{ "count": 26, "next": null, "previous": null, "results": [ { "id": 4808, "url": "https://svs.gsfc.nasa.gov/4808/", "result_type": "Visualization", "release_date": "2020-11-09T00:00:00-05:00", "title": "NASA/JAXA GPM Satellite Eyes Eta Over Florida", "description": "Tropical Storm Eta making landfall over the Florida Keys on Sunday, November 8, 2020 at approximately 23:11Z (11/9/2020 4:11 EST). || eta1109_001.4300_print.jpg (1024x576) [149.3 KB] || eta1109_001.4300_searchweb.png (320x180) [116.5 KB] || eta1109_001.4300_thm.png (80x40) [8.6 KB] || eta1109_001.mp4 (1920x1080) [47.6 MB] || tif (1920x1080) [0 Item(s)] || exr (1920x1080) [0 Item(s)] || eta1109_001.webm (1920x1080) [5.7 MB] || eta1109_001.mp4.hwshow [177 bytes] || ", "hits": 60 }, { "id": 3740, "url": "https://svs.gsfc.nasa.gov/3740/", "result_type": "Visualization", "release_date": "2010-07-08T00:00:00-04:00", "title": "Space Weather Event: The View from L1", "description": "We start from a position 'behind' the Earth, looking towards the Sun. From this position we see the orbit of the Moon as well as three of the heliospheric 'sentinels' (see \"Sentinels of the Heliosphere\"), ACE, SOHO, and Wind patrolling along 'halo orbits' (Wikipedia) around the Sun-Earth Lagrange Point, L1.The CME (orange isosurface) erupts, heading towards the Earth. The density enhancement of the CME is visible in slice of data in the Earth's orbit plane which provides a better sense of when the CME actually reaches the Earth.As the particle density enhancement from the CME strikes the Earth, we see the Earth's magnetosphere respond, with the outer, high density surface (red), 'blown away'. This surface location corresponds roughly to the location of the bow shock. The bow shock has not been eliminated, only some of its particles have been depleted, to be carried off in the CME and solar wind. As the densest material of the CME passes (orange surface), plasma from the CME continues to flow by the Earth, stretching the magnetosphere into a long, thin structure behind the Earth.The magnetosphere slowly recovers from the 'impact', and regions that can confine higher particle densities reform - the red surfaces return. But not for long as the rarefaction behind the CME reaches the Earth. This lower density region provides fewer particles to repopulate the magnetosphere and make it easier for particles confined in the magnetosphere to 'leak' out into the solar wind.For the BATS-R-US model, the isosurface colors are: red=20 AMUs per cubic centimeter, yellow=10.0 AMUs per cubic centimeter, light blue=1.0 AMUs per cubic centimeter, and blue=0.1 AMUs per cubic centimeter. An AMU corresponds to about the mass of a hydrogen atom, the dominant component of the solar wind.This visualization is part of a series of visualizations on space weather modeling. || ", "hits": 37 }, { "id": 3743, "url": "https://svs.gsfc.nasa.gov/3743/", "result_type": "Visualization", "release_date": "2010-07-08T00:00:00-04:00", "title": "Space Weather Event: Close-up on the Earth Environment", "description": "We open with a view from high above the ecliptic plane, at the space between the Sun (left) and the Earth (within the small rectangular box on the right). In the plane of the Earth's orbit, we show a 'slice' of the Enlil model showing the particle density profile of the solar wind (white to yellow for decreasing particle density). The spiral 'rotating water sprinkler' pattern in the density is the Parker spiral (Wikipedia). We zoom down to the Earth as the CME (orange surface) erupts in the direction of the Earth and move into a position above the Earth's orbital plane with the Earth (geospace) environment in view.As the particle density enhancement from the CME strikes the Earth, we see the Earth's magnetosphere respond, with the outer, high density surface (red) 'blown away'. This surface location corresponds roughly to the location of the bow shock. The bow shock has not been eliminated, only some of its particles have been depleted, to be carried off in the CME and solar wind. As the densest material of the CME passes (orange surface), plasma from the CME continues to flow by the Earth, stretching the magnetosphere into a long, thin structure behind the Earth.The magnetosphere slowly recovers from the 'impact', and regions that can confine higher particle densities reform - the red surfaces return. But not for long as the rarefaction (Wikipedia) behind the CME reaches the Earth. This lower