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• Journal article
  Maynard NC, Moen J, Burke WJ, Lester M, Ober DM, Scudder JD, Siebert KD, Weimer DR, Russe CT, Balogh Aet al., 2004,

  Temporal-spatial structure of magnetic merging at the magnetopause inferred from 557.7-nm all-sky images

  , ANNALES GEOPHYSICAE, Vol: 22, Pages: 2917-2942, ISSN: 0992-7689
  • Cite
  • Citations: 5
• Conference paper
  Kucharek H, Möbius E, Scholer M, Mouikis C, Kistler LM, Horbury T, Balogh A, Réme H, Bosqued JMet al., 2004,

  On the origin of field-aligned beams at the quasi-perpendicular bow shock: multi-spacecraft observations by Cluster

  , Meeting on Spatio-Temporal Analysis and Multipoint Measurements in Space, Publisher: COPERNICUS GESELLSCHAFT MBH, Pages: 2301-2308, ISSN: 0992-7689
  • Cite
  • Citations: 64
• Journal article
  Moore LE, Mendillo M, Muller-Wodarg ICF, Murr DLet al., 2004,

  Modeling of global variations and ring shadowing in Saturn's ionosphere

  , ICARUS, Vol: 172, Pages: 503-520, ISSN: 0019-1035
  • Cite
• Conference paper
  Sigsbee K, Kletzing CA, Gurnett DA, Pickett JS, Balogh A, Lucek Eet al., 2004,

  Statistical behavior of foreshock Langmuir waves observed by the Cluster wideband data plasma wave receiver

  , Meeting on Spatio-Temporal Analysis and Multipoint Measurements in Space, Publisher: COPERNICUS GESELLSCHAFT MBH, Pages: 2337-2344, ISSN: 0992-7689
  • Cite
  • Citations: 9
• Conference paper
  Phan TD, Dunlop MW, Paschmann G, Klecker B, Bosqued JM, Rème H, Balogh A, Twitty C, Mozer FS, Carlson CW, Mouikis C, Kistler LMet al., 2004,

  Cluster observations of continuous reconnection at the magnetopause under steady interplanetary magnetic field conditions

  , Meeting on Spatio-Temporal Analysis and Multipoint Measurements in Space, Publisher: COPERNICUS GESELLSCHAFT MBH, Pages: 2355-2367, ISSN: 0992-7689
  • Cite
  • Citations: 120
• Journal article
  Cargill PJ, Dunlop MW, Lavraud B, Elphic RC, Holland DL, Nykyri K, Balogh A, Dandouras I, Rème Het al., 2004,

  CLUSTER encounters with the high altitude cusp: boundary structure and magnetic field depletions

  , ANNALES GEOPHYSICAE, Vol: 22, Pages: 1739-1754, ISSN: 0992-7689
  • Cite
  • Citations: 34
• Journal article
  Owens M, Cargill P, 2004,

  Predictions of the arrival time of Coronal Mass Ejections at 1 AU: an analysis of the causes of errors

  , ANNALES GEOPHYSICAE, Vol: 22, Pages: 661-671, ISSN: 0992-7689
  • Cite
  • Citations: 66
• Journal article
  Meziane K, Mazelle C, Wilber M, LeQueau D, Eastwood JP, Reme H, Dandouras I, Sauvaud JA, Bosqued JM, Parks GK, Kistler LM, McCarthy M, Klecker B, Korth A, Bavassano-Cattaneo MB, Lundin R, Balogh Aet al., 2004,

  Bow shock specularly reflected ions in the presence of low-frequency electromagnetic waves: a case study

