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Conference paperSANDERSON TR, MARSDEN RG, WENZEL KP, et al., 1995, , Publisher: SPRINGER, Pages: 291-296, ISSN: 0038-6308
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- Citations: 17
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Conference paperBALOGH A, GONZALEZESPARZA JA, FORSYTH RJ, et al., 1995, , Publisher: SPRINGER, Pages: 171-180, ISSN: 0038-6308
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- Citations: 101
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Conference paperREUSS MK, KEPPLER E, FRANZ M, et al., 1995, , Publisher: SPRINGER, Pages: 343-346, ISSN: 0038-6308
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- Citations: 5
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Conference paperMURPHY N, SMITH EJ, TSURUTANI BT, et al., 1995, , Publisher: SPRINGER, Pages: 447-453, ISSN: 0038-6308
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- Citations: 49
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Journal articleTSURUTANI BT, SMITH EJ, HO CM, et al., 1995, , SPACE SCIENCE REVIEWS, Vol: 72, Pages: 205-210, ISSN: 0038-6308
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- Citations: 24
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Conference paperMACDOWALL RJ, DESCH MD, KAISER ML, et al., 1995, , Publisher: SPRINGER, Pages: 125-128, ISSN: 0038-6308
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- Citations: 5
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Conference paperFORSYTH RJ, 1995, , Publisher: SPRINGER, Pages: 153-163, ISSN: 0038-6308
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- Citations: 16
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Conference paperSOLOMON J, CORNILLEAUWEHRLIN N, CANU P, et al., 1995, , Publisher: SPRINGER, Pages: 181-184, ISSN: 0038-6308
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- Citations: 3
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Conference paperGOSLING JT, BAME SJ, MCCOMAS DJ, et al., 1995,
Coronal mass ejections at high heliographic latitudes: Ulysses
, 28th ESLAB Symposium - The High Latitude Heliosphere, Pages: 133-136Nine coronal mass ejections (CMEs) have been detected in the solar wind by the Ulysses plasma experiment between 31 degrees and 61 degrees South. One of these events, which was also a magnetic cloud, was directly associated with an event observed by the soft X-ray telescope on Yohkoh in which large magnetic loops formed in the solar corona directly beneath Ulysses. This association suggests that the flux rope topology of the magnetic cloud resulted from reconnection between the ''legs'' of neighboring magnetic loops within the rising CME. The average CME speed (similar to 740 km s(-1)) at these latitudes was comparable to that of the normal solar wind there and is much greater than average CME speeds observed either in the solar wind in the ecliptic plane or in the corona close to the Sun. We suggest that the same basic acceleration process applies to both slow CMEs and the normal solar wind at any latitude.
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Conference paperGOLDSTEIN BE, NEUGEBAUER M, GOSLING JT, et al., 1995,
Ulysses observations of solar wind plasma parameters in the ecliptic from 1.4 to 5.4 AU and out of the ecliptic
, 28th ESLAB Symposium - The High Latitude Heliosphere, Pages: 113-116We report observations of radial and latitudinal gradients of Ulysses plasma parameters. The solar wind velocity increased rapidly with latitude from 0 degrees to 35 degrees, then remained approximately constant at higher latitudes. Solar wind density decreased rapidly from 0 degrees to 35 degrees of latitude, and also was approximately constant beyond that latitude. The mass flux similarly decreased away from the equator (but less than the density), whereas the momentum flux was relatively constant. The radial gradient of the entropy at high latitude indicated a value for the polytrope index of about 1.72 (close to adiabatic); the in-ecliptic estimates of radial gradients for temperature and entropy may be biased by temporal variation. A striking increase in the alpha particle-proton velocity difference with latitude is found.
