|
|
SMART-1 Looks Back
| title |
SMART-1 Looks Back |
| description |
The first picture of Earth taken by the SMART-1 spacecraft on 21 May 2004 from a distance of 70,000 kilometres. The image shows from top left, Scandinavia, Denmark, United Kingdom and clear west and northern France. Southern France and Spain are at the centre under cloud cover. North Africa is bottom right (in the full-resoltion image). The image was taken by the Advanced Moon Micro-Imager Experiment (AMIE) camera. This imaging system has been developed by the Space-X company in Neuchatel, Switzerland. The AMIE camera is a remarkably compact design, a package of dedicated optics, electronics and mechanical interfaces that weighs only 450 grams. Once in orbit around the Moon, AMIE will survey the lunar terrain using visible and near-infrared light, providing clues about its chemical composition and geological history."The image shows clearly that the AMIE camera works well, and that we are really in space," says Principal Investigator Jean Luc Josset, Space-X."This picture is a great view of Earth seen as a planet," says ESA Project Scientist Bernard Foing. "Further synoptic images of Earth obtained during the cruise phase will be used to compare the signature of geophysical processes with what we shall measure on the Moon." *Image Credit*: European Space Agency |
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Hubble Sees 'Comet Galaxy' B
| Title |
Hubble Sees 'Comet Galaxy' Being Ripped Apart By Galaxy Cluster |
|
SOLAR FLARE LEAVES SUN QUAKI
| Description |
SOLAR FLARE LEAVES SUN QUAKING Scientists have shown for the first time that solar flares produce seismic waves in the Sun's interior that closely resemble those created by earthquakes on our planet. The researchers observed a flare-generated solar quake that contained about 40,000 times the energy released in the great earthquake that devastated San Francisco in 1906. The amount of energy released was enough to power the United States for 20 years at its current level of consumption, and was equivalent to an 11.3 magnitude earthquake, scientists calculated. Dr. Alexander G. Kosovichev, a senior research scientist from Stanford University, and Dr. Valentina V. Zharkova from Glasgow (United Kingdom) University found the tell-tale seismic signature in data on the Sun's surface collected by the Michelson Doppler Imager onboard the Solar and Heliospheric Observatory (SOHO) spacecraft immediately following a moderate-sized flare on July 9, 1996. "Although the flare was a moderate one, it still released an immense amount of energy," said Dr. Craig Deforest, a researcher with the SOHO project. "The energy released is equal to completely covering the Earth's continents with a yard of dynamite and detonating it all at once." SOHO is a joint project of the European Space Agency and NASA. The finding is reported in the May 28 issue of the journal Nature, and is the subject of a press conference at the spring meeting of the American Geophysical Union in Boston, Mass., May 27. The solar quake that the science team recorded looks much like ripples spreading from a rock dropped into a pool of water. But over the course of an hour, the solar waves traveled for a distance equal to 10 Earth diameters before fading into the fiery background of the Sun's photosphere. Unlike water ripples that travel outward at a constant velocity, the solar waves accelerated from an initial speed of 22,000 miles per hour to a maximum of 250,000 miles per hour before disappearing. "People have looked for evidence of seismic waves from flares before, but they didn't have a theory so they didn't know where to look," says Kosovichev. Several years ago Kosovichev and Zharkova developed a theory that can explain how a flare, which explodes in space above the Sun's surface, can generate a major seismic wave in the Sun's interior. According to the currently accepted model of solar flares, the primary explosion creates high-energy electrons (electrically charged subatomic particles). These are funneled down into a magnetic flux tube, an invisible tube of magnetic energy, and produce X-rays, microwaves and a shock wave that heats the solar surface. Kosovichev and Zharkova developed a theory that predicts the nature and magnitude of the shock waves that this beam of energetic electrons should create when they slam down into the solar atmosphere. Although their theory directed them to the right area to search for the seismic waves, the waves that they found were 10 times stronger than they had, predicted. "They were so strong that you can see them in the raw data," Kosovichev says. The solar seismic waves appear to be compression waves like the "P" waves generated by an earthquake. They travel throughout the Sun's interior. In fact, the waves should recombine on the opposite side of the Sun from the location of the flare to create a faint duplicate of the original ripple pattern, Kosovichev predicts. Now that they know how to find them, the SOHO scientists say that the seismic waves generated by solar flares should allow them to verify independently some of the conditions in the solar interior that they have inferred from studying the pattern of waves that are continually ruffling the Sun's surface. SOHO is part of the International Solar-Terrestrial Physics (ISTP) program, a global effort to observe and understand our star and its effects on our environment. The ISTP mission includes more than 20 satellites, coupled with with ground-based observatories and modeling centers, that allow scientists to study the Sun, the Earth, and the space between them in unprecedented detail. ISTP is a joint program of NASA, ESA, Japan's Institute for Astronautical Science, and Russia's Space Research Institute. |
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NASA?s Marshall Space Flight
| Name of Image |
NASA?s Marshall Space Flight Center (MSFC) Contributes to Solar B/Hinode |
| Date of Image |
2006-08-09 |
| Full Description |
Hinode (Sunrise), formerly known as Solar-B before reaching orbit, was launched from the Uchinoura Space Center in Japan on September 23, 2006. Hinode was designed to probe into the Sun?s magnetic field to better understand the origin of solar disturbances which interfere with satellite communications, electrical power transmission grids, and the safety of astronauts traveling beyond the Earth?s magnetic field. Hinode is circling Earth in a polar orbit that places the instruments in continuous sunlight for nine months each year and allows data dumps to a high latitude European Space Agency (ESA) ground station every orbit. NASA and other science teams will support instrument operations and data collection from the spacecraft?s operation center at the Japanese Aerospace Exploration Agency?s (JAXA?s) Institute of Space and Aeronautical Science facility located in Tokyo. The Hinode spacecraft is a collaboration among space agencies of Japan, the United States, the United Kingdom, and Europe. The Marshall Space Flight Center (MSFC) managed development of three instruments comprising the spacecraft, the Solar Optical Telescope (SOT), the X-Ray Telescope (XRT), and the Extreme Ultraviolet (EUV) Imaging Spectrometer (EIS). Provided by the Multimedia support group at MSFC, this rendering illustrates the Solar-B Spacecraft in earth orbit with its solar panels partially extended. |
