Analysis of a series of solar flare X-ray spectra

Details Analysis of a series of solar flare X-ray spectra Analysis of a series of solar flare X-ray spectra

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981stin...8225071m&link_type=abstract

Unknown

Physics

Electron Density (Concentration), Emission Spectra, Line Spectra, Solar Flares, Solar Flux, X Ray Spectra, Conductive Heat Transfer, Proportional Counters, Radiative Heat Transfer, Temperature Measurement, Time Series Analysis, X Ray Spectroscopy

Scientific paper

Thirteen X-ray line spectra (7.8 to 23.0 A) acquired during a solar flare that peaked at 2326 UT were analyzed. The data include fluxes of lines excited throughout the temperature range present in the coronal flare. The coronal flare emission measure began to decrease 500 s or less after the broad band X-ray flux peaked. The differential emission measure was calculated from the data by using collision strengths for a small number of the observed lines.

Affiliated with

Also associated with

No associations

Rating

Analysis of a series of solar flare X-ray spectra 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 Analysis of a series of solar flare X-ray spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Analysis of a series of solar flare X-ray spectra will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1443337