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Coronal Mass Ejections (CME): Radio Quiet Variety
This is a simple comparison of SOHO/LASCO/C3 difference images (left side) combined with radio data from Wind/WAVES (right side).

The LASCO difference images are produced from a time series of images by subtracting the previous image from the current image. Moving material therefore appears white on the leading edge and dark behind it. The WAVES spectrograph shows the variation of radio intensity (black is low, violet is high) in frequency (vertical axis) and time(horizontal axis). A vertical white bar marks the time of the LASCO image.

This CME shows no radio-loud emission between 0.2-1.0 MHz.


This movie displays the eruption of the CME synchronized with the radio signal amplitude (color) and frequency.    This movie displays the eruption of the CME synchronized with the radio signal amplitude (color) and frequency.
Duration: 3.0 seconds
Available formats:
  1024x512 (6 fps) MPEG-4   4 MB
  1024x512 (6 fps) Frames
  320x160     PNG           176 KB
  320x160 (30 fps) MPEG-1   545 KB
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Still image showing the CME in eruption. The radio-loud component is not visible (between 0.2-1.0 MHz).    Still image showing the CME in eruption. The radio-loud component is not visible (between 0.2-1.0 MHz).

Available formats:
  1024 x 512       PNG     263 KB
  320 x 160         JPEG     42 KB
  160 x 80           PNG       53 KB
  80 x 40             PNG       14 KB
  320 x 160         PNG     182 KB

Animation Number:3431
Completed:2007-05-23
Animator:Tom Bridgman (GST) (Lead)
Scientist:Natchimuthuk Gopalswamy (NASA/GSFC)
Writer:William Steigerwald (NASA/GSFC)
Platforms/Sensors/Data Sets:Wind/WAVES
 SOHO/Large Angle Spectrometric COronagraph (LASCO)/C3
Data Collected:2005-07-25
Series:CMEs: Radio Loud and Quiet
Keywords:
SVS >> Coronal Mass Ejection
SVS >> Sun
GCMD >> EARTH SCIENCE >> Sun-earth Interactions >> Solar Activity
GCMD >> EARTH SCIENCE >> Sun-earth Interactions >> Solar Activity >> Solar Events
GCMD >> EARTH SCIENCE >> Sun-earth Interactions >> Solar Activity >> Solar Radio Waves
 
 
Please give credit for this item to:
NASA/Goddard Space Flight Center Scientific Visualization Studio


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