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NASA?s Marshall Space Flight
| Name of Image |
NASA?s Marshall Space Flight Center (MSFC) Contributes to Solar B/Hinode |
| Date of Image |
2006-08-09 |
| Full Description |
Hinode (Sunrise), formerly known as Solar-B before reaching orbit, was launched from the Uchinoura Space Center in Japan on September 23, 2006. Hinode was designed to probe into the Sun?s magnetic field to better understand the origin of solar disturbances which interfere with satellite communications, electrical power transmission grids, and the safety of astronauts traveling beyond the Earth?s magnetic field. Hinode is circling Earth in a polar orbit that places the instruments in continuous sunlight for nine months each year and allows data dumps to a high latitude European Space Agency (ESA) ground station every orbit. NASA and other science teams will support instrument operations and data collection from the spacecraft?s operation center at the Japanese Aerospace Exploration Agency?s (JAXA?s) Institute of Space and Aeronautical Science facility located in Tokyo. The Hinode spacecraft is a collaboration among space agencies of Japan, the United States, the United Kingdom, and Europe. The Marshall Space Flight Center (MSFC) managed development of three instruments comprising the spacecraft, the Solar Optical Telescope (SOT), the X-Ray Telescope (XRT), and the Extreme Ultraviolet (EUV) Imaging Spectrometer (EIS). Provided by the Multimedia support group at MSFC, this video clip is an animated illustration of the Solar-B Spacecraft in earth orbit. |
|
NASA?s Marshall Space Flight
| Name of Image |
NASA?s Marshall Space Flight Center (MSFC) Contributes to Solar B/Hinode |
| Date of Image |
2006-08-09 |
| Full Description |
Hinode (Sunrise), formerly known as Solar-B before reaching orbit, was launched from the Uchinoura Space Center in Japan on September 23, 2006. Hinode was designed to probe into the Sun?s magnetic field to better understand the origin of solar disturbances which interfere with satellite communications, electrical power transmission grids, and the safety of astronauts traveling beyond the Earth?s magnetic field. Hinode is circling Earth in a polar orbit that places the instruments in continuous sunlight for nine months each year and allows data dumps to a high latitude European Space Agency (ESA) ground station every orbit. NASA and other science teams will support instrument operations and data collection from the spacecraft?s operation center at the Japanese Aerospace Exploration Agency?s (JAXA?s) Institute of Space and Aeronautical Science facility located in Tokyo. The Hinode spacecraft is a collaboration among space agencies of Japan, the United States, the United Kingdom, and Europe. The Marshall Space Flight Center (MSFC) managed development of three instruments comprising the spacecraft, the Solar Optical Telescope (SOT), the X-Ray Telescope (XRT), and the Extreme Ultraviolet (EUV) Imaging Spectrometer (EIS). Provided by the Multimedia support group at MSFC, this rendering illustrates the Solar-B Spacecraft in earth orbit with its solar panels completely extended. |
|
Solar B/Hinode Image of Suns
| Name of Image |
Solar B/Hinode Image of Sunspot |
| Date of Image |
2005-08-09 |
| Full Description |
Hinode (Sunrise), formerly known as Solar-B before reaching orbit, was launched from the Uchinoura Space Center in Japan on September 23, 2006. Hinode was designed to probe into the Sun?s magnetic field to better understand the origin of solar disturbances which interfere with satellite communications, electrical power transmission grids, and the safety of astronauts traveling beyond the Earth?s magnetic field. Hinode is circling Earth in a polar orbit that places the instruments in continuous sunlight for nine months each year and allows data dumps to a high latitude European Space Agency (ESA) ground station every orbit. NASA and other science teams will support instrument operations and data collection from the spacecraft?s operation center at the Japanese Aerospace Exploration Agency?s (JAXA?s) Institute of Space and Aeronautical Science facility located in Tokyo. The Hinode spacecraft is a collaboration among space agencies of Japan, the United States, the United Kingdom, and Europe. The Marshall Space Flight Center (MSFC) managed development of three instruments comprising the spacecraft, the Solar Optical Telescope (SOT), the X-Ray Telescope (XRT), and the Extreme Ultraviolet (EUV) Imaging Spectrometer (EIS). This image of a sunspot, taken by Hinode, is a prime example of what the spacecraft can offer. |
|
NASA?s Marshall Space Flight
| Name of Image |
NASA?s Marshall Space Flight Center (MSFC) Contributes to Solar B/Hinode |
| Date of Image |
2006-08-09 |
| Full Description |
Hinode (Sunrise), formerly known as Solar-B before reaching orbit, was launched from the Uchinoura Space Center in Japan on September 23, 2006. Hinode was designed to probe into the Sun?s magnetic field to better understand the origin of solar disturbances which interfere with satellite communications, electrical power transmission grids, and the safety of astronauts traveling beyond the Earth?s magnetic field. Hinode is circling Earth in a polar orbit that places the instruments in continuous sunlight for nine months each year and allows data dumps to a high latitude European Space Agency (ESA) ground station every orbit. NASA and other science teams will support instrument operations and data collection from the spacecraft?s operation center at the Japanese Aerospace Exploration Agency?s (JAXA?s) Institute of Space and Aeronautical Science facility located in Tokyo. The Hinode spacecraft is a collaboration among space agencies of Japan, the United States, the United Kingdom, and Europe. The Marshall Space Flight Center (MSFC) managed development of three instruments comprising the spacecraft, the Solar Optical Telescope (SOT), the X-Ray Telescope (XRT), and the Extreme Ultraviolet (EUV) Imaging Spectrometer (EIS). Provided by the Multimedia support group at MSFC, this video clip is an animated illustration of the Solar-B Spacecraft in earth orbit. |
