Partial Halo CME on 20021124 - SOHO/LASCO C3 Data

COMMENTS: The CME was due to a filament eruption, which occured north-east from an AR 0200. The axial component of the erupted magnetic field was northwardly directed. We expect that the Bz component of the IMF will be unsettled, changing from S to N.

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
    BBSO Halpha and SOHO MDI/EIT images are courtesy of Active Region Monitor

    Automaticaly Generated on Mon Nov 25 15:54:18 2002
    Please, send questions and comments to Vasyl Yurchyshyn