dc.contributor.author |
Prasad, D. C |
|
dc.contributor.author |
Chandrasekhar, T |
|
dc.contributor.author |
Desai, J. N |
|
dc.contributor.author |
Ashok, N. M |
|
dc.contributor.author |
Krishan, V |
|
dc.date.accessioned |
2008-09-17T12:20:59Z |
|
dc.date.available |
2008-09-17T12:20:59Z |
|
dc.date.issued |
1989-03 |
|
dc.identifier.citation |
Journal of Astrophysics and Astronomy, Vol. 10, No. 1, pp. 1 - 20 |
en |
dc.identifier.issn |
0250-6335 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3720 |
|
dc.description.abstract |
During the recent apparition of Comet Halley in 1985-86, a transient ionic event in the form of a blob of H2O(+) emission was recorded in the coma at about 0 h UT on March 13, 1986. Observations were carried out using a special filter for H2O(+) emission at 7000 A/175 A, a 35-cm telescope, a Fabry-Perot interferometer, and an image intensifier camera from Gurushikhar, Mt. Abu. A Fabry-Perot interferogram in H-alpha taken a few minutes later at the same location, reveals strong hydrogen emission (H-alpha) associated with the blob. The velocity field in the blob is structured with relative velocities up to about 35 km/sec. The event is interpreted as arising due to the sector boundary crossing of the interplanetary magnetic field by the comet. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Indian Academy of Sciences |
en |
dc.relation.uri |
http://ads.iucaa.ernet.in/abs/1989JApA...10....1D |
en |
dc.subject |
Cometary atmospheres |
en |
dc.subject |
Fabry-perot interferometers |
en |
dc.subject |
Halley's comet |
en |
dc.subject |
Visible spectrum |
en |
dc.subject |
Emission spectra |
en |
dc.subject |
H alpha line |
en |
dc.subject |
Interplanetary magnetic fields |
en |
dc.subject |
Solar wind |
en |
dc.subject |
Spectrum analysis |
en |
dc.subject |
Water |
en |
dc.title |
Optical interferometric observations of a transient event of 1986 March 13 in the coma of Comet Halley |
en |
dc.type |
Article |
en |