On the scaling of magnetic field strength with loop length in solar active regions
Recognizing that loops are the main structures of the solar corona, we investigate how the magnetic field strength of coronal flux tubes depends on the end-to-end length of the tube for a sample of active regions. We use photospheric magnetograms from the Michelson Doppler Imager, aboard the Solar a...
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2005
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03796566_v_n596_p85_Mandrini http://hdl.handle.net/20.500.12110/paper_03796566_v_n596_p85_Mandrini |
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