight Test Squadron and director of the Global Reach Combined Test Force. Following that assignment, she deployed to Iraq as an advisor to the Iraqi Air Force. Her last active duty tour was as an instructor at the Air Force Test Pilot School. She retired from active duty in 2007 with the rank of lieutenant colonel. She received her commission from the U.S. Air Force Academy in 1987 with a Bachelor of Science in astronautical engineering. Latimer earned a Master of Science in astronautics from George Washington University.
Photo Date	March 9, 2007

Christened "Clipper Lindbergh" when it flew for Pan American Airways in the 1970s, the SOFIA 747SP shows evidence of modification to its aft fuselage contours to accommodate a 16-foot-tall opening for a 45,000-pound infrared telescope. This inflight photo was taken on SOFIA's first flight since its modification to become an airborne observatory.

Photo Description	Christened "Clipper Lindbergh" when it flew for Pan American Airways in the 1970s, the SOFIA 747SP shows evidence of modification to its aft fuselage contours to accommodate a 16-foot-tall opening for a 45,000-pound infrared telescope. This inflight photo was taken on SOFIA's first flight since its modification to become an airborne observatory.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 100-inch (2.5 meter) diameter infrared telescope weighing 20 tons mounted in a highly-modified Boeing 747SP aircraft, is approaching the flight test phase as part of a joint program by NASA and DLR Deutsches Zentrum fuer Luft- und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope has been carried out at L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations will be conducted at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif, beginning in 2007. SOFIA's science and mission operations are being planned jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are currently based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	April 26, 2007

747SP - SOFIA maiden flight …

Technicians check out the mounting structure of the 20-metric-ton infrared telescope installed in NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA).

Photo Description	Technicians check out the mounting structure of the 20-metric-ton infrared telescope installed in NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA).
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	April 25, 2007

A technician examines the instrument mounting structure and bulkhead of the German-built infrared telescope installed in NASA's SOFIA airborne observatory.

Photo Description	A technician examines the instrument mounting structure and bulkhead of the German-built infrared telescope installed in NASA's SOFIA airborne observatory.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	April 25, 2007

The NASA and German Aerospace Center SOFIA airborne infrared observatory took flight for the first time April 26, 2007, from its modification center in Waco, Texas.

Photo Description	The NASA and German Aerospace Center SOFIA airborne infrared observatory took flight for the first time April 26, 2007, from its modification center in Waco, Texas.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	April 26, 2007

NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) was airborne for almost two hours during its first check flight at Waco, Texas on April 26, 2007.

Photo Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) was airborne for almost two hours during its first check flight at Waco, Texas on April 26, 2007.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	April 26, 2007

Logos of NASA and the German Aerospace Center (DLR) are displayed prominently on the tail of the Stratospheric Observatory for Infrared Astronomy (SOFIA) 747SP.

Photo Description	Logos of NASA and the German Aerospace Center (DLR) are displayed prominently on the tail of the Stratospheric Observatory for Infrared Astronomy (SOFIA) 747SP.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	April 26, 2007

NASA's modified Boeing 747SP SOFIA airborne observatory taxis along the runway at Waco, Texas after completing its first checkout flight on April 26, 2007.

Photo Description	NASA's modified Boeing 747SP SOFIA airborne observatory taxis along the runway at Waco, Texas after completing its first checkout flight on April 26, 2007.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	April 26, 2007

NASA's SOFIA 747SP shows evidence of modification to its aft fuselage contours to accommodate a 16-foot-tall cavity door for its 45,000-pound infrared telescope.

Photo Description	NASA's SOFIA 747SP shows evidence of modification to its aft fuselage contours to accommodate a 16-foot-tall cavity door for its 45,000-pound infrared telescope.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	April 26, 2007

Photo Description	Christened "Clipper Lindbergh" when it flew for Pan American Airways in the 1970s, the SOFIA 747SP shows evidence of modification to its aft fuselage contours to accommodate a 16-foot-tall opening for a 45,000-pound infrared telescope. This inflight photo was taken on SOFIA's first flight since its modification to become an airborne observatory.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	April 26, 2007

With landing gear extended, the NASA/DLR Stratospheric Observatory for Infared Astronomy (SOFIA) 747SP cruises over central Texas on its first checkout flight.

