Halo CME on 20021219 - SOHO/LASCO C3 Data

COMMENTS: The axial magnetic field in the CME was SN oriented and the azimuthal field was mainly EW directed and slightly inclined to the south. Therefore, we do not expect a strong southward component to be present in the IMF.

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 Fri Dec 20 09:21:56 2002
    Please, send questions and comments to Vasyl Yurchyshyn