CME associations with quiet and active solar features

Details CME associations with quiet and active solar features CME associations with quiet and active solar features

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998newa....3..321r&link_type=abstract

New Astronomy, vol. 5, no. 3, p. 321-333.

Astronomy and Astrophysics

Astronomy

1

Sun: Activity, Sun: Flares, Sun: Corona, Sunspots, Sun: Faculae, Plages

Scientific paper

While studying CME phenomenology the existence of different physical conditions were considered. These conditions are roughly described by the CME association to different solar active phenomena. We considered three different typical locations in which CME and associated solar activity may occur; in sunspots, plages and the large scale magnetic field pattern, which has not been included earlier. No matter the large uncertainty of the CME association to solar features, due to the observational method and the CME scale; from data exploration some tendencies were obtained and discussed. No evidence was found that the process that leads to coronal mass ejections starts before their detection at 1.6 solar radii. This indicates that the whole volume moves upward simultaneously, no matter how deep it reaches into the solar atmosphere.

Affiliated with

Also associated with

No associations

Rating

CME associations with quiet and active solar features 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 CME associations with quiet and active solar features, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CME associations with quiet and active solar features will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1271560