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• Journal article
  THOMPSON P, DOUGHERTY MK, SOUTHWOOD DJ, 1995,

  WAVE BEHAVIOR NEAR-CRITICAL FREQUENCIES IN COLD BI-ION PLASMAS

  , PLANETARY AND SPACE SCIENCE, Vol: 43, Pages: 625-634, ISSN: 0032-0633
  • Author Web Link
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  • Citations: 9
• Conference paper
  Phillips JL, Bame SJ, Gary SP, Gosling JT, Scime EE, Forsyth RJet al., 1995,

  Radial and meridional trends in solar wind thermal electron temperature and anisotropy: Ulysses

  , Pages: 109-112, ISSN: 0038-6308

  Ulysses plasma measurement from 1.15 to 5.31 AU and from S6.4° to S48.3° solar latitude are used to assess the trends in the solar wind thermal electron temperature and anisotropy. Improved spacecraft potential corrections and data products have been incorporated. The radial temperature gradient is steeper than in previous determinations, but flatter than adiabatic. When normalized to 1 AU, temperature decrease with increasing latitude. Little change in the average thermal anisotropy has been seen during the mission. © 1995 Kluwer Academic Publishers.

  • Abstract
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  • Citations: 21
• Conference paper
  McComas DJ, Gosling JT, Hammond CM, Moldwin MB, Phillips JL, Forsyth RJet al., 1995,

  Reconnection on open field lines ahead of coronal mass ejections

  , Pages: 129-132, ISSN: 0038-6308

  Plasma and magnetic field signatures from 29 November 1990 indicate that the Ulysses spacecraft passed through a series of interplanetary structures that were most likely formed by magnetic reconnection on open field lines ahead of a coronal mass ejection (CME). This reconnection changed the magnetic topology of the upstream region by converting normal open interplanetary magnetic field into a pair of regions: one magnetically disconnected from the Sun and the other, a tongue, connected back to the Sun at both ends. This process provides a new method for producing both heat flux dropouts and counterstreaming suprathermal electron signatures in interplanetary space. In this paper we expand upon the 29 November case study and argue that reconnection ahead of CMEs should be less common at high heliolatitudes. © 1995 Kluwer Academic Publishers.

  • Abstract
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  • Citations: 9
• Journal article
  Reiner MJ, Anderson KA, Roelof E, Armstrong T, Hospodarsky GB, Fainberg J, Stone RG, Lanzerotti L, Gurnett DA, Phillips JL, Forsyth Ret al., 1995,

  Ulysses/Galileo observations of type III radio bursts and associated in-situ electrons and Langmuir waves

  , Space Science Reviews, Vol: 72, Pages: 261-266, ISSN: 0038-6308

  Both the Ulysses and Galileo spacecraft detected energetic electrons and Langmuir waves that were associated with a type III radio burst on 10 December 1990. At the time of these observations, these spacecraft were in the ecliptic plane and separated by 0.4 AU, with Galileo near the Earth at 1 AU and Ulysses at 1.36 AU. From the measured electron arrival times, the propagation path lengths of the electrons to both Ulysses and Galileo were estimated to be significantly longer than the length of the Parker spiral. These long path lengths are interpreted as due to draping of the interplanetary magnetic field lines around a CME. The onset times of the Langmuir waves at Ulysses and Galileo coincided with the estimated arrival time of the 9 keV and 14 keV electrons, respectively. © 1995 Kluwer Academic Publishers.

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  • Citations: 5
• Conference paper
  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

  , Publisher: SPRINGER, Pages: 447-453, ISSN: 0038-6308
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  • Citations: 49
• Conference paper
  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

  , Publisher: SPRINGER, Pages: 291-296, ISSN: 0038-6308
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  • Citations: 17
• Conference paper
  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

  , Publisher: SPRINGER, Pages: 197-200, ISSN: 0038-6308
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  • Citations: 13
• 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
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  • Citations: 101
• Conference paper
  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

  , Publisher: SPRINGER, Pages: 285-290, ISSN: 0038-6308
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  • Citations: 10
• Conference paper
  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

