Computer solutions for studying correlations between solar magnetic fields and SKYLAB X-ray observations

Details Computer solutions for studying correlations between solar magnetic fields and SKYLAB X-ray observations Computer solutions for studying correlations between solar magnetic fields and SKYLAB X-ray observations

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...53...97t&link_type=abstract

Solar Physics, vol. 53, July 1977, p. 97-110.

Physics

23

Computer Techniques, H Alpha Line, Skylab Program, Solar Magnetic Field, Solar X-Rays, Correlation, Magnetic Effects, Magnetometers, Photosphere, Solar Spectra

Scientific paper

A method is described which correlates the NASA-Marshall Space Flight Center (MSFC) Image Data Processing System (IDAPS) and MSFC magnetograph data to X-ray and H-alpha observations from the Skylab mission. Solutions of Laplace's equation in three dimensions, based on the magnetograph data, are convolved with observed X-ray and H-alpha regions. Matched filtering (template matching) provides a best fit of the observed X-ray regions to the computed total magnetic vector magnitude between 10,000 and 15,000 km above the photosphere.

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