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  • 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
    WANG Z, KIVELSON MG, JOY S, KHURANA KK, POLANSKEY C, SOUTHWOOD DJ, WALKER RJet al., 1995,

    Solar wind interaction with small bodies .1. Whistler wing signatures near Galileo's closest approach to Gaspra and Ida

    , D1 Symposium of COSPAR Scientific Commission D, at the 30th COSPAR Scientific Assembly, Pages: 47-57

    Data from Galileo's two asteroid flybys reveal magnetic fluctuations that ive interpret as perturbations of the solar wind magnetic field caused by an interaction with the nearby asteroid. The scale sizes of the bodies (similar to 14 km for Gaspra and similar to 30 km for Ida) are intermediate between the ion and electron gyroradii, which implies that the asteroid-imposed perturbations propagate in the whistler mode. Special properties of the whistler mode include phase velocities that can exceed the solar wind speed and confinement of the disturbance to directions nearly aligned with the magnetic field. These features of the interaction impose a structure on the solar wind disturbance that differs greatly from the forms familiar for either magnetized or unmagnetized bodies of magnetohydrodynamic spatial scales. We examine both data and computer simulations of the interaction with special attention to what can be inferred about the interaction itself from analysis of the data.
  • 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
  • Journal article
    Smith EJ, Neugebauer M, Balogh A, Bame SJ, Lepping RP, Tsurutani BTet al., 1995,

    Ulysses observations of latitude gradients in the heliospheric magnetic field: Radial component and variances

    , Space Science Reviews, Vol: 72, Pages: 165-170, ISSN: 0038-6308
  • 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
    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
  • 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.
  • Conference paper
    LANZEROTTI 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 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 GALILEOS DETECTION OF MAGNETIC ROTATIONS TELL US ABOUT GASPRA AND IDA

    , D1 Symposium of COSPAR Scientific Commission D, at the 30th COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 59-68, ISSN: 0273-1177
  • Conference paper
    KIVELSON MG, PREVOST A, CORONITI FV, KHURANA KK, SOUTHWOOD DJet 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: 197-204

    We 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.
  • Conference paper
    WANG Z, KIVELSON MG, JOY S, KHURANA KK, POLANSKEY C, SOUTHWOOD DJ, WALKER RJet al., 1995,

    SOLAR-WIND INTERACTION WITH SMALL BODIES .1. WHISTLER WING SIGNATURES NEAR GALILEOS CLOSEST APPROACH TO GASPRA AND IDA

    , D1 Symposium of COSPAR Scientific Commission D, at the 30th COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 47-57, ISSN: 0273-1177
  • Journal article
    MacDowall RJ, Desch MD, Kaiser ML, Stone RG, Hess RA, Balogh A, Bame SJ, Goldstein BEet 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 article
    Murphy N, Smith EJ, Tsurutani BT, Balogh A, Southwood DJet 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 article
    Reuss MK, Keppler E, Franz M, Witte M, Krupp N, Wilken B, Balogh A, Forsyth RJ, Moussas X, Polygiannakis JM, Kakouris AD, Alevizos Aet 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 article
    Riley P, Sonett CP, Balogh A, Forsyth RJ, Scime EE, Feldman WCet 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
  • Journal article
    Scime EE, Bame SJ, Phillips JL, Balogh Aet al., 1995,

    Latitudinal variations in the solar wind electron heat flux

    , Space Science Reviews, Vol: 72, Pages: 105-108, ISSN: 0038-6308
  • Journal article
    Sanderson TR, Marsden RG, Wenzel KP, Balogh A, Forsyth RJ, Goldstein BEet 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 paper
    HAMMOND CM, FELDMAN WC, PHILLIPS JL, BALOGH Aet 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
  • Journal article
    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

    , Space Science Reviews, Vol: 72, Pages: 171-180, ISSN: 0038-6308

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