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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2658
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dc.contributor.authorRaju, P. K-
dc.contributor.authorDwivedi, B. N-
dc.contributor.authorGupta, A. K-
dc.date.accessioned2008-07-14T06:04:34Z-
dc.date.available2008-07-14T06:04:34Z-
dc.date.issued1994-02-
dc.identifier.citationSolar Physics, Vol. 149, No. 2, pp. 289 - 299en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/2658-
dc.description.abstractLine intensity ratios of extreme ultraviolet (EUV) emission lines from Na VII and Al IX have been considered for electron density and temperature determinations within the chromosphere-corona transition region and the corona. The electron pressure within the emission region has been assumed to be a constant parameter. Theoretical line intensities for these ions have been computed using a model solar atmosphere and compared with the values as observed by the Apollo Telescope Mount (ATM) ultraviolet spectrometer. The observed intensities correspond to the average quiet-Sun conditions near solar minimum.en
dc.format.extent846421 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://www.springerlink.com/content/k31v8541uph2115v/en
dc.relation.urihttp://adsabs.harvard.edu/abs/1994SoPh..149..289Ren
dc.subjectAluminumen
dc.subjectChromosphereen
dc.subjectEmission Spectraen
dc.subjectLine Spectraen
dc.subjectPlasma Densityen
dc.subjectPlasma Diagnosticsen
dc.subjectPlasma Temperatureen
dc.subjectSodiumen
dc.subjectSolar Coronaen
dc.subjectSolar Electronsen
dc.subjectSolar Spectraen
dc.subjectStellar Modelsen
dc.subjectUltraviolet Astronomyen
dc.subjectUltraviolet Spectraen
dc.subjectAstronomical Spectroscopyen
dc.subjectAtmospheric Modelsen
dc.subjectCollision Parametersen
dc.subjectElectron Density (Concentration)en
dc.subjectElectron Pressureen
dc.subjectExtreme Ultraviolet Radiationen
dc.subjectIonsen
dc.subjectMathematical Modelsen
dc.subjectRadiative Transferen
dc.subjectSoho Missionen
dc.subjectSolar Atmosphereen
dc.subjectSolar Cyclesen
dc.subjectUltraviolet Spectrometeen
dc.titleDensity and temperature diagnostics of solar emission lines from NA VII and AL IXen
dc.typeArticleen
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