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Journal articleSmith EJ, Balogh A, Lepping RP, et al., 1995,
Ulysses observations of latitude gradients in the heliospheric magnetic field
, Heliosphere During the Declining Solar Cycle, Vol: 16, Pages: 165-170, ISSN: 0273-1177 -
Journal articleMurphy N, Smith EJ, Tsurutani BT, et al., 1995,
Further studies of waves accompanying the solar wind pick-up of interstellar hydrogen
, Space Science Reviews, Vol: 72, Pages: 447-453, ISSN: 0038-6308 -
Journal articleScime EE, Bame SJ, Phillips JL, et al., 1995,
Latitudinal variations in the solar wind electron heat flux
, Space Science Reviews, Vol: 72, Pages: 105-108, ISSN: 0038-6308 -
Journal articleSanderson TR, Marsden RG, Wenzel KP, et al., 1995,
High-latitude observations of energetic ions during the first Ulysses polar pass
, Space Science Reviews, Vol: 72, Pages: 291-296, ISSN: 0038-6308 -
Conference paperHAMMOND CM, FELDMAN WC, PHILLIPS JL, et al., 1995,
ULYSSES OBSERVATIONS OF DOUBLE ION-BEAMS ASSOCIATED WITH CORONAL MASS EJECTIONS
, E2.2 Symposium of COSPAR Scientific Commission E on Solar Flare, Coronal and Heliospheric Dynamics, at the 13th COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 303-306, ISSN: 0273-1177- Cite
- Citations: 1
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Conference paperKRUPP N, KEPPLER E, KORTH A, et al., 1995, , D1 Symposium of COSPAR Scientific Commission D, at the 30th COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 183-186, ISSN: 0273-1177
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- Citations: 1
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Conference paperKIVELSON MG, PREVOST A, CORONITI FV, et al., 1995,
Galileo flybys of Earth: The nature of the distant shock
, D1 Symposium of COSPAR Scientific Commission D, at the 30th COSPAR Scientific Assembly, Pages: 197-204We report on observations of the Earth's bow shock at unprecedentedly large downtail distances, some as remote as 360 R(E). Surprisingly, we find that even at these large distances, the bow shock signature remains clear. The cases we report are among the weakest shocks ever clearly identified. These shocks reveal patterns of field changes remarkably similar to those observed for stronger shocks. Indeed, several of the shocks could serve as textbook examples because they occur in unusually quiet and steady solar wind conditions. The quasiperpendicular shocks are, in some cases preceded by whistler wave trains. Several of the shocks which have normal vectors in the transitional region between quasiperpendicular and quasiparallel are associated with large amplitude wave disturbances in the downstream plasma. Although low Mach number, these shocks are the source of large amplitude turbulence. We show a range of fits to the locations of the shock crossings, and argue that, for steady solar wind conditions, there is no sign of tail flapping. The displacement of the shock from the tail axis appears to be governed by the interplanetary magnetic field orientation as previously reported for Venus.
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Journal articleBalogh A, GonzalezEsparza JA, Forsyth RJ, et al., 1995,
Interplanetary shock waves: Ulysses observations in and out of the ecliptic plane
, Space Science Reviews, Vol: 72, Pages: 171-180, ISSN: 0038-6308 -
Conference paperKRUPP N, KEPPLER E, KORTH A, et al., 1995,
Ion measurements in the Jovian magnetosphere by the Ulysses EPAC experiment: A comparison between dawn and dusk sectors
, D1 Symposium of COSPAR Scientific Commission D, at the 30th COSPAR Scientific Assembly, Pages: 183-186We report on results from the EPAC experiment on board the Ulysses spacecraft during the Jupiter Flyby in February 1992. We compare ion anisotropies (E = 0.24-0.77 MeV/N) received on the inbound pass in the noon sector at low magnetic latitudes with those from the outbound pass in the dusk sector at high magnetic latitudes. The results can be summarized as follows: (1) The classification of an inner and middle magnetosphere is observed inbound at low magnetic latitudes as well as outbound at high magnetic latitudes. (2) Three-dimensional anisotropies of ions in the noon sector were found in the corotation direction with radial components, whereas in the dusk sector field aligned anisotropies as well as anisotropies in corotation and anti-corotation were observed. (3) The steady increase of He/O with increasing latitude in the inner magnetosphere suggests the ionosphere as an internal He-source. (4) We find a difference in the He/O-ratio between the day- and the dusk side of the magnetosphere.
