Comparison of Solar Magnetic Fields Measured at Different Observatories: Peculiar Strength Ratio Distributions Across the Disk
| Autor: | J. Staude, E. M. Golubeva, M. L. Demidov, V. M. Grigoryev, Horst Balthasar |
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| Rok vydání: | 2008 |
| Předmět: |
Physics
Photosphere Solar observatory Astrophysics::High Energy Astrophysical Phenomena Astrophysics::Instrumentation and Methods for Astrophysics Astronomy Astronomy and Astrophysics Astrophysics Solar disk Spectral line Magnetic field symbols.namesake Space and Planetary Science Observatory Physics::Space Physics symbols Astrophysics::Solar and Stellar Astrophysics Doppler effect Line (formation) |
| Zdroj: | Solar Physics. 250:279-301 |
| ISSN: | 1573-093X 0038-0938 |
| DOI: | 10.1007/s11207-008-9225-5 |
| Popis: | In this paper we analyze the distribution of magnetic strength ratios (MSR) across the solar disk using magnetograms in different spectral lines from the same observatory (Mount Wilson Observatory (MWO) and Sayan Observatory (SO)), magnetograms in the same line from different observatories (MWO, SO, Wilcox Solar Observatory (WSO)), and in different spectral lines from different observatories (the three observatories mentioned above, the National Solar Observatory/Kitt Peak (KP) and Michelson Doppler Imager (MDI) on board Solar and Heliospheric Observatory (SoHO)). We find peculiarities in some combinations of data sets. Besides the expected MSR center-to-limb variations, there is an equator-to-pole asymmetry, especially in the near-limb areas. Therefore, it is generally necessary to use 2D matrices of correction coefficients to reduce one kind of observation into another one. |
| Databáze: | OpenAIRE |
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