density region provides fewer particles to repopulate the magnetosphere and makes it easier for particles confined in the magnetosphere to 'leak' out into the solar wind.For the BATS-R-US model, the isosurface colors are: red=20 AMUs per cubic centimeter, yellow=10.0 AMUs per cubic centimeter, light blue=1.0 AMUs per cubic centimeter, and blue=0.1 AMUs per cubic centimeter. An AMU corresponds to about the mass of a hydrogen atom, the dominant component of the solar wind.This visualization is part of a series of visualizations on space weather modeling. || ", "hits": 39 }, { "id": 3739, "url": "https://svs.gsfc.nasa.gov/3739/", "result_type": "Visualization", "release_date": "2010-07-06T00:00:00-04:00", "title": "Space Weather Event: Incoming View", "description": "We open with a view from high above the ecliptic plane, at the space between the Sun (left) and the Earth (within the small rectangular box on the right). In the plane of the Earth's orbit, we show a 'slice' of the Enlil model showing the particle density profile of the solar wind (white to yellow for decreasing particle density). The spiral 'rotating water sprinkler' pattern in the density is the Parker spiral (Wikipedia). The nested grid pattern centered on the Earth, provides a sense of scale to the scene. The smallest grid square in the opening view is 1,000 Earth radii on each side. The scale changes by a factor of ten for each step larger or smaller in size.We zoom down to the Earth as the CME (orange surface) erupts in the direction of the Earth, then move into a position behind the Earth with the Sun visible in the distance.As the particle density enhancement from the CME strikes the Earth, we see the Earth's magnetosphere respond, with the outer, high density surface (red) 'blown away'. This surface location corresponds roughly to the location of the bow shock. The bow shock has not been eliminated, only some of its particles have been depleted, to be carried off in the CME and solar wind. As the densest material of the CME passes (orange surface), plasma from the CME continues to flow by the Earth, stretching the magnetosphere into a long, thin structure behind the Earth.The magnetosphere slowly recovers from the 'impact', and regions that can confine higher particle densities reform - the red surfaces return. But not for long as the rarefaction (Wikipedia) behind the CME reaches the Earth. This lower density region provides fewer particles to repopulate the magnetosphere and makes it easier for particles confined in the magnetosphere to 'leak' out into the solar wind.For the BATS-R-US model, the isosurface colors correpond to densities of: red=20 AMUs per cubic centimeter, yellow=10.0 AMUs per cubic centimeter, light blue=1.0 AMUs per cubic centimeter, and blue=0.1 AMUs per cubic centimeter. An AMU corresponds to about the mass of a hydrogen atom, so the value roughly corresponds to the number of atoms per cubic centimeter.This visualization is part of a series of visualizations on space weather modeling. || ", "hits": 23 }, { "id": 3746, "url": "https://svs.gsfc.nasa.gov/3746/", "result_type": "Visualization", "release_date": "2010-07-01T20:00:00-04:00", "title": "Hurricane Alex Makes Landfall in Northeastern Mexico", "description": "NASA's TRMM spacecraft observed this view of Hurricane Alex on June 30, 2010 at 2103 UTC (5:02 PM EST). At this time, Hurricane Alex was increasing in intensity and had become a category 2 storm with estimated winds at 75 knots (~86.4 mph) and a pressure reading of 962 mb. The rain structure is taken by TRMM's Tropical Microwave Imager (TMI) and TRMM's Precitation Radar (PR) instruments. The TMI rainfall analysis shows that Alex had a well defined eye containing powerful thounderstorms that were dropping extreme amounts of rain. The clouds are taken by TRMM's visible-infrared radiometer (VIRS) and the National Oceanic and Atmospheric Administration (NOAA) Geostationary Operational Environmental Satellite (GOES-13) infrared instrument. TRMM looks underneath of the storm's clouds to reveal the underlying rain structure. The colored isosurface under the clouds show the rain seen by the PR instrument. Areas of extremely heavy rainfall are colored in red. Heavy rainfall are colored in yellow, moderate rainfall are colored in green, and light rain are in blue. || ", "hits": 75 }, { "id": 3744, "url": "https://svs.gsfc.nasa.gov/3744/", "result_type": "Visualization", "release_date": "2010-06-29T00:00:00-04:00", "title": "Tropical