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| Natura: | Preprint |
| Pubblicazione: |
2023
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| Accesso online: | https://arxiv.org/abs/2311.15693 |
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| _version_ | 1866929697493876736 |
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| author | Bommier, Véronique |
| author_facet | Bommier, Véronique |
| contents | All magnetic field vector measurements lead to ambiguous results. We show that observations in two different lines belonging to the same multiplet but having different absorption coefficients so that they are formed at two different depths like Fe I 6302.5 A and 6301.5 A, enable the resolution of the azimuth ambiguity remaining from the Zeeman signal interpretation. What is measured by interpretation of the Zeeman effect is the magnetic field H, and not the divergence-free magnetic induction B. We analyze how the anisotropy of the photosphere, which is strongly stratified due to gravity and density at the star surface, affects divH and how the ambiguity resolution has to be performed in these conditions. As a consequence, two ambiguity-resolved field vector maps are obtained at two different but close altitudes, which enable the derivation of the current density full vector via curlH=J. This reveals the horizontal component of the current density, which is generally found markedly larger than the better known vertical one. We observe some systematical trends, of which we present examples in the paper, like circular currents wrapping spots clockwise about a positive polarity spot and anticlockwise about a negative polarity spot and strong horizontal current components crossing active region neutral lines. We finally remark that the Na I D1 and D2 lines form another such line pair. We propose them as an access to the low chromosphere where they are formed. However, a better spatial resolution for both observations and analysis would probably be necessary in such a medium. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2311_15693 |
| institution | arXiv |
| publishDate | 2023 |
| record_format | arxiv |
| spellingShingle | Magnetometry: solving the fundamental ambiguity from line pair inversion Bommier, Véronique Solar and Stellar Astrophysics All magnetic field vector measurements lead to ambiguous results. We show that observations in two different lines belonging to the same multiplet but having different absorption coefficients so that they are formed at two different depths like Fe I 6302.5 A and 6301.5 A, enable the resolution of the azimuth ambiguity remaining from the Zeeman signal interpretation. What is measured by interpretation of the Zeeman effect is the magnetic field H, and not the divergence-free magnetic induction B. We analyze how the anisotropy of the photosphere, which is strongly stratified due to gravity and density at the star surface, affects divH and how the ambiguity resolution has to be performed in these conditions. As a consequence, two ambiguity-resolved field vector maps are obtained at two different but close altitudes, which enable the derivation of the current density full vector via curlH=J. This reveals the horizontal component of the current density, which is generally found markedly larger than the better known vertical one. We observe some systematical trends, of which we present examples in the paper, like circular currents wrapping spots clockwise about a positive polarity spot and anticlockwise about a negative polarity spot and strong horizontal current components crossing active region neutral lines. We finally remark that the Na I D1 and D2 lines form another such line pair. We propose them as an access to the low chromosphere where they are formed. However, a better spatial resolution for both observations and analysis would probably be necessary in such a medium. |
| title | Magnetometry: solving the fundamental ambiguity from line pair inversion |
| topic | Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2311.15693 |