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Chilly Temperatures During t …
Title Chilly Temperatures During the Maunder Minimum
Description Many things can change temperatures on Earth: a volcano erupts, swathing the Earth with bright haze that blocks sunlight, and temperatures drop, greenhouse gases trap heat in the atmosphere, and temperatures climb. From 1650 to 1710, temperatures across much of the Northern Hemisphere plunged when the Sun entered a quiet phase now called the Maunder Minimum. During this period, very few sunspots appeared on the surface of the Sun, and the overall brightness of the Sun decreased slightly. Already in the midst of a colder-than-average period called the Little Ice Age, Europe and North America went into a deep freeze: alpine glaciers extended over valley farmland, sea ice crept south from the Arctic, and the famous canals in the Netherlands froze regularly—an event that is rare today. The impact of the solar minimum is clear in this image, which shows the temperature difference between 1680, a year at the center of the Maunder Minimum, and 1780, a year of normal solar activity, as calculated by a general circulation model. Deep blue across eastern and central North America and northern Eurasia illustrates where the drop in temperature was the greatest. Nearly all other land areas were also cooler in 1680, as indicated by the varying shades of blue. The few regions that appear to have been warmer in 1680 are Alaska and the eastern Pacific Ocean (left), the North Atlantic Ocean south of Greenland (left of center), and north of Iceland (top center). If energy from the Sun decreased only slightly, why did temperatures drop so severely in the Northern Hemisphere? Climate scientist Drew Shindell and colleagues at the NASA Goddard Institute for Space Studies tackled that question by combining temperature records gleaned from tree rings, ice cores, corals, and the few measurements recorded in the historical record, with an advanced computer model of the Earth's climate. The group first calculated the amount of energy coming from the Sun during the Maunder Minimum and entered the information into a general circulation model. The model is a mathematical representation of the way various Earth systems—ocean surface temperatures, different layers of the atmosphere, energy reflected and absorbed from land, and so forth—interact to produce the climate. When the model started with the decreased solar energy and returned temperatures that matched the paleoclimate record, Shindell and his colleagues knew that the model was showing how the Maunder Minimum could have caused the extreme drop in temperatures. The model showed that the drop in temperature was related to ozone [ http://earthobservatory.nasa.gov/Library/Ozone/ozone_2.html ], in the stratosphere, the layer of the atmosphere that is between 10 and 50 kilometers from the Earth's surface. Ozone is created when high-energy ultraviolet light from the Sun interacts with oxygen. During the Maunder Minimum, the Sun emitted less strong ultraviolet light, and so less ozone formed. The decrease in ozone affected planetary waves, the giant wiggles in the jet stream that we are used to seeing on television weather reports. The change to the planetary waves kicked the North Atlantic Oscillation (NAO) [ http://earthobservatory.nasa.gov/Study/NAO_200307/NAO.html ]—the balance between a permanent low-pressure system near Greenland and a permanent high-pressure system to its south—into a negative phase. When the NAO is negative, both pressure systems are relatively weak. Under these conditions, winter storms crossing the Atlantic generally head eastward toward Europe, which experiences a more severe winter. (When the NAO is positive, winter storms track farther north, making winters in Europe milder.) The model results, shown above, illustrate that the NAO was more negative on average during the Maunder Minimum, and Europe remained unusually cold. These results matched the paleoclimate record. By creating a model that could reproduce temperatures recorded in paleoclimate records, Shindell and colleagues reached a better understanding of how changes in the stratosphere influence weather patterns. With such an understanding, scientists are better poised to understand what factors could influence Earth's climate in the future. To read more about how ancient temperature records are used to improve climate models, see Paleoclimatology: Understanding the Past to Predict the Future, [ http://earthobservatory.nasa.gov/Study/Paleoclimatology_Understanding/paleoclimatology_understanding.html ] the final installment of a series of articles [ http://earthobservatory.nasa.gov/Study/Paleoclimatology/paleoclimatology_intro.html ] about paleoclimatology on the Earth Observatory. Map adapted from Shindell et al., 2001, copyright AAAS 2001. Terms and conditions of use for material copyright AAAS: Readers may view, browse, and/or download material for temporary copying purposes only, provided these uses are for noncommercial personal purposes. Except as provided by law, this material may not be further reproduced, distributed, transmitted, modified, adapted, performed, displayed, published, or sold in whole or in part, without prior written permission from the publisher.
