Results
- Showing results for:
- Reset all filters
Search results
-
Journal articlePickering JC, 1996, , ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, Vol: 107, Pages: 811-822, ISSN: 0067-0049
- Cite
- Citations: 60
-
Journal articleBothmer V, Desai MI, Marsden RG, et al., 1996,
Ulysses observations of open and closed magnetic field lines within a coronal mass ejection
, ASTRONOMY & ASTROPHYSICS, Vol: 316, Pages: 493-498, ISSN: 0004-6361- Cite
- Citations: 27
-
Journal articlePickering JC, Thorne AP, 1996, , ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, Vol: 107, Pages: 761-809, ISSN: 0067-0049
- Cite
- Citations: 53
-
Journal articleNilsson H, Kirkwood S, Lilensten J, et al., 1996, , ANNALES GEOPHYSICAE-ATMOSPHERES HYDROSPHERES AND SPACE SCIENCES, Vol: 14, Pages: 1462-1472, ISSN: 0992-7689
- Cite
- Citations: 20
-
Journal articleBurton ME, Smith EJ, Balogh A, et al., 1996,
Ulysses out-of-ecliptic observations of interplanetary shocks
, ASTRONOMY & ASTROPHYSICS, Vol: 316, Pages: 313-322, ISSN: 0004-6361- Cite
- Citations: 25
-
Journal articleWeiss LA, Gosling JT, McAllister AH, et al., 1996,
A comparison of interplanetary coronal mass ejections at Ulysses with Yohkoh soft X-ray coronal events
, ASTRONOMY & ASTROPHYSICS, Vol: 316, Pages: 384-395, ISSN: 0004-6361- Cite
- Citations: 24
-
Journal articleZook HA, Gr眉n E, Baguhl M, et al., 1996, , Science, Vol: 274, Pages: 1501-1503, ISSN: 0036-8075
From September 1991 to October 1992, the cosmic dust detector on the Ulysses spacecraft recorded 11 short bursts, or streams, of dust. These dust grains emanated from the jovian system, and their trajectories were strongly affected by solar wind magnetic field forces. Analyses of the on-board measurements of these fields, and of stream approach directions, show that stream-associated dust grain masses are of the order of 10(-18) gram and dust grain velocities exceed 200 kilometers per second. These masses and velocities are, respectively, about 10(3) times less massive and 5 to 10 times faster than earlier reported.
-
Journal articleForsyth RJ, Balogh A, Smith EJ, et al., 1996, , GEOPHYSICAL RESEARCH LETTERS, Vol: 23, Pages: 3281-3282, ISSN: 0094-8276
-
Journal articleDougherty MK, Balogh A, Southwood DJ, et al., 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 24929-24941, ISSN: 2169-9380
- Cite
- Citations: 16
-
Journal articleZhong WY, Toumi R, Haigh JD, 1996, , GEOPHYSICAL RESEARCH LETTERS, Vol: 23, Pages: 3183-3186, ISSN: 0094-8276
- Cite
- Citations: 17
-
Journal articleSchwartz SJ, Burgess D, Moses JJ, 1996, , ANNALES GEOPHYSICAE-ATMOSPHERES HYDROSPHERES AND SPACE SCIENCES, Vol: 14, Pages: 1134-1150, ISSN: 0992-7689
- Cite
- Citations: 182
-
Journal articleSchwartz SJ, Burgess D, Moses JJ, 1996, , Annales Geophysicae, Vol: 14, Pages: 1134-1150-1134-1150
-
Journal articleKivelson MG, Khurana KK, Walker RJ, et al., 1996, , SCIENCE, Vol: 274, Pages: 396-398, ISSN: 0036-8075
- Cite
- Citations: 161
-
Journal articleHoogeveen GW, Phillips JL, Dougherty MK, 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 21439-21446, ISSN: 2169-9380
- Cite
- Citations: 1
-
Conference paperBalogh A, 1996, , Publisher: SPRINGER, Pages: 15-28, ISSN: 0038-6308
- Cite
- Citations: 6
-
Journal articleBekki S, Pyle JA, Zhong W, et al., 1996, , GEOPHYSICAL RESEARCH LETTERS, Vol: 23, Pages: 2669-2672, ISSN: 0094-8276
- Cite
- Citations: 79
-
Journal articleThompson P, Southwood DJ, Goodman S, 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 19849-19858, ISSN: 2169-9380
- Cite
- Citations: 5
-
Journal articleRiley P, Sonett CP, Tsurutani BT, et al., 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 19987-19993, ISSN: 2169-9380
- Cite
- Citations: 52
-
Journal articleKivelson MG, Southwood DJ, 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 17365-17371, ISSN: 2169-9380
- Cite
- Citations: 154
-
Journal articleGonzalezEsparza JA, Balogh A, Forsyth RJ, et al., 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 17057-17071, ISSN: 2169-9380
- Cite
- Citations: 25
-
Journal articleKivelson MG, Khurana KK, Walker RJ, et al., 1996, , SCIENCE, Vol: 273, Pages: 337-340, ISSN: 0036-8075
- Cite
- Citations: 94
-
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
-
Journal articleCowley SWH, Balogh A, Dougherty MK, et al., 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 15197-15210, ISSN: 2169-9380
- Cite
- Citations: 52
-
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
- Cite
- Citations: 6
-
Journal articleHaigh JD, 1996, , SCIENCE, Vol: 272, Pages: 981-984, ISSN: 0036-8075
- Cite
- Citations: 551
-
Journal articleTsurutani BT, Ho CM, Arballo JK, et al., 1996, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 11027-11038, ISSN: 2169-9380
- Cite
- Citations: 60
-
Journal articleToumi R, Haigh JD, Law KS, 1996, , GEOPHYSICAL RESEARCH LETTERS, Vol: 23, Pages: 1037-1040, ISSN: 0094-8276
- Cite
- Citations: 39
-
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>
-
Journal articleStaines K, Balogh A, Cowley SWH, et al., 1996, , PLANETARY AND SPACE SCIENCE, Vol: 44, Pages: 341-&, ISSN: 0032-0633
- Cite
- Citations: 17
-
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
- Cite
- Citations: 5
This data is extracted from the Web of Science and reproduced under a licence from Thomson Reuters. You may not copy or re-distribute this data in whole or in part without the written consent of the Science business of Thomson Reuters.