The solar MG I spectrum from ATMOS. I - Identification and preliminary discussion

Details The solar MG I spectrum from ATMOS. I - Identification and preliminary discussion The solar MG I spectrum from ATMOS. I - Identification and preliminary discussion

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...377..337j&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 377, Aug. 10, 1991, p. 337-342.

Astronomy and Astrophysics

Astrophysics

24

Infrared Spectra, Magnesium, Solar Spectra, Spacelab Payloads, High Resolution, Quantum Numbers, Signal To Noise Ratios

Scientific paper

As an initial step in a program to understand some puzzling aspects of the infrared solar Mg I spectrum, the set of high-resolution, high SNR lines of this spectrum are examined in the 1985 ATMOS experiment on Spacelab 3. Wavenumbers were obtained for the Mg I transitions lying in or near the range covered by ATMOS, namely 650 to 4800/cm. Lines involving principal quantum numbers up to n = 10 are seen in the data; some striking features of the Mg I spectrum are described and some directions of interest for future analytical studies and for future flights of the experiment are indicated.

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