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  • Journal article
    Bogdanov AT, Glassmeier KH, Musmann G, Dougherty MK, Kellock S, Slootweg P, Tsurutani Bet al., 2003,

    , ANNALES GEOPHYSICAE, Vol: 21, Pages: 2043-2057, ISSN: 0992-7689
  • Journal article
    Czaja A, 2003,

    , QUARTERLY JOURNAL OF THE ROYAL METEOROLOGICAL SOCIETY, Vol: 129, Pages: 2867-2878, ISSN: 0035-9009
  • Journal article
    Zong QG, Fritz TA, Spence H, Dunlop M, Pu ZY, Korth A, Daly PW, Balogh A, Reme Het al., 2003,

    , PLANETARY AND SPACE SCIENCE, Vol: 51, Pages: 821-830, ISSN: 0032-0633
    • Cite
    • Citations: 27
  • Journal article
    Mazelle C, Meziane K, LeQu茅au D, Wilber M, Eastwood JP, R猫me H, Sauvaud JA, Bosqued JM, Dandouras I, McCarthy M, Kistler LM, Klecker B, Korth A, Bavassano-Cattaneo MB, Pallocchia G, Lundin R, Balogh Aet al., 2003,

    , PLANETARY AND SPACE SCIENCE, Vol: 51, Pages: 785-795, ISSN: 0032-0633
    • Cite
    • Citations: 90
  • Journal article
    Brindley HE, Allan RP, 2003,

    , QUARTERLY JOURNAL OF THE ROYAL METEOROLOGICAL SOCIETY, Vol: 129, Pages: 2971-2988, ISSN: 0035-9009
    • Cite
    • Citations: 11
  • Journal article
    Sanderson TR, Marsden RG, Tranquille C, Dalla S, Forsyth RJ, Gosling JT, McKibben RBet al., 2003,

    , GEOPHYSICAL RESEARCH LETTERS, Vol: 30, ISSN: 0094-8276
    • Cite
    • Citations: 15
  • Journal article
    Dalla S, Balogh A, Krucker S, Posner A, M眉ller-Mellin R, Anglin JD, Hofer MY, Marsden RG, Sanderson TR, Tranquille C, Heber B, Zhang M, McKibben RBet al., 2003,

    , GEOPHYSICAL RESEARCH LETTERS, Vol: 30, ISSN: 0094-8276
    • Cite
    • Citations: 64
  • Journal article
    Reisenfeld DB, Gosling JT, Forsyth RJ, Riley P, St Cyr OCet al., 2003,

    , GEOPHYSICAL RESEARCH LETTERS, Vol: 30, ISSN: 0094-8276
    • Cite
    • Citations: 44
  • Journal article
    Hofer MY, Marsden RG, Sanderson TR, Tranquille C, Forsyth RJet al., 2003,

    , GEOPHYSICAL RESEARCH LETTERS, Vol: 30, ISSN: 0094-8276
  • Journal article
    Jones GH, Balogh A, Smith EJ, 2003,

    , GEOPHYSICAL RESEARCH LETTERS, Vol: 30, ISSN: 0094-8276
    • Cite
    • Citations: 35
  • Journal article
    Rees A, Forsyth RJ, 2003,

    , GEOPHYSICAL RESEARCH LETTERS, Vol: 30, ISSN: 0094-8276
    • Cite
    • Citations: 10
  • Journal article
    Lin NG, Kellogg PJ, MacDowall RJ, McComas DJ, Balogh Aet al., 2003,

    , GEOPHYSICAL RESEARCH LETTERS, Vol: 30, ISSN: 0094-8276
    • Cite
    • Citations: 10
  • Journal article
    Sahraoui F, Pin莽on JL, Belmont G, Rezeau L, Cornilleau-Wehrlin N, Robert P, Mellul L, Bosqued JM, Balogh A, Canu P, Chanteur Get al., 2003,

    , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 108, ISSN: 2169-9380
    • Cite
    • Citations: 93
  • Conference paper
    Reisenfeld DB, Gosling JT, Steinberg JT, Riley P, Forsyth RJ, Cyr OCSet al., 2003,

