Zobrazeno 1 - 6
of 6
pro vyhledávání: '"R. S. Flagg"'
Publikováno v:
Icarus. 29:463-475
Morphological analyses of high-resolution spectral recordings of Jovian decametric radiation show a regime of phenomena not seen at lower resolutions. Observed emissions range from narrow-band (50 kHz) simple quasi-periodic bursts to wide-band emissi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::af0a2ad4b94c297b3bb1d777edebb3b7
https://doi.org/10.1016/0019-1035(76)90066-x
https://doi.org/10.1016/0019-1035(76)90066-x
Autor:
J.J. Riihimaa, Jorge Levy, G. R. Lebo, W. B. Greenman, P. P. Gombola, Thomas D. Carr, R. S. Flagg
Publikováno v:
Icarus. 48:298-307
High-resolution dynamic spectra of Jovian S-bursts frequently reveal sloping gaps crossing bands of L-burst emission with drift rates comparable to those of S-bursts. These “fast-drift shadow” (FDS) events are often sharply bounded on one edge by
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d76eb67c203b007b236698cd26e6a0e6
https://doi.org/10.1016/0019-1035(81)90111-1
https://doi.org/10.1016/0019-1035(81)90111-1
Publikováno v:
Radio Science. 20:1625-1638
A variety of techniques and instruments have been developed at the University of Florida to study the decametric radio emissions from the planet Jupiter. Several types of radio spectrograph are being utilized, each offering a unique advantage in spee
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a8d336f8bdaa2d543a27db4322023bc2
https://doi.org/10.1029/rs020i006p01625
https://doi.org/10.1029/rs020i006p01625
Publikováno v:
Icarus. 29:477-482
Analysis of the bandlike Jovian decametric emission is presented. A model for the active region that accounts for the observed radiation characteristics is described using the measured parameters of the bandlike emission and a model of the Jovian mag
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fff696e4b18049f9228e8f5f49f8248c
https://doi.org/10.1016/0019-1035(76)90067-1
https://doi.org/10.1016/0019-1035(76)90067-1
Publikováno v:
Solar Physics. 90:111-115
High-time resolution spectral measurements of solar radio emission close to 264 MHz are reported. Instrumental resolutions of the order of a few kHz in frequency and tenths of milliseconds in time were used to resolve the burst fine structure in the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::879505372384a8d307f2d2215387a847
https://doi.org/10.1007/bf00153788
https://doi.org/10.1007/bf00153788
Publikováno v:
Nature. 272:38-40
Drift rates for S-burst emissions from Jupiter are studied. The burst spectra, recorded in the frequency range near 32 MHz, provide a qualitative illustration of the behavior of electron bunches shortly after injection into the Io-associated magnetic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b69f536a682d8a68e47ce310591db5e8
https://doi.org/10.1038/272038a0
https://doi.org/10.1038/272038a0