A physical parameter method for the design of broad-band X-ray imaging systems to do coronal plasma diagnostics

Physics

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Plasma Diagnostics, Solar Corona, Temperature Effects, X Ray Imagery, Broadband, Pressure Measurement, X Ray Spectra, X Ray Telescopes

Scientific paper

The technique commonly used for the analysis of data from broad-band X-ray imaging systems for plasma diagnostics is the filter ratio method. This requires the use of two or more broad-band filters to derive temperatures and line-of-sight emission integrals or emission measure distributions as a function of temperature. Here an alternative analytical approach is proposed in which the temperature response of the imaging system is matched to the physical parameter being investigated. The temperature response of a system designed to measure the total radiated power along the line of sight of any coronal structure is calculated. Other examples are discussed.

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