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Therese Kucera



Movie   ID   Roles   Title
The camera transitions to a coordinate system moving with the Earth, keeping the Earth stationary in the field of view while the rest of the solar system spins around it.   3591 Scientist
  STEREO Visits the Lagrange Points - L4 and L5
We finally bring in the view of the HI-2 instrument which shows the outer regions of the dust corona and stars.  Some constellations are visible.  The dark region on the left side of the image is part of the 'Earth Occulter' in the HI-2 instrument.   3405 Scientist
  STEREO Panoramic View
A full-resolution image from STEREO-A/EUVI in 171 Ångstrom ultraviolet light.   3407 Scientist
  STEREO's Extreme UltraViolet Imager (EUVI)
As the CME moves out, the leading edge appears bright while the trailing edge appears dark in difference images.   3406 Scientist
  STEREO Coronal Mass Ejection: From the EUVI to HI-2
While STEREO A continues outward, STEREO B doesn't have quite enough speed and curves back Earthward, receiving an extra boost from the Moon. This is the 'no date' version.   3364 Scientist
  STEREO's Routes to Solar Orbits
We begin our flight through the loops, noting that the more prominent regions on the surface have a higher density of field lines.   3346 Scientist
  Grand Tour of the Coronal Loops Model
This is a stereo version of the movie.  Note the stereo appearance is not that effective because of the predominant green coloration of the movie.<img src='/images/stereoicon.png'>   3286 Scientist
  Flight through the Coronal Loops
Another angle of the model showing a number of active regions.   3287 Scientist
  Rotating Tour of Solar Coronal Loops
  10066 Scientist
  Model for Coronal Mass Ejections
  10064 Scientist
  STEREO Watches the Active Sun
Stereo spacecraft looks at the sun   10060 Scientist
  STEREO On-Station
Stereo uses lunar gravity   10061 Scientist
  STEREO Enroute: The Lunar Flyby
Stereo Beauty Pass   10062 Scientist
  STEREO Spacecraft Beauty-Pass
Stereo: Earth Flyby   10063 Scientist
  STEREO Enroute: Earth Flyby


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