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Conference paperMCKIBBEN RB, SIMPSON JA, ZHANG M, et al., 1995, , Publisher: SPRINGER, Pages: 403-408, ISSN: 0038-6308
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- Citations: 45
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Conference paperSCIME EE, BAME SJ, PHILLIPS JL, et al., 1995, , Publisher: SPRINGER, Pages: 105-108, ISSN: 0038-6308
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- Citations: 8
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Conference paperMCCOMAS DJ, GOSLING JT, HAMMOND CM, et al., 1995, , Publisher: SPRINGER, Pages: 129-132, ISSN: 0038-6308
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- Citations: 9
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Conference paperPHILLIPS JL, BAME SJ, GARY SP, et al., 1995, , Publisher: SPRINGER, Pages: 109-112, ISSN: 0038-6308
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- Citations: 26
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Conference paperWINTERHALTER D, NEUGEBAUER M, GOLDSTEIN BE, et al., 1995, , Publisher: SPRINGER, Pages: 201-204, ISSN: 0038-6308
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- Citations: 58
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Journal articleEVANS SJ, HAIGH JD, 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 695-698, ISSN: 0094-8276
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- Citations: 3
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Journal articleRUZMAIKIN AA, FEYNMAN J, GOLDSTEIN BE, et al., 1995, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 100, Pages: 3395-3403, ISSN: 2169-9380
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- Citations: 82
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Journal articleBUTTIGHOFFER A, PICK M, ROELOF EC, et al., 1995, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 100, Pages: 3369-3381, ISSN: 2169-9380
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- Citations: 17
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Journal articlePantellini FGE, Schwartz SJ, 1995, , \jgr, Vol: 100, Pages: 3539-3549-3539-3549
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Journal articleLEAMON RJ, DOUGHERTY MK, SOUTHWOOD DJ, et al., 1995, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 100, Pages: 1829-1835, ISSN: 2169-9380
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- Citations: 10
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Conference paperBALOGH A, 1995, , 14th European Cosmic Ray Symposium (14th ECRS) - Cosmic Rays 94: Solar, Heliospheric, Astrophysical and High-Energy Aspects, Publisher: ELSEVIER, Pages: 69-74, ISSN: 0550-3213
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- Citations: 3
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Journal articleGosling JT, McComas DJ, Phillips JL, et al., 1995, , Geophysical Research Letters, Vol: 22, Pages: 1753-1756, ISSN: 0094-8276
A solar wind disturbance produced by a fast coronal mass ejection, CME, that departed from the Sun on Feburary 20, 1994 was observed in the ecliptic plane at 1 AU by IMP 8 and at high heliographic latitudes at 3.53 AU by Ulysses. In the ecliptic the disturbance included a strong forward shock but no reverse shock, while at high latitudes the disturbance was bounded by a relatively weak forward鈥恟everse shock pair. It is clear that the disturbance in the ecliptic plane was driven primarily by the relative speed between the CME and a slower ambient solar wind ahead, whereas at higher latitudes the disturbance was driven by expansion of the CME. The combined IMP 8 and Ulysses observations thus provide a graphic illustration of how a single fast CME can produce very different types of solar wind disturbances at low and high heliographic latitudes. Simple numerical simulations help explain observed differences at the two spacecraft. Copyright 1995 by the American Geophysical Union.
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Journal articleZHONG WY, HAIGH JD, 1995, , JOURNAL OF THE ATMOSPHERIC SCIENCES, Vol: 52, Pages: 124-138, ISSN: 0022-4928
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- Citations: 54
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Journal articleHORBURY T, BALOGH A, FORSYTH RJ, et al., 1995,
ULYSSES MAGNETIC-FIELD OBSERVATIONS OF FLUCTUATIONS WITHIN POLAR CORONAL FLOWS
, ANNALES GEOPHYSICAE-ATMOSPHERES HYDROSPHERES AND SPACE SCIENCES, Vol: 13, Pages: 105-107, ISSN: 0992-7689- Cite
- Citations: 25
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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 articleReuss MK, Keppler E, Franz M, et al., 1995,
A particle event at 5 AU and 20 degrees southern latitude from measurements with the EPAC instrument on Ulysses
, Space Science Reviews, Vol: 72, Pages: 343-346, ISSN: 0038-6308 -
Journal articleRiley P, Sonett CP, Balogh A, et al., 1995,
Alfvenic fluctuations in the solar wind: A case study using Ulysses measurements
, Space Science Reviews, Vol: 72, Pages: 197-200, ISSN: 0038-6308 -
Conference paperKIVELSON MG, WANG Z, JOY S, et al., 1995,
Solar wind interaction with small bodies .2. What can Galileo's detection of magnetic rotations tell us about Gaspra and Ida
, D1 Symposium of COSPAR Scientific Commission D, at the 30th COSPAR Scientific Assembly, Pages: 59-68As the Galileo spacecraft passed the asteroids Gaspra in 1990 and Ida in 1993, the magnetometer recorded changes in the solar wind magnetic field that we associate with the presence of the nearby body. This paper focuses on the types of interactions that can produce perturbations in the solar wind. We have suggested that the interaction at Gaspra is consistent with expectations of flow diversion by a magnetic dipole moment and an associated ''magnetosphere'' whose scale size is much larger than the diameter of the solid body. The conditions for the Ida flyby leave more room for ambiguity. The observations could plausibly be related to either interaction with a magnetized body or with a conducting body. We will report on details of the observations that may enable us to distinguish between the different types of interaction and to provide quantitative estimates of the physical properties of the asteroids themselves.
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Conference paperLANZEROTTI LJ, MACLENNAN CG, FORSYTH RJ, 1995,
INTERPLANETARY MAGNETIC-FIELD CONTROL OF HEAVY-ION ABUNDANCES AT SIMILAR-TO-5.2 AU
, 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: 307-310, ISSN: 0273-1177 -
Conference paperKIVELSON MG, WANG Z, JOY S, et al., 1995, , D1 Symposium of COSPAR Scientific Commission D, at the 30th COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 59-68, ISSN: 0273-1177
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- Citations: 17
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