RBSP is designed to help us understand the sun's influence on the Earth and near-Earth space by studying the planet's radiation belts on various scales of space and time.
Understanding the radiation belt environment and its variability has extremely important practical applications in the areas of spacecraft operations, spacecraft and spacecraft system design, mission planning, and astronaut safety.
RBSP is scheduled to launch no earlier than 4:08 a.m. Thursday, Aug. 23 from Cape Canaveral Air Force Station in Florida. The twin probes will lift off on a United Launch Alliance Atlas V rocket.
News conference panelists are:
— Madhulika Guhathakurta, Living With a Star program scientist, NASA Headquarters, Washington
— Mona Kessel, RBSP program scientist, NASA Headquarters
— Barry Mauk, RBSP project scientist, Johns Hopkins University Applied Physics Laboratory (APL), Laurel, Md.
— Rick Fitzgerald, RBSP project manager, APL, Laurel, Md.", "items": [], "extra_data": {} }, { "id": 348409, "url": "https://svs.gsfc.nasa.gov/11027/#media_group_348409", "widget": "Single image", "title": "", "caption": "", "description": "Living with a Star Overview
This image provides the rationale for LWS Program \"Science with relevance to life and society\". The upper half shows the sun's influence on Earth's magnetosphere, ionosphere, mesosphere, interaction with the atmosphere of other planets and understanding basic physical processes of magnetized plasma. The lower half shows the increasing vulnerability of human society to solar flares and coronal mass ejections.
Credit: NASA", "items": [ { "id": 317976, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473378, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/LG_Viz1_Web.jpg", "filename": "LG_Viz1_Web.jpg", "media_type": "Image", "alt_text": "Living with a Star OverviewThis image provides the rationale for LWS Program \"Science with relevance to life and society\". The upper half shows the sun's influence on Earth's magnetosphere, ionosphere, mesosphere, interaction with the atmosphere of other planets and understanding basic physical processes of magnetized plasma. The lower half shows the increasing vulnerability of human society to solar flares and coronal mass ejections.Credit: NASA", "width": 3282, "height": 2473, "pixels": 8116386 } }, { "id": 317977, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473379, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/LG_Viz1_Web_web.jpg", "filename": "LG_Viz1_Web_web.jpg", "media_type": "Image", "alt_text": "Living with a Star OverviewThis image provides the rationale for LWS Program \"Science with relevance to life and society\". The upper half shows the sun's influence on Earth's magnetosphere, ionosphere, mesosphere, interaction with the atmosphere of other planets and understanding basic physical processes of magnetized plasma. The lower half shows the increasing vulnerability of human society to solar flares and coronal mass ejections.Credit: NASA", "width": 320, "height": 241, "pixels": 77120 } } ], "extra_data": {} }, { "id": 348410, "url": "https://svs.gsfc.nasa.gov/11027/#media_group_348410", "widget": "Single image", "title": "", "caption": "", "description": "To track CMEs from the sun to Earth, STEREO uses five digital cameras, from a telescope pointed straight at the sun to a wide-field camera that sees Earth and Venus more than 45 degrees away. By distorting the many fields-of-view into radial coordinates, STEREO scientists can easily watch the CME's transit in a single video.