Smoke Over Northern Europe a …
Title Smoke Over Northern Europe and the Atlantic
Description Although skies may have been mostly cloud-free over Ireland and the United Kingdom on May 10, 2006, a pall of haze dimmed the day. The white haze drifts from the Atlantic Ocean northwest of Ireland, over the island country, and southeast over the Celtic Sea and the English Channel in this photo-like image taken by the Moderate Resolution Imaging Spectroradiometer (MODIS [ http://modis.gsfc.nasa.gov ]) on NASA's Aqua [ http://aqua.nasa.gov/ ] satellite. The smoke is coming from hundreds of fires [ http://earthobservatory.nasa.gov/NaturalHazards/natural_hazards_v2.php3?img_id=13539 ] burning in western Russia, most of which are probably agricultural fires. The fires have been burning since late April, and in that time, the smoke has drifted northwest over Scandinavia, the Norwegian Sea, Iceland, and the Atlantic Ocean before curving south to blanket Ireland. Unrelated to the smoke, the ocean southwest of Ireland is brilliant green-blue where a large phytoplankton bloom is growing. Phytoplankton are microscopic plants that grow in the sun-lit surface waters of the ocean. When large colonies develop, the blooms are visible from space by the bright color they lend the normally dark water. The large image provided above has a resolution of 250 meters per pixel. The image is available in additional resolutions [ http://rapidfire.sci.gsfc.nasa.gov/subsets/subsets.php?Europe.2006130.aqua.2km ] from the MODIS Rapid Response Team. NASA image courtesy the MODIS Rapid Response Team [ http://rapidfire.sci.gsfc.nasa.gov ] at NASA GSFC.
Aurora Over Clouds
Title Aurora Over Clouds
Explanation Aurorae usually occur high above the clouds. The auroral glow [ http://www.geo.mtu.edu/weather/aurora/ ] is created when fast-moving particles ejected [ http://antwrp.gsfc.nasa.gov/apod/ap000309.html ] from the Sun [ http://www.nineplanets.org/sol.html ] impact air molecules high in the Earth's atmosphere [ http://csep10.phys.utk.edu/astr161/lect/earth/atmosphere.html ]. An oxygen molecule [ http://pearl1.lanl.gov/periodic/elements/8.html ], for example, will glow in a green light when reacquiring an electron [ http://www.aip.org/history/electron/ ] lost during a collision with a solar particle. The lowest part of an aurora [ http://www.rog.nmm.ac.uk/leaflets/aurora/aurora.html ] will typically occur at 100 kilometers up, while most clouds [ http://www.cloudyskies.net/clouds.html ] usually exist only below about 10 kilometers. The relative heights of clouds and aurorae are shown clearly in the above picture [ http://www.iww.is/art/shs/pages/page22.html ] from Iceland [ http://www.cia.gov/cia/publications/factbook/geos/ic.html ], where aurorae are relatively common. Over the past weekend, one of the largest sunspot groups [ http://www.sunspot.noao.edu/INFO/INTRODUCTION/sunspot-mar272001.html ] ever recorded has been associated with explosive solar activity [ http://antwrp.gsfc.nasa.gov/apod/ap000403.html ] and expansive terrestrial aurora displays [ http://apod.gsfc.nasa.gov/cgi-bin/apod/apod_search?aurora+AND+Earth ]. Although in Earth's northern hemisphere aurorae [ http://www.pfrr.alaska.edu/~pfrr/AURORA/INDEX.HTM ] are usually seen only in the far north, these aurorae [ http://www.spaceweather.com ] were so prevalent they were imaged by a continuous nighttime camera [ http://concam.net/kp/about.html ] operating in southern Arizona [ http://www.state.az.us/ ]!