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Double Exposure Image of Spa
| Name of Image |
Double Exposure Image of Spacelab-1 in Cargo Bay of Orbiter Columbia |
| Date of Image |
1983-01-01 |
| Full Description |
This double exposure image shows Spacelab-1 in the cargo bay of orbiter Columbia. From top to bottom inside the cargo bay are the Spacelab Access Turnel, which is connected to the mid-deck of the orbiter, the Spacelab module, a pressurized module in which scientists conduct experiments not possible on Earth, and Spacelab pallets, which can hold instruments for the experiments requiring direct exposure to space. The first Spacelab mission, Spacelab-1, sponsored jointly and shared equally by NASA and the European Space Agency, was a multidisciplinary mission, that is, investigations were performed in several different fields of scientific research. The overall goal of the mission was to verify Spacelab performance through a variety of scientific experiments. The disciplines represented by these experiments were astronomy and solar physics, earth observations, space plasma physics, materials sciences, atmospheric physics, and life sciences. International in nature, Spacelab-1 conducted experiments from the United States, Japan, the Netherlands, United Kingdom, Beluga, France, Germany, Italy, and Switzerland. Spacelab-1 was launched from the Kennedy Space Center on November 28, 1983 aboard the orbiter Columbia (STS-9). The Marshall Space Flight Center was responsible for managing the Spacelab missions. |
|
Spacelab-1 Module
| Name of Image |
Spacelab-1 Module |
| Date of Image |
1983-01-01 |
| Full Description |
This photograph shows the Spacelab-1 module and Spacelab access turnel being installed in the cargo bay of orbiter Columbia for the STS-9 mission. The oribiting laboratory, built by the European Space Agency, is capable of supporting many types of scientific research that can best be performed in space. The Spacelab access tunnel, the only major piece of Spacelab hardware made in the U.S., connects the module with the mid-deck level of the orbiter cabin. The first Spacelab mission, Spacelab-1, sponsored jointly and shared equally by NASA and the European Space Agency, was a multidisciplinary mission, that is, investigations were performed in several different fields of scientific research. The overall goal of the mission was to verify Spacelab performance through a variety of scientific experiments. The disciplines represented by these experiments were: astronomy and solar physics, earth observations, space plasma physics, materials sciences, atmospheric physics, and life sciences. International in nature, Spacelab-1 conducted experiments from the United States, Japan, the Netherlands, United Kingdom, Beluga, France, Germany, Italy, and Switzerland. Spacelab-1, was launched from the Kennedy Space Center on November 28, 1983 aboard the orbiter Columbia (STS-9). The Marshall Space Flight Center was responsible for managing the Spacelab missions. |
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International Space Station
| Name of Image |
International Space Station |
| Date of Image |
1998-01-01 |
| Full Description |
This artist's digital concept depicts the completely assembled International Space Station (ISS) passing over Florida. As a gateway to permanent human presence in space, the Space Station Program is to expand knowledge benefiting all people and nations. The ISS is a multidisciplinary laboratory, technology test bed, and observatory that will provide unprecedented undertakings in scientific, technological, and international experimentation. Experiments to be conducted in the ISS include: microgravity research, Earth science, space science, life sciences, space product development, and engineering research and technology. The sixteen countries participating the ISS are: United States, Russian Federation, Canada, Japan, United Kingdom, Germany, Italy, France, Norway, Netherlands, Belgium, Spain, Denmark, Sweden, Switzerland, and Brazil. |
|
International Space Station
| Name of Image |
International Space Station |
| Date of Image |
1998-01-01 |
| Full Description |
This artist's concept depicts the completely assembled International Space Station (ISS) passing over Florida and the Bahamas. As a gateway to permanent human presence in space, the Space Station Program is to expand knowledge benefiting all people and nations. The ISS is a multidisciplinary laboratory, technology test bed, and observatory that will provide unprecedented undertakings in scientific, technological, and international experimentation. Experiments to be conducted in the ISS include: microgravity research, Earth science, space science, life sciences, space product development, and engineering research and technology. The sixteen countries participating in the ISS are: United States, Russian Federation, Canada, Japan, United Kingdom, Germany, Italy, France, Norway, Netherlands, Belgium, Spain, Denmark, Sweden, Switzerland, and Brazil. |
|
International Space Station
| Name of Image |
International Space Station |
| Date of Image |
1998-01-01 |
| Full Description |
This artist's concept depicts the completely assembled International Space Station (ISS) passing over the Straits of Gibraltar and the Mediterranean Sea. As a gateway to permanent human presence in space, the Space Station Program is to expand knowledge benefiting all people and nations. The ISS is a multidisciplinary laboratory, technology test bed, and observatory that will provide unprecedented undertakings in scientific, technological, and international experimentation. Experiments to be conducted in the ISS include: microgravity research, Earth science, space science, life sciences, space product development, and engineering research and technology. The sixteen countries participating the ISS are: United States, Russian Federation, Canada, Japan, United Kingdom, Germany, Italy, France, Norway, Netherlands, Belgium, Spain, Denmark, Sweden, Switzerland, and Brazil. |
|
International Space Station
| Name of Image |
International Space Station Assembly |
| Date of Image |
1999-01-01 |
| Full Description |