Photo Description	With landing gear extended, the NASA/DLR Stratospheric Observatory for Infared Astronomy (SOFIA) 747SP cruises over central Texas on its first checkout flight.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	April 26, 2007

NASA's highly modified Boeing 747SP SOFIA observatory banks low over the Texas countryside as it heads for landing at Waco to conclude its second check flight.

Photo Description	NASA's highly modified Boeing 747SP SOFIA observatory banks low over the Texas countryside as it heads for landing at Waco to conclude its second check flight.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	May 10, 2007

Erik Lindbergh, grandson of aviator Charles Lindbergh, unveiled a plaque commemorating his grandfather on the 80th anniversary of Charles Lindbergh's transatlantic flight. The event was a dedication of the 747 Clipper Lindbergh, a NASA airborne infrared observatory that is beginning test flights in preparation for conducting world-class airborne astronomy. The project is known as the Stratospheric Observatory for Infrared Astronomy, or SOFIA.

Photo Description	Erik Lindbergh, grandson of aviator Charles Lindbergh, unveiled a plaque commemorating his grandfather on the 80th anniversary of Charles Lindbergh's transatlantic flight. The event was a dedication of the 747 Clipper Lindbergh, a NASA airborne infrared observatory that is beginning test flights in preparation for conducting world-class airborne astronomy. The project is known as the Stratospheric Observatory for Infrared Astronomy, or SOFIA.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	05/21/2007

Photo Description	Erik Lindbergh, grandson of aviator Charles Lindbergh, unveiled a plaque commemorating his grandfather on the 80th anniversary of Charles Lindbergh's transatlantic flight. The event was a dedication of the 747 Clipper Lindbergh, a NASA airborne infrared observatory that is beginning test flights in preparation for conducting world-class airborne astronomy. The project is known as the Stratospheric Observatory for Infrared Astronomy, or SOFIA.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	05/21/2007

Erik Lindbergh christens NASA's 747 Clipper Lindbergh, the Stratospheric Observatory for Infrared Astronomy, with a special commemorative concoction representing local, NASA, and industry partners. The liquid consisted of a small amount of California wine representing NASA Dryden where the aircraft will be stationed, a small amount of Dr. Pepper (a Waco, TX invention), a quantity of French bottled water (to symbolize Charles Lindbergh's flight to Paris on this date), and a dash of German beer to represent the SOFIA German industry partners.

Photo Description	Erik Lindbergh christens NASA's 747 Clipper Lindbergh, the Stratospheric Observatory for Infrared Astronomy, with a special commemorative concoction representing local, NASA, and industry partners. The liquid consisted of a small amount of California wine representing NASA Dryden where the aircraft will be stationed, a small amount of Dr. Pepper (a Waco, TX invention), a quantity of French bottled water (to symbolize Charles Lindbergh's flight to Paris on this date), and a dash of German beer to represent the SOFIA German industry partners.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	05/21/2007

NASA's Boeing 747SP SOFIA airborne observatory soars over a bed of puffy clouds during its second checkout flight over the Texas countryside on May 10, 2007.

Photo Description	NASA's Boeing 747SP SOFIA airborne observatory soars over a bed of puffy clouds during its second checkout flight over the Texas countryside on May 10, 2007.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	May 10, 2007

NASA's Stratospheric Observatory for Infrared Astronomy is silhouetted against the sky as it soars on its second check flight near Waco, Texas on May 10, 2007.

Photo Description	NASA's Stratospheric Observatory for Infrared Astronomy is silhouetted against the sky as it soars on its second check flight near Waco, Texas on May 10, 2007.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	May 10, 2007

NASA's SOFIA airborne observatory is shadowed by a NASA F/A-18 safety chase aircraft during its second checkout flight near Waco, Texas on May 10, 2007.

Photo Description	NASA's SOFIA airborne observatory is shadowed by a NASA F/A-18 safety chase aircraft during its second checkout flight near Waco, Texas on May 10, 2007.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	May 10, 2007

Two NASA F/A-18s flown by NASA Dryden research pilots Jim Smolka and Nils Larson cruise over the Texas landscape after supporting a SOFIA check flight in May 2007.

