Plasma diagnostics for SUMER on board the SOHO mission

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