The emergence of different polarity photospheric flux as the cause of CMEs and interplanetary shocks

Details The emergence of different polarity photospheric flux as the cause of CMEs and interplanetary shocks The emergence of different polarity photospheric flux as the cause of CMEs and interplanetary shocks

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.conf...59b&link_type=abstract

Universidad Nacional Autonoma de Mexico, International Solar Wind 8 Conference, p. 59

Physics

Coronas, Interplanetary Medium, Photosphere, Solar Atmosphere, Stellar Mass Ejection, Magnetic Flux, Shock Waves, Interplanetary Magnetic Fields, Polarity, Magnetic Field Configurations, Solar Wind

Scientific paper

Here we discuss the effect that the emergence of flux with a polarity opposed to that previously established in a certain photospheric region. can have on the magnetic structure of the solar atmosphere. We show that such a flux emergence may lead to the ejection of coronal material into the interplanetary medium (a CME) and also to a rapid change in the velocity of the solar wind from the region, which may eventually lead to the formation of an interplanetary shock.

Affiliated with

Also associated with

No associations

Rating

The emergence of different polarity photospheric flux as the cause of CMEs and interplanetary shocks 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 The emergence of different polarity photospheric flux as the cause of CMEs and interplanetary shocks, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The emergence of different polarity photospheric flux as the cause of CMEs and interplanetary shocks will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-759902