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Aug. 1 Solar Eclipse Image S
On August 1, a total solar e
8/4/08
| Description |
On August 1, a total solar eclipse was visible in parts of Canada, northern Greenland, the Arctic, central Russia, Mongolia and China. The eclipse swept across Earth in a narrow path that began in Canada's northern province of Nunavut and ended in northern China's Silk Road region. Though the eclipse was not visible in most of North America, NASA TV and the Exploratorium made streaming video of the event available online. These images are taken from that video. The sun appears differently in some of the images because of the different filters used to capture the event. Times listed are approximate. At 6:54 a.m. ET, clouds began to roll in, threatening to block out the total eclipse. The clouds began to break at 7:06 a.m., and the sky cleared long enough for views of totality at 7:10 a.m. > Larger, unlabeled image Credit: NASA TV/The Exploratorium |
| Date |
8/4/08 |
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California Fires Mid-Novembe
One hundred eighty-seven hom
11/27/08
| Description |
One hundred eighty-seven homes were destroyed by the Freeway Fire in Southern California in mid-November 2008. Driven by Santa Ana winds, the fire exploded out of the Chino Hills into communities at the foothills of the mountains. More than 30,000 acres were scorched by the fire. This natural-color image of the burned area was captured by the Advanced Land Imager (ALI) on NASA's Earth Observing-1 satellite on November 18, 2008. The top image shows the Chino Hills north of Riverside Freeway and west of Chino Valley Freeway, a mostly undeveloped area that encompasses Chino Hills State Park. Small cities and residential areas encircle the mountains. The burned area is charcoal, and it stretches across most of the Chino Hills. The lower image is a detailed view of the edge of the burned area in northwestern Yorba Linda. The fire crossed Telegraph Canyon and made forays southwestward into neighborhoods. One arm of the fire encircled Carbon Canyon Regional Park. Southeast of the Riverside Freeway (shown in the large image), is a part of Chino Hills State Park called the Coal Canyon area. The area has a dull greenish-brown color that is typical for the dry woodland/chaparral ecosystems native to the area. (In this part of California, bright green vegetation is the product of irrigation, for example, golf courses and lawns.) The Coal Canyon area was added to China Hills State Park in 2000, and it was the only part of the 14,000-acre park that was not burned, according to local news reports. NASA image by Robert Simmon, based on data provided by the EO-1 Mission Office. Caption by Rebecca Lindsey. |
| Date |
11/27/08 |
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Far East Russian Fires
Large fires were burning in
5/28/09
| Description |
Large fires were burning in the forests of Siberia between the Amur River (known as Heilong Jiang in China) and the Bureya River on May 24, 2009, when the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA's Aqua satellite captured this image. Places where the sensor detected actively burning fires are marked in red. Dark brownish-purple patches on the landscape are burn scars from previous fires. Thick smoke in the eastern part of the image may be from these fires as well as fires farth er west, south of Lake Baikal. Both accidental and natural forest fires are common in spring and summer in Russia. The large image provided above is at MODIS' maximum spatial resolution (level of detail) of 250 meters per pixel. The MODIS Rapid Response Team provides a georeferenced version of this image for use in Google Earth. NASA image by Jeff Schmaltz, MODIS Rapid Response Team. Caption by Rebecca Lindsey. |
| Date |
5/28/09 |
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Harrier Cockpit Restoration
Ed Swan and Gray Creech disc
8/20/08
| Description |
Ed Swan and Gray Creech discuss AV-8A Harrier cutting and retrieval challenges at the Naval Air Warfare Center Weapons Division at China Lake. The former Marine Corps aircraft had been a weapons survivability test aircraft. |
| Date |
8/20/08 |
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Great Wall of China
These radar images show two
8/3/95
| Date |
8/3/95 |
| Description |
