Plasma diagnostics for SUMER on board the SOHO mission

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1818

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DC Field	Value	Language
dc.contributor.author	Dwivedi, B. N	-
dc.date.accessioned	2007-09-21T11:47:43Z	-
dc.date.available	2007-09-21T11:47:43Z	-
dc.date.issued	1996	-
dc.identifier.citation	BASI, Vol.24 No. 2 pp. 333-337	en
dc.identifier.uri	http://hdl.handle.net/2248/1818	-
dc.description.abstract	We 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 physics	en
dc.format.extent	480394 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1996BASI...24..333D	en
dc.subject	Line diagnostics	en
dc.subject	Density and temperature diagnostics	en
dc.subject	Spectroscopic diagnostics for solar ions	en
dc.title	Plasma diagnostics for SUMER on board the SOHO mission	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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