Depression ALEX hits Mexico's Yucatan Peninsula", "description": "NASA's TRMM spacecraft observed this view of Tropical Depression Alex on June 27, 2010 at 2214 UTC (6:14 PM EST). Tropical depression Alex was near the western coast of Mexico's Yucatan Peninsula. Alex had weakened and wasn't dropping the very heavy rainfall that had occurred a day earlier causing deadly flooding. At the time of this image, Alex had winds estimated at 35 knots (~40.3 mph) and a pressure reading of 991 mb. The rain structure is taken by TRMM's Tropical Microwave Imager (TMI) and TRMM's Precitation Radar (PR) instruments. The clouds are taken by TRMM's visible-infrared radiometer (VIRS) and the National Oceanic and Atmospheric Administration (NOAA) Geostationary Operational Environmental Satellite (GOES-13) infrared instrument. TRMM looks underneath of the storm's clouds to reveal the underlying rain structure. The colored isosurface under the clouds show the rain seen by the PR instrument. Areas of extremely heavy rainfall are colored in red. Heavy rainfall are colored in yellow, moderate rainfall are colored in green, and light rain are in blue. || ", "hits": 30 }, { "id": 3660, "url": "https://svs.gsfc.nasa.gov/3660/", "result_type": "Visualization", "release_date": "2009-11-09T12:00:00-05:00", "title": "Tropical Storm Ida Observed on November 9, 2009 at 1218 UTC", "description": "NASA's TRMM spacecraft observed this view of Tropical Storm Ida on November 9, 2009 at 1218 UTC (7:18 AM EST). Scattered convective thunderstorms are shown producing moderate to heavy rainfall of over 50 millimeters per hour (~2 inches) north of IDA's center of circulation and in a strong band on the eastern side. At the time of this image IDA had winds estimated at 70 knots (~80.5 mph). IDA is predicted by the National Hurricane Center in Miami, Florida to hit the Gulf coast near Pensacola, Florida on Tuesday morning. The rain structure is taken by TRMM's Tropical Microwave Imager (TMI) and TRMM's Precitation Radar(PR) instruments. TRMM looks underneath of the storm's clouds to reveal the underlying rain structure. The colored isosurface under the clouds show the rain seen by the PR instrument. || ", "hits": 14 }, { "id": 3626, "url": "https://svs.gsfc.nasa.gov/3626/", "result_type": "Visualization", "release_date": "2009-08-17T12:00:00-04:00", "title": "Hurricane Bill on August 17, 2009 at 1133 UTC", "description": "NASA's TRMM spacecraft observed this view of Hurricane Bill on August 17, 2009 at 1133 UTC. At this time the storm was a category 1 hurricane with sustained winds of 56 knots (64 mph), a pressure reading of 994 millibars. The cloud cover in this animation is taken by TRMM's Visible and Infrared Scanner(VIRS) and the GOES spacecraft. The rain structure is taken by TRMM's Tropical Microwave Imager (TMI) and TRMM's Precitation Radar(PR) instruments. TRMM looks underneath of the storm's clouds to reveal the underlying rain structure. The colored isosurface under the clouds show the rain seen by the PR instrument. || ", "hits": 20 }, { "id": 3559, "url": "https://svs.gsfc.nasa.gov/3559/", "result_type": "Visualization", "release_date": "2008-09-11T12:00:00-04:00", "title": "Hurricane Ike on September 10, 2008 at 1745 UTC", "description": "NASA's TRMM spacecraft observed this view of Hurricane Ike on September 10, 2008 at 1745 UTC or 1:45PM EST. At this time the storm was a category 2 hurricane with sustained winds of 85 knots (97.75 mph), a pressure reading of 958 millibars, and a diameter of 100 miles. The cloud cover in this animation is taken by TRMM's Visible and Infrared Scanner(VIRS) and the GOES spacecraft. The rain structure is taken by TRMM's Tropical Microwave Imager (TMI) and TRMM's Precitation Radar(PR) instruments. TRMM looks underneath of the storm's clouds to reveal the underlying rain structure. The colored isosurface uner the clouds show the rain seen by the PR instrument. This surface is colored according to cloud height where yellow represents 10 km thunderclouds and red represents 15 km or more intense thunderclouds. Ike is expected to generate a 10 to 15 foot storm surge along a 100 mile stretch of the Texas Coast from the eye landfall location. || ", "hits": 22 }, { "id": 3558, "url": "https://svs.gsfc.nasa.gov/3558/", "result_type": "Visualization", "release_date": "2008-09-10T12:00:00-04:00", "title": "Hurricane Ike Strengthens in the Gulf of Mexico on September 10, 