Halo CME on 20031111 - SOHO/LASCO C3 Data

COMMENTS: The direction of the magnetic field is hard to determine due to close proximity to the solar limb. The estimates below are given for the southward magnetic field.

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 Thu Nov 13 11:06:40 2003
    Please, send questions and comments to Vasyl Yurchyshyn