    , Pages: 210-213, ISSN: 0094-243X

    From September through November 2001, Ulysses was almost continuously immersed in polar coronal hole (CH) flow during its northern polar pass of the Sun. For much of this time, the flow was fast (> 700 km/s) and steady, quite similar to the steady unstructured flow observed during Ulysses' first polar orbit near solar minimum. During the three months Ulysses transited the northern polar CH it observed 5 coronal mass ejections (CMEs). Of these, two were clearly over-expanding and two were at least partially driven by overexpansion. The phenomenon of over-expansion was frequently observed at high latitudes during Ulysses' first orbit. The recurrence of over-expanding CMEs during the second orbit at high latitudes indicates that this is a phenomenon apparently unique to and typical of CMEs embedded in polar CH flow. Ulysses was nearly above the solar limb during this three-month interval, providing an opportunity to use LASCO/SOHO observations to study the initial velocity profiles of the CMEs observed further out by Ulysses. These initial conditions were used as inputs into a hydrodynamic code, the results of which are reported here.
  • Conference paper
    Lin N, Kellogg PJ, MacDowall RJ, McComas DJ, Balogh A, Forsyth RJet al., 2003,

    , Pages: 534-537, ISSN: 0094-243X

    We have compared observations of VLF waves (0.2 to 448 Hz) made by Ulysses during its second fast latitude scan (near the solar maximum) with the wave observations during the first fast latitude scan in 1995, when the solar activity was approaching a minimum. The occurrences and properties of the waves are found to be similar during the solar maximum and solar minimum periods for slow and intermediate speed solar wind. The maximum intensity of the electromagnetic waves for the two solar cycle periods is comparable. These similarities suggest that the plasma conditions for the waves' excitation are similar for the slow and intermediate solar wind in both solar maximum and minimum phases. It is also found that the electric field noise detected in the low band channels, which are measuring less than 9 Hz signals, is contaminated by the spin modulation of the electric field due to photoelectrons around the spacecraft, especially when the ambient plasma density is low. This noise increases with increasing solar aspect angle.
  • Conference paper
    Qureshi MNS, Pallocchia G, Bruno R, Cattaneo MB, Formisano V, Reme H, Bosqued JM, Dandouras I, Sauvaud JA, Kistler LM, Möbius E, Klecker B, Carlson CW, McFadden JP, Parks GK, McCarthy M, Korth A, Lundin R, Balogh A, Shah HAet al., 2003,

    , Pages: 489-492, ISSN: 0094-243X

    One of the major issues in space plasma physics is that in spite of the inhomogeneity of interplanetary plasma and the complicated magnetic field topology we do not find strong deviations from Maxwellian distributions as it would be expected for a quasi-collisionless plasma. However, the presence of high energy tail and shoulders in the profile of distribution function stimulate to look for a better analytic representation of the observed distributions. Therefore, here we adopt a non-Maxwellian distribution function such as the Ellipsian distribution function, which is the generalized form of the Kappa distribution function. In this paper we have analysed the solar wind data recorded by Cluster s/c during early 2001 and 2002 when the s/c were repeatedly immersed in the solar wind, ahead of the Earth's bow shock. Data were modeled with the help of the Ellipsian distribution function and values of the best fit parameters were successively used to characterize the solar wind kinetics at different locations of one of the four Cluster s/c.
  • Journal article
    Messnarz D, Jaritz N, Arcimowicz B, Zilio VO, Engleman R, Pickering JC, J盲ger H, Guth枚hrlein GH, Windholz Let al., 2003,

    , PHYSICA SCRIPTA, Vol: 68, Pages: 170-191, ISSN: 0031-8949
    • Cite
    • Citations: 19
  • Journal article
    V枚r枚s Z, Baumjohann W, Nakamura R, Runov A, Zhang TL, Volwerk M, Eichelberger HU, Balogh A, Horbury TS, Glassmeier KH, Klecker B, R猫me Het al., 2003,

    Multi-scale magnetic field intermittence in the plasma sheet

    , ANNALES GEOPHYSICAE, Vol: 21, Pages: 1955-1964, ISSN: 0992-7689
    • Cite
    • Citations: 60
  • Journal article
    Sergeev VA, Sauvaud JA, Reme H, Balogh A, Daly P, Zong QG, Angelopoulos V, Andre M, Vaivads Aet al., 2003,

