The X-ray line and continuum emission from a solar active region

Details The X-ray line and continuum emission from a solar active region The X-ray line and continuum emission from a solar active region

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...42..209l&link_type=abstract

Solar Physics, vol. 42, May 1975, p. 209-214.

Physics

Continuous Spectra, Emission Spectra, Line Spectra, Solar Activity, Solar X-Rays, X Ray Spectra, Astronomical Models, Rocket-Borne Instruments, Solar Spectra, Spectrum Analysis

Scientific paper

The X-ray spectrum of the quiet sun in the energy range of 2.3-6.9 keV was observed from an Aerobee rocket using an uncollimated graphite crystal spectrometer. These results and spatial measurements made with an onboard modulation collimator are analyzed using solar models. Several methods of estimating coronal temperatures are used in the analysis and all yield results within the range of (4 plus or minus 1) million K.

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