The International Space Station (ISS) is an unparalleled international scientific and technological cooperative venture that will usher in a new era of human space exploration and research and provide benefits to people on Earth. On-Orbit assembly began on November 20, 1998, with the launch of the first ISS component, Zarya, on a Russian Proton rocket. The Space Shuttle followed on December 4, 1998, carrying the U.S.-built Unity cornecting Module. Sixteen nations are participating in the ISS program: the United States, Canada, Japan, Russia, Brazil, Belgium, Denmark, France, Germany, Italy, the Netherlands, Norway, Spain, Sweden, Switzerland, and the United Kingdom. The ISS will include six laboratories and be four times larger and more capable than any previous space station. The United States provides two laboratories (United States Laboratory and Centrifuge Accommodation Module) and a habitation module. There will be two Russian research modules, one Japanese laboratory, referred to as the Japanese Experiment Module (JEM), and one European Space Agency (ESA) laboratory called the Columbus Orbital Facility (COF). The station's internal volume will be roughly equivalent to the passenger cabin volume of two 747 jets. Over five years, a total of more than 40 space flights by at least three different vehicles - the Space Shuttle, the Russian Proton Rocket, and the Russian Soyuz rocket - will bring together more than 100 different station components and the ISS crew. Astronauts will perform many spacewalks and use new robotics and other technologies to assemble ISS components in space. |
|
Payload Operations Center (P
| Name of Image |
Payload Operations Center (POC) for the International Space Station (ISS) |
| Date of Image |
2001-02-01 |
| Full Description |
The International Space Station (ISS) Payload Operations Center (POC) at NASA's Marshall Space Flight Center (MSFC) in Huntsville, Alabama, is the world's primary science command post for the International Space Station (ISS), the most ambitious space research facility in human history. The Payload Operations team is responsible for managing all science research experiments aboard the Station. The center is also home for coordination of the mission-plarning work of variety of international sources, all science payload deliveries and retrieval, and payload training and safety programs for the Station crew and all ground personnel. Within the POC, critical payload information from the ISS is displayed on a dedicated workstation, reading both S-band (low data rate) and Ku-band (high data rate) signals from a variety of experiments and procedures operated by the ISS crew and their colleagues on Earth. The POC is the focal point for incorporating research and experiment requirements from all international partners into an integrated ISS payload mission plan. This photograph is an overall view of the MSFC Payload Operations Center displaying the flags of the countries participating the ISS. The flags at the left portray The United States, Canada, France, Switzerland, Netherlands, Japan, Brazil, and Sweden. The flags at the right portray The Russian Federation, Italy, Germany, Belgium, Spain, United Kingdom, Denmark, and Norway. |
|
Payload Operations Center (P
| Name of Image |
Payload Operations Center (POC) for the International Space Station (ISS) |
| Date of Image |
2000-02-01 |
| Full Description |
The International Space Station (ISS) Payload Operations Center (POC) at NASA's Marshall Space Flight Center (MSFC) in Huntsville, Alabama, is the world's primary science command post for the (ISS), the most ambitious space research facility in human history. The Payload Operations team is responsible for managing all science research experiments aboard the Station. The center is also home for coordination of the mission-plarning work of variety of international sources, all science payload deliveries and retrieval, and payload training and safety programs for the Station crew and all ground personnel. Within the POC, critical payload information from the ISS is displayed on a dedicated workstation, reading both S-band (low data rate) and Ku-band (high data rate) signals from a variety of experiments and procedures operated by the ISS crew and their colleagues on Earth. The POC is the focal point for incorporating research and experiment requirements from all international partners into an integrated ISS payload mission plan. This photograph is an overall view of the MSFC Payload Operations Center displaying the flags of the countries participating in the ISS. The flags at the left portray The United States, Canada, France, Switzerland, Netherlands, Japan, Brazil, and Sweden. The flags at the right portray The Russian Federation, Italy, Germany, Belgium, Spain, United Kingdom, Denmark, and Norway. |
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Heat Wave in Western Europe
| Title |
Heat Wave in Western Europe |
| Description |
Western Europe continued to bake in late July 2006. Following an unusually warm spell between July 12 and 19, [ http://earthobservatory.nasa.gov/NaturalHazards/natural_hazards_v2.php3?img_id=13743 ] temperatures across most of the region remained much warmer than normal. This image shows land surface (as opposed to air) temperatures collected from July 20-27, 2006, compared to the average temperatures for that period over the past six years (2000-2005). Places that were up to ten degrees Celsius warmer than average are deep red, while places that were up to ten degrees cooler than average are deep blue. Places where the temperatures were average are white. The temperatures were measured by the Moderate Resolution Imaging Spectroradiometer (MODIS) [ http://modis.gsfc.nasa.gov ] on NASA's Terra [ http://terra.nasa.gov ] satellite. In the center of the image, deep red areas of very warm temperatures spread across Germany, as well as France (to the west), and Poland (to the east). To the north (top center), both Norway (west) and Sweden (east) were much warmer than average. Only small pockets of the region were cooler than average: northeastern Spain, the "toe" of Italy's boot and the western half of the island of Sicily, and parts of Greece (lower right). July 2006 was a record-breaking month for heat in many Western European countries, coming in as the hottest July on record in several countries, including Belgium, Denmark, Ireland, the Netherlands, and the United Kingdom. NASA image created by Jesse Allen, Earth Observatory, using data provided courtesy of Zhengming Wan, MODIS Land Surface Temperature Group, Institute for Computational Earth System Science [ http://www.icess.ucsb.edu/ ], University of California, Santa Barbara. |
|
European Heat Wave
| Title |
European Heat Wave |
| Description |