These radar images show two segments of the Great Wall of China in a desert region of north-central China, about 700 kilometers (434 miles) west of Beijing. The wall appears as a thin orange band, running from the top to the bottom of the left image, and from the middle upper-left to the lower-right of the right image. These segments of the Great Wall were constructed in the 15th century, during the Ming Dynasty. The wall is between 5 and 8 meters high (16 to 26 feet) in these areas. The entire wall is about 3,000 kilometers (1,864 miles) long and about 150 kilometers (93 miles) of the wall appear in these two images. The wall is easily detected from space by radar because its steep, smooth sides provide a prominent surface for reflection of the radar beam. Near the center of the left image, two dry lake beds have been developed for salt extraction. Rectangular patterns in both images indicate agricultural development, primarily wheat fields. The images were acquired by the Spaceborne Imaging Radar-C/X-Band Synthetic Aperture Radar (SIR-C/X-SAR) onboard the space shuttle Endeavour on April 10, 1994. SIR-C/X-SAR, a joint mission of the German, Italian and the United States space agencies, is part of NASA's Mission to Planet Earth. The left image is centered at 37.7 degrees North latitude and 107.5 degrees East longitude. The right image is centered at 37.5 degrees North latitude and 108.1 degrees East longitude. North is toward the upper right. Each area shown measures 25 kilometers by 75 kilometers (15.5 miles by 45.5 miles). The colors in the image are assigned to different frequencies and polarizations of the radar as follows: red is L- band horizontally transmitted, horizontally received, green is L- band horizontally transmitted, vertically received, blue is C-band horizontally transmitted, vertically received. ##### |
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Karakax Valley, China 3-D Vi
This three-dimensional persp
11/6/95
| Date |
11/6/95 |
| Description |
This three-dimensional perspective of the remote Karakax Valley in the northern Tibetan Plateau of western China was created by combining two spaceborne radar images using a technique known as interferometry. Visualizations like this are helpful to scientists because they reveal where the slopes of the valley are cut by erosion, as well as the accumulations of gravel deposits at the base of the mountains. These gravel deposits, called alluvial fans, are a common landform in desert regions that scientists are mapping in order to learn more about Earth's past climate changes. Higher up the valley side is a clear break in the slope, running straight, just below the ridge line. This is the trace of the Altyn Tagh fault, which is much longer than California's San Andreas fault. Geophysicists are studying this fault for clues it may be able to give them about large faults. Elevations range from 4000 m (13,100 ft) in the valley to over 6000 m (19,700 ft) at the peaks of the glaciated Kun Lun mountains running from the front right towards the back. Scale varies in this perspective view, but the area is about 20 km (12 miles) wide in the middle of the image, and there is no vertical exaggeration. The two radar images were acquired on separate days during the second flight of the Spaceborne Imaging Radar- C/X-band Synthetic Aperture Radar (SIR-C/X-SAR) aboard the space shuttle Endeavour in October 1994. The interferometry technique provides elevation measurements of all points in the scene. The resulting digital topographic map was used to create this view, looking northwest from high over the valley. Variations in the colors can be related to gravel, sand and rock outcrops. This image is centered at 36.1 degrees north latitude, 79.2 degrees east longitude. Radar image data are draped over the topography to provide the color with the following assignments: Red is L- band vertically transmitted, vertically received, green is the average of L-band vertically transmitted, vertically received and C-band vertically transmitted, vertically received, and blue is C-band vertically transmitted, vertically received. SIR-C/X-SAR, a joint mission of the German, Italian and United States space agencies, is part of NASA's Mission to Planet Earth. ##### |
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Mineral Resources, China L a
This spaceborne radar image
| Description |