Credit: NASA/SwRI/STEREO
The video can be found here.", "items": [ { "id": 317978, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473380, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/LG_Viz2a_Still.png", "filename": "LG_Viz2a_Still.png", "media_type": "Image", "alt_text": "To track CMEs from the sun to Earth, STEREO uses five digital cameras, from a telescope pointed straight at the sun to a wide-field camera that sees Earth and Venus more than 45 degrees away. By distorting the many fields-of-view into radial coordinates, STEREO scientists can easily watch the CME's transit in a single video. Credit: NASA/SwRI/STEREOThe video can be found here.", "width": 1280, "height": 720, "pixels": 921600 } }, { "id": 317979, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473381, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/LG_Viz2a_Still_web.png", "filename": "LG_Viz2a_Still_web.png", "media_type": "Image", "alt_text": "To track CMEs from the sun to Earth, STEREO uses five digital cameras, from a telescope pointed straight at the sun to a wide-field camera that sees Earth and Venus more than 45 degrees away. By distorting the many fields-of-view into radial coordinates, STEREO scientists can easily watch the CME's transit in a single video. Credit: NASA/SwRI/STEREOThe video can be found here.", "width": 320, "height": 180, "pixels": 57600 } } ], "extra_data": {} }, { "id": 348411, "url": "https://svs.gsfc.nasa.gov/11027/#media_group_348411", "widget": "Single image", "title": "", "caption": "", "description": "Reprocessed images from NASA's STEREO-A spacecraft allow scientists to trace the anatomy of the December 2008 CME as it moves and changes on its journey from the Sun to the Earth, identify the origin and structure of the material that impacted Earth, and connect the image data directly with measurements at Earth at the time of impact.
Credit: NASA/Goddard Space Flight Center/SwRI/STEREO
The video can be found here.", "items": [ { "id": 317982, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473384, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/LG_Viz2b_Still.jpg", "filename": "LG_Viz2b_Still.jpg", "media_type": "Image", "alt_text": "Reprocessed images from NASA's STEREO-A spacecraft allow scientists to trace the anatomy of the December 2008 CME as it moves and changes on its journey from the Sun to the Earth, identify the origin and structure of the material that impacted Earth, and connect the image data directly with measurements at Earth at the time of impact. Credit: NASA/Goddard Space Flight Center/SwRI/STEREOThe video can be found here.", "width": 1280, "height": 720, "pixels": 921600 } }, { "id": 317981, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473383, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/LG_Viz2b_Still_web.png", "filename": "LG_Viz2b_Still_web.png", "media_type": "Image", "alt_text": "Reprocessed images from NASA's STEREO-A spacecraft allow scientists to trace the anatomy of the December 2008 CME as it moves and changes on its journey from the Sun to the Earth, identify the origin and structure of the material that impacted Earth, and connect the image data directly with measurements at Earth at the time of impact. Credit: NASA/Goddard Space Flight Center/SwRI/STEREOThe video can be found here.", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 317980, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473382, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/LG_Viz2b_Still.tif", "filename": "LG_Viz2b_Still.tif", "media_type": "Image", "alt_text": "Reprocessed images from NASA's STEREO-A spacecraft allow scientists to trace the anatomy of the December 2008 CME as it moves and changes on its journey from the Sun to the Earth, identify the origin and structure of the material that impacted Earth, and connect the image data directly with measurements at Earth at the time of impact. Credit: NASA/Goddard Space Flight Center/SwRI/STEREOThe video can be found here.", "width": 1280, "height": 720, "pixels": 921600 } } ], "extra_data": {} }, { "id": 348412, "url": "https://svs.gsfc.nasa.gov/11027/#media_group_348412", "widget": "Video player", "title": "", "caption": "", "description": "Earth's Magnetosphere
The simulation shows the magnetosphere and its response to the onset of the January 10, 1997 magnetic storm, solar wind arriving from the left. The translucent surface represents the shape and extent of Earth's magnetic field. The colormap indicates plasma density and shows the sunward shock wave around the Earth.