Photo Description	Two NASA F/A-18s flown by NASA Dryden research pilots Jim Smolka and Nils Larson cruise over the Texas landscape after supporting a SOFIA check flight in May 2007.
Project Description	unknown
Photo Date	May 10, 2007

The SOFIA flight crew, consisting of Co-pilot Gordon Fullerton, DFRC, Pilot Bill Brocket, DFRC, Test Conductor Marty Trout, DFRC, Test Engineer Don Stonebrook, L-3, and Flight Engineer Larry Larose, JSC, descend the stairs after ferrying the 747SP airborne observatory from Waco, Texas, to its new home at NASA's Dryden Flight Research Center in California. NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, arrived at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif. on May 31, 2007. The heavily modified Boeing 747SP was ferried to Dryden from Waco, Texas, where L-3 Communications Integrated Systems installed a German-built 2.5-meter infrared telescope and made other major modifications over the past several years. SOFIA is scheduled to undergo installation and integration of mission systems and a multi-phase flight test program at Dryden over the next three years that is expected to lead to a full operational capability to conduct astronomy missions in about 2010. During its expected 20-year lifetime, SOFIA will be capable of "Great Observatory" class astronomical science, providing astronomers with access to the visible, infrared and sub-millimeter spectrum with optimized performance in the mid-infrared to sub-millimeter range.

The SOFIA flight crew descen …

Photo Description	The SOFIA flight crew, consisting of Co-pilot Gordon Fullerton, DFRC, Pilot Bill Brocket, DFRC, Test Conductor Marty Trout, DFRC, Test Engineer Don Stonebrook, L-3, and Flight Engineer Larry Larose, JSC, descend the stairs after ferrying the 747SP airborne observatory from Waco, Texas, to its new home at NASA's Dryden Flight Research Center in California. NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, arrived at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif. on May 31, 2007. The heavily modified Boeing 747SP was ferried to Dryden from Waco, Texas, where L-3 Communications Integrated Systems installed a German-built 2.5-meter infrared telescope and made other major modifications over the past several years. SOFIA is scheduled to undergo installation and integration of mission systems and a multi-phase flight test program at Dryden over the next three years that is expected to lead to a full operational capability to conduct astronomy missions in about 2010. During its expected 20-year lifetime, SOFIA will be capable of "Great Observatory" class astronomical science, providing astronomers with access to the visible, infrared and sub-millimeter spectrum with optimized performance in the mid-infrared to sub-millimeter range.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	May 31, 2007

NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) Boeing 747SP flares for landing at Edwards AFB after a ferry flight from Waco, Texas. NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, arrived at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif. on May 31, 2007. The heavily modified Boeing 747SP was ferried to Dryden from Waco, Texas, where L-3 Communications Integrated Systems installed a German-built 2.5-meter infrared telescope and made other major modifications over the past several years. SOFIA is scheduled to undergo installation and integration of mission systems and a multi-phase flight test program at Dryden over the next three years that is expected to lead to a full operational capability to conduct astronomy missions in about 2010. During its expected 20-year lifetime, SOFIA will be capable of "Great Observatory" class astronomical science, providing astronomers with access to the visible, infrared and sub-millimeter spectrum with optimized performance in the mid-infrared to sub-millimeter range.

Photo Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) Boeing 747SP flares for landing at Edwards AFB after a ferry flight from Waco, Texas. NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, arrived at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif. on May 31, 2007. The heavily modified Boeing 747SP was ferried to Dryden from Waco, Texas, where L-3 Communications Integrated Systems installed a German-built 2.5-meter infrared telescope and made other major modifications over the past several years. SOFIA is scheduled to undergo installation and integration of mission systems and a multi-phase flight test program at Dryden over the next three years that is expected to lead to a full operational capability to conduct astronomy missions in about 2010. During its expected 20-year lifetime, SOFIA will be capable of "Great Observatory" class astronomical science, providing astronomers with access to the visible, infrared and sub-millimeter spectrum with optimized performance in the mid-infrared to sub-millimeter range.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	May 31, 2007

