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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/282
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dc.contributor.authorLivingston, W-
dc.contributor.authorHarvey, J-
dc.contributor.authorDoe, L. A-
dc.contributor.authorGillespie, B-
dc.contributor.authorLadd, G-
dc.date.accessioned2005-02-03T02:57:37Z-
dc.date.available2005-02-03T02:57:37Z-
dc.date.issued1980-06-
dc.identifier.citationBASI, Vol. 8, Nos. 2&3, pp. 43-47en
dc.identifier.urihttp://hdl.handle.net/2248/282-
dc.description.abstractMulti-slit spectra of (Fe XIV 5303) plus neon comparisons were successfully obtained on February 16, 1980 at the Japal-Rangapur site. The objective is to confirm our previous results of March 1970 and June 1973, viz. that the corona is remarkably quiescent (random velocities = 0.5 Km/s r.m.s.) and that the majority of detected flows at 0.3 - 1.0 Ro are directed towards the Sun.en
dc.format.extent1161387 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherTata Institute of Fundamental Research, Bombayen
dc.subjectCoronal Velocityen
dc.subjectKitt Peak Coronal Velocity Experimenten
dc.titleThe Kitt Peak Coronal Velocity Experimenten
dc.typeArticleen
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