Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976jgr....81.4508b&link_type=abstract
Journal of Geophysical Research, vol. 81, Sept. 1, 1976, p. 4508-4516. Research supported by the Osservatorio Astrofisico di Ar
Astronomy and Astrophysics
Astronomy
15
Emission Spectra, Geomagnetism, Kp Index, Magnetic Field Configurations, Solar Corona, Solar Wind Velocity, Autocorrelation, Brightness Temperature, Isophotes, Magnetic Effects, Oso-7, Solar Magnetic Field
Scientific paper
The method of superposed epochs is used to determine the average solar wind velocity and the Kp index following central meridian passage of coronal weak and bright features identified from OSO 7 isophotograms of the Fe XV (284 A) emission line. It is found that bright coronal regions possess magnetic fields of closed configuration, thus reducing particle escape, while coronal holes possess open magnetic field lines favorable to particle escape or enhanced outflow of the solar wind.
Bell Barbara
Noci Giancarlo
No associations
LandOfFree
Intensity of the Fe XV emission line corona, the level of geomagnetic activity, and the velocity of the solar wind 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 Intensity of the Fe XV emission line corona, the level of geomagnetic activity, and the velocity of the solar wind, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Intensity of the Fe XV emission line corona, the level of geomagnetic activity, and the velocity of the solar wind will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1415636