This spaceborne radar image of a mineral-rich region in southern China is being used by geologists to identify potential new areas for mineral exploration. The area shown is the vicinity of the city of Zhao Qing, the light blue area along the banks of the River Xi Jiang in the lower left. This is in the southern Chinese province of Guangdong, about 75 kilometers (46 miles) west of Guangzhou (Canton). The largest gold mine in southern China is located in the far upper left of the image along a brightly reflective mountain ridge. Using the radar image as a guide, geologists are tracing the extension of the ridge structure to the east (right) to identify possible mining areas. Radar imaging is especially useful for this purpose because of its sensitivity to subtle topographic structure, even in areas such as these, which have a dense vegetation cover. The Xi Jiang area is one of the most productive mining regions in China, with deposits of tungsten, lead, zinc and gold. The image was acquired by the Spaceborne Imaging Radar-C/X-Band Synthetic Aperture Radar (SIR-C/X-SAR) onboard the space shuttle Endeavour on April 17, 1994. The image is centered at 37.2 degrees north latitude and 112.5 degrees east longitude. North is toward the upper right. The image shows an area 60 kilometers by 38 kilometers (37.2 miles by 23.6 miles) The colors are assigned to different frequencies and polarizations of the radar as follows: red is L- band, horizontally transmitted, horizontally received, green is L-band, horizontally transmitted, vertically received, blue is C- band, horizontally transmitted, vertically received. SIR-C/X-SAR, a joint mission of the German, Italian and United States space agencies, is part of NASA's Mission to Planet Earth program. ##### |
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Great Wall of China L and C
These spaceborne radar image
4/18/96
| Date |
4/18/96 |
| Description |
These spaceborne radar images show a segment of the Great Wall of China in a desert region of north-central China, about 700 kilometers (434 miles) west of Beijing. The wall appears as a thin orange band, running from the top to the bottom of the color image on the left. The black and white images on the right correspond to the area outlined by the box and represent the four radar channels of the Spaceborne Imaging Radar-C (SIR-C). Each channel is sensitive to different aspects of the terrain, including two generations of the Great Wall. The L-band image (24 cm wavelength, horizontally transmitted and horizontally received polarizations) provides the clearest image of the two wall segments. The bright continuous line running from top to bottom in this image is the younger wall, built during the Ming Dynasty about 600 years ago. Immediately to the right of this wall is a bright discontinuous line that is the remnant of an older version of the wall, built during the Sui Dynasty, about 1500 years ago. The two generations of the wall are seen less distinctly in the L-band image (horizontally transmitted, vertically received) and C-band image (6 cm wavelength, horizontally transmitted, horizontally received). Orchards and other trees lining a road parallel to the wall show up as bright rectangles on the these two images because the L and C channels are sensitive to complex vegetation structure. The Ming Dynasty wall is between 5 meters and 8 meters high (16 feet to 26 feet) in these areas. The entire wall is about 3,000 kilometers (1,864 miles) long, but only a 75-kilometer (45.5-mile) long segment is shown in this image. The wall is easily detected from space by radar because its steep, smooth sides provide a prominent surface for reflection of the radar beam. Detection of the remnant Sui Dynasty wall by radar is allowing Chinese researchers to trace the former location of the wall across vast and remote areas. In some areas, the Sui wall is buried by sand that has been blown across the desert. The images were acquired by the Spaceborne Imaging Radar-C/X-Band Synthetic Aperture Radar (SIR-C/X-SAR) onboard the space shuttle Endeavour on April 10, 1994. The left image is centered at 37.7 degrees north latitude and 107.5 degrees east longitude. North is toward the upper right. The left image shows an area 25 kilometers by 75 kilometers (15.5 miles by 45.5 miles), and the right images show an area 3.1 kilometers by 2.2 kilometers (1.9 miles by 1.4 miles). The colors in the left image are assigned to different frequencies and polarizations of the radar as follows: red is L- band, horizontally transmitted, horizontally received, green is L-band, horizontally transmitted, vertically received, blue is C-band, horizontally transmitted, vertically received. SIR-C/X-SAR, a joint mission of the German, Italian and United States space agencies, is part of NASA's Mission to Planet Earth program. ##### |
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Hong Kong L & C bands
This spaceborne radar image
6/13/96
| Date |
6/13/96 |
| Description |