2008", "description": "NASA's TRMM spacecraft observed this view of Hurricane Ike on September 10, 2008 as slammed into Cuba . At this time the storm was a category 1 hurricane with sustained winds of 75 knots (86.25 mph) and a pressure reading of 963 millibars. At this time, TRMM's data and aircraft reports confirm the small inner eye is eroding as the outer bands, shown here as red towers, are becoming better defined. This could limit rapid intensity development in the very near term, but the storm is projected to strengthen before it makes landfall. The cloud cover in this animation is taken by TRMM's Visible and Infrared Scanner(VIRS) and the GOES spacecraft. The rain structure is taken by TRMM's Tropical Microwave Imager (TMI) and TRMM's Precitation Radar(PR) instruments. TRMM looks underneath of the storm's clouds to reveal the underlying rain structure. The colored isosurface uner the clouds show the rain seen by the PR instrument. This surface is colored according to cloud height where yellow represents 10 km thunderclouds and red represents 12 km more intense thunderclouds. || ", "hits": 18 }, { "id": 3485, "url": "https://svs.gsfc.nasa.gov/3485/", "result_type": "Visualization", "release_date": "2007-12-10T00:00:00-05:00", "title": "THEMIS and the March 2007 Substorm", "description": "NASA's Time History of Events and Macroscale Interactions during Substorms (THEMIS) mission observed the dynamics of a rapidly developing substorm in March of 2007. This visualization combines the orbits of the THEMIS satellites with a magnetohydrodynamical simulation of the Earth's magnetosphere corresponding to this time. || ", "hits": 28 }, { "id": 3016, "url": "https://svs.gsfc.nasa.gov/3016/", "result_type": "Visualization", "release_date": "2004-09-22T12:00:00-04:00", "title": "TRMM Precipiation Radar Observes Rain Structure of Hurricane Jeanne on September 23, 2004", "description": "NASA's TRMM spacecraft is used by meteorologists to understand Hurricane Jeanne. TRMM recorded this view of Hurricane Jeanne on September 23, 2004. The cloud cover is taken by TRMM's Visible and Infrared Scanner(VIRS) and the rain structure is seen by TRMM's Precipitation Radar (PR). It looks underneath of the storm's clouds to reveal the underlying rain structure. Blue represents areas with at least 0.25 inches of rain per hour. Green shows at least 0.5 inches of rain per hour. Yellow is at least 1.0 inches of rain and Red is at least 2.0 inches of rain per hour. || ", "hits": 11 }, { "id": 2970, "url": "https://svs.gsfc.nasa.gov/2970/", "result_type": "Visualization", "release_date": "2004-08-05T12:00:00-04:00", "title": "Volumetric Visualization of the Convection-generated Stresses in Earth", "description": "The fundamental problem of the deformation of the Earth involves stress conditions on the basis of the crust caused by the mantle convection. Based on decades of satellite gravity data, a harmonic analytical model of the convection flow has been developed at GSFC. The magnitudes and directions of the resultant stresses in the crust were obtained at 64,000 grid points for each of 18 layers from 150 km to 600 km under the Earth. In this project, we explored three dimensional volumetric visualization methods for the data. To overcome the typical volumetric visualization obstacles such as enormous amount of data and opacity of objects in the scene, we developed an interactive and transparent isosurface model to render the volumetric data. a) Animated isosurfaces of earth stress below Hawaii. The blue objects indicate the shape of the stress distribution and the yellow objects indicate the high stress areas. b) Interactive global earth stress. To view the model, please use the QuickTime Player (similarly, please select the QuickTime version of the movie). Hold the left button and drag the mouse horizontally to view areas on the earth at the same depth. Hold the left button and drag the mouse vertically to view the different layers of the stress distributions inside the earth, between 150 km to 600 km deep. || ", "hits": 35 }, { "id": 2820, "url": "https://svs.gsfc.nasa.gov/2820/", "result_type": "Visualization", "release_date": "2003-09-30T12:00:00-04:00", "title": "Recipe of a Hurricane (Part 2) — Clouds and Isosurfaces (Match Rendered)", "description": "This visualization was created in support of the 'Recipe for a Hurricane' live shot campaign. This is a visualization of Hurricane Erin on September 10, 2001. This is the main