  , Annales Geophysicae, Vol: 22, Pages: 2325-2335

  An energetic ion (E less than or equal to40 keV) event observed by the CLUSTER/CIS experiment upstream of the Earth's bow shock is studied in detail. The ion event is observed in association with quasi-monochromatic ULF MHD-like waves, which we show modulate the ion fluxes. According to three statistical bow shock position models, the Cluster spacecrafts are located at similar to0.5 R-E from the shock and the averaged bow shock theta(Bno) is about similar to30degrees. The analysis of the three-dimensional angular distribution indicates that ions propagating roughly along the magnetic field direction are observed at the onset of the event. Later on, the angular distribution is gyrophase-bunched and the pitch-angle distribution is peaked at alpha(o)similar totheta(Bno), consistent with the specular reflection production mechanism. The analysis of the waves shows that they are left-handed in the spacecraft frame of reference (right-handed in the solar wind frame) and propagate roughly along the ambient magnetic field; we have found that they are in cyclotron-resonance with the field-aligned beam observed just upstream. Using properties of the waves and particles, we explain the observed particle flux-modulation in the context Of theta(Bn) changes at the shock caused by the convected ULF waves. We have found that the high count rates coincide with particles leaving the shock when theta(Bn) angles are less than similar to40degrees, consistent with the specular reflection hypothesis as the production mechanism of ions.

  • Abstract
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• Journal article
  Haaland SE, Sonnerup B, Dunlop MW, Balogh A, Georgescu E, Hasegawa H, Klecker B, Paschmann G, Puhl-Quinn P, Rème H, Vaith H, Vaivads Aet al., 2004,

  Four-spacecraft determination of magnetopause orientation, motion and thickness: comparison with results from single-spacecraft methods

  , ANNALES GEOPHYSICAE, Vol: 22, Pages: 1347-1365, ISSN: 0992-7689
  • Cite
  • Citations: 94
• Journal article
  Sahraoui F, Belmont G, Pinçon JL, Rezeau L, Balogh A, Robert P, Cornilleau-Wehrlin Net al., 2004,

  Magnetic turbulent spectra in the magnetosheath: new insights

  , ANNALES GEOPHYSICAE, Vol: 22, Pages: 2283-2288, ISSN: 0992-7689
  • Cite
  • Citations: 67
• Journal article
  Hasegawa H, Sonnerup B, Dunlop MW, Balogh A, Haaland SE, Klecker B, Paschmann G, Lavraud B, Dandouras I, Rème Het al., 2004,

  Reconstruction of two-dimensional magnetopause structures from Cluster observations: verification of method

  , ANNALES GEOPHYSICAE, Vol: 22, Pages: 1251-1266, ISSN: 0992-7689
  • Cite
  • Citations: 78
• Conference paper
  Pickett JS, Kahler SW, Chen LJ, Huff RL, Santolík O, Khotyaintsev Y, Décréau PM, Winningham D, Frahm R, Goldstein ML, Lakhina GS, Tsurutani BT, Lavraud B, Gurnett DA, André M, Fazakerley A, Balogh A, Rème Het al., 2004,

  Solitary waves observed in the auroral zone: the Cluster multi-spacecraft perspective

  , 5th International Workshops on Nonlinear Waves and Chaos in Space Plasmas, Publisher: COPERNICUS GESELLSCHAFT MBH, Pages: 183-196, ISSN: 1023-5809
  • Cite
  • Citations: 96
• Report
  Allen AJ, Schwartz SJ, Harvey C, Perry C, Huc C, Robert Pet al., 2004,

  Cluster exchange format - data file syntax

  , DSQMWTN0010
  • Cite
• Journal article
  Bale SD, Mozer FS, Horbury TS, 2003,

  Density-transition scale at quasiperpendicular collisionless shocks

  , PHYSICAL REVIEW LETTERS, Vol: 91, ISSN: 0031-9007
  • Author Web Link
  • Cite
  • Citations: 79
• Journal article
  Nykyri K, Cargill PJ, Lucek EA, Horbury TS, Balogh A, Lavraud B, Dandouras I, Rème Het al., 2003,

  Ion cyclotron waves in the high altitude cusp:: CLUSTER observations at varying spacecraft separations -: art. no. 2263

  , GEOPHYSICAL RESEARCH LETTERS, Vol: 30, ISSN: 0094-8276
  • Author Web Link
  • Cite
  • Citations: 35
• Journal article
  Mozer FS, Bale SD, Phan TD, Osborne JAet al., 2003,

