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There are a total of 13 record(s) matching your query.
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Bursts of relativistic electrons from Jupiter observed in interplanetary space with the time variation of the planetary rotation period
Author(s): Chenette, D. L.; Conlon, T. F.; Simpson, J. A.
Abstract: Bursts of Jovian electrons in the energy range 3 to 30 Mev have been detected to distances of the order of 1 AU from the planet. The duration of each burst was about two to three days, and the maximum intensity increased ...
NASA Center: NASA (non Center Specific)
Publication Year: 1974
Added to NTRS: 2004-11-03
Accession Number: 74A43656; Document ID: 19740060906
Voyager 2 - Energetic ions and electrons in the Jovian magnetosphere
Author(s): Vogt, R. E.; Cummings, A. C.; Garrard, T. L.; Gehrels, N.; Stone, E. C.; Trainor, J. H.; Schardt, A. W.; Conlon, T. F.; Mcdonald, F. B.
Abstract: The passage of Voyager 2 through the Jovian magnetosphere demonstrated that this magnetosphere is highly variable, even as close as 10 Jupiter radii from the planet. The cosmic-ray subsystem measured the flux, elemental ...
NASA Center: Goddard Space Flight Center
Publication Year: 1979
Added to NTRS: 2004-11-03
Accession Number: 80A12849; Document ID: 19800028679
Progress report on the radial gradients of cosmic ray nuclei 0.5 MeV per nucleon to relativistic energies and electrons 6 to 30 MeV
Author(s): Simpson, J. A.; Conlon, T. F.; Mckibben, R. B.; Tuzzolino, A. J.; Ogallagher, J. J.
Abstract: No Abstract Available
NASA Center: NASA (non Center Specific)
Publication Year: 1974
Added to NTRS: 2004-11-03
Accession Number: 75A28020; Document ID: 19750043948
Source variations of interplanetary Jovian electrons - Voyagers 1 and 2 results
Author(s): Conlon, T. F.; Mcdonald, F. B.; Schardt, A. W.; Trainor, J. H.
Abstract: The large intensity of interplanetary Jovian electrons at 1 AU and near the Jovian magnetosphere have been attributed to the large scale solar wind structure. The only variations that can be definitely attributed to the ...
NASA Center: Goddard Space Flight Center
Publication Year: 1980
Added to NTRS: 2004-11-03
Accession Number: 81A12469; Document ID: 19810028065
Observations in interplanetary space of relativistic electrons from Jupiter
Author(s): Chenette, D. L.; Conlon, T. F.; Simpson, J. A.
Abstract: Evidence for the presence of Jovian electrons in interplanetary space as much as 1 AU inside the orbit of Jupiter is summarized. Electron flux patterns at Pioneer 10 can only rarely be correlated with solar activity. Clear ...
NASA Center: NASA (non Center Specific)
Publication Year: 1975
Added to NTRS: 2004-11-03
Accession Number: 75A46247; Document ID: 19750062175
Jovian electron bursts - Correlation with the interplanetary field direction and hydromagnetic waves
Author(s): Smith, E. J.; Tsurutani, B. T.; Chenette, D. L.; Conlon, T. F.; Simpson, J. A.
Abstract: The bursts of relativistic electrons detected on Pioneer 10 upstream from Jupiter and within 400 Jovian radii of the planet have been found to be correlated with the interplanetary magnetic field. In three examples, ...
NASA Center: Jet Propulsion Laboratory
Publication Year: 1976
Added to NTRS: 2004-11-03
Accession Number: 76A19836; Document ID: 19760036870
The effect of coronal transport of energetic solar particles
Author(s): Conlon, T. F.; Van Hollebeke, M. A. I.; Mcdonald, F. B.; Trainor, J. H.
Abstract: A single active center was the origin of several solar flares observed in September, 1977. The longitude of the flares ranged from approximately 115 deg E to approximately 117 deg W. During this period Helios 1, Helios 2, ...
NASA Center: Goddard Space Flight Center
Publication Year: 1980
Added to NTRS: 2004-11-03
Accession Number: 81A12458; Document ID: 19810028054
Acceleration of nucleons in interplanetary space and modulation of Jovian electrons at distances of 1 to 10 AU by corotating regions of solar origin
Author(s): Barnes, C. W.; Chenette, D. L.; Conlon, T. F.; Pyle, K. R.; Simpson, J. A.
Abstract: Corotating interaction regions (CIRs) are formed in interplanetary space when a fast solar-plasma flow overtakes a slow solar-wind stream. This paper shows that CIRs are closely related to two unusual phenomena observed ...
NASA Center: NASA (non Center Specific)
Publication Year: 1977
Added to NTRS: 2004-11-03
Accession Number: 77A32859; Document ID: 19770050007
Observations of Jovian electrons at 1 AU throughout the 13 month Jovian synodic year
Author(s): Chenette, D. L.; Conlon, T. F.; Pyle, K. R.; Simpson, J. A.
Abstract: A study of Jovian electron-flux increases observed aboard the IMP-8 earth-orbiting satellite reveals that, contrary to previous reports of a 4-8-month Jovian electron 'season', Jovian electron-intensity increases were ...
NASA Center: NASA (non Center Specific)
Publication Year: 1977
Added to NTRS: 2004-11-03
Accession Number: 77A39444; Document ID: 19770056592
The interplanetary modulation and transport of Jovian electrons
Author(s): Conlon, T. F.
Abstract: Based on simultaneous measurements by Pioneer 11 of the 3-6 MeV Jovian electron flux, interplanetary magnetic field magnitude, and solar wind speed, the interplanetary transport of energetic particles is studied. It is found ...
NASA Center: NASA (non Center Specific)
Publication Year: 1978
Added to NTRS: 2004-11-03
Accession Number: 78A26080; Document ID: 19780042171
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