section of the visualization that shows the GOES and TRMM/VIRS based cloud tops (extruded), the TRMM/PR based rain isosurface, and the CAMEX-4/dropsonde-based heat isosurface. This visualization was match-frame rendered to two other visualizations (winds and isosurfaces) and was intended to be shown edited together. || ", "hits": 14 }, { "id": 2821, "url": "https://svs.gsfc.nasa.gov/2821/", "result_type": "Visualization", "release_date": "2003-09-30T12:00:00-04:00", "title": "Recipe of a Hurricane - Spin Around Clouds and Isosurfaces", "description": "This visualization was created in support of the 'Recipe for a Hurricane' live shot campaign. This is a visualization of hurricane Erin on September 10, 2001. This version of the visualization is a slow spin around the GOES and TRMM/VIRS based cloud tops (extruded), the TRMM/PR based rain isosurface, and the CAMEX-4/dropsonde-based heat isosurface. || ", "hits": 14 }, { "id": 2826, "url": "https://svs.gsfc.nasa.gov/2826/", "result_type": "Visualization", "release_date": "2003-09-30T12:00:00-04:00", "title": "Hurricane Isabel Prepares to Make Landfall in North Carolina, September 17, 2003", "description": "This animation is of Hurricane Isabel on September 17, 2003 as it barrels toward the East Coast of the United States. At this time, Isabel was packing winds of 115 MPH and is classified as a Category 3 storm. The animation peels away the cloud layer and reveals the storm's rain structure. The yellow isosurface represents areas where at least 0.5 inches ofrain fell per hour. The green isosurface show 1.0 inches of rain per hour and red displays where more than 2 inches of rain fell per hour. || ", "hits": 19 }, { "id": 2827, "url": "https://svs.gsfc.nasa.gov/2827/", "result_type": "Visualization", "release_date": "2003-09-30T12:00:00-04:00", "title": "Hurricane Isabel Batters North Carolina, September 18, 2003", "description": "This animation is of Hurricane Isabel on September 18, 2003 as it barrels toward the East Coast of the United States. At this time, Isabel waspacking winds of 105 MPH and was downgraded to a Category 2 storm. The animation peels away the cloud layer and reveals the storm's rain structure. The yellow isosurface represents areas where at least 0.5 inches ofrain fell per hour. The green isosurface show 1.0 inches of rain per hour and red displays where more than 2 inches of rain fell per hour. || ", "hits": 22 }, { "id": 2804, "url": "https://svs.gsfc.nasa.gov/2804/", "result_type": "Visualization", "release_date": "2003-09-16T12:00:00-04:00", "title": "Hurricane Isabel Barrels Down on the East Coast, September 15, 2003", "description": "This animation is of Hurricane Isabel on September 15, 2003 as it barrels toward the East Coast of the United States. At this time, Isabel had maximum sustained winds of 150 mph with gusts up to 160 mph. The eye of the storm has a diameter of 40 nautical miles. The storm is moving to the west-northwest at 7mph. The animation peels away the cloud layer and reveals the storm's rain structure. The yellow isosurface represents areas where at least 0.5 inches of rain fell per hour. The green isosurface show 1.0 inches of rain per hour and red displays where more than 2 inches of rain fell per hour. || ", "hits": 20 }, { "id": 2799, "url": "https://svs.gsfc.nasa.gov/2799/", "result_type": "Visualization", "release_date": "2003-09-11T12:00:00-04:00", "title": "Typhoon Maemi, September 11, 2003", "description": "This animation shows TRMM's view of Typhoon Maemi. Typhoon Maemi was located approximately 400 miles south-southest of Okinawa, Japan. At the time this image was taken, Maemi was classified as a Category 5 storm under the Saffir-Simpson scale because it was packing sustained winds of 172 mph with gusts to 200 mph. The Tropical Rainfall Measuring Mission (TRMM) has provided some remarkable images of Super Typhoon Maemi. During the storm's most intense phase, TRMM was able to capture the evolution of Maemi's eyewall structure as it was starting to undergo a process known as 'eyewall replacement,' whereby two concentric eyewalls are present before the outer eyewall collapses down to replace the original inner eyewall. This process can occur in very intense typhoons and hurricanes. || ", "hits": 31 }, { "id": 2797, "url": "https://svs.gsfc.nasa.gov/2797/", "result_type": "Visualization", "release_date": "2003-09-10T12:00:00-04:00", "title": "Hurricane Ignacio on August 25, 2003", "description": "This