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Morosin, Roberta; de la Cruz Rodríguez, Jaime; Vissers, Gregal J. M.; Yadav, Rahul (2020). "Stratification of canopy magnetic fields in a plage region. Constraints from a spatially-regularized weak-field approximation method".
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Pietrow, A. G. M.; Kiselman, D.; de la Cruz Rodríguez, J.; Díaz Baso, C. J.; Pastor Yabar, A.; Yadav, R. (2020). "Inference of the chromospheric magnetic field configuration of solar plage using the Ca II 8542 Å line".
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below. The magnetic field of plage is confined to the intergranular lanes in the photosphere with a strength of around 1500 G, but expands into a volume filling canopy in the chromosphere with a field of around 450G.
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It is believed that plage is formed from decaying emerging flux regions, and often acts as a footprint for coronal loops and fibrils, which makes them an important interface for
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is often believed to be poetically taken from the French word for "beach"; however, this is likely a misunderstanding of an 1893 article by
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In this near true color photograph, taken through a narrowband hydrogen-alpha filter, plages are visible as overexposed patches.
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Physical properties of chromospheric features: Plage, peacock jets, and calibrating it all
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127:. With modern imaging, most researchers now identify plage based on the
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Classically, plage have been defined as regions that are bright in
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was suggested. In the article, Deslandres also refers to them as
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Encyclopedia of
Astrobiology, Astronomy & Spaceflight: Plage
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186:. In Landsberg, Helmut E.; Van Mieghem, J. (eds.).
182:Athay, R. Grant; Warwick, Constance S. (1961).
65:. Historically, they have been referred to as
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190:. Vol. 8. Elsevier Science. p. 30.
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848:List of heliophysics missions
220:(PhD). Stockholm University.
894:This article related to the
853:Category:Missions to the Sun
326:10.1051/0004-6361/202038754
272:10.1051/0004-6361/202038750
226:10.13140/RG.2.2.36047.76968
184:"Indices of Solar Activity"
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296:Astronomy and Astrophysics
242:Astronomy and Astrophysics
97:Henri-Alexandre Deslandres
53:is a bright region in the
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829:G-type main-sequence star
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692:In mythology and culture
214:Pietrow, A.G.M. (2022).
123:and other chromospheric
318:2020A&A...642A.210M
264:2020A&A...644A..43P
559:Supra-arcade downflows
188:Advances in Geophysics
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539:Coronal mass ejection
75:chromospheric faculae
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803:Standard solar model
773:Solar radio emission
591:List of solar cycles
79:photospheric faculae
623:Magnetic switchback
813:Sunlight radiation
408:Internal structure
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748:Solar energy
743:Solar dynamo
704:Heliophysics
534:Coronal loop
529:Coronal hole
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836:Exploration
714:Solar deity
661:Heliosheath
643:Heliosphere
613:Wolf number
586:Solar cycle
450:Photosphere
153:Solar cycle
115:Description
943:Categories
788:Solar time
709:In culture
666:Heliopause
618:Solar wind
549:Prominence
441:Atmosphere
426:Tachocline
309:2006.14487
255:2006.14486
169:References
107:, meaning
959:Sun stubs
671:Bow shock
578:Variation
544:Nanoflare
334:220055552
280:220055853
89:The term
85:Etymology
73:, and as
871:Category
147:See also
687:Eclipse
680:Related
501:Spicule
473:Sunspot
468:Faculae
463:Granule
387:The Sun
314:Bibcode
302:: 642.
260:Bibcode
248:: 644.
133:faculae
516:Corona
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898:is a
628:Flare
496:Plage
330:S2CID
304:arXiv
276:S2CID
250:arXiv
92:plage
29:plage
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