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Conference paperWANG Z, KIVELSON MG, JOY S, et al., 1995, , D1 Symposium of COSPAR Scientific Commission D, at the 30th COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 47-57, ISSN: 0273-1177
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- Citations: 15
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Journal articleMacDowall RJ, Desch MD, Kaiser ML, et al., 1995,
The three-dimensional extent of a high speed solar wind stream
, Space Science Reviews, Vol: 72, Pages: 125-128, ISSN: 0038-6308 -
Journal articleSCIME EE, BAME SJ, FELDMAN WC, et al., 1994, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 99, Pages: 23401-23410, ISSN: 2169-9380
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- Citations: 112
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Journal articleWINTERHALTER D, NEUGEBAUER M, GOLDSTEIN BE, et al., 1994, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 99, Pages: 23371-23381, ISSN: 2169-9380
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- Citations: 195
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Journal articlePantellini FGE, Burgess D, Schwartz SJ, 1994, , Physics of Plasmas, Vol: 1, Pages: 3784-3791-3784-3791
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Conference paperBALOGH A, 1994, , Discussion Meeting on the Solar System - A Review of Results from Space Missions, Publisher: ROYAL SOC, Pages: 227-236, ISSN: 1364-503X
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- Citations: 5
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Journal articleCOWLEY SWH, RUNCORN SK, SOUTHWOOD DJ, 1994, , PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES, Vol: 349, Pages: 169-170, ISSN: 1364-503X
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Conference paperSOUTHWOOD DJ, 1994, , Discussion Meeting on the Solar System - A Review of Results from Space Missions, Publisher: ROYAL SOC, Pages: 261-271, ISSN: 1364-503X
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- Citations: 1
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Journal articleYOSHINO K, MURRAY JE, ESMOND JR, et al., 1994, , CANADIAN JOURNAL OF PHYSICS, Vol: 72, Pages: 1101-1108, ISSN: 0008-4204
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- Citations: 30
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Journal articleGOSLING JT, MCCOMAS DJ, PHILLIPS JL, et al., 1994, , GEOPHYSICAL RESEARCH LETTERS, Vol: 21, Pages: 2271-2274, ISSN: 0094-8276
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- Citations: 109
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Journal articleTSURUTANI BT, HO CM, SMITH EJ, et al., 1994, , GEOPHYSICAL RESEARCH LETTERS, Vol: 21, Pages: 2267-2270, ISSN: 0094-8276
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- Citations: 138
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Journal articleHAIGH J, 1994,
WRONG SEX
, NEW SCIENTIST, Vol: 144, Pages: 57-57, ISSN: 0262-4079 -
Journal articleHAIGH JD, 1994, , NATURE, Vol: 370, Pages: 544-546, ISSN: 0028-0836
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- Citations: 341
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Journal articleMCCOMAS DJ, GOSLING JT, HAMMOND CM, et al., 1994, , GEOPHYSICAL RESEARCH LETTERS, Vol: 21, Pages: 1751-1754, ISSN: 0094-8276
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- Citations: 39
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Journal articleARMSTRONG TP, HAGGERTY D, LANZEROTTI LJ, et al., 1994, , GEOPHYSICAL RESEARCH LETTERS, Vol: 21, Pages: 1747-1750, ISSN: 0094-8276
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- Citations: 30
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Journal articleGiacalone J, Schwartz SJ, Burgess D, 1994, , Annales Geophysicae, Vol: 12, Pages: 591-601-591-601
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Journal articleGIACALONE J, SCHWARTZ SJ, BURGESS D, 1994, , ANNALES GEOPHYSICAE-ATMOSPHERES HYDROSPHERES AND SPACE SCIENCES, Vol: 12, Pages: 591-601, ISSN: 0992-7689
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- Citations: 17
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Journal articleLENGYELFREY D, FARRELL WM, STONE RG, et al., 1994, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 99, Pages: 13325-13334, ISSN: 2169-9380
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- Citations: 29
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Journal articleMURRAY JE, YOSHINO K, ESMOND JR, et al., 1994, , JOURNAL OF CHEMICAL PHYSICS, Vol: 101, Pages: 62-73, ISSN: 0021-9606
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- Citations: 43
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Journal articlePHILLIPS JL, BALOGH A, BAME SJ, et al., 1994, , GEOPHYSICAL RESEARCH LETTERS, Vol: 21, Pages: 1105-1108, ISSN: 0094-8276
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- Citations: 116
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Journal articleSANDERSON TR, MARSDEN RG, WENZEL KP, et al., 1994, , GEOPHYSICAL RESEARCH LETTERS, Vol: 21, Pages: 1113-1116, ISSN: 0094-8276
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- Citations: 42
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