NASA's SOFIA 747SP bearing a German-built 2.5-meter infrared telescope in its rear fuselage taxis up to NASA Dryden's ramp after a ferry flight from Waco, Texas. NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, arrived at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif. on May 31, 2007. The heavily modified Boeing 747SP was ferried to Dryden from Waco, Texas, where L-3 Communications Integrated Systems installed a German-built 2.5-meter infrared telescope and made other major modifications over the past several years. SOFIA is scheduled to undergo installation and integration of mission systems and a multi-phase flight test program at Dryden over the next three years that is expected to lead to a full operational capability to conduct astronomy missions in about 2010. During its expected 20-year lifetime, SOFIA will be capable of "Great Observatory" class astronomical science, providing astronomers with access to the visible, infrared and sub-millimeter spectrum with optimized performance in the mid-infrared to sub-millimeter range.

NASA's SOFIA 747SP bearing a …

Photo Description	NASA's SOFIA 747SP bearing a German-built 2.5-meter infrared telescope in its rear fuselage taxis up to NASA Dryden's ramp after a ferry flight from Waco, Texas. NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, arrived at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif. on May 31, 2007. The heavily modified Boeing 747SP was ferried to Dryden from Waco, Texas, where L-3 Communications Integrated Systems installed a German-built 2.5-meter infrared telescope and made other major modifications over the past several years. SOFIA is scheduled to undergo installation and integration of mission systems and a multi-phase flight test program at Dryden over the next three years that is expected to lead to a full operational capability to conduct astronomy missions in about 2010. During its expected 20-year lifetime, SOFIA will be capable of "Great Observatory" class astronomical science, providing astronomers with access to the visible, infrared and sub-millimeter spectrum with optimized performance in the mid-infrared to sub-millimeter range.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	May 31, 2007

NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) Boeing 747SP flies over NASA's Dryden Flight Research Center after a ferry flight from Waco, Texas. NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, arrived at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif. on May 31, 2007. The heavily modified Boeing 747SP was ferried to Dryden from Waco, Texas, where L-3 Communications Integrated Systems installed a German-built 2.5-meter infrared telescope and made other major modifications over the past several years. SOFIA is scheduled to undergo installation and integration of mission systems and a multi-phase flight test program at Dryden over the next three years that is expected to lead to a full operational capability to conduct astronomy missions in about 2010. During its expected 20-year lifetime, SOFIA will be capable of "Great Observatory" class astronomical science, providing astronomers with access to the visible, infrared and sub-millimeter spectrum with optimized performance in the mid-infrared to sub-millimeter range.

Photo Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) Boeing 747SP flies over NASA's Dryden Flight Research Center after a ferry flight from Waco, Texas. NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, arrived at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif. on May 31, 2007. The heavily modified Boeing 747SP was ferried to Dryden from Waco, Texas, where L-3 Communications Integrated Systems installed a German-built 2.5-meter infrared telescope and made other major modifications over the past several years. SOFIA is scheduled to undergo installation and integration of mission systems and a multi-phase flight test program at Dryden over the next three years that is expected to lead to a full operational capability to conduct astronomy missions in about 2010. During its expected 20-year lifetime, SOFIA will be capable of "Great Observatory" class astronomical science, providing astronomers with access to the visible, infrared and sub-millimeter spectrum with optimized performance in the mid-infrared to sub-millimeter range.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	May 31, 2007

NASA's SOFIA airborne observatory lands at Edwards AFB after being flown from Waco, Texas to NASA Dryden for systems installation, integration and flight test. NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, arrived at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif. on May 31, 2007. The heavily modified Boeing 747SP was ferried to Dryden from Waco, Texas, where L-3 Communications Integrated Systems installed a German-built 2.5-meter infrared telescope and made other major modifications over the past several years. SOFIA is scheduled to undergo installation and integration of mission systems and a multi-phase flight test program at Dryden over the next three years that is expected to lead to a full operational capability to conduct astronomy missions in about 2010. During its expected 20-year lifetime, SOFIA will be capable of "Great Observatory" class astronomical science, providing astronomers with access to the visible, infrared and sub-millimeter spectrum with optimized performance in the mid-infrared to sub-millimeter range.

