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Badalyan, O. G., Obridko, V. N. (2006) Two Regularities in the Coronal Green-Line Brightness – Magnetic Field Coupling and the Heating of the Corona. Solar Physics, 238 (2). 271-292 doi:10.1007/s11207-006-0214-2

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Reference TypeJournal (article/letter/editorial)
TitleTwo Regularities in the Coronal Green-Line Brightness – Magnetic Field Coupling and the Heating of the Corona
JournalSolar Physics
AuthorsBadalyan, O. G.Author
Obridko, V. N.Author
Year2006 (November)Volume238
Issue2
PublisherSpringer Science and Business Media LLC
DOIdoi:10.1007/s11207-006-0214-2Search in ResearchGate
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Mindat Ref. ID8922656Long-form Identifiermindat:1:5:8922656:4
GUID0
Full ReferenceBadalyan, O. G., Obridko, V. N. (2006) Two Regularities in the Coronal Green-Line Brightness – Magnetic Field Coupling and the Heating of the Corona. Solar Physics, 238 (2). 271-292 doi:10.1007/s11207-006-0214-2
Plain TextBadalyan, O. G., Obridko, V. N. (2006) Two Regularities in the Coronal Green-Line Brightness – Magnetic Field Coupling and the Heating of the Corona. Solar Physics, 238 (2). 271-292 doi:10.1007/s11207-006-0214-2
In(2006, November) Solar Physics Vol. 238 (2) Springer Science and Business Media LLC

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Badalyan, O. G., Obridko, V. N., Sýkora, J. (2004) Space–time distributions of the coronal green-line brightness and solar magnetic fields. Astronomical & Astrophysical Transactions, 23. 555-566 doi:10.1080/10556790412331335336
Badalyan, O. G., Obridko, V. N. (2018) Magnetic Field as a Tracer for Studying the Differential Rotation of the Solar Corona. Solar Physics, 293 (9). doi:10.1007/s11207-018-1349-7
Badalyan, Olga G., Obridko, V. N., Sýkora, J. (2004) Cyclic variations in distribution of the coronal green line brightness and solar magnetic field. Proceedings of the International Astronomical Union, 2004. 69-72 doi:10.1017/s1743921304005125
Badalyan, Olga G., Obridko, V. N. (2004) Relationship between the coronal green line brightness and magnetic field strength. Proceedings of the International Astronomical Union, 2004. 371-372 doi:10.1017/s1743921304006155
Badalyan, O. G., Obridko, V. N. (2004) Solar magnetic fields and the intensity of the green coronal line. Astronomy Reports, 48. 678-687 doi:10.1134/1.1787070
Badalyan, O. G., Obridko, V. N., Sýkora, J. (2005) Cyclic variation in the spatial distribution of the coronal green line brightness. Astronomy Reports, 49. 477-484 doi:10.1134/1.1941490
Badalyan, O. G., Obridko, V. N. (2007) To the problem of solar coronal heating. Astronomy Letters, 33. 182-191 doi:10.1134/s106377370703005x
Badalyan, O. G., Obridko, V. N. (2018) Differential Rotation of the Solar Corona from Magnetic Field Data. Astronomy Letters, 44. 727-733 doi:10.1134/s1063773718110014
Badalyan, O. G., Obridko, V. N., Sýkora, J. (2008) Quasi-Biennial Oscillations in the North – South Asymmetry of Solar Activity. Solar Physics, 247 (2). 379-397 doi:10.1007/s11207-008-9120-0
Badalyan, O. G., Obridko, V. N., Sýkora, J. (2006) Cyclic variations in the differential rotation of the solar corona. Astronomy Reports, 50. 312-324 doi:10.1134/s1063772906040056
Bludova, N. G., Badalyan, O. G. (2006) Relation of the coronal green line intensity to magnetic fields and sunspot areas in the solar cycle. Astronomy Letters, 32. 698-706 doi:10.1134/s1063773706100057
 
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