Credit: C. Goodrich
", "items": [ { "id": 317983, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473385, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/LG_Viz3_Still.png", "filename": "LG_Viz3_Still.png", "media_type": "Image", "alt_text": "Earth's MagnetosphereThe simulation shows the magnetosphere and its response to the onset of the January 10, 1997 magnetic storm, solar wind arriving from the left. The translucent surface represents the shape and extent of Earth's magnetic field. The colormap indicates plasma density and shows the sunward shock wave around the Earth. Credit: C. Goodrich", "width": 640, "height": 481, "pixels": 307840 } }, { "id": 317984, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473386, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/LG_Viz3_Still_web.jpg", "filename": "LG_Viz3_Still_web.jpg", "media_type": "Image", "alt_text": "Earth's MagnetosphereThe simulation shows the magnetosphere and its response to the onset of the January 10, 1997 magnetic storm, solar wind arriving from the left. The translucent surface represents the shape and extent of Earth's magnetic field. The colormap indicates plasma density and shows the sunward shock wave around the Earth. Credit: C. Goodrich", "width": 319, "height": 240, "pixels": 76560 } }, { "id": 317987, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473389, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/505283main_ION-MS1-MPEG4_1280X720_29.97.webmhd.webm", "filename": "505283main_ION-MS1-MPEG4_1280X720_29.97.webmhd.webm", "media_type": "Movie", "alt_text": "Earth's MagnetosphereThe simulation shows the magnetosphere and its response to the onset of the January 10, 1997 magnetic storm, solar wind arriving from the left. The translucent surface represents the shape and extent of Earth's magnetic field. The colormap indicates plasma density and shows the sunward shock wave around the Earth. Credit: C. Goodrich", "width": 960, "height": 540, "pixels": 518400 } }, { "id": 317985, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473387, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/505283main_ION-MS1-MPEG4_1280X720_29.97.mp4", "filename": "505283main_ION-MS1-MPEG4_1280X720_29.97.mp4", "media_type": "Movie", "alt_text": "Earth's MagnetosphereThe simulation shows the magnetosphere and its response to the onset of the January 10, 1997 magnetic storm, solar wind arriving from the left. The translucent surface represents the shape and extent of Earth's magnetic field. The colormap indicates plasma density and shows the sunward shock wave around the Earth. Credit: C. Goodrich", "width": 640, "height": 480, "pixels": 307200 } }, { "id": 317986, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473388, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/505283main_ION-MS1-QuickTime_H.264.mov", "filename": "505283main_ION-MS1-QuickTime_H.264.mov", "media_type": "Movie", "alt_text": "Earth's MagnetosphereThe simulation shows the magnetosphere and its response to the onset of the January 10, 1997 magnetic storm, solar wind arriving from the left. The translucent surface represents the shape and extent of Earth's magnetic field. The colormap indicates plasma density and shows the sunward shock wave around the Earth. Credit: C. Goodrich", "width": 640, "height": 480, "pixels": 307200 } } ], "extra_data": {} }, { "id": 348413, "url": "https://svs.gsfc.nasa.gov/11027/#media_group_348413", "widget": "Single image", "title": "", "caption": "", "description": "Top - Comparison of 81-day smoothed sunspot numbers (red), with magnetic activity as represented by the AA-index (yearly averaged (blue) and monthly mean (grey)). The average predictions for sunspot number in solar cycle 24 by the NOAA Solar Cycle Prediction Panel are indicated by dashed lines.
Bottom - Percentage of days per year with solar wind structures of co-rotating high speed streams from coronal holes (blue), transient structures that include CMEs and other transient flows (red), and slow speed flows (green).
