MgH as a diagnostic tool for fluctuations in the solar photosphere

Details MgH as a diagnostic tool for fluctuations in the solar photosphere MgH as a diagnostic tool for fluctuations in the solar photosphere

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...234..530k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 234, no. 1-2, Aug. 1990, p. 530-534.

Astronomy and Astrophysics

Astrophysics

5

Line Spectra, Magnesium Compounds, Metal Hydrides, Photosphere, Pressure Oscillations, Solar Atmosphere, Oscillator Strengths, Temperature Dependence

Scientific paper

A linear perturbation method is used to calculate the behavior of an MgH spectral line at 5175 A as a function of temperature and pressure fluctuations. Particular attention is given to the MgH spectral lines of the A2Pi-X2Sigma(+) (0,0)-system in solar active and quiet regions. It is found that Mgh 5175 A is sensitive to temperature perturbations in the height range of 0 to 300 km with a peak in the response function near 100 km.

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