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Journal articleForsyth RJ, Balogh A, Smith EJ, et al., 1996, , GEOPHYSICAL RESEARCH LETTERS, Vol: 23, Pages: 3281-3282, ISSN: 0094-8276
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Journal articleDougherty MK, Balogh A, Southwood DJ, et al., 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 24929-24941, ISSN: 2169-9380
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- Citations: 16
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Journal articleZhong WY, Toumi R, Haigh JD, 1996, , GEOPHYSICAL RESEARCH LETTERS, Vol: 23, Pages: 3183-3186, ISSN: 0094-8276
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- Citations: 17
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Journal articleSchwartz SJ, Burgess D, Moses JJ, 1996, , ANNALES GEOPHYSICAE-ATMOSPHERES HYDROSPHERES AND SPACE SCIENCES, Vol: 14, Pages: 1134-1150, ISSN: 0992-7689
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- Citations: 182
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Journal articleSchwartz SJ, Burgess D, Moses JJ, 1996, , Annales Geophysicae, Vol: 14, Pages: 1134-1150-1134-1150
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Journal articleKivelson MG, Khurana KK, Walker RJ, et al., 1996, , SCIENCE, Vol: 274, Pages: 396-398, ISSN: 0036-8075
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- Citations: 161
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Journal articleHoogeveen GW, Phillips JL, Dougherty MK, 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 21439-21446, ISSN: 2169-9380
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- Citations: 1
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Conference paperBalogh A, 1996, , Publisher: SPRINGER, Pages: 15-28, ISSN: 0038-6308
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- Citations: 6
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Journal articleBekki S, Pyle JA, Zhong W, et al., 1996, , GEOPHYSICAL RESEARCH LETTERS, Vol: 23, Pages: 2669-2672, ISSN: 0094-8276
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- Citations: 79
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Journal articleThompson P, Southwood DJ, Goodman S, 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 19849-19858, ISSN: 2169-9380
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- Citations: 5
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Journal articleRiley P, Sonett CP, Tsurutani BT, et al., 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 19987-19993, ISSN: 2169-9380
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- Citations: 52
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Journal articleKivelson MG, Southwood DJ, 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 17365-17371, ISSN: 2169-9380
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- Citations: 154
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Journal articleGonzalezEsparza JA, Balogh A, Forsyth RJ, et al., 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 17057-17071, ISSN: 2169-9380
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- Citations: 25
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Journal articleKivelson MG, Khurana KK, Walker RJ, et al., 1996, , SCIENCE, Vol: 273, Pages: 337-340, ISSN: 0036-8075
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- Citations: 94
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Journal articleZHONG W, HAIGH JD, TOUMI R, et al., 1996, , Quarterly Journal of the Royal Meteorological Society, Vol: 122, Pages: 1459-1466, ISSN: 0035-9009
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Journal articleCowley SWH, Balogh A, Dougherty MK, et al., 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 15197-15210, ISSN: 2169-9380
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- Citations: 52
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Journal articleZhong WY, Haigh JD, Toumi R, et al., 1996, , QUARTERLY JOURNAL OF THE ROYAL METEOROLOGICAL SOCIETY, Vol: 122, Pages: 1459-1466, ISSN: 0035-9009
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- Citations: 6
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Journal articleHaigh JD, 1996, , SCIENCE, Vol: 272, Pages: 981-984, ISSN: 0036-8075
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- Citations: 551
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Journal articleTsurutani BT, Ho CM, Arballo JK, et al., 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 11027-11038, ISSN: 2169-9380
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- Citations: 60
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Journal articleToumi R, Haigh JD, Law KS, 1996, , GEOPHYSICAL RESEARCH LETTERS, Vol: 23, Pages: 1037-1040, ISSN: 0094-8276
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- Citations: 39
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Journal articleLim TL, Quenby JJ, Reuss MK, et al., 1996, , Annales Geophysicae, Vol: 14, Pages: 400-410
<jats:p>Abstract. During November 1992, a series of forward and reverse shocks passed the ULYSSES spacecraft. Spectral and anisotropy measurements are reported for protons and alpha particles between 0.28 and 6 MeV observed by the Energetic Particle Composition Experiment, data recorded by the Magnetometer Experiment and the high-energy (2.7–300 MeV) proton data from the Kiel Electron Telescope. An analysis of energetic particle, plasma and magnetometer data from ULYSSES has allowed a unique study of the corresponding arrival of fare particles, particles within a corotating interaction region and particles transported with a coronal mass ejection. We present an analysis of these data in terms of possible diffusive shock acceleration but conclude that this is likely to be incompatible with the short transit time of the particles. Shock drift acceleration of particles with energies 0.3 MeV/nucleon or solar acceleration followed by particle trapping behind the shock front are alternative possibilities. </jats:p>
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Journal articleStaines K, Balogh A, Cowley SWH, et al., 1996, , PLANETARY AND SPACE SCIENCE, Vol: 44, Pages: 341-&, ISSN: 0032-0633
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- Citations: 17
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Journal articleLim TL, Quenby JJ, Reuss MK, et al., 1996, , ANNALES GEOPHYSICAE-ATMOSPHERES HYDROSPHERES AND SPACE SCIENCES, Vol: 14, Pages: 400-410, ISSN: 0992-7689
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- Citations: 5
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Journal articleEdwards TM, Balogh A, Cowley SWH, et al., 1996, , PLANETARY AND SPACE SCIENCE, Vol: 44, Pages: 371-386, ISSN: 0032-0633
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- Citations: 6
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Journal articleForsyth RJ, Horbury TS, Balogh A, et al., 1996, , GEOPHYSICAL RESEARCH LETTERS, Vol: 23, Pages: 595-598, ISSN: 0094-8276
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- Citations: 53
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Journal articleMotschmann U, Woodward TI, Glassmeier KH, et al., 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 4961-4965, ISSN: 2169-9380
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- Citations: 89
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Journal articleFlowerdew RJ, Haigh JD, 1996, , GEOPHYSICAL RESEARCH LETTERS, Vol: 23, Pages: 351-354, ISSN: 0094-8276
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- Citations: 34
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Journal articleCrooker NU, Burton ME, Phillips JL, et al., 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 2467-2474, ISSN: 2169-9380
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- Citations: 56
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Journal articlePrange R, Rego D, Southwood D, et al., 1996, , Nature, Vol: 379, Pages: 323-325
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Journal articlePrange R, Rego D, Southwood D, et al., 1996, , Nature, Vol: 379, Pages: 323-325
THE electrodynamic interaction between Jupiter and the closest of its large moons, Io, is unique in the Solar system. Io's volcanoes eject a considerable amount of material into the inner jovian system (>1 tonne per second), much of it in the form of ions(1); the motion of Io through Jupiter's powerful magnetic field in turn generates a million-ampere current(2) between the charged near-Io environment and the planet's ionosphere. This current is presumably carried by Alfven waves(3), the electromagnetic equivalent of sound waves. Here we present far-ultraviolet observations of the atmospheric footprint of this current, which demonstrate that most of the energy is dissipated rapidly when the waves first encounter Jupiter's ionosphere; the position of the footprint varies with time, We see no evidence for the multiple ionospheric interactions that have been proposed to explain the structure of the radio emissions associated with these waves(4).
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