Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1818
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dc.contributor.authorDwivedi, B. N-
dc.date.accessioned2007-09-21T11:47:43Z-
dc.date.available2007-09-21T11:47:43Z-
dc.date.issued1996-
dc.identifier.citationBASI, Vol.24 No. 2 pp. 333-337en
dc.identifier.urihttp://hdl.handle.net/2248/1818-
dc.description.abstractWe highlight a rich source of high-resolution EUV observations that the Solar Ultraviolet Measurements of Emitted Radiation (SUMER) instrument, on board the SOHO mission, is capable of making in the broad spectral range from less than 500 angstrom to 1610 angstrom , and which is further extended to shorter wavelengths by the Coronal Diagnostic Spectrometer (CDS)instrument. This will provide a unique opportunity to study in greater detail than previously done, the diagnostics and dynamics of the solar plasma from the upper chromosphere to the corona. We also briefly present the spectroscopic diagnostics for several ions relevant to the SUMER/CDS spectral range for the inference of the physical parameters and discuss underlying coronal physicsen
dc.format.extent480394 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996BASI...24..333Den
dc.subjectLine diagnosticsen
dc.subjectDensity and temperature diagnosticsen
dc.subjectSpectroscopic diagnostics for solar ionsen
dc.titlePlasma diagnostics for SUMER on board the SOHO missionen
dc.typeArticleen
Appears in Collections:BASI Publications

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