Determination of the energy or pressure of a solar X-ray structure using X-ray filtergrams from a single filter

Details Determination of the energy or pressure of a solar X-ray structure using X-ray filtergrams from a single filter Determination of the energy or pressure of a solar X-ray structure using X-ray filtergrams from a single filter

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...48..255k&link_type=abstract

Solar Physics, vol. 48, June 1976, p. 255-259.

Astronomy and Astrophysics

Astronomy

25

Filtergrams, Plasma Flux Measurement, Solar Flux Density, Solar X-Rays, Spaceborne Astronomy, X Ray Telescopes, Optical Filters, Skylab Program, Solar Temperature, X Ray Density Measurement

Scientific paper

While the X-ray fluxes measured through two different broadband filters can be used to derive the temperatures and emission measures of solar plasmas, it is generally assumed that no plasma parameters can be measured quantitatively with a single filtergram alone. It is shown that the thermal energy density (or pressure) of a solar plasma can be measured with an ideal single filtergram. Calculations have been done to compare the properties of the Skylab S-054 X-ray telescope filters with those of the ideal filter.

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