This spaceborne radar image shows part of the British territory of Hong Kong, adjacent to mainland China. The South China Sea is shown in dark blue and red on the image. Land surfaces are seen in shades of lighter blue and gold, including Hong Kong Island in the lower center, the Kowloon Peninsula in the upper right and many other small islands. The brightest yellow areas are the densely developed areas of Hong Kong's business and residential districts. The small yellow dots in the water are the many ships that make Hong Kong one of the busiest seaports in the Far East. Images such as this can be used by land-use planners to monitor urban development and its effect on the tropical environment. The image was acquired by the Spaceborne Imaging Radar-C/X-band Synthetic Aperture Radar (SIR- C/X-SAR) onboard the space shuttle Endeavour on October 10, 1994. The image is 23 kilometers by 31 kilometers (14 miles by 19 miles) and is centered at 22.3 degrees north latitude, 114.1 degrees east longitude. North is toward the upper right. The colors are assigned to different radar frequencies and polarizations of the radar as follows: red is L-band, vertically transmitted and received, green is C-band, vertically transmitted and received, and blue is C-band minus L-band, both vertically transmitted and received. SIR-C/X-SAR, a joint mission of the German, Italian and United States space agencies, is part of NASA's Mission to Planet Earth. ##### |
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NSCAT global image
This is a global image of la
11/18/96
| Date |
11/18/96 |
| Description |
This is a global image of land surfaces as seen by the NASA Scatterometer (NSCAT) onboard Japan's Advanced Earth Observing Satellite. The scatterometer's primary function is to study winds over the oceans, but scientists have devised a way of studying changes in the instrument's radar backscatter to look at land surfaces as well. The scatterometer's radar is sensitive to conditions on the Earth's surface. The brightest regions in this image are glacial ice sheets in Greenland and Antarctica. Tropical rainforests along the equator in South America, Africa and Southeast Asia are relatively bright due to their vegetation and soil moisture. Very dry, sandy deserts show up as black in this image. Some examples are the Empty Quarter in Saudia Arabia, the Gobi Desert in Western China and the Sahara Desert in North Africa. The light area just below the wide, dark band in Africa is known as the Sahel, a region that lightens and darkens with the changing seasons and drought conditions in Africa. The seasonal radar response of the Sahel is thought to be a sensitive indicator of desertification due to global warming and climate change. NSCAT was launched from Japan on August 16, 1996. The mission represents the first major collaboration between the two nations in Earth remote-sensing. JPL developed, built and manages the NSCAT instrument for NASA's Office of Mission to Planet Earth. ##### |
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Dust clouds over eastern Chi
The desert takes to the skie
5/9/01
| Date |
5/9/01 |
| Description |
The desert takes to the skies in these images of eastern China from NASA's Multi-angle Imaging SpectroRadiometer (MISR). A hazy summer view from July 9, 2000, (left) compares with a spectacularly dusty spring view from April 7, 2001, (middle). The two images cover an area from central Manchuria near the top to portions of North and South Korea at the bottom. The image on the right is a higher resolution MISR nadir- camera view of a portion of the April 7, 2001, dust cloud. When viewed at full magnification, a number of atmospheric wave features, like the ridges and valleys of a fingerprint, are apparent. These are probably induced by surface topography, which can disturb the wind flow. A few small cumulus clouds are also visible and are casting shadows on the thick lower dust layer. According to the Xinhua News Agency in China, nearly one million tons of Gobi Desert dust blow into Beijing each year. During a similar dust outbreak last year, the Associated Press reported that the visibility in Beijing had been reduced to the point where buildings were barely visible across city streets and airline schedules were significantly disrupted. The dust has also been implicated in adverse health effects such as respiratory discomfort and eye irritation. Asia's desert areas are prone to soil erosion, as underground water tables are lowered by prolonged drought and by industrial and agricultural water use. Heavy winds blowing eastward across the arid and sparsely vegetated surfaces of