Identification of driver gas-associated BZ events and prediction of their orientation

Details Identification of driver gas-associated BZ events and prediction of their orientation Identification of driver gas-associated BZ events and prediction of their orientation

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992stin...9228059z&link_type=abstract

Unknown

Physics

Identifying, Photosphere, Solar Atmosphere, Solar Flares, Solar Magnetic Field, Solar Physics, Sun, Comparison, Models, Regions, Rotation

Scientific paper

An approach for identifying a driver gas-associated Bz event and its solar source is introduced. Seven newly identified events are used to further test the model developed by Hoeksema and Zhao 1991 for prediction of the magnetic orientation of some driver gas-associated Bz events from photospheric field observations. Comparison of the model predictions with observations confirms that the model may be appropriate only for those driver gas-associated Bz events which have magnetic structures lacking large internal field rotation and are associated with active region-CMEs.

Affiliated with

Also associated with

No associations

Rating

Identification of driver gas-associated BZ events and prediction of their orientation does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Identification of driver gas-associated BZ events and prediction of their orientation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Identification of driver gas-associated BZ events and prediction of their orientation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-941194