Europe is experiencing an historic heat wave that has been responsible for at 3,000 deaths in France alone. Compared to July 2001, temperatures in July 2003 were sizzling. This image shows the differences in day time land surface temperatures collected in the two years by the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA's Terra satellite. A blanket of deep red across southern and eastern France (left of image center) shows where temperatures were 10 degrees Celsius (18 degrees Fahrenheit) hotter this summer. White areas show where temperatures were similar, and blue shows where temperatures were cooler in 2003 than 2001. Even the Alps, which arc across southeastern France, Switzerland, Austria, and northern Italy (just below image center), are very warm this year. Glaciers are melting rapidly and swelling rivers and lakes to dangerously high levels. Climbers had to be evacuated from Switzerland's famous Matterhorn after melting triggered the collapse of a rock face. The popular climbing destination has been closed while geologists assess the possibility of further collapses. The heat wave stretches northward all the way to the United Kingdom, particularly southern England (bottom of island) and Scotland (top of island). In London, trains were shut down over fears that tracks would buckle in the heat, while in Scotland the high temperatures combined with falling water levels in rivers and streams are threatening the spawning and survival of salmon. Throughout France, Spain, Portugal, and Italy, the intense heat and dry conditions sparked devastating forest fires that killed at least 15 people. Image by Reto Stockli and Robert Simmon, NASA?s Earth Observatory Team. |
|
Severe Winter Storm in North
| Title |
Severe Winter Storm in Northern Europe |
| Description |
The clouds over Northern Europe have the menacing curl of a low pressure system associated with severe winter storms. This particular storm lashed the United Kingdom, Scandinavia, northern Germany, and Russia with hurricane-force winds and intense rains. According to news reports, 14 people died in the storm, many from being hit by falling trees or blowing debris. The storm brought severe floods to northern England and Scotland, submersing the English town of Carlisle entirely. Across Northern Europe, train services were halted and electricity flickered out under the onslaught of winds that gusted up to 180 kilometers per hour (112 mph). This image of the storm was acquired by the Moderate Resolution Imaging Spectroradiometer (MODIS [ http://modis.gsfc.nasa.gov ]) on NASA's Terra [ http://terra.nasa.gov/ ] satellite on January 9, 2005. NASA image created by Jesse Allen, Earth Observatory, using data obtained from the MODIS Rapid Response team. |
|
Silent Earthquake: Shahdad,
| Title |
Silent Earthquake: Shahdad, Iran |
| Description |
A magnitude 6.6 earthquake struck a sparsely inhabited area of southeast Iran on March 14, 1998, at 11:10 p.m. local time. While using satellite-based radar data to study the fault rupture of the 1998 earthquake, a team of scientists from the United States and the United Kingdom discovered that a second fault 10 to 30 kilometers (6 to 19 miles) to the east of the primary fault also moved in the six months after the quake. Named after a nearby town, the Shahdad Thrust Fault did not cause any detectable seismic waves when it slipped after the 1998 quake, and so scientists refer to the event as aseismic, or a "silent earthquake." The two images above show a three-dimensional view of the region affected by the 1998 quake. The images cover an area roughly 50 kilometers (30 miles) wide, and they are displayed with North along the right edge. (Imagine you are standing on the ground at the bottom of the image looking due west.) The image on top shows the region's surface geology, while the image on the bottom shows where the event deformed the surface. The light gray linear features running from lower left to upper right across the top image are small ridges that are related to the Shahdad Fault. The rainbow colors in the bottom image show contours of the motion of the surface. The big loops in red tones sweeping out across the low ridges show where the Shahdad Fault slipped eastward (toward you as you are standing at the bottom of the image) in the six months after the main earthquake. The top image was made from Landsat satellite data, while the bottom image is the result of the scientists' analysis of radar data collected by the European Remote Sensing (ERS) satellites. The March 1998 earthquake struck a valley on the other side of the mountains in the background of this view. Calculations of the transfer of stress in the Earth indicate that the earthquake probably caused the slip on the Shahdad Fault, and that the additional stresses were released by the "silent" slip. Scientists estimate that this silent earthquake would have been equivalent to a magnitude 6.0 earthquake if it had caused seismic waves. If other thrust faults in places such as Los Angeles manage to move aseismically, then they might release stresses that would otherwise build up to cause earthquakes. Radar data used in this research were acquired by the ERS satellites operated by the European Space Agency, which kindly made these data available for research. Part of this research was performed at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the U.S. National Aeronautics and Space Administration. Research was also performed at the Centre for the Observation and Modeling of Earthquakes and Tectonics supported by the U.K. Natural Environment Research Council, and at Stanford University. Landsat has been providing visible and infrared views of the Earth since 1972. The Landsat archive is managed by the U.S. Geological Survey's Eros Data, Center (USGS EDC). For more information, see the following recently published paper: Fielding, E.J., Wright, T.J., Muller, J., Parsons, B.E. and Walker, R. (2004) Aseismic deformation of a fold-and-thrust belt imaged by SAR interferometry near Shahdad, southeast Iran, Geology, v. 32, no. 7. Image Courtesy NASA/JPL/ESA |
|
Snow Hammers Europe
| Title |
Snow Hammers Europe |
| Description |
Clouds still lingered over much of Europe after winter snow blanketed much of the continent during the last week of February 2005. The snow closed roads and delayed flights in France, the United Kingdom, Italy, and Germany. This image, taken on February 24, 2005, hints at the extent of the snowfall under the clouds. To differentiate between white clouds and white snow, this image was created with both shortwave infrared and visible light. The resulting combination makes the snow appear dark red, while clouds are white and lighter peach. A band of snow stretches down the spine of Italy, and patches of snow are spread across France, left. Germany and all countries to its east and southeast appear to be entirely covered with snow. The Moderate Resolution Imaging Spectroradiometer (MODIS [ http://modis.gsfc.nasa.gov ]) flying aboard NASA's Terra [ http://terra.nasa.gov/ ] satellite acquired the image. NASA image created by Jesse Allen, Earth Observatory, using data courtesy of the MODIS Rapid Response team. |