Mongolia and western China pick up large quantities of yellow dust. Airborne dust clouds from the April 2001 storm blew across the Pacific Ocean and were carried as far as North America. The minerals transported in this manner are believed to provide nutrients for both oceanic and land ecosystems. The left-hand and middle images are from Terra orbits 2,967 and 6,928 respectively. They are approximately 380 kilometers (236 miles) in width. The right-hand image covers an area roughly 250 kilometers (155 miles) wide by 470 kilometers (292 miles) high. Analyses of images such as these constitute one phase of MISR's participation in the Asian-Pacific Regional Aerosol Characterization Experiment, an international campaign aimed at studying the offshore transport of airborne particles from the Asian continent. More information about this international endeavor is available online at http://saga.pmel.noaa.gov/aceasia/ . MISR, built and managed by NASA's Jet Propulsion Laboratory, is one of several Earth-observing experiments aboard Terra, launched in December 1999. MISR acquires images of the Earth at nine angles simultaneously, using nine separate cameras pointed forward, downward, and backward along its flight path. More information about MISR is available at http://www-misr.jpl.nasa.gov . JPL is a division of the California Institute of Technology in Pasadena. Image credit: NASA/GSFC/LaRC/JPL, MISR Team. # # # # # |
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A Shocking Surprise in Steph
| Title |
A Shocking Surprise in Stephan's Quintet |
| Description |
This false-color composite image of the Stephan's Quintet galaxy cluster clearly shows one of the largest shock waves ever seen (green arc), produced by one galaxy falling toward another at over a million miles per hour. It is made up of data from NASA's Spitzer Space Telescope and a ground-based telescope in Spain. Four of the five galaxies in this image are involved in a violent collision, which has already stripped most of the hydrogen gas from the interiors of the galaxies. The centers of the galaxies appear as bright yellow-pink knots inside a blue haze of stars, and the galaxy producing all the turmoil, NGC7318b, is the left of two small bright regions in the middle right of the image. One galaxy, the large spiral at the bottom left of the image, is a foreground object and is not associated with the cluster. The titanic shock wave, larger than our own Milky Way galaxy, was detected by the ground-based telescope using visible-light wavelengths. It consists of hot hydrogen gas. As NGC7318b collides with gas spread throughout the cluster, atoms of hydrogen are heated in the shock wave, producing the green glow. Spitzer pointed its infrared spectrograph at the peak of this shock wave (middle of green glow) to learn more about its inner workings. This instrument breaks light apart into its basic components. Data from the instrument are referred to as spectra and are displayed as curving lines that indicate the amount of light coming at each specific wavelength. The Spitzer spectrum showed a strong infrared signature for incredibly turbulent gas made up of hydrogen molecules. This gas is caused when atoms of hydrogen rapidly pair-up to form molecules in the wake of the shock wave. Molecular hydrogen, unlike atomic hydrogen, gives off most of its energy through vibrations that emit in the infrared. This highly disturbed gas is the most turbulent molecular hydrogen ever seen. Astronomers were surprised not only by the turbulence of the gas, but by the incredible strength of the emission. The reason the molecular hydrogen emission is so powerful is not yet completely understood. Stephan's Quintet is located 300 million light-years away in the Pegasus constellation. This image is composed of three data sets: near-infrared light (blue) and visible light called H-alpha (green) from the Calar Alto Observatory in Spain, operated by the Max Planck Institute in Germany, and 8-micron infrared light (red) from Spitzer's infrared array camera. |
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First Class of Female Astron
| Title |
First Class of Female Astronauts |
| Full Description |