Credit: Defined as in Emery et al., 2009, JASTP. Doi: 10.1016/j.jastp.2008.08.005", "items": [ { "id": 317988, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473390, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/LG_Viz4_Web.jpg", "filename": "LG_Viz4_Web.jpg", "media_type": "Image", "alt_text": "Top - Comparison of 81-day smoothed sunspot numbers (red), with magnetic activity as represented by the AA-index (yearly averaged (blue) and monthly mean (grey)). The average predictions for sunspot number in solar cycle 24 by the NOAA Solar Cycle Prediction Panel are indicated by dashed lines.Bottom - Percentage of days per year with solar wind structures of co-rotating high speed streams from coronal holes (blue), transient structures that include CMEs and other transient flows (red), and slow speed flows (green). Credit: Defined as in Emery et al., 2009, JASTP. Doi: 10.1016/j.jastp.2008.08.005", "width": 2999, "height": 2249, "pixels": 6744751 } }, { "id": 317989, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473391, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/LG_Viz4_Web_web.jpg", "filename": "LG_Viz4_Web_web.jpg", "media_type": "Image", "alt_text": "Top - Comparison of 81-day smoothed sunspot numbers (red), with magnetic activity as represented by the AA-index (yearly averaged (blue) and monthly mean (grey)). The average predictions for sunspot number in solar cycle 24 by the NOAA Solar Cycle Prediction Panel are indicated by dashed lines.Bottom - Percentage of days per year with solar wind structures of co-rotating high speed streams from coronal holes (blue), transient structures that include CMEs and other transient flows (red), and slow speed flows (green). Credit: Defined as in Emery et al., 2009, JASTP. Doi: 10.1016/j.jastp.2008.08.005", "width": 319, "height": 239, "pixels": 76241 } } ], "extra_data": {} }, { "id": 348414, "url": "https://svs.gsfc.nasa.gov/11027/#media_group_348414", "widget": "Single image", "title": "", "caption": "", "description": "Model of the Earth's Van Allen radiation belts with the 2 satellites from NASA's Radiation Belt Storm Probes pictured.\r
Credit: NASA", "items": [ { "id": 317990, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473392, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/MK_Viz1_Web.jpg", "filename": "MK_Viz1_Web.jpg", "media_type": "Image", "alt_text": "Model of the Earth's Van Allen radiation belts with the 2 satellites from NASA's Radiation Belt Storm Probes pictured.\rCredit: NASA", "width": 2999, "height": 1495, "pixels": 4483505 } }, { "id": 317991, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473393, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/MK_Viz1_Web_web.jpg", "filename": "MK_Viz1_Web_web.jpg", "media_type": "Image", "alt_text": "Model of the Earth's Van Allen radiation belts with the 2 satellites from NASA's Radiation Belt Storm Probes pictured.\rCredit: NASA", "width": 319, "height": 159, "pixels": 50721 } } ], "extra_data": {} }, { "id": 348415, "url": "https://svs.gsfc.nasa.gov/11027/#media_group_348415", "widget": "Single image", "title": "", "caption": "", "description": "Left to right pictured: Carl McIIwain, James Van Allen, George Ludwig, Ernie Ray.
Credit: University of Iowa", "items": [ { "id": 317992, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473394, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/MK_Viz2_Web.jpg", "filename": "MK_Viz2_Web.jpg", "media_type": "Image", "alt_text": "Left to right pictured: Carl McIIwain, James Van Allen, George Ludwig, Ernie Ray.Credit: University of Iowa", "width": 2583, "height": 1819, "pixels": 4698477 } }, { "id": 317993, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473395, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/MK_Viz2_Web_web.jpg", "filename": "MK_Viz2_Web_web.jpg", "media_type": "Image", "alt_text": "Left to right pictured: Carl McIIwain, James Van Allen, George Ludwig, Ernie Ray.Credit: University of Iowa", "width": 320, "height": 225, "pixels": 72000 } } ], "extra_data": {} }, { "id": 348416, "url": "https://svs.gsfc.nasa.gov/11027/#media_group_348416", "widget": "Single image", "title": "", "caption": "", "description": "Left to right pictured Pickering, James Van Allen, Werner Von Braun holding up a model of Explorer 1 after its successful launch in 1958.
Credit: NASA", "items": [ { "id": 317994, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473396, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/MK_Viz3_Web.jpg", "filename": "MK_Viz3_Web.jpg", "media_type": "Image", "alt_text": "Left to right pictured Pickering, James Van Allen, Werner Von Braun holding up a model of Explorer 1 after its successful launch in 1958.Credit: NASA", "width": 2231, "height": 2830, "pixels": 6313730 } }, { "id": 317995, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473397, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/MK_Viz3_Web_web.jpg", "filename": "MK_Viz3_Web_web.jpg", "media_type": "Image", "alt_text": "Left to right pictured Pickering, James Van Allen, Werner Von Braun holding up a model of Explorer 1 after its successful launch in 1958.Credit: NASA", "width": 319, "height": 405, "pixels": 129195 } } ], "extra_data": {} }, { "id": 348417, "url": "https://svs.gsfc.nasa.gov/11027/#media_group_348417", "widget": "Single image", "title": "", "caption": "", "description": "left: Van Allen's sketch of the inner and outer zones of the radiation belt made after Pioneer 1 and 3 data returns, as the sketch was presented in a paper by J. A. Van Allen and L. A. Frank, in the science journal Nature in 1959. The two lines that go from the upper left to the lower right are the paths of the satellite. The plot is of the radiation dosages received by the two satellites as they pass into and out of the radiation belt zones. Through multiple rocket launches and satellite studies, the general scope and strength of the belts was eventually determined.