Photo Description	NASA's SOFIA airborne observatory lands at Edwards AFB after being flown from Waco, Texas to NASA Dryden for systems installation, integration and flight test. NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, arrived at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif. on May 31, 2007. The heavily modified Boeing 747SP was ferried to Dryden from Waco, Texas, where L-3 Communications Integrated Systems installed a German-built 2.5-meter infrared telescope and made other major modifications over the past several years. SOFIA is scheduled to undergo installation and integration of mission systems and a multi-phase flight test program at Dryden over the next three years that is expected to lead to a full operational capability to conduct astronomy missions in about 2010. During its expected 20-year lifetime, SOFIA will be capable of "Great Observatory" class astronomical science, providing astronomers with access to the visible, infrared and sub-millimeter spectrum with optimized performance in the mid-infrared to sub-millimeter range.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	May 31, 2007

SOFIA Airborne Observatory A …

Erik Lindbergh, grandson of famed aviator Charles Lindbergh, yanks the bunting to reveal the Clipper Lindbergh name on NASA's SOFIA Boeing 747SP on June 27, 2007. More than 250 VIPs, news media and guests joined NASA, DLR, USRA and other SOFIA staff for the debut of the airborne observatory at NASA Dryden.

Photo Description	Erik Lindbergh, grandson of famed aviator Charles Lindbergh, yanks the bunting to reveal the Clipper Lindbergh name on NASA's SOFIA Boeing 747SP on June 27, 2007. More than 250 VIPs, news media and guests joined NASA, DLR, USRA and other SOFIA staff for the debut of the airborne observatory at NASA Dryden.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	June 27, 2007

Erik Lindbergh, grandson of famed aviator Charles Lindbergh, rededicated the SOFIA Boeing 747SP as the Clipper Lindbergh at NASA Dryden on June 27, 2007.

Photo Description	Erik Lindbergh, grandson of famed aviator Charles Lindbergh, rededicated the SOFIA Boeing 747SP as the Clipper Lindbergh at NASA Dryden on June 27, 2007.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	June 27, 2007

More than 250 VIPs, news media and guests joined NASA, DLR, USRA and other SOFIA staff for the debut of the airborne observatory at NASA DFRC on June 27, 2007.

Photo Description	More than 250 VIPs, news media and guests joined NASA, DLR, USRA and other SOFIA staff for the debut of the airborne observatory at NASA DFRC on June 27, 2007.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	June 27, 2007

Relocation Flight of SOFIA f …

Debut of NASA's Stratospheri …

NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, arrived at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif. on May 31, 2007. The heavily modified Boeing 747SP was ferried to Dryden from Waco, Texas, where L-3 Communications Integrated Systems installed a German-built 2.5-meter infrared telescope and made other major modifications over the past several years. SOFIA is scheduled to undergo installation and integration of mission systems and a multi-phase flight test program at Dryden over the next three years that is expected to lead to a full operational capability to conduct astronomy missions in about 2010. During its expected 20-year lifetime, SOFIA will be capable of "Great Observatory" class astronomical science, providing astronomers with access to the visible, infrared and sub-millimeter spectrum with optimized performance in the mid-infrared to sub-millimeter range.

NASA's SOFIA infrared observ …

Photo Description	NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, arrived at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif. on May 31, 2007. The heavily modified Boeing 747SP was ferried to Dryden from Waco, Texas, where L-3 Communications Integrated Systems installed a German-built 2.5-meter infrared telescope and made other major modifications over the past several years. SOFIA is scheduled to undergo installation and integration of mission systems and a multi-phase flight test program at Dryden over the next three years that is expected to lead to a full operational capability to conduct astronomy missions in about 2010. During its expected 20-year lifetime, SOFIA will be capable of "Great Observatory" class astronomical science, providing astronomers with access to the visible, infrared and sub-millimeter spectrum with optimized performance in the mid-infrared to sub-millimeter range.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	October 11, 2007

Photo Description	NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, arrived at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif. on May 31, 2007. The heavily modified Boeing 747SP was ferried to Dryden from Waco, Texas, where L-3 Communications Integrated Systems installed a German-built 2.5-meter infrared telescope and made other major modifications over the past several years. SOFIA is scheduled to undergo installation and integration of mission systems and a multi-phase flight test program at Dryden over the next three years that is expected to lead to a full operational capability to conduct astronomy missions in about 2010. During its expected 20-year lifetime, SOFIA will be capable of "Great Observatory" class astronomical science, providing astronomers with access to the visible, infrared and sub-millimeter spectrum with optimized performance in the mid-infrared to sub-millimeter range.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	October 11, 2007