From left to right are Shannon W. Lucid, Margaret Rhea Seddon, Kathryn D. Sullivan, Judith A. Resnik, Anna L. Fisher, and Sally K. Ride. NASA selected all six women as their first female astronaut candidates in January 1978, allowing them to enroll in a training program that they completed in August 1979. Shannon W. Lucid was born on January 14, 1943 in Shanghai, China but considers Bethany, Oklahoma to be her hometown. She spent many years at the University of Oklahoma, receiving a Bachelor in chemistry in 1963, a Master in biochemistry in 1970, and a Doctorate in biochemistry in 1973. Dr. Lucid flew on the STS-51G Discovery, STS-34 Atlantis, STS-43 Atlantis, and STS-58 Columbia shuttle missions, setting the record for female astronauts by logging 838 hours and 54 minutes in space. She also currently holds the United States single mission space flight endurance record for her 188 days on the Russian Space Station Mir. From February 2002 to September 2003, she served as chief scientist at NASA Headquarters before returning to JSC to help with the Return to Flight program after the STS-107 accident. Born November 8, 1947, in Murfreesboro, Tennessee, Margaret Rhea Seddon received a Doctorate of Medicine in 1973 from the University of Tennessee. She flew on space missions STS-51 Discovery, STS-40 Columbia, and STS-58 Columbia for a total of over 722 hours in space. Dr. Seddon retired from NASA in November 1997, taking on a position as the Assistant Chief Medical Officer of the Vanderbilt Medical Group in Nashville, Tennessee. Kathryn Sullivan was born October 3, 1951 in Patterson, New Jersey but considers Woodland Hills, California to be her hometown. She received a Bachelor in Earth Sciences from the University of California, Santa Cruz in 1973 and a Doctorate in Geology from Dalhousie University in Halifax, Nova Scotia in 1978. She flew on space missions STS-41G, STS-31, and STS-45 and logged a total of 532 hours in space. Dr. Sullivan left NASA in August 1992 to assume the position of Chief Scientist of the National Oceanic and Atmospheric Administration (NOAA). She later went on to serve as President and CEO of the Center of Science and Industry in Columbus, Ohio. Dr. Judith Resnik was born April 5, 1949 in Akron, Ohio. She received a Bachelor of Science degree in Electrical Engineering from Carnegie-Mellon University in 1970, and a Doctorate in Electrical Engineering from University of Maryland in 1977. Dr. Resnik left a job as a senior systems engineer in product development with Xerox Corporation at El Segundo, California to work for NASA in 1978. She died on January 28, 1986 on her second mission, during the launch of Challenger STS-51-L. Anna Fisher was born August 24, 1949 in New York City, New York hometown. She received a Doctorate in Medicine in 1976 and a Master of Science in Chemistry in 1987, both from the University of California, Los Angeles. Dr. Fisher flew on STS-51A, the Space Shuttle Discovery's November 8, 1984, mission, and logged 192 hours in space, her second schedule mission was cancelled after the Space Shuttle Challenger STS-51L accident. She remains with NASA, where she has filled many positions over decades of service. Dr. Sally Ride was the first American woman in space. Born on May 26, 1951 in Los Angeles, California, she went on to receive a Bachelor in Physics and English in 1973 from Stanford University and, later, a Master in Physics in 1975 and a Doctorate in Physics in 1978, also from Stanford. She began her astronaut career as a mission specialist on STS-7, which launched from Kennedy Space Center, Florida on June 18, 1983, and later went on to fly on STS-41G. She withdrew from training for her third scheduled mission in order to serve on the investigative committee for the Space Shuttle Challenger accident and never returned to training, although she went on to work for headquarters and later to serve on the Columbia Accident Investigation Board before returning to the private sector as a physics professor. |
| Date |
02/28/1979 |
| NASA Center |
Johnson Space Center |
|
Visit of Chinese Vice Premie
| Title |
Visit of Chinese Vice Premier Deng Xiaoping to Johnson Space Center |
| Full Description |
Deng Xiaoping, Vice Premier of the People's Republic of China state council, and his wife are briefed by Johnson Space Center director Dr. Christopher C. Kraft. A complete review of NASA's manned space program was given, using exhibit scale models and flight simulators. |
| Date |
02/02/1979 |
| NASA Center |
Johnson Space Center |
|
Just like its "cousin" nine
| Description |