Ring of Fire Revisited
Title Ring of Fire Revisited
Explanation Early on Saturday [ http://skyandtelescope.com/observing/objects/eclipses/ article_924_1.asp ], May 31 (UT) the new Moon will once again slide across the Sun's fiery disk, and once again [ http://antwrp.gsfc.nasa.gov/apod/ap020610.html ] an annular solar eclipse [ http://sunearth.gsfc.nasa.gov/eclipse/ASE2003/ ASE2003.html ] will be the result -- since the Moon's apparent diameter [ http://www.rc-astro.com/composite/sun_moon.htm ] will be a little too small to completely cover the Sun [ http://www.earthview.com/tutorial/tutorial.htm ]. But this time celestial geometry [ http://members.aol.com/atsinclair/ecl2003.htm ] has conspired to produce a broad D-shaped region [ http://sunearth.gsfc.nasa.gov/eclipse/ASE2003/ASE2003gif/ ASE2003-1b.GIF ] for viewing the annular phase that extends into the far northern hemisphere, rather than creating a thin track racing across land and sea. The characteristic ring of fire will be visible from northern Scotland, Iceland, and parts of Greenland. Otherwise a partial eclipse will be more widely visible as across Europe, along with parts of Asia and North America, the Moon will appear to take a "bite" out of the Sun. While the northerly observers might certainly expect a dramatic view [ http://www.astrosurf.com/alphaweb/10mai94/ ], it will probably not look quite like this one [ http://www.skyscapes.com/Shadows%20in%20the%20Sky/ RingFire.htm ], recorded with a foreground of palm trees during a 1992 annular eclipse. Want to watch Saturday's eclipse on the web? Check out the planned webcasts from Astronet [ http://www.xs4all.nl/~carlkop/zoneclips/eclipse.html ].
Chilly Temperatures During t …
nasa, nasaimageofthedaygalle …
Many things can change tempe …
maunder_minimum_temperature
mediatype IMAGE
mediatype image
date 2006-08-10
creator NASA -- Map adapted from Shindell et al., 2001, copyright AAAS 2001. Terms and conditions of use for material copyright AAAS: Readers may view, browse, and/or download material for temporary copying purposes only, provided these uses are for noncommercial personal purposes. Except as provided by law, this material may not be further reproduced, distributed, transmitted, modified, adapted, performed, displayed, published, or sold in whole or in part, without prior written permission from the publisher.
identifier maunder_minimum_temperature
Smoke Over Northern Europe a …
nasa, nasanaturalhazards
Although skies may have been …
Ireland_AMO_2006130
mediatype IMAGE
mediatype image
date 2006-05-10
creator NASA -- NASA Image Of The Day
identifier Ireland_AMO_2006130
Ganges Chasma Sands
PIA03990
Sol (our sun)
Mars Orbiter Camera
Title Ganges Chasma Sands
Original Caption Released with Image 8 July 2005 This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows dark, windblown sand in the form of dunes and a broad, relatively flat, sand sheet in Ganges Chasma, part of the eastern Valles Marineris trough complex. The winds responsible for these dunes blew largely from the north. Sand dunes on Mars, unlike their Earthly counterparts, are usually dark in tone. This is a reflection of their composition, which includes minerals that are more rich in iron and magnesium than the common silica-rich dunes of Earth. Similar dark sands on Earth are found in volcanic regions such as Iceland and Hawaii. A large dune field of iron/magnesium-rich grains, in the form fragments of the volcanic rock, basalt, occurs south of Moses Lake, Washington, in the U.S. "Location near": 7.7°S, 45.3°W"Image width": ~3 km (~1.9 mi) "Illumination from": lower left "Season": Southern Spring
Small Volcano in Tempe Terra
PIA01468
Sol (our sun)
Mars Orbiter Camera
Title Small Volcano in Tempe Terra
Original Caption Released with Image (closest point to the planet during the orbit). The local time (on Mars) was late in the afternoon--the Sun was only 10° above the horizon--equivalent to about 5:20 p.m. Malin Space Science Systems and the California Institute of Technology built the MOC using spare hardware from the Mars Observer mission. MSSS operates the camera from its facilities in San Diego, CA. The Jet Propulsion Laboratory's Mars Surveyor Operations Project operates the Mars Global Surveyor spacecraft with its industrial partner, Lockheed Martin Astronautics, from facilities in Pasadena, CA and Denver, CO., Mars is famous for its giant volcanoes, such as Elysium Mons--observed by Mars Global Surveyor in July 1998--and the colossal Olympus Mons--3 times the height of Mt. Everest and as big as the U.S. state of Arizona. However, not all martian volcanoes are large. One of Mars Global Surveyor's most recent pictures, indeed, highlights one of Mars' tiniest volcanoes--a small "shield" volcano with a 2 kilometer (1.2 mile-) long depression at its summit. The small volcano is located in the Tempe-Mareotis Fossae region of Tempe Terra (local context Viking 1 Orbiter image 627a28). Centered at 36.2°N, 85.1°W, this is one of many small volcanoes on Mars. The Mars Global Surveyor MOC image presented here is the first close-up view of one of these small volcanoes. This volcano is similar in both shape and size to many of the small basalt shield volcanoes found on the Snake River Plain in southern Idaho, U.S.A. Other