A NEW METHOD FOR STUDYING CELESTIAL EMISSION SPECTRUM

A NEW METHOD FOR STUDYING CELESTIAL EMISSION SPECTRUM

<正> Ⅰ. INTRODUCTION A pure Doppler profile without self-absorption is a Gaussian profile If the source function is not frequency dependent in the region of spectrum and selfabsorption exists, we can write Eq. (1) into

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Veröffentlicht in:科学通报：英文版 1981 (1), p.48-52
1. Verfasser: 朱灿生 史忠先
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Sprache:eng
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Zusammenfassung:<正> Ⅰ. INTRODUCTION A pure Doppler profile without self-absorption is a Gaussian profile If the source function is not frequency dependent in the region of spectrum and selfabsorption exists, we can write Eq. (1) into
ISSN:2095-9273