Just like its "cousin" nine days ago, yet another small comet appeared in the lower left area of the field of view of SOHO's C3 coronagraph instrument (February 14-15, 2007 and streaked right towards the Sun. This "sungrazer" comet followed almost exactly the same trajectory as the comet observed on Feb. 6. They both most likely belonged to the Kreutz comet group. Kreutz comets are a family of comets that we often spot passing near the Sun. The members of the Kreutz group are believed to have all originated as part of the same parent comet that broke up in the past near perihelion (the closest approach to the Sun). In this case, due to a day long data gap in these images, we do not get to follow it into the Sun, but it is a fair assumption that it too was vaporized as it got too close. This comet is SOHO-1270 and was discovered by Hua Su (China) -- the third (almost second) most successful SOHO comet hunter with approx 140 comet finds! Some of you may not know that amateur comet hunters using the Internet have discovered about 75% of the SOHO comets. |
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Panda Habitat Deforestation:
| Title |
Panda Habitat Deforestation: Highlighting Wolong Preserve |
| Abstract |
Zoom into China, hightlighting the Wolong Preserve. |
| Completed |
2001-04-06 |
|
Panda Habitat Deforestation:
| Title |
Panda Habitat Deforestation: Highlighting Wolong Preserve |
| Abstract |
Zoom into China, hightlighting the Wolong Preserve. |
| Completed |
2001-04-06 |
|
China Dust Storm seen by Ear
| Title |
China Dust Storm seen by Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6 and 7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and the United States. |
| Completed |
2003-12-01 |
|
China Dust Storm seen by Ear
| Title |
China Dust Storm seen by Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6 and 7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and the United States. |
| Completed |
2003-12-01 |
|
China Dust Storm seen by Ear
| Title |
China Dust Storm seen by Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6 and 7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and the United States. |
| Completed |
2003-12-01 |
|
China Dust Storm seen by Ear
| Title |
China Dust Storm seen by Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6 and 7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and the United States. |
| Completed |
2003-12-01 |
|
China Dust Storm seen by Ear
| Title |
China Dust Storm seen by Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6 and 7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and the United States. |
| Completed |
2003-12-01 |
|
China Dust Storm seen by Ear
| Title |
China Dust Storm seen by Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6 and 7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and the United States. |
| Completed |
2003-12-01 |
|
China Dust Storm seen by Ear
| Title |
China Dust Storm seen by Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6 and 7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and the United States. |
| Completed |
2003-12-01 |
|
China Dust Storm seen by Ear
| Title |
China Dust Storm seen by Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6 and 7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and the United States. |
| Completed |
2003-12-01 |
|
China Dust Storm seen by Ear
| Title |
China Dust Storm seen by Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6 and 7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and the United States. |
| Completed |
2003-12-01 |
|
China Dust Storm seen by Ear
| Title |
China Dust Storm seen by Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6 and 7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and the United States. |
| Completed |
2003-12-01 |
|
China Dust Storm seen by Ear
| Title |
China Dust Storm seen by Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6 and 7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and the United States. |
| Completed |
2003-12-01 |
|
China Dust Storm seen by Ear
| Title |
China Dust Storm seen by Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6 and 7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and the United States. |
| Completed |
2003-12-01 |
|
China Dust Storm seen by Ear
| Title |
China Dust Storm seen by Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6 and 7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and the United States. |
| Completed |
2003-12-01 |
|
Transient Aerosol Features:
| Title |
Transient Aerosol Features: Great China Fire from April through May 1987 |
| Completed |
1996-06-15 |
|
The Shenzhen Special Economi
| Title |
The Shenzhen Special Economic Zone |
| Abstract |
Landsat Thematic Mapper views Shenzhen, China, located on the Pearl River, in 1988, 1992, and 1995. The band combination used in these images is 432. To view related animations, please see animations 942, 1396, 1397, and 1398. |
| Completed |
1999-04-09 |
|
Typhoon Utor from TRMM: July
| Title |
