High-resolution photography of the solar chromosphere. XXI Determination of the physical conditions in an H-alpha active-region loop

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Astronomical Photography, Chromosphere, Coronal Loops, Solar Prominences, Doppler Effect, Electron Density (Concentration), Electron Energy, H Alpha Line, High Resolution, Solar Spectra

Scientific paper

Values of the electron temperature, electron density, gas density, gas pressure, degree of hydrogen ionization, and other physical conditions are determined at seven locations along the axis of an H-alpha active-region loop observed on the solar disk. Combining these data with earlier results, a fairly complete description is presented of the true geometry, flow velocities, and thermodynamic conditions in such a loop at one moment of time. The physical conditions show a marked variation along the loop. The variations in density and pressure exhibit a wavelike nature, with an apparent wavelength of some 50,000-60,000 km. The results offer the prospect of putting observational constraints on theoretical models of coronal loops and of identifying the types of flows and waves present.

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