Identification of CrH and CrD Molecular Lines in the Sunspot Umbral Spectrum

High-resolution Fourier transform spectrometer sunspot umbral spectra obtained at the National Solar Observatory/Kitt Peak were used to identify molecular rotational lines arising from the infrared band systems of CrH and CrD molecules. Measurement of the equivalent width used the Gaussian-profile a...

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Veröffentlicht in:Solar physics 2009-07, Vol.257 (2), p.261-269
Hauptverfasser: Viswanathan, B., Shanmugavel, R., Bagare, S. P., Rajamanickam, N., Sriramachandran, P.
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container_issue 2
container_start_page 261
container_title Solar physics
container_volume 257
creator Viswanathan, B.
Shanmugavel, R.
Bagare, S. P.
Rajamanickam, N.
Sriramachandran, P.
description High-resolution Fourier transform spectrometer sunspot umbral spectra obtained at the National Solar Observatory/Kitt Peak were used to identify molecular rotational lines arising from the infrared band systems of CrH and CrD molecules. Measurement of the equivalent width used the Gaussian-profile approximation method, which is suitable especially for faint lines. Equivalent widths are measured for an adequate number of best lines of the A – X (0,0) band of CrH and the A – X (0,0;1,0) bands of CrD and, thereby, the effective rotational temperatures are estimated.
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subjects Approximation method
Astrophysics
Astrophysics and Astroparticles
Atmospheric Sciences
Fourier transforms
Physics
Physics and Astronomy
Solar physics
Space Exploration and Astronautics
Space Sciences (including Extraterrestrial Physics
Sunspots
Temperature
title Identification of CrH and CrD Molecular Lines in the Sunspot Umbral Spectrum
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