Credit: NASA/Goddard Space Flight Center, Time", "items": [ { "id": 317996, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473398, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/MK_Viz4_Web.jpg", "filename": "MK_Viz4_Web.jpg", "media_type": "Image", "alt_text": "left: Van Allen's sketch of the inner and outer zones of the radiation belt made after Pioneer 1 and 3 data returns, as the sketch was presented in a paper by J. A. Van Allen and L. A. Frank, in the science journal Nature in 1959. The two lines that go from the upper left to the lower right are the paths of the satellite. The plot is of the radiation dosages received by the two satellites as they pass into and out of the radiation belt zones. Through multiple rocket launches and satellite studies, the general scope and strength of the belts was eventually determined. Credit: NASA/Goddard Space Flight Center, Time", "width": 2999, "height": 2249, "pixels": 6744751 } }, { "id": 317997, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473399, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/MK_Viz4_Web_web.jpg", "filename": "MK_Viz4_Web_web.jpg", "media_type": "Image", "alt_text": "left: Van Allen's sketch of the inner and outer zones of the radiation belt made after Pioneer 1 and 3 data returns, as the sketch was presented in a paper by J. A. Van Allen and L. A. Frank, in the science journal Nature in 1959. The two lines that go from the upper left to the lower right are the paths of the satellite. The plot is of the radiation dosages received by the two satellites as they pass into and out of the radiation belt zones. Through multiple rocket launches and satellite studies, the general scope and strength of the belts was eventually determined. Credit: NASA/Goddard Space Flight Center, Time", "width": 319, "height": 239, "pixels": 76241 } } ], "extra_data": {} }, { "id": 348418, "url": "https://svs.gsfc.nasa.gov/11027/#media_group_348418", "widget": "Video player", "title": "", "caption": "", "description": "Movie of the changing radiation belts as measured by SAMPEX/LICA from January 1, 1998 to March 1, 2005.
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Credit: NASA/Johns Hopkins University Applied Physics Laboratory
For complete transcript, click here.", "items": [ { "id": 318076, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473471, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/Assembly_Still.png", "filename": "Assembly_Still.png", "media_type": "Image", "alt_text": "This compilation of integration and testing footage shows: solar array deployment testing; electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) magnetometer boom deployment testing; stacked spacecraft vibration testing; magnetic swing testing; launch vehicle separation testing; Electric Field and Waves Suite (EFW) instrument antenna testing; thermal and vacuum testing; spin testing (55 RPM). 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Credit: NASA/Johns Hopkins University Applied Physics LaboratoryFor complete transcript, click here.", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 318069, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473472, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/RBSP_chron2_press_conf_8912_ProRes_1920x1080_29.97.mov", "filename": "RBSP_chron2_press_conf_8912_ProRes_1920x1080_29.97.mov", "media_type": "Movie", "alt_text": "This compilation of integration and testing footage shows: solar array deployment testing; electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) magnetometer boom deployment testing; stacked spacecraft vibration testing; magnetic swing testing; launch vehicle separation testing; Electric Field and Waves Suite (EFW) instrument antenna testing; thermal and vacuum testing; spin testing (55 RPM). Credit: NASA/Johns Hopkins University Applied Physics LaboratoryFor complete transcript, click here.", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 318070, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473473, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/RBSP_chron2_press_conf_8912-H264_Best_1920x1080_29.97.mov", "filename": "RBSP_chron2_press_conf_8912-H264_Best_1920x1080_29.97.mov", "media_type": "Movie", "alt_text": "This compilation of integration and testing footage shows: solar array deployment testing; electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) magnetometer boom deployment testing; stacked spacecraft vibration testing; magnetic swing testing; launch vehicle separation testing; Electric Field and Waves Suite (EFW) instrument antenna testing; thermal and vacuum testing; spin testing (55 RPM). Credit: NASA/Johns Hopkins University Applied Physics LaboratoryFor complete transcript, click here.", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 318071, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473474, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/RBSP_chron2_press_conf_8912-H264_Good_1920x1080_29.97.mov", "filename": "RBSP_chron2_press_conf_8912-H264_Good_1920x1080_29.97.mov", "media_type": "Movie", "alt_text": "This