  Observations of electron diffusion regions at the subsolar magnetopause

  , PHYSICAL REVIEW LETTERS, Vol: 91, ISSN: 0031-9007
  • Author Web Link
  • Cite
  • Citations: 39
• Journal article
  Slavin JA, Owen CJ, Dunlop MW, Borälv E, Moldwin MB, Sibeck DG, Tanskanen E, Goldstein ML, Fazakerley A, Balogh A, Lucek E, Richter I, Reme H, Bosqued JMet al., 2003,

  Cluster four spacecraft measurements of small traveling compression regions in the near-tail - art. no. 2208

  , GEOPHYSICAL RESEARCH LETTERS, Vol: 30, ISSN: 0094-8276
  • Cite
  • Citations: 38
• Journal article
  Volwerk M, Nakamura R, Baumjohann W, Treumann RA, Runov A, Vörös Z, Zhang TL, Asano Y, Klecker B, Richter I, Balogh A, Rème Het al., 2003,

  A statistical study of compressional waves in the tail current sheet - art. no. 1429

  , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 108, ISSN: 2169-9380
  • Cite
  • Citations: 39
• Journal article
  Fitzenreiter RJ, Ogilvie KW, Bale SD, Viñas AFet al., 2003,

  Modification of the solar wind electron velocity distribution at interplanetary shocks - art. no. 1415

  , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 108, ISSN: 2169-9380
  • Cite
  • Citations: 22
• Conference paper
  Da Silva Curiel A, Meerman M, Liddle D, Schwartz S, Underwood C, Sweeting Met al., 2003,

  FRISBEE - A platform for a small satellite science swarms

  , Pages: 3671-3678

  The FRISBEE multi-mission platform is presented, alongside the mission concept for SWARM (Space Weather Advanced Research Mission), a fleet of 30 or more microsatellites launched in groups of 5 and covering a range of local times and inclinations. The aim of this mission is to develop an understanding of the dynamic, global, and multiscale solar terrestrial interactions. The scientific payload is restricted to a dc magnetometer and electrostatic charged particle (ion and electron) analyser, providing both high time resolution and characterisation of collisionless plasma processes, together with a miniaturised radiation environment monitor, CEDEX-2, to measure total-ionising radiation dose and the higher energy protons and heavy ions associated with single-event-effect activity. The baseline satellite swarm can be launched in a variety of configurations and be augmented by future launches of identical satellites to provide greater coverage and density of measurement. The satellites require only loose formation control to ensure equal separation throughout the set of orbits defined in this document. The individual satellites are spin stabilized and each have a mass < 25 kg.

  • Abstract
  • Cite
  • Citations: 1
• Conference paper
  Hodgson E, Sidgreaves R, Braham S, Hoffman J, Carr C, Lee P, Marmolejo J, Miller J, Rosenberg I, Schwartz Set al., 2003,

  Requirements and potential for enhanced EVA information interfaces

  NASA has long recognized the advantages of providing improved information interfaces to EVA astronauts and has pursued this goal through a number of development programs over the past decade. None of these activities or parallel efforts in industry and academia has so far resulted in the development of an operational system to replace or augment the current extravehicular mobility unit (EMU) Display and Controls Module (DCM) display and cuff checklist. Recent advances in display, communications, and information processing technologies offer exciting new opportunities for EVA information interfaces that can better serve the needs of a variety of NASA missions. Hamilton Sundstrand Space Systems International (HSSSI) has been collaborating with Simon Fraser University and others on the NASA Haughton Mars Project and with researchers at the Massachusetts Institute of Technology (MIT), Boeing, and Symbol Technologies in investigating these possibilities. The objectives of this research so far have been to better understand the ways in which an improved information interface may be applied in a variety of mission settings and to refine the definition of system design requirements to best support those applications. Research efforts have combined the results of concept definition and mission requirements studies with experiments in pressurized spacesuits in the laboratory and in lower fidelity test-beds in field settings. Several promising approaches for the integration of highly capable information interfaces with EVA systems have evolved and have been evaluated in preliminary proof-of-concept tests. The results show considerable promise that an advanced information interface could be adapted to support near-term orbital EVA missions and could be evolved to provide robust support for future planetary exploration missions. Copyright © 2003 Hamilton Sundstrand Space Systems International, Inc.