  , Publisher: SPRINGER, Pages: 165-170, ISSN: 0038-6308
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  • Citations: 58
• Conference paper
  GOLDSTEIN BE, NEUGEBAUER M, GOSLING JT, BAME SJ, PHILLIPS JL, MCCOMAS DJ, BALOGH Aet al., 1995,

  ULYSSES OBSERVATIONS OF SOLAR-WIND PLASMA PARAMETERS IN THE ECLIPTIC FROM 1.4-AU TO 5.4-AU AND OUT OF THE ECLIPTIC

  , Publisher: SPRINGER, Pages: 113-116, ISSN: 0038-6308
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  • Citations: 11
• Conference paper
  GOSLING JT, BAME SJ, MCCOMAS DJ, PHILLIPS JL, BALOGH A, STRONG KTet al., 1995,

  CORONAL MASS EJECTIONS AT HIGH HELIOGRAPHIC LATITUDES - ULYSSES

  , Publisher: SPRINGER, Pages: 133-136, ISSN: 0038-6308
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  • Citations: 21
• Journal article
  TSURUTANI BT, SMITH EJ, HO CM, NEUGEBAUER M, GOLDSTEIN BE, MOK JSet al., 1995,

  INTERPLANETARY DISCONTINUITIES AND ALFVEN WAVES

  , SPACE SCIENCE REVIEWS, Vol: 72, Pages: 205-210, ISSN: 0038-6308
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  • Citations: 24
• Conference paper
  MCCOMAS DJ, GOSLING JT, HAMMOND CM, MOLDWIN MB, PHILLIPS JL, FORSYTH RJet al., 1995,

  RECONNECTION ON OPEN-FIELD LINES AHEAD OF CORONAL MASS EJECTIONS

  , Publisher: SPRINGER, Pages: 129-132, ISSN: 0038-6308
  • Cite
  • Citations: 9
• Conference paper
  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

  , Publisher: SPRINGER, Pages: 201-204, ISSN: 0038-6308
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  • Citations: 58
• Conference paper
  SCIME EE, BAME SJ, PHILLIPS JL, BALOGH Aet al., 1995,

  LATITUDINAL VARIATIONS IN THE SOLAR-WIND ELECTRON HEAT-FLUX

  , Publisher: SPRINGER, Pages: 105-108, ISSN: 0038-6308
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  • Citations: 8
• Conference paper
  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

  , Publisher: SPRINGER, Pages: 403-408, ISSN: 0038-6308
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  • Citations: 45
• Conference paper
  GOLDSTEIN BE, NEUGEBAUER M, GOSLING JT, BAME SJ, PHILLIPS JL, MCCOMAS DJ, BALOGH Aet 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: 113-116

  We 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.

  • Abstract
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• Conference paper
  GOSLING JT, BAME SJ, MCCOMAS DJ, PHILLIPS JL, BALOGH A, STRONG KTet al., 1995,

  Coronal mass ejections at high heliographic latitudes: Ulysses

  , 28th ESLAB Symposium - The High Latitude Heliosphere, Pages: 133-136

  Nine 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.

  • Abstract
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• Conference paper
  PHILLIPS JL, BAME SJ, GARY SP, GOSLING JT, SCIME EE, FORSYTH RJet al., 1995,

  RADIAL AND MERIDIONAL TRENDS IN SOLAR-WIND THERMAL ELECTRON-TEMPERATURE AND ANISOTROPY - ULYSSES

  , Publisher: SPRINGER, Pages: 109-112, ISSN: 0038-6308
  • Cite
  • Citations: 26
• 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
  • Cite
  • Citations: 5
• Conference paper
  FORSYTH RJ, 1995,

  THE HIGH-LATITUDE HELIOSPHERIC MAGNETIC-FIELD

  , Publisher: SPRINGER, Pages: 153-163, ISSN: 0038-6308
  • Cite
  • Citations: 16
• 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
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  • Citations: 3
• Conference paper
  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

  , Publisher: SPRINGER, Pages: 343-346, ISSN: 0038-6308
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  • Citations: 5
• 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
  • Author Web Link
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  • Citations: 3
• 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
  • Cite
• 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
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  • Citations: 10
• 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
  • Cite
  • Citations: 3

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