compilation of integration and testing footage shows: solar array deployment testing; electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) magnetometer boom deployment testing; stacked spacecraft vibration testing; magnetic swing testing; launch vehicle separation testing; Electric Field and Waves Suite (EFW) instrument antenna testing; thermal and vacuum testing; spin testing (55 RPM). Credit: NASA/Johns Hopkins University Applied Physics LaboratoryFor complete transcript, click here.", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 318072, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473475, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/RBSP_chron2_press_conf_8912-H264_1280x720_30.mov", "filename": "RBSP_chron2_press_conf_8912-H264_1280x720_30.mov", "media_type": "Movie", "alt_text": "This compilation of integration and testing footage shows: solar array deployment testing; electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) magnetometer boom deployment testing; stacked spacecraft vibration testing; magnetic swing testing; launch vehicle separation testing; Electric Field and Waves Suite (EFW) instrument antenna testing; thermal and vacuum testing; spin testing (55 RPM). Credit: NASA/Johns Hopkins University Applied Physics LaboratoryFor complete transcript, click here.", "width": 1280, "height": 720, "pixels": 921600 } }, { "id": 318073, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473476, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/RBSP_chron2_press_conf_8912-H264_960x720_29.97_Apple_TV.m4v", "filename": "RBSP_chron2_press_conf_8912-H264_960x720_29.97_Apple_TV.m4v", "media_type": "Movie", "alt_text": "This compilation of integration and testing footage shows: solar array deployment testing; electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) magnetometer boom deployment testing; stacked spacecraft vibration testing; magnetic swing testing; launch vehicle separation testing; Electric Field and Waves Suite (EFW) instrument antenna testing; thermal and vacuum testing; spin testing (55 RPM). Credit: NASA/Johns Hopkins University Applied Physics LaboratoryFor complete transcript, click here.", "width": 960, "height": 720, "pixels": 691200 } }, { "id": 318075, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473478, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/RBSP_chron2_press_conf_8912-MPEG4_1920x1080_29.97.mp4", "filename": "RBSP_chron2_press_conf_8912-MPEG4_1920x1080_29.97.mp4", "media_type": "Movie", "alt_text": "This compilation of integration and testing footage shows: solar array deployment testing; electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) magnetometer boom deployment testing; stacked spacecraft vibration testing; magnetic swing testing; launch vehicle separation testing; Electric Field and Waves Suite (EFW) instrument antenna testing; thermal and vacuum testing; spin testing (55 RPM). Credit: NASA/Johns Hopkins University Applied Physics LaboratoryFor complete transcript, click here.", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 318078, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473480, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/RBSP_chron2_press_conf_8912-H264_960x720_29.97_Apple_TV.webmhd.webm", "filename": "RBSP_chron2_press_conf_8912-H264_960x720_29.97_Apple_TV.webmhd.webm", "media_type": "Movie", "alt_text": "This compilation of integration and testing footage shows: solar array deployment testing; electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) magnetometer boom deployment testing; stacked spacecraft vibration testing; magnetic swing testing; launch vehicle separation testing; Electric Field and Waves Suite (EFW) instrument antenna testing; thermal and vacuum testing; spin testing (55 RPM). Credit: NASA/Johns Hopkins University Applied Physics LaboratoryFor complete transcript, click here.", "width": 960, "height": 540, "pixels": 518400 } }, { "id": 318074, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473477, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/RBSP_chron2_press_conf_8912.mov", "filename": "RBSP_chron2_press_conf_8912.mov", "media_type": "Movie", "alt_text": "This compilation of integration and testing footage shows: solar array deployment testing; electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) magnetometer boom deployment testing; stacked spacecraft vibration testing; magnetic swing testing; launch vehicle separation testing; Electric Field and Waves Suite (EFW) instrument antenna testing; thermal and vacuum testing; spin testing (55 RPM). Credit: NASA/Johns Hopkins University Applied Physics LaboratoryFor complete transcript, click here.", "width": 640, "height": 360, "pixels": 230400 } } ], "extra_data": {} }, { "id": 348432, "url": "https://svs.gsfc.nasa.gov/11027/#media_group_348432", "widget": "Single image", "title": "", "caption": "", "description": "CAD rendering of the RBSP spacecraft and enclosing rocket.