|
Total Lunar Eclipse Tonight
| Title |
Total Lunar Eclipse Tonight |
| Explanation |
Go outside tonight and see the total lunar eclipse. Tonight's eclipse [ http://sunearth.gsfc.nasa.gov/eclipse/LEmono/TLE2004Oct28/TLE2004Oct28.html ] is easy and convenient for much of the world to see. Anyone who can spot a full Moon [ http://antwrp.gsfc.nasa.gov/apod/ap010906.html ] can see it fade out as the Earth's shadow [ http://www.mreclipse.com/Special/LEprimer.html ] engulfs it. No protective glasses or expensive telescopes are needed, just a little moxie [ http://blogs.law.harvard.edu/desultor/2003/08/19 ]. The above illustration [ http://sunearth.gsfc.nasa.gov/eclipse/LEmono/TLE2004Oct28/TLE2004Oct28.html ] shows how the eclipse will appear across the Earth. The total lunar eclipse [ http://antwrp.gsfc.nasa.gov/apod/ap960926.html ] starts at 9:14 pm Eastern Daylight Time [ http://aa.usno.navy.mil/faq/docs/us_tzones.html ], equivalent to 1:14 am UT [ http://aa.usno.navy.mil/faq/docs/UT.html ] in the morning for sky enthusiasts in the United Kingdom [ http://www.cia.gov/cia/publications/factbook/geos/uk.html ]. From the moment the first part of the Moon disappears [ http://antwrp.gsfc.nasa.gov/apod/ap040829.html ] to the moment that the last part of the Moon reappears will be 3 hours and 40 minutes. For those unfortunate enough to suffer clouds [ http://www.ucar.edu/educ_outreach/webweather/cloud3.html ], the eclipse can also be followed over several live [ http://NightSkyLive.net/ ] web [ http://sunearth.gsfc.nasa.gov/eclipse/LEmono/TLE2004Oct28/TLE2004Oct28.html#webcast ]casts [ http://www.xs4all.nl/~carlkop/verdmaan/leclips2004b.html ]. |
|
Ship Tracks off British Colu
nasa, nasanaturalhazards
KMZ file of the ship tracks
ships_amo_2008021
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2008-01-21 |
| creator |
NASA -- NASA Image Of The Day |
| identifier |
ships_amo_2008021 |
|
European Heat Wave: Natural
nasa, nasanaturalhazards
Europe is experiencing an hi
modis_lst_europe_2001-2003
| mediatype |
IMAGE |
| mediatype |
image |
| date |
July 31, 2003 |
| creator |
NASA -- NASA Image Of The Day |
| identifier |
modis_lst_europe_2001-2003 |
|
London, England: Image of th
nasa, nasaimageofthedaygalle
For almost 2,000 years, the
PIA04301
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2001-10-12 |
| creator |
NASA -- Image courtesy NASA/GSFC/MITI/ERSDAC/JAROS, and U.S./Japan asterweb.jpl.nasa.gov/ ASTER Science Team |
| identifier |
PIA04301 |
|
Ship Traffic on the Suez Can
nasa, nasaimageofthedaygalle
This astronaut photograph ca
ISS013-E-44847
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2006-06-30 |
| creator |
NASA -- Astronaut photograph eol.jsc.nasa.gov/scripts/sseop/photo.pl?mission=ISS013&roll=E&frame=44847 ISS013-E-44847 was acquired June 30, 2006, with a Kodak 760C digital camera using an 800 mm lens, and is provided by the ISS Crew Earth Observations experiment and the Image Science & Analysis Group, Johnson Space Center. The image in this article has been cropped and enhanced to improve contrast. The spaceflight.nasa.gov/home/index.html International Space Station Program supports the laboratory to help astronauts take pictures of Earth that will be of the greatest value to scientists and the public, and to make those images freely available on the Internet. Additional images taken by astronauts and cosmonauts can be viewed at the eol.jsc.nasa.gov/ NASA/JSC Gateway to Astronaut Photography of Earth. |
| identifier |
ISS013-E-44847 |
|
Snow Hammers Europe: Natural
nasa, nasanaturalhazards
Clouds still lingered over m
weurope_tmo_24feb05
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2005-02-24 |
| creator |
NASA -- NASA Image Of The Day |
| identifier |
weurope_tmo_24feb05 |
|
Heat Wave in Western Europe:
nasa, nasanaturalhazards
Western Europe continued to
weuropelsta_tmo_2006201
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2006-07-28 |
| creator |
NASA -- NASA Image Of The Day |
| identifier |
weuropelsta_tmo_2006201 |
|
Ship Tracks off British Colu
nasa, nasaimageofthedaygalle
They may look like airplane
ge_08430
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2008-01-21 |
| creator |
NASA -- NASA Image Of The Day |
| identifier |
ge_08430 |
|
Ship Tracks off British Colu
nasa, nasaimageofthedaygalle
They may look like airplane
ge_08430
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2008-01-21 |
| creator |
NASA -- NASA Image Of The Day |
| identifier |
ge_08430 |
|
NASA Launches Aura Satellite
nasa, nasaimageofthedaygalle
* eoimages.gsfc.nasa.gov/ima
Aura_launch
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2004-07-15 |
| creator |
NASA -- NASA images and animations of Aura satellite by Jesse Allen and Reto Stöckli, Earth Observatory. Photo of Delta II rocket courtesy Boeing/Thom Baur. |
| identifier |
Aura_launch |
|
Severe Winter Storm in North
nasa, nasanaturalhazards
The clouds over Northern Eur
terra_neurope_08jan05
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2005-01-09 |
| creator |
NASA -- NASA Image Of The Day |
| identifier |
terra_neurope_08jan05 |
|
Silent Earthquake: Shahdad,
nasa, nasaimageofthedaygalle
A magnitude 6.6 earthquake s
PIA06310
| mediatype |
IMAGE |
| mediatype |
image |
| date |
1998-09-14 |
| creator |
NASA -- Image Courtesy NASA/JPL/ESA |
| identifier |
PIA06310 |
|
London, England
PIA04301
Sol (our sun)
ASTER
| Title |
London, England |
| Original Caption Released with Image |
For almost 2,000 years, the River Thames has served as the life force of London, capital of the United Kingdom and one of the world's most famous cities. In AD 43 the Romans established the trading settlement of Londinium at a favorable crossing point on the river. The Romans remained until the 5th century, when the city came under Saxon control. The early 17th century saw enormous growth, but the deadly plague of 1664 and 1665 ravaged the population, and in the following year the Great Fire, which burned for four days, destroyed most of the city. A public transportation system and other city services in the early 19th century eased many of the increasing urban problems of the burgeoning capital of the wealthy British Empire. After coping with the devastating effects of bombing during World War II and the gradual dismantling of the empire, London today thrives as a vital modern metropolis. London is one of 100 cities being studied using ASTER data to map and monitor urban use patterns and growth. This image was acquired on October 12, 2001 by the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) on NASA's Terra satellite. With its 14 spectral bands from the visible to the thermal infrared wavelength region, and