STEREO Coronal Mass Ejection: From the EUVI to HI-2

This movie collects imagery from SOHO and STEREO-A of a coronal mass ejection (CME) during January of 2007. The instruments in this view, from left to right, are STEREO/HI-1, STEREO/HI-2, SOHO/LASCO/C3, SOHO/LASCO/C2, and STEREO/EUVI. The Heliospheric Imager, HI-2, shows some of the tail of comet McNaught. The dark trapezoidal shape on the left edge of the image in HI-2 is the Earth occulter which will block out the disk of the Earth when it moves into view (since the planet will appear so bright as to saturate the detectors). Due to ongoing work with the STEREO coronagraphs, COR1 and COR2, the SOHO/LASCO coronagraphs are used for this movie. The blue Sun in the center of the coronagraphs is STEREO/EUVI ultraviolet images.

There is a 22 hour gap in the data coverage for HI-2 which creates the appearance of a jump in the playback.

These are not standard images but are called 'running difference' images which highlight changes in the view. White pixels correspond to increases in brightness, while dark pixels reflect a decrease in brightness, with respect to the immediately previous image.

'Running differencing' generates some unusual effects. For example, the mottled background is created by the motion of the stars through the field-of-view as the spacecraft pointing direction slowly changes (the Andromeda galaxy is the oblong 'smudge' near the upper left corner). The planets Venus (right edge of HI-2) and Mercury are visible (near center of HI-1), their column of pixels saturated due to their brightness.

  • STEREO: Solar TErrestrial RElations Observatory
  • SOHO: SOlar Heliospheric Observatory
  • LASCO: Large Angle and Spectrometric Coronagraph
  • EUVI: Extreme UltraViolet Imager

  • Visualization Credits

    Tom Bridgman (GST): Lead Animator
    Therese Kucera (NASA/GSFC): Scientist
    Russ Howard (NRL): Scientist
    Angelos Vourlidas (NRL): Scientist
    Michael Kaiser (NASA/GSFC): Scientist
    Please give credit for this item to:
    NASA/Goddard Space Flight Center Scientific Visualization Studio

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    Data Used:
    SOHO/Large Angle Spectrometric COronagraph (LASCO)/C2 2007-01-24 to 2007-01-27
    STEREO-A/Heliospheric Imager 2 (HI-2) 2007-01-24 to 2007-01-27
    STEREO-A/Heliospheric Imager 1 (HI-1) 2007-01-24 to 2007-01-27
    STEREO-A/Extreme UltraViolet Imager (EUVI) 2007-01-24 to 2007-01-27
    STEREO 2007-01-24 to 2007-01-27
    SOHO/Large Angle Spectrometric COronagraph (LASCO)/C3 2007-01-24 to 2007-01-27

    This item is part of this series:
    STEREO Post-Launch

    SVS >> Coronal Mass Ejection
    SVS >> HDTV
    SVS >> Heliosphere
    SVS >> SOHO
    SVS >> Sun
    GCMD >> Earth Science >> Sun-earth Interactions
    GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity >> Coronal Properties
    GCMD >> Location >> Corona
    SVS >> Space Weather
    SVS >> Coronagraph
    NASA Science >> Sun

    GCMD keywords can be found on the Internet with the following citation: Olsen, L.M., G. Major, K. Shein, J. Scialdone, S. Ritz, T. Stevens, M. Morahan, A. Aleman, R. Vogel, S. Leicester, H. Weir, M. Meaux, S. Grebas, C.Solomon, M. Holland, T. Northcutt, R. A. Restrepo, R. Bilodeau, 2013. NASA/Global Change Master Directory (GCMD) Earth Science Keywords. Version