similar volcanic vents are found in Hawaii and Iceland. Basalt is the dark, iron- and magnesium-rich silicate rock found in places like the Snake River Plain, Hawaii, and Iceland. Basalt is also common on the floor of Earth's oceans and on the flat plains of the Moon known as "maria". The volcano seen in this MOC image does not show many of the features generally found around volcanoes of this size on Earth. Instead of the lava flows and leveed channels found on Earth, we see only a faint pattern of subtle, somewhat sinuous ridges and troughs that are radial to the long, elliptical summit depression (or "caldera"). This pattern gives the surface of the volcano and its surroundings quite a rough appearance. Much of the appearance of this "sandpaper-like" texture appears to be unrelated to the volcano, but is instead an expression of the eroded "regolith"--"soil"--that covers the old lava flows. The MOC image suggests that a person hiking around on this small martian volcano would find the walk pretty difficult (especially in a spacesuit). But what an exciting and fascinating walk that would be. Not only would one be able to look, and even hike down, into the 150 m (460 foot) deep caldera, but one could also inspect the spectacular, regularly-spaced ridges seen on the floors of nearby troughs ("e.g.," in the lower 1/3 of this MOC image). These ridges are formed by wind and are probably composed of a mixture of sand and granules--perhaps reworked cinders from ancient volcanic eruptions in the region. Some windblown ridges can also be seen in the shadows on the floor of the volcano's linear caldera. The MOC image was taken at 6:57 a.m. (PDT) on August 22, 1998, during the 506th orbit of Mars Global Surveyor as the spacecraft was nearing its 507th "periapsis"
Small Volcano in Tempe Terra
PIA01468
Sol (our sun)
Mars Orbiter Camera
Title Small Volcano in Tempe Terra
Original Caption Released with Image (closest point to the planet during the orbit). The local time (on Mars) was late in the afternoon--the Sun was only 10° above the horizon--equivalent to about 5:20 p.m. Malin Space Science Systems and the California Institute of Technology built the MOC using spare hardware from the Mars Observer mission. MSSS operates the camera from its facilities in San Diego, CA. The Jet Propulsion Laboratory's Mars Surveyor Operations Project operates the Mars Global Surveyor spacecraft with its industrial partner, Lockheed Martin Astronautics, from facilities in Pasadena, CA and Denver, CO., Mars is famous for its giant volcanoes, such as Elysium Mons--observed by Mars Global Surveyor in July 1998--and the colossal Olympus Mons--3 times the height of Mt. Everest and as big as the U.S. state of Arizona. However, not all martian volcanoes are large. One of Mars Global Surveyor's most recent pictures, indeed, highlights one of Mars' tiniest volcanoes--a small "shield" volcano with a 2 kilometer (1.2 mile-) long depression at its summit. The small volcano is located in the Tempe-Mareotis Fossae region of Tempe Terra (local context Viking 1 Orbiter image 627a28). Centered at 36.2°N, 85.1°W, this is one of many small volcanoes on Mars. The Mars Global Surveyor MOC image presented here is the first close-up view of one of these small volcanoes. This volcano is similar in both shape and size to many of the small basalt shield volcanoes found on the Snake River Plain in southern Idaho, U.S.A. Other similar volcanic vents are found in Hawaii and Iceland. Basalt is the dark, iron- and magnesium-rich silicate rock found in places like the Snake River Plain, Hawaii, and Iceland. Basalt is also common on the floor of Earth's oceans and on the flat plains of the Moon known as "maria". The volcano seen in this MOC image does not show many of the features generally found around volcanoes of this size on Earth. Instead of the lava flows and leveed channels found on Earth, we see only a faint pattern of subtle, somewhat sinuous ridges and troughs that are radial to the long, elliptical summit depression (or "caldera"). This pattern gives the surface of the volcano and its surroundings quite a rough appearance. Much of the appearance of this "sandpaper-like" texture appears to be unrelated to the volcano, but is instead an expression of the eroded "regolith"--"soil"--that covers the old lava flows. The MOC image suggests that a person hiking around on this small martian volcano would find the walk pretty difficult (especially in a spacesuit). But what an exciting and fascinating walk that would be. Not only would one be able to look, and even hike down, into the 150 m (460 foot) deep caldera, but one could also inspect the spectacular, regularly-spaced ridges seen on the floors of nearby troughs ("e.g.," in the lower 1/3 of this MOC image). These ridges are formed by wind and are probably composed of a mixture of sand and granules--perhaps reworked cinders from ancient volcanic eruptions in the region. Some windblown ridges can also be seen in the shadows on the floor of the volcano's linear caldera. The MOC image was taken at 6:57 a.m. (PDT) on August 22, 1998, during the 506th orbit of Mars Global Surveyor as the spacecraft was nearing its 507th "periapsis"
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.
