Collisional influence on the differential Hanle effect method applied to the second solar spectrum of the A^2Π–X^2Σ⁺ (0, 0) band of MgH

V. Bommier; E. Landi Degl’Innocenti; N. Feautrier; G. Molodij

doi:10.1051/0004-6361:20054591

August 4, 2006Astronomy and AstrophysicsOpen Access

Collisional influence on the differential Hanle effect method applied to the second solar spectrum of the A^2Π–X^2Σ⁺ (0, 0) band of MgH

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Abstract

Aims.This paper presents an analysis of the lines of the Q band of the A-X (0, 0) transition of MgH, whose linear polarization was measured 4 arcsec inside the solar limb in a quiet region (North Pole) with THEMIS on 21 November 2004.

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synapsesocial.com/papers/6a7c82258a815a5ddccc453f https://doi.org/10.1051/0004-6361:20054591

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Collisional influence on the differential Hanle effect method applied to the second solar spectrum of the A^2Π–X^2Σ⁺ (0, 0) band of MgH

Abstract

Discussion

Cite This Study

Collisional influence on the differential Hanle effect method applied to the second solar spectrum of the A^2Π–X^2Σ⁺ (0, 0) band of MgH

Abstract

Discussion

Cite This Study

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