The evolution and the secondary maximum of the green line intensity

Details The evolution and the secondary maximum of the green line intensity The evolution and the secondary maximum of the green line intensity

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...76..181x&link_type=abstract

Solar Physics, vol. 76, Feb. 1982, p. 181-190.

Physics

9

Line Spectra, Solar Corona, Solar Cycles, Solar Protons, Solar Spectra, Spectral Energy Distribution, Maxima, Solar Activity, Solar Magnetic Field

Scientific paper

A new relation is given for calculating the intensity of the green line of the solar corona at 5303 A as a function of the number of proton events and the solar activity index. The relation is available for the 19th and 20th solar cycles. In addition, a theoretical justification is given for the relationship, taking into account as a new parameter the evolution of the coronal magnetic field during the solar cycle.

Affiliated with

Also associated with

No associations

Rating

The evolution and the secondary maximum of the green line intensity 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 evolution and the secondary maximum of the green line intensity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The evolution and the secondary maximum of the green line intensity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1648590