Sand Dunes in Noachis Terra
PIA05293
Sol (our sun)
Mars Orbiter Camera
Title Sand Dunes in Noachis Terra
Original Caption Released with Image 11 February 2004 This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows dark-toned sand dunes in a crater in eastern Noachis Terra. Most big martian dunes tend to be dark, as opposed to the more familiar light-toned dunes of Earth. This difference is a product of the composition of the dunes, on Earth, most dunes contain abundant quartz. Quartz is usually clear (transparent), though quartz sand grains that have been kicked around by wind usually develop a white, frosty surface. On Mars, the sand is mostly made up of the darker minerals that comprise iron- and magnesium-rich volcanic rocks--i.e., like the black sand beaches found on volcanic islands like Hawaii. Examples of dark sand dunes on Earth are found in central Washington state and Iceland, among other places. This picture is located near 49.0°S, 326.3°W. Sunlight illuminates this scene from the upper left, the image covers an area 3 km (1.9 mi) wide.
Olympus Mons Lava Flows
PIA03763
Sol (our sun)
Thermal Emission Imaging Sys …
Title Olympus Mons Lava Flows
Original Caption Released with Image (Released 05 April 2002) Olympus Mons stands 26 km above the surrounding plains, which is three times taller than Mt. Everest, and is the tallest volcano in the solar system. Olympus Mons is also wider (585 km) than the state of Arizona. Although these are impressive dimensions an astronaut would find walking these slopes easy, as they are typically only 2 to 5 degrees. This image contains numerous lava flows, leveed lava channels, a discontinuous sinuous rille (thought to be a collapsed lava tube) and lava plains. Close examination of the sinuous rille reveals that portions of the roof of the lava tube have not completely collapsed. All of these features can be seen in basaltic (iron and magnesium rich black rock) volcanic regions on Earth like Hawaii and Iceland. Impact craters are scarce, indicating a relatively young age (several hundred million years old) for these surfaces.
Olympus Mons Lava Flows
PIA03763
Sol (our sun)
Thermal Emission Imaging Sys …
Title Olympus Mons Lava Flows
Original Caption Released with Image (Released 05 April 2002) Olympus Mons stands 26 km above the surrounding plains, which is three times taller than Mt. Everest, and is the tallest volcano in the solar system. Olympus Mons is also wider (585 km) than the state of Arizona. Although these are impressive dimensions an astronaut would find walking these slopes easy, as they are typically only 2 to 5 degrees. This image contains numerous lava flows, leveed lava channels, a discontinuous sinuous rille (thought to be a collapsed lava tube) and lava plains. Close examination of the sinuous rille reveals that portions of the roof of the lava tube have not completely collapsed. All of these features can be seen in basaltic (iron and magnesium rich black rock) volcanic regions on Earth like Hawaii and Iceland. Impact craters are scarce, indicating a relatively young age (several hundred million years old) for these surfaces.
