Abstract
No fluctuations in polarization have been found during a 7 GHz solar burst showing 17s periodic pulses in intensity. Polarization effects can be produced by the propagation media in the active centre, which are not affected directly by the burst source, but situated more deeply than the observed heights at that microwave frequency.
Kaufmann, P
[1]
- Universidade Mackenzie, Sao Paulo (Brazil). Centro de Radio-Astronomia e Astrofisica
Citation Formats
Kaufmann, P.
Polarization of a periodic solar microwave burst.
Netherlands: N. p.,
1976.
Web.
Kaufmann, P.
Polarization of a periodic solar microwave burst.
Netherlands.
Kaufmann, P.
1976.
"Polarization of a periodic solar microwave burst."
Netherlands.
@misc{etde_7311918,
title = {Polarization of a periodic solar microwave burst}
author = {Kaufmann, P}
abstractNote = {No fluctuations in polarization have been found during a 7 GHz solar burst showing 17s periodic pulses in intensity. Polarization effects can be produced by the propagation media in the active centre, which are not affected directly by the burst source, but situated more deeply than the observed heights at that microwave frequency.}
journal = []
volume = {50:1}
journal type = {AC}
place = {Netherlands}
year = {1976}
month = {Sep}
}
title = {Polarization of a periodic solar microwave burst}
author = {Kaufmann, P}
abstractNote = {No fluctuations in polarization have been found during a 7 GHz solar burst showing 17s periodic pulses in intensity. Polarization effects can be produced by the propagation media in the active centre, which are not affected directly by the burst source, but situated more deeply than the observed heights at that microwave frequency.}
journal = []
volume = {50:1}
journal type = {AC}
place = {Netherlands}
year = {1976}
month = {Sep}
}