Typhoon Utor from TRMM: July 5, 2001 |
| Abstract |
Typhoon Utor hits Taiwan on its way towards mainland China. This data from TRMM was taken at about 6:45 UTC on July 5, 2001. Isosurfaces are: Yellow=0.5 inches/hour, Green=1.0 inches/hour, Red=2.0 inches/hour on rainfall rates. |
| Completed |
2001-07-05 |
|
Typhoon Utor from TRMM: July
| Title |
Typhoon Utor from TRMM: July 5, 2001 |
| Abstract |
Typhoon Utor hits Taiwan on its way towards mainland China. This data from TRMM was taken at about 6:45 UTC on July 5, 2001. Isosurfaces are: Yellow=0.5 inches/hour, Green=1.0 inches/hour, Red=2.0 inches/hour on rainfall rates. |
| Completed |
2001-07-05 |
|
Typhoon Utor from TRMM: July
| Title |
Typhoon Utor from TRMM: July 5, 2001 |
| Abstract |
Typhoon Utor hits Taiwan on its way towards mainland China. This data from TRMM was taken at about 6:45 UTC on July 5, 2001. Isosurfaces are: Yellow=0.5 inches/hour, Green=1.0 inches/hour, Red=2.0 inches/hour on rainfall rates. |
| Completed |
2001-07-05 |
|
Pearl River, Region 3 (542)
| Title |
Pearl River, Region 3 (542) |
| Abstract |
Superseded by animation 942. |
| Completed |
1999-04-09 |
|
Ground Photographs from Sout
| Title |
Ground Photographs from Southern China: Road Construction |
| Completed |
1999-04-09 |
|
Haze over China
| Title |
Haze over China |
| Abstract |
NASA satellite image of eastern Asia shows a dense blanket of polluted air over central eastern China -- dense enough that the coastline around Shanghai virtually disappears. The 'Asian Brown Cloud' is a toxic mix of ash, acids and airborne particles from car and factory emissions, as well as from low-tech polluters like wood-burning stoves. |
| Completed |
2003-01-10 |
|
Haze over China
| Title |
Haze over China |
| Abstract |
NASA satellite image of eastern Asia shows a dense blanket of polluted air over central eastern China -- dense enough that the coastline around Shanghai virtually disappears. The 'Asian Brown Cloud' is a toxic mix of ash, acids and airborne particles from car and factory emissions, as well as from low-tech polluters like wood-burning stoves. |
| Completed |
2003-01-10 |
|
Haze over China
| Title |
Haze over China |
| Abstract |
NASA satellite image of eastern Asia shows a dense blanket of polluted air over central eastern China -- dense enough that the coastline around Shanghai virtually disappears. The 'Asian Brown Cloud' is a toxic mix of ash, acids and airborne particles from car and factory emissions, as well as from low-tech polluters like wood-burning stoves. |
| Completed |
2003-01-10 |
|
SeaWiFS: Typhoon Bilis
| Title |
SeaWiFS: Typhoon Bilis |
| Abstract |
'Super' Typhoon Bilis was one of the largest Typhoons on record. On August 23, 2000, it slammed Taiwan on its way to China. |
| Completed |
2000-08-15 |
|
SeaWiFS: Typhoon Bilis
| Title |
SeaWiFS: Typhoon Bilis |
| Abstract |
'Super' Typhoon Bilis was one of the largest Typhoons on record. On August 23, 2000, it slammed Taiwan on its way to China. |
| Completed |
2000-08-15 |
|
Flyover of Songhua Floods: A
| Title |
Flyover of Songhua Floods: August 20, 1998 |
| Completed |
1998-08-20 |
|
Flyover of Songhua Floods: A
| Title |
Flyover of Songhua Floods: August 20, 1998 |
| Completed |
1998-08-20 |
|
Flyover of Songhua Floods: A
| Title |
Flyover of Songhua Floods: August 20, 1998 |
| Completed |
1998-08-20 |
|
Pearl River, China (with win
| Title |
Pearl River, China (with window) |
| Completed |
1999-04-09 |
|
China Dust Storm seen by Ter
| Title |
China Dust Storm seen by Terra/MODIS and Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6-7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and The United States. |
| Completed |
2003-12-01 |
|
China Dust Storm seen by Ter
| Title |
China Dust Storm seen by Terra/MODIS and Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6-7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and The United States. |
| Completed |
2003-12-01 |
|
China Dust Storm seen by Ter
| Title |
China Dust Storm seen by Terra/MODIS and Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6-7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and The United States. |
| Completed |
2003-12-01 |
|
China Dust Storm seen by Ter
| Title |
China Dust Storm seen by Terra/MODIS and Earth Probe/TOMS in April of 2001 |
| Abstract |
A thick shroud of dust appears over China on April 6-7, 2001. The densest portion of the aerosol pollution travels east over China, Russia, Japan, the Pacific Ocean, Canada, and The United States. |
| Completed |
2003-12-01 |
|
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