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  • Conference paper
    MACDOWALL RJ, DESCH MD, KAISER ML, STONE RG, HESS RA, BALOGH A, BAME SJ, GOLDSTEIN BEet al., 1995,

    THE 3-DIMENSIONAL EXTENT OF A HIGH-SPEED SOLAR-WIND STREAM

    , Publisher: SPRINGER, Pages: 125-128, ISSN: 0038-6308
  • Conference paper
    FORSYTH RJ, 1995,

    THE HIGH-LATITUDE HELIOSPHERIC MAGNETIC-FIELD

    , Publisher: SPRINGER, Pages: 153-163, ISSN: 0038-6308
  • Conference paper
    SOLOMON J, CORNILLEAUWEHRLIN N, CANU P, LENGYELFREY D, BAME SJ, SCIME EE, BALOGH A, FORSYTH Ret al., 1995,

    INTERACTION BETWEEN WHISTLER-MODE WAVES AND ELECTRONS IN THE VICINITY OF INTERPLANETARY SHOCKS AS SEEN BY ULYSSES - A PRELIMINARY-STUDY

    , Publisher: SPRINGER, Pages: 181-184, ISSN: 0038-6308
  • Conference paper
    BALOGH A, GONZALEZESPARZA JA, FORSYTH RJ, BURTON ME, GOLDSTEIN BE, SMITH EJ, BAME SJet al., 1995,

    INTERPLANETARY SHOCK-WAVES - ULYSSES OBSERVATIONS IN AND OUT OF THE ECLIPTIC-PLANE

    , Publisher: SPRINGER, Pages: 171-180, ISSN: 0038-6308
    • Cite
    • Citations: 101
  • Journal article
    EVANS SJ, HAIGH JD, 1995,

    THE RETRIEVAL OF TOTAL OPTICAL DEPTH AND EFFECTIVE DROPLET RADIUS OF CLOUDS FROM SOLAR REFLECTION MEASUREMENTS USING THE ALONG-TRACK SCANNING RADIOMETER-2 (ATSR-2)

    , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 695-698, ISSN: 0094-8276
  • Journal article
    BUTTIGHOFFER A, PICK M, ROELOF EC, HOANG S, MANGENEY A, LANZEROTTI LJ, FORSYTH RJ, PHILLIPS JLet al., 1995,

    CORONAL ELECTRON STREAM AND LANGMUIR WAVE DETECTION INSIDE A PROPAGATION CHANNEL AT 4.3 AU

    , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 100, Pages: 3369-3381, ISSN: 2169-9380
    • Cite
    • Citations: 17
  • Journal article
    RUZMAIKIN AA, FEYNMAN J, GOLDSTEIN BE, SMITH EJ, BALOGH Aet al., 1995,

    INTERMITTENT TURBULENCE IN SOLAR-WIND FROM THE SOUTH POLAR HOLE

    , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 100, Pages: 3395-3403, ISSN: 2169-9380
    • Cite
    • Citations: 82
  • Journal article
    Pantellini FGE, Schwartz SJ, 1995,

    Electron temperature effects in the linear proton mirror instability

    , \jgr, Vol: 100, Pages: 3539-3549-3539-3549
  • Journal article
    LEAMON RJ, DOUGHERTY MK, SOUTHWOOD DJ, HAYNES PLet al., 1995,

    MAGNETIC NULLS IN THE OUTER MAGNETOSPHERE OF JUPITER - DETECTIONS BY PIONEER AND VOYAGER SPACECRAFT

    , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 100, Pages: 1829-1835, ISSN: 2169-9380
  • Conference paper
    BALOGH A, 1995,

    MAGNETIC-FIELDS IN THE HIGH-LATITUDE HELIOSPHERE

    , 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
  • Journal article
    ZHONG WY, HAIGH JD, 1995,

    IMPROVED BROAD-BAND EMISSIVITY PARAMETERIZATION FOR WATER-VAPOR COOLING RATE CALCULATIONS

    , JOURNAL OF THE ATMOSPHERIC SCIENCES, Vol: 52, Pages: 124-138, ISSN: 0022-4928
  • Journal article
    Gosling JT, McComas DJ, Phillips JL, Pizzo VJ, Goldstein BE, Forsyth RJ, Lepping RPet al., 1995,

    A CME‐driven solar wind disturbance observed at both low and high heliographic latitudes

    , 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‐reverse 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.
  • Journal article
    HORBURY T, BALOGH A, FORSYTH RJ, SMITH EJet 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
  • Journal article
    Hammond CM, Feldman WC, Phillips JL, Balogh Aet al., 1995,

    Ulysses observations of double ion beams associated with coronal mass ejections

    , Solar Flare, Coronal and Heliospheric Dynamics, Vol: 17, Pages: 303-306, ISSN: 0273-1177
  • Conference paper
    SMITH EJ, BALOGH A, LEPPING RP, NEUGEBAUER M, PHILLIPS J, TSURUTANI BTet al., 1995,