    , GEOPHYSICAL RESEARCH LETTERS, Vol: 30, ISSN: 0094-8276
    • Cite
    • Citations: 14
  • Journal article
    Wild JA, Milan SE, Cowley SWH, Dunlop MW, Owen CJ, Bosqued JM, Taylor MGGT, Davies JA, Lester M, Sato N, Yukimatu AS, Fazakerley AN, Balogh A, R猫me Het al., 2003,

    , ANNALES GEOPHYSICAE, Vol: 21, Pages: 1807-1826, ISSN: 0992-7689
    • Cite
    • Citations: 40
  • Journal article
    Lanchester BS, Galand M, Robertson SC, Rees MH, Lummerzheim D, Furniss I, Peticolas LM, Frey HU, Baumgardner J, Mendillo Met al., 2003,

    , ANNALES GEOPHYSICAE, Vol: 21, Pages: 1629-1643, ISSN: 0992-7689
    • Cite
    • Citations: 12
  • Journal article
    Eastwood JP, Balogh A, Lucek EA, Mazelle C, Dandouras Iet al., 2003,

    , ANNALES GEOPHYSICAE, Vol: 21, Pages: 1457-1465, ISSN: 0992-7689
    • Cite
    • Citations: 52
  • Journal article
    Louarn P, Budnik E, Sauvaud JA, Parks G, Meziane K, Bosqued JM, Dandouras I, R猫me H, Mall U, Daly P, Dunlop M, Balogh A, Kistler LM, Amata Eet al., 2003,

    , ANNALES GEOPHYSICAE, Vol: 21, Pages: 1483-1495, ISSN: 0992-7689
  • Journal article
    Petrukovich AA, Baumjohann W, Nakamura R, Balogh A, Mukai T, Glassmeier KH, Reme H, Klecker Bet al., 2003,

    , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 108, ISSN: 2169-9380
    • Cite
    • Citations: 30
  • Journal article
    Runov A, Nakamura R, Baumjohann W, Treumann RA, Zhang TL, Volwerk M, V枚r枚s Z, Balogh A, Glassmeier KH, Klecker B, R猫me H, Kistler Let al., 2003,

    , GEOPHYSICAL RESEARCH LETTERS, Vol: 30, ISSN: 0094-8276
    • Cite
    • Citations: 245
  • Journal article
    Wahlund JE, Yilmaz A, Backrud M, Sundkvist D, Vaivads A, Winningham D, Andr茅 M, Balogh A, Bonnell J, Buchert S, Carozzi T, Cornilleau N, Dunlop M, Eriksson AI, Fazakerley A, Gustafsson G, Parrot M, Robert P, Tjulin Aet al., 2003,

    , GEOPHYSICAL RESEARCH LETTERS, Vol: 30, ISSN: 0094-8276
    • Cite
    • Citations: 25
  • Journal article
    McKibben RB, Connell JJ, Lopate C, Zhang M, Anglin JD, Balogh A, Dalla S, Sanderson TR, Marsden RG, Hofer MY, Kunow H, Posner A, Heber Bet al., 2003,

    , ANNALES GEOPHYSICAE, Vol: 21, Pages: 1217-1228, ISSN: 0992-7689
    • Cite
    • Citations: 63
  • Journal article
    Dalla S, Balogh A, Krucker S, Posner A, M眉ller-Mellin R, Anglin JD, Hofer MY, Marsden RG, Sanderson TR, Heber B, Zhang M, McKibben RBet al., 2003,

    , ANNALES GEOPHYSICAE, Vol: 21, Pages: 1367-1375, ISSN: 0992-7689
    • Cite
    • Citations: 37
  • Journal article
    Jones GH, Balogh A, 2003,

    , ANNALES GEOPHYSICAE, Vol: 21, Pages: 1377-1382, ISSN: 0992-7689
    • Cite
    • Citations: 10
  • Journal article
    Mozer FS, Phan TD, Bale SD, 2003,

    , PHYSICS OF PLASMAS, Vol: 10, Pages: 2480-2485, ISSN: 1070-664X
    • Cite
    • Citations: 14

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