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William Steigerwald
Movie   ID   Roles   Title
This short narrated feature describes how LRO's instruments are used collectively to scout for safe landing sites. The crater depicted in this stereoscopic visualization is ficticious and only intended for illustrative purposes. This set provides stereoscopic content (Left and Right Eye separate) of the visualization.<p><p><p>For complete transcript, click <a href='http://svs.gsfc.nasa.gov/vis/a000000/a003500/a003587/script_9206_00.html'>here</a>.   3587 Writer
  LRO Scouts for Safe Landing Sites - Stereoscopic Version
This set provides stereoscopic images (Left and Right Eye separate) of the visualization. The raw frames provided here have alpha channels and no text labels, so this element can be overlaid over other visuals.   3567 Writer
  How LRO Will Find Safe Landing Sites on the Moon - Stereoscopic Version
This short video feature describes how LRO's instruments are used collectively to scout for safe landing sites. The crater depicted in this animation is ficticious and only intended for illustrative purposes.<p><p>For complete transcript, click <a href='/vis/a010000/a010300/a010349/LRO_Safe_Landings_transcript.htm'>here</a>.   10349 Writer
  LRO Scouts for Safe Landing Sites (Narrated)
The crater depicted in this animation is ficticious and only intended for illustrative purposes. The animation begins with the reveal of a digital elevation map showing sample lunar topography illustrating the kind of data that LRO's LOLA instrument will collect. From this topographic data level surface areas can be derived as the first step to determining safe landing sites. Next, an example temperature map of the lunar surface is revealed to show the sort of data Diviner will collect. Changes in surface temperature will help determine small rock hazards, since they retain and release heat at a different rate than the surrounding regolith. Large rock hazards can be found with LROC's surface imagery. Finally, removing rock hazard areas from level surface areas reveals potential safe landing sites for future lunar missions.   3533 Writer
  How LRO Will Find Safe Landing Sites on the Moon (No Narration)
June 23, 2007   3484 Writer
  The First Season of Noctilucent Clouds from AIM
Still image showing the CME in eruption. The radio-loud component is not visible (between 0.2-1.0 MHz).   3431 Writer
  Coronal Mass Ejections (CME): Radio Quiet Variety
Still image showing the CME in eruption and the radio-loud component of the emission, the bright yellow-orange band between 0.2-1.0 MHz.   3432 Writer
  Coronal Mass Ejections (CME): Radio Loud Variety
In this case, we see the PFSS model matches the TRACE coronal loops very well.   3211 Writer
  Space Weather Forecasting: Quiet Times Ahead
The PFSS model is a poor match for the TRACE coronal loops.   3212 Writer
  Space Weather Forecasting: Active Times Ahead
The X17 event shown here launched a CME at the Earth whose <a href='http://svs.gsfc.nasa.gov/vis/a000000/a002900/a002964'>impact was observed the next day by Earth-orbiting satellites</a>.   2959 Writer
  Halloween Solar Storms from SOHO/EIT, 195 Ångstroms
A solar prominence appears clearly in this band, yet has no obvious counterpart visible in the 195 Angstrom band.   2960 Writer
  Halloween Solar Storms from SOHO/EIT, 304 Ångstroms
The last big X-class flare as the active region rotates back to the far side of the Sun.   2961 Writer
  Halloween Solar Storms from SOHO/EIT and SOHO/LASCO
In the case of low solar wind pressure, the sunward side of the ionosphere is thick (the red region) and some of the atmosphere can be seen trailing off behind the planet.   2962 Writer
  Computer Simulations of the Martian Atmosphere Interacting with the Solar Wind
The particle flux increases dramatically over the polar cap, as they are carried Earthward along the magetic field lines.   2963 Writer
  The NOAA POES Satellite Detects Record Particle Flows into the Earth's Upper Atmosphere
A snapshot of a high-intensity time in the storm. The bright linear structure in the upper left is an artifact created by the edge of the instrument field-of-view.   2964 Writer
  IMAGE Views of the Aurora from Space
As the fast CME engulfs the slower one, another burst of radio emission is detected.   2936 Writer
  The fastest CME of Cycle 23 overtakes another fast CME
A bright moment for the proton aurora - the bright spot near the center.   2861 Writer
  Reconnection: Solar Wind Breaches the Earth's Magnetic Shield
When the solar wind speed is low, the heliosphere is small.   2856 Writer
  Model of the Heliosphere Over the Solar Cycle
The 2.2MeV gamma-ray emission is prominent.   2750 Writer
  RHESSI Observes 2.2 MeV Line Emission from a Solar Flare
The X3.0 flare at AR 10030   2495 Writer
  SOHO/EIT views solar 'Grand Slam'
The X4.8 flare at AR 10039   2496 Writer
  SOHO/EIT Views Solar 'Grand Slam' with Zoom
A view of the oxygen atom flux near the Earths poles at low intensity.   2444 Writer
  IMAGE/HENA Views Oxygen in the Magnetosphere (Rainbow Version)
The polar regions begin to brighten due to increased influx of oxygen atoms onto the upper atmosphere.   2445 Writer
  IMAGE/HENA Views Oxygen in the Magnetosphere (Blue Version)
Oxygen atoms (green) blowing off from the Earths atmosphere.   2435 Writer
  IMAGE/LENA Observes Oxygen Atoms in the near-Earth Environment


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