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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2667
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dc.contributor.authorSingh, J-
dc.contributor.authorJain, S. K-
dc.contributor.authorVenkatakrishnan, P-
dc.date.accessioned2008-07-14T06:44:58Z-
dc.date.available2008-07-14T06:44:58Z-
dc.date.issued1994-03-
dc.identifier.citationSolar Physics, Vol. 150, No. 1-2, pp. 49 - 59en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/2667-
dc.description.abstractWe have studied the time-dependent behavior of the He I 10830 A line. These studies show that (1) the fluctuations of the line width are uncorrelated with the equivalent-width fluctuations and (2) the autocorrelation curves for the equivalent-width fluctuations are broader than those for line-width fluctuations. These results could be interpreted as the signatures of the eruption of density inhomogeneities, like spicules, into the altitudes of formation of the He I 10830 A line.en
dc.format.extent803186 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://adsabs.harvard.edu/abs/1994SoPh..150...49Sen
dc.relation.urihttp://www.springerlink.com/content/5g63058x23754h74/en
dc.subjectHeliumen
dc.subjectInfrared Astronomyen
dc.subjectInfrared Spectraen
dc.subjectLine Spectraen
dc.subjectSolar Atmosphereen
dc.subjectSolar Coronaen
dc.subjectSolar Spectraen
dc.subjectSpectral Line Widthen
dc.subjectSpectrum Analysisen
dc.subjectSpiculesen
dc.subjectTime Dependenceen
dc.subjectUltraviolet Spectraen
dc.subjectCross Correlationen
dc.subjectMagnetic Signaturesen
dc.subjectPlasma Densityen
dc.subjectPlasma Turbulenceen
dc.subjectSignal To Noise Ratiosen
dc.subjectSolar Rotationen
dc.subjectStatistical Analysisen
dc.subjectTime Series Analysisen
dc.titleTime variability of the He I 10830 A line profileen
dc.typeArticleen
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