The Land of Ice and Fire
PIA03426
Sol (our sun)
Multi-angle Imaging SpectroR …
Title The Land of Ice and Fire
Original Caption Released with Image . Each image represents an area of about 200 by 340 kilometers. Two of Iceland's larger icecaps, Langjökull (located just below image center) and Hofsjökull (just above center) can be clearly seen. The western edge of Vatnajökull is also visible at the top of the image, and a portion of Myrdalsjökull can be seen through the clouds in the upper right. Langjökull (the Long Glacier, 1287 meters maximum elevation)is the second largest icecap in Iceland. It supplies water to Lake Pingvallavatn, the largest lake in the country (visible in the lower right), and to several other lakes and geothermal areas. Hofsjökull (the Temple Glacier, 1760 meters) is the third largest icecap in Iceland. The landscape under the ice is the great mountain mass if of a central subglacial volcano. The brighter, rounded area atop the icecap is a vast, ice filled caldera. The Pjórsá, Iceland's longest and largest river, is fed by the Hofsjökull icecap. The river can be seen running adjacent to the icecap toward the Atlantic Ocean at image right. Iceland has a very vigorous climate, and the high-energy coastline and glacial melt waters result in the movement of a large amount of sediment to the sea, visible herein the turbid waters of the Pjórsá. The capital city of Reykjavík is visible in the lower right as a greyish region along the coast, to the west of (below) a bank of cumulus clouds. Reykjavík is located about 20 kilometers west of the Reykjanes-Langjökull volcanic zone, and the name of the city, the "Bay of Smokes", is testimony to the region's geothermal activity. MISR was built and is managed by NASA's Jet Propulsion Laboratory, Pasadena, CA, for NASA's Office of Earth Science, Washington, DC. The Terra satellite is managed by NASA's Goddard Space Flight Center, Greenbelt, MD. JPL is a division of the California Institute of Technology., Due to an unusual combination of tectonic settings, many icecaps and glaciers of Iceland rest above active volcanoes. This landnation is located on the northern edge of the Mid-Atlantic ridge, at the intersection of the North American and Eurasian plates, and is one of the few places on Earth where a mid-ocean ridge is exposed above sea level. The land is built from erupted and intruded magmas concentrated around a hot spot beneath the spreading ridge. These late summer views of central and southwestern Iceland were obtained by the Multi-angle Imaging SpectroRadiometer on August 16,2001, during Terra orbit 8842. The upper image is a true-color view from the instrument's vertical-viewing (nadir) camera. The lower image is a stereo anaglyph generated from the instrument's nadir and 60-degree forward-viewing cameras. Viewing the anaglyph in 3-D requires the use of red/blue glasses with the red filter placed over your left eye. The images have been oriented with north at the left in order to facilitate stereo viewing. Information on ordering glasses is available here [ http://photojournal.jpl.nasa.gov/Help/VendorList.html#Glasses ]
A Vortex Street in the Arcti …
PIA03448
Sol (our sun)
Multi-angle Imaging SpectroR …
Title A Vortex Street in the Arctic
Original Caption Released with Image Marine stratocumulus clouds frequently form parallel rows, or "cloud streets", along the direction of wind flow. When the flow is interrupted by an obstacle such as an island, a series of organized eddies can appear within the cloud layer downwind of the obstacle. These turbulence patterns are known as von Karman vortex streets. In these images from NASA's Multi-angle Imaging SpectroRadiometer, an impressive vortex pattern continues for over three hundred kilometers southward of Jan Mayen island. Jan Mayen is an isolated territory of Norway, located about 650 kilometers northeast of Iceland in the north Atlantic Ocean. Jan Mayen's Beerenberg volcano rises about 2.2 kilometers above the ocean surface, providing a significant impediment to wind flow. These MISR images were captured on June 6, 2001, during Terra orbit 7808. The entire vortex street can be seen in the top panel, which is a natural-color view from the instrument's nadir (downward-looking) camera. The area covered measures 365 kilometers x 158 kilometers, and a cloud-clearing effect is apparent at the vortex centers until finally closing on the sixteenth"hole." The bottom panel is a stereo anaglyph of a portion of the vortex street, compiled using data from MISR's 26-degree forward and 70-degree backward viewing cameras. This view covers an area of about 183 kilometers x 96 kilometers. Despite the vertical exaggeration afforded by using widely separated angles, the relatively modest height variation in the cloud layer implies a vertically stable atmosphere. To facilitate stereo viewing, the images have been oriented with north at the left. Red/blue glasses should be used with the red filter placed over your left eye. Information on ordering glasses can be found here [ http://photojournal.jpl.nasa.gov/Help/VendorList.html#Glasses ]. Fluid dynamicist Theodore von Karman was the first to derive the conditions under which these turbulence patterns occur. Von Karman was a professor of aeronautics at the California Institute of Technology and one of the principal founders of NASA's Jet Propulsion Laboratory. MISR was built and is managed by NASA's Jet Propulsion Laboratory, Pasadena, CA, for NASA's Office of Earth Science, Washington, DC. The Terra satellite is managed by NASA's Goddard Space Flight Center, Greenbelt, MD. JPL is a division of the California Institute of Technology.