animation is of Hurricane Ignacio as it attacks the coast of Baja, California. The animation peels away the cloud layer and reveals the storm's rain structure. The yellow isosurface represents areas where at least 0.5 inches of rain fell per hour. The green isosurface show 1.0 inches of rain per hour and red displays where more than 2 inches of rain fell per hour. || ", "hits": 31 }, { "id": 2794, "url": "https://svs.gsfc.nasa.gov/2794/", "result_type": "Visualization", "release_date": "2003-09-04T12:00:00-04:00", "title": "Hurricane Fabian Approaches Bermuda, September 4, 2003", "description": "This animation is of Hurricane Fabian on September 4, 2003 as it churns towards Bermuda. At this time, Fabian had maximum sustained winds of 120 mph and was moving to the north-northwest at 12 mph. The animation peels away the cloud layer and reveals the storm's rain structure. The yellow isosurface represents areas where at least 0.5 inches of rain fell per hour. The green isosurface show 1.0 inches of rain per hour and red displays where more than 2 inches of rain fell per hour. || ", "hits": 11 }, { "id": 2676, "url": "https://svs.gsfc.nasa.gov/2676/", "result_type": "Visualization", "release_date": "2003-03-18T12:00:00-05:00", "title": "Tour of the Magnetosphere", "description": "Tour of the Earth's magnetosphere generated for 'Live from the Aurora'. This viz pulls out from the Earth and fades in components of the magnetosphere. || ", "hits": 38 }, { "id": 2659, "url": "https://svs.gsfc.nasa.gov/2659/", "result_type": "Visualization", "release_date": "2002-12-30T12:00:00-05:00", "title": "Tropical Cyclone Crystal on December 25, 2002", "description": "Tropical Cyclone Crystal approaches the island of Mauritius in the Indian Ocean. The storm packed sustained winds of 80 miles per hour with gusts up to 96 miles per hour. Mauritius is situated east of Madagascar off of the Africa's southeastern coast. This animation shows the storm's rain structure with 5 different isosurfaces. The first isosurface is gray and depicts areas with 0.5 inches of rain per hour. The second is light blue and reflects 1.0 inches of rain per hour. The third is green and shows 1.7 inches of rain per hour. The fourth is yellow and represents 2.0 inches of rain per hour. The last isosurface is red and shows 2.2 inches or more of rain. || ", "hits": 46 }, { "id": 2647, "url": "https://svs.gsfc.nasa.gov/2647/", "result_type": "Visualization", "release_date": "2002-11-21T12:00:00-05:00", "title": "Tropical Cyclone Boura on November 17, 2002", "description": "Tropical Cyclone Boura approaches Madagascar on November 17, 2002. The storm has intensified over night. The rain structure is depicted with 5 different isosurfaces. The first isosurface is gray and depicts areas with 0.5 inches of rain per hour. The second is light blue and reflects 1.0 inches of rain per hour. The third is green and shows 1.7 inches of rain per hour. The forth is yellow and represents 2.0 inches of rain per hour. The last isosurface is red and shows 2.2 inches or more of rain per hour. || ", "hits": 21 }, { "id": 2734, "url": "https://svs.gsfc.nasa.gov/2734/", "result_type": "Visualization", "release_date": "1999-11-05T12:00:00-05:00", "title": "A Lagrangian Trajectory Filter for the Assimilation of Stratospheric Chemical Observation", "description": "A presentation for the HPCC ESS project. It consists of five separate visualizations on the same data set: a Moving Grid, a Methane Mixing Ratio in Lagrangian Frame, the Methane Mixing Ratio in Eulerian Frame, an Isosurface (see animation 259), and the Methane Mixing Ratio in Cylindrical Projection. || ", "hits": 10 }, { "id": 259, "url": "https://svs.gsfc.nasa.gov/259/", "result_type": "Visualization", "release_date": "1997-11-01T12:00:00-05:00", "title": "Global Methane Isosurface Wave", "description": "An animation of a three-dimensional isosurface of global methane in the atmosphere evolving over time, from a global data assimilation model. The globe of the Earth starts out opaque, then becomes transparent in order to more clearly see the structure of the isosurface. The isosurface exhibits wave breaking in the southern hemisphere. || a000259_thm.png (80x40) [4.6 KB] || a000259_pre.jpg (320x238) [6.2 KB] || a000259_pre_searchweb.jpg (320x180) [38.5 KB] || preview_made_from_dv.00030_print.png (352x240) [99.1 KB] || a000259.webmhd.webm (960x540) [5.2 MB] || a000259.mpg (352x240) [11.5 MB] || ", "hits": 28 } ] }