Photo Description	NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, arrived at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif. on May 31, 2007. The heavily modified Boeing 747SP was ferried to Dryden from Waco, Texas, where L-3 Communications Integrated Systems installed a German-built 2.5-meter infrared telescope and made other major modifications over the past several years. SOFIA is scheduled to undergo installation and integration of mission systems and a multi-phase flight test program at Dryden over the next three years that is expected to lead to a full operational capability to conduct astronomy missions in about 2010. During its expected 20-year lifetime, SOFIA will be capable of "Great Observatory" class astronomical science, providing astronomers with access to the visible, infrared and sub-millimeter spectrum with optimized performance in the mid-infrared to sub-millimeter range.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	October 11, 2007

NASA Dryden's mockup Orion crew module is located in Dryden's Shuttle hangar, where abort flight test equipment is being positioned.

Photo Description	NASA Dryden's mockup Orion crew module is located in Dryden's Shuttle hangar, where abort flight test equipment is being positioned.
Project Description	A mockup Orion crew module has been constructed by NASA Dryden Flight Research Center's Fabrication Branch. The mockup is being used to develop integration procedures for avionics and instrumentation in advance of the arrival of the first abort flight test article. The Abort Flight Test effort is managed by NASA Dryden under the leadership of the Project Orion Flight Test Office at NASA's Johnson Space Center, Houston, Texas.
Photo Date	September 25, 2007

Rogers Dry Lake serves as a backdrop for a mockup Orion crew module built by NASA Dryden Flight Research Center's Fabrication Branch. The module was relocated to Dryden's Shuttle hangar on Sept. 25, 2007.

Photo Description	Rogers Dry Lake serves as a backdrop for a mockup Orion crew module built by NASA Dryden Flight Research Center's Fabrication Branch. The module was relocated to Dryden's Shuttle hangar on Sept. 25, 2007.
Project Description	A mockup Orion crew module has been constructed by NASA Dryden Flight Research Center's Fabrication Branch. The mockup is being used to develop integration procedures for avionics and instrumentation in advance of the arrival of the first abort flight test article. The Abort Flight Test effort is managed by NASA Dryden under the leadership of the Project Orion Flight Test Office at NASA's Johnson Space Center, Houston, Texas.
Photo Date	September 25, 2007

A mockup Orion crew module built by NASA Dryden Flight Research Center's Fabrication Branch gets a lift from its construction site to its new home in Dryden's Shuttle hangar.

Photo Description	A mockup Orion crew module built by NASA Dryden Flight Research Center's Fabrication Branch gets a lift from its construction site to its new home in Dryden's Shuttle hangar.
Project Description	A mockup Orion crew module has been constructed by NASA Dryden Flight Research Center's Fabrication Branch. The mockup is being used to develop integration procedures for avionics and instrumentation in advance of the arrival of the first abort flight test article. The Abort Flight Test effort is managed by NASA Dryden under the leadership of the Project Orion Flight Test Office at NASA's Johnson Space Center, Houston, Texas.
Photo Date	September 25, 2007

