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- W3100731429 abstract "Context. Small scale magnetic fields can be observed on the Sun in G-band filtergrams as magnetic bright points (MBPs) or identified in spectro-polarimetric measurements due to enhanced signals of Stokes profiles. These magnetic fields and their dynamics play a crucial role in understanding the coronal heating problem and also in surface dynamo models. MBPs can theoretically be described to evolve out of a patch of a solar photospheric magnetic field with values below the equipartition field strength by the so-called convective collapse model. After the collapse, the magnetic field of MBPs reaches a higher stable magnetic field level." @default.
- W3100731429 created "2020-11-23" @default.
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- W3100731429 date "2013-06-01" @default.
- W3100731429 modified "2023-10-13" @default.
- W3100731429 title "Magnetic field strength distribution of magnetic bright points inferred from filtergrams and spectro-polarimetric data" @default.
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- W3100731429 doi "https://doi.org/10.1051/0004-6361/201116894" @default.
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