Solar flare gamma-ray line spectroscopy

Details Solar flare gamma-ray line spectroscopy Solar flare gamma-ray line spectroscopy

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..253m&link_type=abstract

In its 19th Intern. Cosmic Ray Conf., Vol. 4 p 253-256 (SEE N85-34729 23-92)

Computer Science

Numerical Analysis

Abundance, Compton Effect, Density (Number/Volume), Fluence, Gamma Ray Spectra, Ion Scattering, Line Spectra, Protons, Solar Flares, Spectroscopy, Ionizing Radiation, Mathematical Models, Numerical Analysis, Photon Density, Spectral Emission

Scientific paper

The techniques and the results of solar elemental abundance determinations using observations of gamma ray lines from the April 27 1981 solar flare were outlined. The techniques are elaborated on and observed and the best-fitting theoretical spectra are presented. Numerical values for the photon fluences and the total number of protons involved in the thick-target production of these gamma rays are derived.

Affiliated with

Also associated with

No associations

Rating

Solar flare gamma-ray line spectroscopy 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 Solar flare gamma-ray line spectroscopy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar flare gamma-ray line spectroscopy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-756047