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Study of molecular lines in the solar photospheric spectrum

N. Grevesse, +1 more
- 01 Aug 1973 - 
- Vol. 27, pp 29
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This article is published in Astronomy and Astrophysics.The article was published on 1973-08-01 and is currently open access. It has received 39 citations till now. The article focuses on the topics: Chromosphere.

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Line strengths and updated molecular constants for the C2 Swan system

TL;DR: In this paper, the rotational line strengths for the C2 Swan system (d Π g 3 − a Π u 3 ) have been calculated for vibrational bands with v ǫ = 0 − 10 and v à = 0 - 9, and J values up to J=34-96, using previous observations in 33 vibrational band.
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The valence states of C2: A configuration interaction study

K. Kirby, +1 more
TL;DR: In this paper, the potential curves for all 62 valence states of C2 have been computed using configuration interaction wavefunctions within the valence orbital space, using a multiconfiguration self-consistent field calculation using a properly dissociating set of configurations for the 3Πu state.
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New observations of the A1Πu-X1Σg+ transition (Phillips system) of C2

TL;DR: In this article, the infrared part of the A 1 Π u - X 1 Σ g + (Phillips system) of C 2 was analyzed and improved molecular constants were derived.
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MARVEL analysis of the measured high-resolution spectra of 14NH3

TL;DR: In this paper, the energy levels of the imidogen free radical (14 NH) were determined for four low-lying electronic states (X 3 Σ -, A 3 Π, A 4 Π, a 1 Δ, and c 1 Π ) using the MARVEL (measured active rotational vibrational vibration energy levels) technique.
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Ab initio configuration interaction study of the low‐lying electronic states of MgH

TL;DR: In this paper, Ab initio configuration interaction calculations have been performed on the X 2Σ+, A 2Π, and B 2 Σ+ states of MgH for 23 internuclear distances between 2.2 and 9.5 a 0.161.