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Credit: NASA/ULA/KSC", "items": [ { "id": 318083, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473485, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/Rick_Fritzgerald_5a_300ppi.jpg", "filename": "Rick_Fritzgerald_5a_300ppi.jpg", "media_type": "Image", "alt_text": "The stacked RBSP spacecraft just prior to encapsulation at Astrotech Space Operations in Florida, along with the RBSP team. Credit: NASA/ULA/KSC", "width": 5333, "height": 3000, "pixels": 15999000 } }, { "id": 318084, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473486, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/Rick_Fritzgerald_5a_300ppi_smaller.jpg", "filename": "Rick_Fritzgerald_5a_300ppi_smaller.jpg", "media_type": "Image", "alt_text": "The stacked RBSP spacecraft just prior to encapsulation at Astrotech Space Operations in Florida, along with the RBSP team. Credit: NASA/ULA/KSC", "width": 2500, "height": 1406, "pixels": 3515000 } }, { "id": 318085, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 473487, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011027/Rick_Fritzgerald_5a_300ppi_smaller_web.png", "filename": "Rick_Fritzgerald_5a_300ppi_smaller_web.png", "media_type": "Image", "alt_text": "The stacked RBSP spacecraft just prior to encapsulation at Astrotech Space Operations in Florida, along with the RBSP team. 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Observations from NASA's Van Allen Probes reveal an isolated third ring in the outer radiation belt. || ", "release_date": "2013-02-28T14:00:00-05:00", "update_date": "2023-05-03T13:52:21.659027-04:00", "main_image": { "id": 467722, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011200/a011212/Mona_3_web.png", "filename": "Mona_3_web.png", "media_type": "Image", "alt_text": "NASA's Living With a Star (LWS) program is a space-weather focused and applications driven research program. Its goal is to develop the scientific understanding necessary to effectively address those aspects of the connected sun-Earth system that directly affect life and society. The program is implemented by a series of inter-related science missions, space environment testbeds, and a targeted theory, modeling, and data analysis program. The Van Allen Probes are the second mission in the LWS program. Credit: NASA", "width": 320, "height": 468, "pixels": 149760 } }, { "id": 11073, "url": "https://svs.gsfc.nasa.gov/11073/", "page_type": "Produced Video", "title": "Earth's Song", "description": "Suspended in the dark cosmos, Earth sings to itself in a high-pitched chorus of chirps and beeps. This song is a product of very low frequency radio waves generated by lightning strikes or excited electrons zipping through the Van Allen Belts, two vast swaths of radiation surrounding Earth. While ham radio operators have long detected this eerie planetary sound using inexpensive receivers, the recent recording by specially designed antennas on NASA's twin Van Allen Probes is one of the clearest examples ever captured. But could Earth's chorus be a siren song? The probes are now on a quest to find out whether these radio waves might be powering up otherwise harmless electrons in the Van Allen Belts, turning them into \"killer electrons\" capable of damaging satellites and astronauts. Watch the videos to hear and learn more about this rare recording. || ", "release_date": "2012-11-27T00:00:00-05:00", "update_date": "2023-05-03T13:52:34.760947-04:00", "main_image": { "id": 470922, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011073/SPBoomsFlybyStill_1024x576.jpg", "filename": "SPBoomsFlybyStill_1024x576.jpg", "media_type": "Image", "alt_text": "In space, no one can hear you scream. So how did two NASA probes record Earth singing?", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 11069, "url": "https://svs.gsfc.nasa.gov/11069/", "page_type": "Produced Video", "title": "Van