dc.contributor.author |
Chandrasekhar, T |
|
dc.contributor.author |
Ashok, N. M |
|
dc.contributor.author |
Desai, J. N |
|
dc.contributor.author |
Pasachoff, J. M |
|
dc.contributor.author |
Sivaraman, K. R |
|
dc.date.accessioned |
2009-01-16T14:15:41Z |
|
dc.date.available |
2009-01-16T14:15:41Z |
|
dc.date.issued |
1984-02 |
|
dc.identifier.citation |
Applied Optics , Vol. 23, pp. 508 - 511 |
en |
dc.identifier.issn |
0003-6935 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/4265 |
|
dc.description |
Restricted Access |
|
dc.description.abstract |
A dual-channel Fabry-Perot interferometric system was used to study simultaneously the coronal emission lines at 5303 Å (Fe XIV) and at 6374 Å (Fe X). Initial results indicate an emission corona confined largely within 1.2 R_sun;. Doppler temperatures derived from the width of the 5303-Å line appear to be appreciably lower than similar temperatures determined during the solar-maximum eclipse of 1980. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Optical society of America |
en |
dc.relation.uri |
http://www.opticsinfobase.org/abstract.cfm?id=27279 |
en |
dc.rights |
© Optical Society of America |
en |
dc.subject |
Fabry-Perot Interferometers |
en |
dc.subject |
Solar Corona |
en |
dc.subject |
Solar Eclipses |
en |
dc.subject |
Solar Instruments |
en |
dc.subject |
Solar Spectra |
en |
dc.subject |
Collimation |
en |
dc.subject |
Emission Spectra |
en |
dc.subject |
Image Filters |
en |
dc.title |
Fabry-Perot interferometric observations of the coronal red and green lines during the 1983 Indonesian eclipse |
en |
dc.type |
Article |
en |