Streamlined Hills of Maja Va …
PIA04523
Sol (our sun)
Thermal Emission Imaging Sys …
Title Streamlined Hills of Maja Vallis
Original Caption Released with Image Released 16 May 2003 Classic catastrophic flood morphology (streamlined hills and longitudinal grooves) is captured in this image of Lunae Planum. Similar features (although much smaller in size) are seen in terrestrial catastrophic flood regions such as Channeled Scabland of Washington state and in Iceland. Image information: VIS instrument. Latitude 14.8, Longitude 301.8East (58.2). 19 meter/pixel resolution. Note: this THEMIS visual image has not been radiometrically nor geometrically calibrated for this preliminary release. An empirical correction has been performed to remove instrumental effects. A linear shift has been applied in the cross-track and down-track direction to approximate spacecraft and planetary motion. Fully calibrated and geometrically projected images will be released through the Planetary Data System in accordance with Project policies at a later time. NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Office of Space Science, Washington, D.C. The Thermal Emission Imaging System (THEMIS) was developed by Arizona State University, Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing. The THEMIS investigation is led by Dr. Philip Christensen at Arizona State University. Lockheed Martin Astronautics, Denver, is the prime contractor for the Odyssey project, and developed and built the orbiter. Mission operations are conducted jointly from Lockheed Martin and from JPL, a division of the California Institute of Technology in Pasadena.
Streamlined Hills of Maja Va …
PIA04523
Sol (our sun)
Thermal Emission Imaging Sys …
Title Streamlined Hills of Maja Vallis
Original Caption Released with Image Released 16 May 2003 Classic catastrophic flood morphology (streamlined hills and longitudinal grooves) is captured in this image of Lunae Planum. Similar features (although much smaller in size) are seen in terrestrial catastrophic flood regions such as Channeled Scabland of Washington state and in Iceland. Image information: VIS instrument. Latitude 14.8, Longitude 301.8East (58.2). 19 meter/pixel resolution. Note: this THEMIS visual image has not been radiometrically nor geometrically calibrated for this preliminary release. An empirical correction has been performed to remove instrumental effects. A linear shift has been applied in the cross-track and down-track direction to approximate spacecraft and planetary motion. Fully calibrated and geometrically projected images will be released through the Planetary Data System in accordance with Project policies at a later time. NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Office of Space Science, Washington, D.C. The Thermal Emission Imaging System (THEMIS) was developed by Arizona State University, Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing. The THEMIS investigation is led by Dr. Philip Christensen at Arizona State University. Lockheed Martin Astronautics, Denver, is the prime contractor for the Odyssey project, and developed and built the orbiter. Mission operations are conducted jointly from Lockheed Martin and from JPL, a division of the California Institute of Technology in Pasadena.
Dark Barchan Dunes
PIA05920
Sol (our sun)
Mars Orbiter Camera
Title Dark Barchan Dunes
Original Caption Released with Image 13 May 2004 This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows north polar sand dunes in the summertime. During winter and early spring, north polar dunes are covered with bright frost. When the frost sublimes away, the dunes appear darker than their surroundings. To a geologist, sand has a very specific meaning. A sand grain is defined independently of its composition, it is a particle with a size between 62.5 and 2000 microns. Two thousand microns equals 2 millimeters. The dunes are dark because they are composed of sand grains made of dark minerals and/or rock fragments. Usually, dark grains indicate the presence of unoxidized iron, for example, the dark volcanic rocks of Hawaii, Iceland, and elsewhere. This dune field is located near 71.7°N, 51.3°W. Dune slip faces indicate winds that blow from the upper left toward lower right. This picture covers an area approximately 3 km (1.9 mi) across and is illuminated by sunlight from the lower left.
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