Air-to-Air Video of SOFIA Ai …

SOFIA Airborne Observatory T …

SOFIA Airborne Observatory S …

Photo Description	NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, arrived at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif. on May 31, 2007. The heavily modified Boeing 747SP was ferried to Dryden from Waco, Texas, where L-3 Communications Integrated Systems installed a German-built 2.5-meter infrared telescope and made other major modifications over the past several years. SOFIA is scheduled to undergo installation and integration of mission systems and a multi-phase flight test program at Dryden over the next three years that is expected to lead to a full operational capability to conduct astronomy missions in about 2010. During its expected 20-year lifetime, SOFIA will be capable of "Great Observatory" class astronomical science, providing astronomers with access to the visible, infrared and sub-millimeter spectrum with optimized performance in the mid-infrared to sub-millimeter range.
Project Description	NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) is being developed as a world-class observatory complementing the Hubble Space Telescope. The observatory, which features a German-built 98.4-inch (2.5 meter) diameter infrared telescope weighing 20 metric tons mounted in a highly-modified Boeing 747SP aircraft, has begun its flight test phase in a joint program by NASA and DLR Deutsches Zentrum fur Luft und Raumfahrt (German Aerospace Center). Major aircraft modifications and installation of the telescope was performed by L-3 Communications Integrated Systems facility at Waco, Texas. Systems integration and flight test operations are being conducted at NASA's Dryden Flight Resarch Center at Edwards Air Force Base, Calif. SOFIA's science and mission operations are managed jointly by the Universities Space Research Association (USRA) and the Deutsches SOFIA Institut (DSI), and are based at NASA's Ames Research Center at Moffett Field near San Jose, Calif. Once operational in the 2009-2010 period, SOFIA will be the world's primary infrared observatory during a mission lasting up to 20 years, as well as an outstanding laboratory for developing and testing instrumentation and detector technology.
Photo Date	October 11, 2007

Floods in Kansas and Missour …

Title	Floods in Kansas and Missouri
Description	The skies over southeastern Kansas were filled with a mix of cloud and haze on July 2, 2007, when the Moderate Resolution Imaging Spectroradiometer (MODIS [ http://modis.gsfc.nasa.gov ]) on NASA's Terra [ http://terra.nasa.gov/ ] satellite captured the top image. But beneath the clouds, the flood-swollen Neosho and Verdigris Rivers and tributaries can be seen. Normally these river rivers would be too small to be visible in MODIS images (as shown by the lower image from June 8, 2007), but on July 2, the rivers paint a wide blue ribbon across the Kansas plains. Water is normally black in this type of false-color image, which is made with visible and infrared light. On July 2, the rivers are blue partly because sediment colors the water and partly because sunlight is reflecting off the surface of the water. Clouds are light turquoise and white, plant-covered land is green, and bare earth (largely freshly planted, rectangular farm fields) is tan. Additional flooding in western Missouri is visible in the large images. By July 2, the floods had forced thousands from their homes throughout Kansas, Missouri, Oklahoma, and Texas, reported CNN. The flood-swollen Verdigris River, image center, surrounded an oil refinery in Coffeyville, Kansas, where more than 42,000 gallons of crude oil spilled into the river, said CNN. The polluted portion of the river is under clouds in this image. The storms and the flooding in Kansas led President Bush to declare a major disaster in the state, CNN added. The Neosho River, along the right side of the image, crested at 35 feet, 10 feet above flood stage, at its highest point on July 2, and the Verdigris reached its highest point, 49 feet, 19 feet above flood stage, in Independence, Kansas, said the National Weather Service. [ http://www.nws.noaa.gov/oh/hic/dirlistings/data/ICT/021424_ICT_Hydrologic_Summary ]Daily images [ http://rapidfire.sci.gsfc.nasa.gov/subsets/?USA7/2007183 ] of Kansas are available from the MODIS Rapid Response System. NASA images courtesy the MODIS Rapid Response Team [ http://rapidfire.sci.gsfc.nasa.gov ] at NASA GSFC.

