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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/80
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dc.contributor.authorVenkatakrishnan, P-
dc.contributor.authorJain, S. K-
dc.date.accessioned2004-12-09T03:07:38Z-
dc.date.available2004-12-09T03:07:38Z-
dc.date.issued1983-
dc.identifier.citationBulletin of the Astronomical Society of India, Vol. 11, pp. 369-370en
dc.identifier.urihttp://hdl.handle.net/2248/80-
dc.description.abstractThe possible applications of the time-dependent measurements of the equivalent width of the He I 10830 A line for a better understanding of the growth of spicules and the evolution of coronal holes and x-ray bright points on the sun are discussed-
dc.format.extent25651671 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectSun-spiculesen
dc.subjectHe I 10830 Aen
dc.titleOn the absorption of He I 10830 Å line by spiculesen
dc.typeArticleen
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