Allen Probes Overview", "description": "The Van Allen Probes (formerly the Radiation Belt Storm Probes, RBSP) will explore the Van Allen Radiation Belts in the Earth's magnetosphere. The charged particles in these regions can be hazardous to both spacecraft and astronauts. Project Scientist Dr. David Sibeck explains the how the mission will explore space weather — changes in Earth's space environment caused by the sun — that can disable satellites, create power grid failures and disrupt GPS service. The mission also will allow researchers to understand fundamental radiation and particle acceleration processes throughout the universe.The 2-year mission launched Thursday, Aug. 23 from Cape Canaveral Air Force Station in Florida. The twin probes lifted off on a United Launch Alliance Atlas V rocket. || ", "release_date": "2012-11-09T12:00:00-05:00", "update_date": "2023-05-03T13:52:38.728118-04:00", "main_image": { "id": 473343, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011000/a011069/RBSP320.jpg", "filename": "RBSP320.jpg", "media_type": "Image", "alt_text": "RBSP Mission OverviewThe two-year RBSP mission will help scientists develop an understanding of Earth's Van Allen radiation belts and related regions that pose hazards to human and robotic explorersFor complete transcript, click here.", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 10809, "url": "https://svs.gsfc.nasa.gov/10809/", "page_type": "Produced Video", "title": "NASA Spacecraft Track Solar Storms From Sun To Earth", "description": "NASA's STEREO spacecraft and new data processing techniques have succeeded in tracking space weather events from their origin in the Sun's ultrahot corona to impact with the Earth 93 million miles away, resolving a 40-year mystery about the structure of the structures that cause space weather: how the structures that impact the Earth relate to the corresponding structures in the solar corona.Despite many instruments that monitor the Sun and a fleet of near-earth probes, the connection between near-Earth disturbances and their counterparts on the Sun has been obscure, because CMEs and the solar wind evolve and change during the 93,000,000 mile journey from the Sun to the Earth.STEREO includes \"heliospheric imager\" cameras that monitor the sky at large angles from the Sun, but the starfield and galaxy are 1,000 times brighter than the faint rays of sunlight reflected by free-floating electron clouds inside CMEs and the solar wind; this has made direct imaging of these important structures difficult or impossible, and limited understanding of the connection between space storms and the coronal structures that cause them.Newly released imagery reveals absolute brightness of detailed features in a large geoeffective CME in late 2008, connecting the original magnetized structure in the Sun's corona to the intricate anatomy of an interplanetary storm as it impacted the Earth three days later. At the time the data were collected, in late 2008, STEREO-A was nearly 45 degrees ahead of the Earth in its orbit, affording a very clear view of the Earth-Sun line.For the press conference Visual 1, a visualization of the STEREO orbits and the 2008 CME, go here.For Visual 7, a CME and reconnection animation, go here.For Visual 8, footage of the October 2003 solar storms, go here. || ", "release_date": "2011-08-18T13:00:00-04:00", "update_date": "2025-01-06T01:15:33.192602-05:00", "main_image": { "id": 484335, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010800/a010809/Main_Science_Still_2.jpg", "filename": "Main_Science_Still_2.jpg", "media_type": "Image", "alt_text": "Short, narrated video about the new ability to track space weather from the sun to the Earth.For complete transcript, click here.", "width": 1280, "height": 720, "pixels": 921600 } } ], "sources": [], "products": [], "newer_versions": [], "older_versions": [], "alternate_versions": [] }