Floods in Kansas and Missour …

Title	Floods in Kansas and Missouri
Description	The skies over southeastern Kansas were filled with a mix of cloud and haze on July 2, 2007, when the Moderate Resolution Imaging Spectroradiometer (MODIS [ http://modis.gsfc.nasa.gov ]) on NASA's Terra [ http://terra.nasa.gov/ ] satellite captured the top image. But beneath the clouds, the flood-swollen Neosho and Verdigris Rivers and tributaries can be seen. Normally these river rivers would be too small to be visible in MODIS images (as shown by the lower image from June 8, 2007), but on July 2, the rivers paint a wide blue ribbon across the Kansas plains. Water is normally black in this type of false-color image, which is made with visible and infrared light. On July 2, the rivers are blue partly because sediment colors the water and partly because sunlight is reflecting off the surface of the water. Clouds are light turquoise and white, plant-covered land is green, and bare earth (largely freshly planted, rectangular farm fields) is tan. Additional flooding in western Missouri is visible in the large images. By July 2, the floods had forced thousands from their homes throughout Kansas, Missouri, Oklahoma, and Texas, reported CNN. The flood-swollen Verdigris River, image center, surrounded an oil refinery in Coffeyville, Kansas, where more than 42,000 gallons of crude oil spilled into the river, said CNN. The polluted portion of the river is under clouds in this image. The storms and the flooding in Kansas led President Bush to declare a major disaster in the state, CNN added. The Neosho River, along the right side of the image, crested at 35 feet, 10 feet above flood stage, at its highest point on July 2, and the Verdigris reached its highest point, 49 feet, 19 feet above flood stage, in Independence, Kansas, said the National Weather Service. [ http://www.nws.noaa.gov/oh/hic/dirlistings/data/ICT/021424_ICT_Hydrologic_Summary ]Daily images [ http://rapidfire.sci.gsfc.nasa.gov/subsets/?USA7/2007183 ] of Kansas are available from the MODIS Rapid Response System. NASA images courtesy the MODIS Rapid Response Team [ http://rapidfire.sci.gsfc.nasa.gov ] at NASA GSFC.

Floods in Texas and Oklahoma

Title	Floods in Texas and Oklahoma
Description	Heavy rains pounded the Southern Plains of the United States during mid-June when moisture from the Gulf of Mexico streamed northward into a slow-moving frontal system. The result was extensive flooding over parts of Texas and Oklahoma. On Monday, June 18, 2007, six flood-related deaths were reported in northern Texas as storms dumped up to 8 inches (abut 200 millimeters) of rain in the area. On Tuesday, additional storms dumped heavy rains over parts of northwestern Oklahoma, forcing several road closures, said news reports. This image shows rainfall totals for June 14 through June 20, 2007. The rainfall totals are from the near-real-time, Multi-satellite Precipitation Analysis (MPA), which is based on measurements taken by the Tropical Rainfall Measuring Mission (TRMM [ http://trmm.gsfc.nasa.gov/ ]) satellite. The MPA analysis indicates that during this time more than 200 millimeters (about 8 inches, red area) of rain fell in northern Texas just south of the Oklahoma border, where flooding was reported. A much broader area of at least 150 to 200 millimeters (about 6 to 8 inches) of rain covers most of northwest Oklahoma. Based on these totals, the TRMM team predicted that flooding was likely or occurring. The group produces a global map [ http://trmm.gsfc.nasa.gov/publications_dir/potential_flood.html ] indicating where there is a high potential for flooding based on rainfall totals. TRMM is a joint mission between NASA and the Japanese space agency, JAXA. Image produced by Hal Pierce (SSAI/NASA GSFC) and caption by Hal Pierce and Steve Lang (SSAI/NASA GSFC).

Floods in Texas and Oklahoma

Title	Floods in Texas and Oklahoma
Description	June 2007 was exceptionally wet for the Southern Plains of the United States because a stagnant weather pattern focused moisture and storms over Texas and Oklahoma. The latest round of heavy storms dumped up to 460 millimeters (18 inches) of rain in parts of central Texas on the night of Tuesday, June 26, said news reports. For Austin, the state's capital, more than 30 inches of rain has fallen since January, making 2007 the wettest year on record so far according to local news reports. This image shows rainfall totals from the near-real-time, Multi-satellite Precipitation Analysis (MPA), which is based on rainfall data collected by the Tropical Rainfall Measuring Mission TRMM [ http://trmm.gsfc.nasa.gov/ ]) satellite. The totals shown here indicate how much rain fell between June 20 and June 28, 2007. Splotches of red over central Texas and southern Oklahoma indicate where the MPA tallied up to 200 millimeters (8 inches) of rain. A broad area of at least 50 mm (about 2 inches) of rainfall covers almost all of Texas and Oklahoma. These totals fall short of totals reported on the ground because the satellites used in the MPA can't see areas of localized heavy rain. These satellites "zoom in" to approximately 30 kilometers (20 miles), and so miss smaller areas of intense rain. TRMM is a joint mission between NASA and the Japanese space agency, JAXA. Image produced by Hal Pierce (SSAI/NASA GSFC) and caption by and Steve Lang (SSAI/NASA GSFC).

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