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  • 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
    Smith EJ, Balogh A, Lepping RP, Neugebauer M, Phillips J, Tsurutani BTet 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 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
  • Conference paper
    KRUPP N, KEPPLER E, KORTH A, FRANZ M, REUSS MK, BALOGH A, DOUGHERTY MKet 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: 183-186

    We 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.
  • 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, Publisher: PERGAMON PRESS LTD, Pages: 197-204, ISSN: 0273-1177
  • 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
    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
  • Journal article
    Winterhalter D, Neugebauer M, Goldstein BE, Smith EJ, Tsurutani BT, Bame SJ, Balogh Aet al., 1995,

    Magnetic holes in the solar wind and their relation to mirror-mode structures

    , Space Science Reviews, Vol: 72, Pages: 201-204, ISSN: 0038-6308
  • Conference paper
    SOUTHWOOD DJ, DOUGHERTY MK, LEAMON RJ, HAYNES PLet al., 1995,

    ORIGIN AND DYNAMICS OF FIELD NULLS DETECTED IN THE JOVIAN MAGNETOSPHERE

    , D1 Symposium of COSPAR Scientific Commission D, at the 30th COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 177-181, ISSN: 0273-1177
  • Conference paper
    KRUPP N, KEPPLER E, KORTH A, FRANZ M, REUSS MK, BALOGH A, DOUGHERTY MKet 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, Publisher: PERGAMON PRESS LTD, Pages: 183-186, ISSN: 0273-1177
  • 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
  • Journal article
    SCIME EE, BAME SJ, FELDMAN WC, GARY SP, PHILLIPS JL, BALOGH Aet al., 1994,

    REGULATION OF THE SOLAR-WIND ELECTRON HEAT-FLUX FROM 1-AU TO 5-AU - ULYSSES OBSERVATIONS

    , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 99, Pages: 23401-23410, ISSN: 2169-9380
    • Cite
    • Citations: 112
  • Journal article
    WINTERHALTER D, NEUGEBAUER M, GOLDSTEIN BE, SMITH EJ, BAME SJ, BALOGH Aet al., 1994,

    ULYSSES FIELD AND PLASMA OBSERVATIONS OF MAGNETIC HOLES IN THE SOLAR-WIND AND THEIR RELATION TO MIRROR-MODE STRUCTURES

    , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 99, Pages: 23371-23381, ISSN: 2169-9380
    • Cite
    • Citations: 195
  • Journal article
    Pantellini FGE, Burgess D, Schwartz SJ, 1994,

    Phase space evolution in linear instabilities

    , Physics of Plasmas, Vol: 1, Pages: 3784-3791-3784-3791
  • Conference paper
    SOUTHWOOD DJ, 1994,

    RECENT MAGNETIC-FIELD RESULTS FROM THE GALILEO AND ULYSSES SPACECRAFT

    , Discussion Meeting on the Solar System - A Review of Results from Space Missions, Publisher: ROYAL SOC, Pages: 261-271, ISSN: 1364-503X
  • Conference paper
    BALOGH A, 1994,

    THE HELIOSPHERE AND THE ULYSSES MISSION

    , Discussion Meeting on the Solar System - A Review of Results from Space Missions, Publisher: ROYAL SOC, Pages: 227-236, ISSN: 1364-503X
  • Journal article
    COWLEY SWH, RUNCORN SK, SOUTHWOOD DJ, 1994,

    THE SOLAR-SYSTEM - A REVIEW OF RESULTS FROM SPACE MISSIONS

    , PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES, Vol: 349, Pages: 169-170, ISSN: 1364-503X
  • Journal article
    YOSHINO K, MURRAY JE, ESMOND JR, SUN Y, PARKINSON WH, THORNE AP, LEARNER RCM, COX Get al., 1994,

    FOURIER-TRANSFORM SPECTROSCOPY OF THE HERZBERG-I BANDS OF O-2

    , CANADIAN JOURNAL OF PHYSICS, Vol: 72, Pages: 1101-1108, ISSN: 0008-4204

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