Halo CME on 20031026 - SOHO/LASCO C3 Data

COMMENTS: The CME originated in AR0484 and it is a fast one, so there are good chances that the corresponding solar wind disturbance may have a significant southward Bz component when it reaches the earth. The numbers below are estimates of the upper bound for the Bz and the Dst.

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 Mon Oct 27 16:32:50 2003
    Please, send questions and comments to Vasyl Yurchyshyn