  • Abstract
  • Cite
  • Citations: 4
• Journal article
  Cui HL, Jin SP, Liu SL, Liu ZX, Balogh Aet al., 2003,

  Observation and simulation of flux rope structures at the dayside magnetopause

  , CHINESE SCIENCE BULLETIN, Vol: 48, Pages: 2634-2639, ISSN: 1001-6538
  • Author Web Link
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• Journal article
  Jones GH, Balogh A, McComas DJ, MacDowall RJet al., 2003,

  Strong interplanetary field enhancements at Ulysses - evidence of dust trails' interaction with the solar wind?

  , ICARUS, Vol: 166, Pages: 297-310, ISSN: 0019-1035
  • Cite
  • Citations: 16
• Journal article
  Maynard NC, Ober DM, Burke WJ, Scudder JD, Lester M, Dunlop M, Wild JA, Grocott A, Farrugia CJ, Lund EJ, Russell CT, Weimer DR, Siebert KD, Balogh A, Andre M, Rème Het al., 2003,

  Polar, Cluster and SuperDARN evidence for high-latitude merging during southward IMF: temporal/spatial evolution

  , ANNALES GEOPHYSICAE, Vol: 21, Pages: 2233-2258, ISSN: 0992-7689
  • Cite
  • Citations: 22
• Conference paper
  Sandford MCW, Allan PM, Caldwell ME, Delderfield J, Oliver MB, Sawyer E, Harries JE, Ashmall J, Brindley H, Kellock S, Mossavati R, Wrigley R, Llewellyn-Jones D, Blake O, Butcher G, Cole R, Nelms N, DeWitte S, Gloesener P, Fabbrizzi Fet al., 2003,

  The geostationary Earth radiation budget (GERB) instrument on EUMETSAT's MSG satellite

  , 51st International Astronautical Congress, Publisher: PERGAMON-ELSEVIER SCIENCE LTD, Pages: 909-915, ISSN: 0094-5765
  • Author Web Link
  • Cite
  • Citations: 5
• Journal article
  Smith EJ, Marsden RG, Balogh A, Gloeckler G, Geiss J, McComas DJ, McKibben RB, MacDowall RJ, Lanzerotti LJ, Krupp N, Krueger H, Landgraf Met al., 2003,

  The Sun and heliosphere at solar maximum

  , SCIENCE, Vol: 302, Pages: 1165-1169, ISSN: 0036-8075
  • Cite
  • Citations: 61
• Journal article
  Jones GH, Balogh A, Russell CT, Dougherty MKet al., 2003,

  Possible distortion of the interplanetary magnetic field by the dust trail of comet 122P/de Vico

  , ASTROPHYSICAL JOURNAL, Vol: 597, Pages: L61-L64, ISSN: 0004-637X
  • Author Web Link
  • Cite
  • Citations: 12
• Journal article
  Kivelson MG, Southwood DJ, 2003,

  First evidence of IMF control of Jovian magnetospheric boundary locations: Cassini and Galileo magnetic field measurements compared

  , PLANETARY AND SPACE SCIENCE, Vol: 51, Pages: 891-898, ISSN: 0032-0633
  • Author Web Link
  • Cite
  • Citations: 16
• Journal article
  Brindley HE, Harries JE, 2003,

  Observations of the infrared outgoing spectrum of the Earth from space: The effects of temporal and spatial sampling

  , JOURNAL OF CLIMATE, Vol: 16, Pages: 3820-3833, ISSN: 0894-8755
  • Author Web Link
  • Cite
  • Citations: 10
• Journal article
  Cheung ASC, Wong AL, Lo DHY, Leung KWS, Yoshino K, Thorne AP, Murray JE, Imajo T, Ito K, Matsui Tet al., 2003,

  Application of a VUV Fourier transform spectrometer and synchrotron radiation source to measurements of.: VI.: The ε(0,0) band of NO

  , JOURNAL OF CHEMICAL PHYSICS, Vol: 119, Pages: 8373-8378, ISSN: 0021-9606
  • Author Web Link
  • Cite
  • Citations: 9

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