Conductive flux in the chromosphere derived from line linear polarization observation

It is shown that quantitative information on the mechanisms of energy transport which take place in solar flares can be obtained by measurement of impact line polarization. Linear polarization in two chromospheric lines (H-alpha and SI 1437 A) observed in the gradual phase of solar flares was invest...

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Veröffentlicht in:	Solar physics 1983-07, Vol.86 (1-2), p.115-122
Hauptverfasser:	Henoux, J.-C., Chambe, G., Heristchi, D., Semel, M., Woodgate, B., Shine, D., Beckers, J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Chromosphere and chromosphere-corona transition. Spicules Earth, ocean, space Exact sciences and technology Solar Physics Solar system
Online-Zugang:	Volltext
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