Halo CME on 20050822 - SOHO/LASCO C3 Data

COMMENTS:It is a very fast CME, however, because it originated very close to the limb it does not have a potential to produce an intense geomagnetic storm. The upper values for Bz and Dst are estimated to be about -20nT and -140nT, respectively.

1Numbers in red are estimates. Numbers in parenthesis (if any) are actual measured values
*These estimates should be compared to the observed 1 hour averaged ACE and Dst values

  • Real Time Dst from World Data Center for Geomagnetism, Kyoto
  • Predicted Dst from Nonlinear Dynamics and Space Physics group
  • Real Time ACE data
  • Today's Space Weather

    Full Disk Halpha Full Disk SOHO/MDI Full Disk SOHO/EIT195
    Active Region Halpha Active Region SOHO/MDI Active Region /EIT195
    Images are courtesy of Active Region Monitor

    Automaticaly Generated on Tue Aug 23 15:42:26 2005
    Please, send questions and comments to Vasyl Yurchyshyn