its high spatial resolution of 15 to 90 meters (about 50 to 300 feet), ASTER images Earth to map and monitor the changing surface of our planet. ASTER is one of five Earth-observing instruments launched December 18, 1999, on NASA's Terra satellite. The instrument was built by Japan's Ministry of Economy, Trade and Industry. A joint U.S./Japan science team is responsible for validation and calibration of the instrument and the data products. The broad spectral coverage and high spectral resolution of ASTER will provide scientists in numerous disciplines with critical information for surface mapping, and monitoring of dynamic conditions and temporal change. Example applications are: monitoring glacial advances and retreats, monitoring potentially active volcanoes, identifying crop stress, determining cloud morphology and physical properties, wetlands evaluation, thermal pollution monitoring, coral reef degradation, surface temperature mapping of soils and geology, and measuring surface heat balance. Dr. Anne Kahle at NASA's Jet Propulsion Laboratory, Pasadena, California, is the U.S. Science team leader, Bjorn Eng of JPL is the project manager. The Terra mission is part of NASA's Earth Science Enterprise, a long- term research effort to understand and protect our home planet. Through the study of Earth, NASA will help to provide sound science to policy and economic decision-makers so as to better life here, while developing the technologies needed to explore the universe and search for life beyond our home planet. Size: 39.5 x 55.3 km (24.5 x 34.3 miles) Location: 51.5 deg. North lat., 0.1 deg. West long. Orientation: North at top Image Data: ASTER bands 1,2, and 3. Original Data Resolution: 15 m Date Acquired:, October 12, 2001 |
|
AIRS First Light Data: North
PIA00345
Sol (our sun)
Atmospheric Infrared Sounder
| Title |
AIRS First Light Data: Northern Europe, July 20, 2002 |
| Original Caption Released with Image |
These images, taken over northern Europe on July 20, 2002, depict a few of the different views of Earth and its atmosphere that are produced by the Atmospheric Infrared Sounder experiment system operating on NASA's Aqua spacecraft. The image in Figure 1 is from an infrared channel from the AIRS instrument that measures the surface temperature in clear areas and cloud top temperatures in cloudy areas. The image reveals very warm conditions in France and a storm off the east coast of the United Kingdom. The image in Figure 2 represents a microwave channel from the Advanced Microwave Sounding Unit instrument that sees through most clouds and observes surface conditions everywhere. The image in Figure 3 is a microwave channel from the Humidity Sounder for Brazil instrument that is very sensitive to humidity and does not see the surface at all, but instead reveals the structure of moisture streams in the troposphere. The infrared and microwave data from the AIRS experiment are integrated to retrieve a single set of temperature, moisture, and cloud values. These three channels represent only a small portion of the 2,400-channel multispectral experiment, whose primary objectives are to improve the accuracy of weather forecasts and to study climate change. The AIRS experiment system also takes pictures of the Earth at four visible and near-infrared wavelengths that can be combined into a color picture. This image shows a swirling low-pressure system over England, clear skies over much of France, and frontal systems in the North Atlantic. Because AIRS is sensitive to different wavelengths than your eye, the colors shown are different from what you would see. For example, plants appear very red to AIRS. There are also subtle color differences in the clouds that relate to their altitude and thickness (compare the white clouds over England with the slightly grey-green ones near Iceland). These images are used in conjunction with other AIRS, AMSU-A, and HSB measurements to get a full 3-D view of the atmosphere. The Atmospheric Infrared Sounder is an instrument onboard NASA's Aqua satellite under the space agency's Earth Observing System. The sounding system is making highly accurate measurements of air temperature, humidity, clouds and surface temperature. Data will be used to better understand weather and climate. It will also be used by the National Weather Service and the National Oceanic and Atmospheric Administration to improve the accuracy of their weather and climate models. The instrument was designed and built by Lockheed Infrared Imaging Systems (recently acquired by British Aerospace) under contract with JPL. The Aqua satellite mission is managed by NASA's Goddard Space Flight Center. |
|
AIRS First Light Data: North
PIA00345
Sol (our sun)
Atmospheric Infrared Sounder
| Title |
AIRS First Light Data: Northern Europe, July 20, 2002 |
| Original Caption Released with Image |
These images, taken over northern Europe on July 20, 2002, depict a few of the different views of Earth and its atmosphere that are produced by the Atmospheric Infrared Sounder experiment system operating on NASA's Aqua spacecraft. The image in Figure 1 is from an infrared channel from the AIRS instrument that measures the surface temperature in clear areas and cloud top temperatures in cloudy areas. The image reveals very warm conditions in France and a storm off the east coast of the United Kingdom. The image in Figure 2 represents a microwave channel from the Advanced Microwave Sounding Unit instrument that sees through most clouds and observes surface conditions everywhere. The image in Figure 3 is a microwave channel from the Humidity Sounder for Brazil instrument that is very sensitive to humidity and does not see the surface at all, but instead reveals the structure of moisture streams in the troposphere. The infrared and microwave data from the AIRS experiment are integrated to retrieve a single set of temperature, moisture, and cloud values. These three channels represent only a small portion of the 2,400-channel multispectral experiment, whose primary objectives are to improve the accuracy of weather forecasts and to study climate change. The AIRS experiment system also takes pictures of the Earth at four visible and near-infrared wavelengths that can be combined into a color picture. This image shows a swirling low-pressure system over England, clear skies over much of France, and frontal systems in the North Atlantic. Because AIRS is sensitive to different wavelengths than your eye, the colors shown are different from what you would see. For example, plants appear very red to AIRS. There are also subtle color differences in the clouds that relate to their altitude and thickness (compare the white clouds over England with the slightly grey-green ones near Iceland). These images are used in conjunction with other AIRS, AMSU-A, and HSB measurements to get a full 3-D view of the atmosphere. The Atmospheric Infrared Sounder is an instrument onboard NASA's Aqua satellite under the space agency's Earth Observing System. The sounding system is making highly accurate measurements of air temperature, humidity, clouds and surface temperature. Data will be used to better understand weather and climate. It will also be used by the National Weather Service and the National Oceanic and Atmospheric Administration to improve the accuracy of their weather and climate models. The instrument was designed and built by Lockheed Infrared Imaging Systems (recently acquired by British Aerospace) under contract with JPL. The Aqua satellite mission is managed by NASA's Goddard Space Flight Center. |