    ULYSSES OBSERVATIONS OF LATITUDE GRADIENTS IN THE HELIOSPHERIC MAGNETIC-FIELD

    , D1 1 Symposium of COSPAR Scientific Commission D on the Heliosphere During the Declining Solar Cycle, at the 30th COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 165-170, ISSN: 0273-1177
  • Conference paper
    Hoang S, Lacombe C, Mangeney A, Pantellini F, Balogh A, Bame SJ, Forsyth RJ, Phillips JLet al., 1995,

    Interplanetary shocks observed by Ulysses in the ecliptic plane as a function of the heliocentric distance

    , D2.1 Symposium Symposium of COSPAR Scientific Commission D on Physics of Collisionless Shocks, at the 30th COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 371-374, ISSN: 0273-1177
  • Journal article
    Keppler E, Franz M, Korth A, Krupp N, Reuss MK, Wilken B, Balogh A, Forsyth RJ, Quenby JJ, Blake Bet al., 1995,

    Energetic particle observations at high heliographic latitudes

    , Space Science Reviews, Vol: 72, Pages: 285-290, ISSN: 0038-6308
  • Conference paper
    Lim TL, Quenby JJ, Reuss MK, Keppler E, Kunow H, Heber B, Forsyth RJet al., 1995,

    Can diffusive shock acceleration work fast enough in interplanetary shocks? Evidence from the November 1992 event

    , Urbino, 24th international cosmic ray conference (xxiv icrc) AUG 28-SEP 08, 1995 ROME, ITALY, Publisher: Argalia Editore Delle Arti Grafiche Editoriali Srl, Pages: 353-356
  • Journal article
    Schwartz SJ, 1995,

    Hot flow anomalies near the Earth’s bow shock

    , Advances in Space Research, Vol: 15, Pages: 107-116-107-116
  • Journal article
    Leckband JA, Burgess D, Pantellini FGE, Schwartz SJet al., 1995,

    Ion distributions associated with mirror waves in the Earth’s magnetosheath

    , Advances in Space Research, Vol: 15, Pages: 345-348-345-348
  • Journal article
    Pantellini FGE, Burgess D, Schwartz SJ, 1995,

    On the non-linear mirror instability

    , Advances in Space Research, Vol: 15, Pages: 341-344-341-344
  • Journal article
    Chisham G, Burgess D, Schwartz SJ, 1995,

    Electron distributions in the ion foreshock

    , Advances in Space Research, Vol: 15, Pages: 141-145-141-145
  • Conference paper
    Leckband JA, Burgess D, Pantellini FGE, Schwartz SJet al., 1995,

    Ion distributions associated with mirror waves in the Earth's magnetosheath

    , D2.1 Symposium Symposium of COSPAR Scientific Commission D on Physics of Collisionless Shocks, at the 30th COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 345-348, ISSN: 0273-1177
  • Conference paper
    Baring MG, Ogilvie KW, Ellison DC, Forsyth Ret al., 1995,

    Acceleration of solar wind ions by oblique interplanetary shocks

    , D2.1 Symposium Symposium of COSPAR Scientific Commission D on Physics of Collisionless Shocks, at the 30th COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 385-388, ISSN: 0273-1177
  • Journal article
    Balogh A, 1995,

    Magnetic fields in the high latitude heliosphere

    , Nuclear Physics B, Pages: 69-74, ISSN: 0550-3213
  • Journal article
    Pickering JC, Thorne AP, Rosberg M, 1995,

    UV Fourier transform spectroscopy and term analysis of Co I and Co II

    , Laboratory and Astronomical High Resolution Spectra, Vol: 81, Pages: 204-211
  • Conference paper
    Lim TL, Quenby JJ, Reuss MK, Keppler E, Kunow H, Heber B, Forsyth RJet al., 1995,

    Can diffusive shock acceleration work fast enough in interplanetary shocks? Evidence from the November 1992 event

    , Urbino, 24th international cosmic ray conference (xxiv icrc) AUG 28-SEP 08, 1995 ROME, ITALY, Publisher: Argalia Editore Delle Arti Grafiche Editoriali Srl, Pages: 353-356
  • Journal article
    McKibben RB, Simpson JA, Zhang M, Bame S, Balogh Aet al., 1995,

    Ulysses out-of-ecliptic observations of ''27-day'' variations in high energy cosmic ray intensity

    , Space Science Reviews, Vol: 72, Pages: 403-408, ISSN: 0038-6308
  • Journal article
    Learner RCM, Thorne AP, Murray JE, Semeniuk JIet al., 1995,

    UV Fourier transform spectroscopy of emission line spectra

    , Laboratory and Astronomical High Resolution Spectra, Vol: 81, Pages: 227-228
  • Conference paper
    KIVELSON MG, WANG Z, JOY S, KHURANA KK, POLANSKEY C, SOUTHWOOD DJ, WALKER RJet 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: 59-68

    As 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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