Improvements of the Longitudinal Magnetic Field Measurement from the Solar Magnetic Field Telescope at the Huairou Solar Observing Station
The weak-field approximation, implying a linear relationship between Stokes- V / I and the longitudinal magnetic field [ B ∥ ], often suffers from saturation observed in strong magnetic-field regions such as sunspot umbrae. In this work, we seek to improve the magnetic-field observations carried out...
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| Published in | Solar physics Vol. 296; no. 11 |
|---|---|
| Main Authors | , , , , , , |
| Format | Journal Article |
| Language | English |
| Published |
Dordrecht
Springer Netherlands
01.11.2021
Springer Nature B.V |
| Subjects | |
| Online Access | Get full text |
| ISSN | 0038-0938 1573-093X |
| DOI | 10.1007/s11207-021-01901-6 |
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| Summary: | The weak-field approximation, implying a linear relationship between Stokes-
V
/
I
and the longitudinal magnetic field [
B
∥
], often suffers from saturation observed in strong magnetic-field regions such as sunspot umbrae. In this work, we seek to improve the magnetic-field observations carried out by the
Solar Magnetic Field Telescope
(SMFT) at the Huairou Solar Observing Station, China. We propose using a non-linear relationship between Stokes-
V
/
I
and
B
∥
to derive the magnetic field. To determine the form of the relationship, we perform a cross-calibration of the observed SMFT data and magnetograms provided by the
Helioseismic and Magnetic Imager
onboard the
Solar Dynamics Observatory
. The algorithm for the magnetic-field derivation is described in detail. We show that using a non-linear relationship between Stokes-
V
/
I
and
B
∥
allows us to eliminate magnetic-field saturation inside the sunspot umbra. The proposed technique enables one to enhance the reliability of the SMFT magnetic-field data obtained even long before the space-based instrumentation era, since 1987. |
|---|---|
| Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 14 |
| ISSN: | 0038-0938 1573-093X |
| DOI: | 10.1007/s11207-021-01901-6 |