|
AIRS First Light Data: North
PIA00345
Sol (our sun)
Atmospheric Infrared Sounder
| Title |
AIRS First Light Data: Northern Europe, July 20, 2002 |
| Original Caption Released with Image |
These images, taken over northern Europe on July 20, 2002, depict a few of the different views of Earth and its atmosphere that are produced by the Atmospheric Infrared Sounder experiment system operating on NASA's Aqua spacecraft. The image in Figure 1 is from an infrared channel from the AIRS instrument that measures the surface temperature in clear areas and cloud top temperatures in cloudy areas. The image reveals very warm conditions in France and a storm off the east coast of the United Kingdom. The image in Figure 2 represents a microwave channel from the Advanced Microwave Sounding Unit instrument that sees through most clouds and observes surface conditions everywhere. The image in Figure 3 is a microwave channel from the Humidity Sounder for Brazil instrument that is very sensitive to humidity and does not see the surface at all, but instead reveals the structure of moisture streams in the troposphere. The infrared and microwave data from the AIRS experiment are integrated to retrieve a single set of temperature, moisture, and cloud values. These three channels represent only a small portion of the 2,400-channel multispectral experiment, whose primary objectives are to improve the accuracy of weather forecasts and to study climate change. The AIRS experiment system also takes pictures of the Earth at four visible and near-infrared wavelengths that can be combined into a color picture. This image shows a swirling low-pressure system over England, clear skies over much of France, and frontal systems in the North Atlantic. Because AIRS is sensitive to different wavelengths than your eye, the colors shown are different from what you would see. For example, plants appear very red to AIRS. There are also subtle color differences in the clouds that relate to their altitude and thickness (compare the white clouds over England with the slightly grey-green ones near Iceland). These images are used in conjunction with other AIRS, AMSU-A, and HSB measurements to get a full 3-D view of the atmosphere. The Atmospheric Infrared Sounder is an instrument onboard NASA's Aqua satellite under the space agency's Earth Observing System. The sounding system is making highly accurate measurements of air temperature, humidity, clouds and surface temperature. Data will be used to better understand weather and climate. It will also be used by the National Weather Service and the National Oceanic and Atmospheric Administration to improve the accuracy of their weather and climate models. The instrument was designed and built by Lockheed Infrared Imaging Systems (recently acquired by British Aerospace) under contract with JPL. The Aqua satellite mission is managed by NASA's Goddard Space Flight Center. |
|
AIRS First Light Data: North
PIA00345
Sol (our sun)
Atmospheric Infrared Sounder
| Title |
AIRS First Light Data: Northern Europe, July 20, 2002 |
| Original Caption Released with Image |
These images, taken over northern Europe on July 20, 2002, depict a few of the different views of Earth and its atmosphere that are produced by the Atmospheric Infrared Sounder experiment system operating on NASA's Aqua spacecraft. The image in Figure 1 is from an infrared channel from the AIRS instrument that measures the surface temperature in clear areas and cloud top temperatures in cloudy areas. The image reveals very warm conditions in France and a storm off the east coast of the United Kingdom. The image in Figure 2 represents a microwave channel from the Advanced Microwave Sounding Unit instrument that sees through most clouds and observes surface conditions everywhere. The image in Figure 3 is a microwave channel from the Humidity Sounder for Brazil instrument that is very sensitive to humidity and does not see the surface at all, but instead reveals the structure of moisture streams in the troposphere. The infrared and microwave data from the AIRS experiment are integrated to retrieve a single set of temperature, moisture, and cloud values. These three channels represent only a small portion of the 2,400-channel multispectral experiment, whose primary objectives are to improve the accuracy of weather forecasts and to study climate change. The AIRS experiment system also takes pictures of the Earth at four visible and near-infrared wavelengths that can be combined into a color picture. This image shows a swirling low-pressure system over England, clear skies over much of France, and frontal systems in the North Atlantic. Because AIRS is sensitive to different wavelengths than your eye, the colors shown are different from what you would see. For example, plants appear very red to AIRS. There are also subtle color differences in the clouds that relate to their altitude and thickness (compare the white clouds over England with the slightly grey-green ones near Iceland). These images are used in conjunction with other AIRS, AMSU-A, and HSB measurements to get a full 3-D view of the atmosphere. The Atmospheric Infrared Sounder is an instrument onboard NASA's Aqua satellite under the space agency's Earth Observing System. The sounding system is making highly accurate measurements of air temperature, humidity, clouds and surface temperature. Data will be used to better understand weather and climate. It will also be used by the National Weather Service and the National Oceanic and Atmospheric Administration to improve the accuracy of their weather and climate models. The instrument was designed and built by Lockheed Infrared Imaging Systems (recently acquired by British Aerospace) under contract with JPL. The Aqua satellite mission is managed by NASA's Goddard Space Flight Center. |
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