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• Book chapter
  Horbury TS, Osman KT, 2008,

  Multi-Spacecraft Turbulence Analysis Methods

  , Multi-Spacecraft Analysis Methods Revisited, Editors: Paschmann, Daly, Noordwijk, Publisher: ESA Communications, Pages: 55-64
  • Cite
• Journal article
  Volwerk M, Zhang TL, Glassmeier KH, Runov A, Baumjohann W, Balogh A, Reme H, Klecker B, Carr Cet al., 2008,
  , ADVANCES IN SPACE RESEARCH, Vol: 41, Pages: 1593-1597, ISSN: 0273-1177
  • Cite
  • Citations: 8
• Conference paper
  Buchlin E, Cargill PJ, Bradshaw SJ, Velli Met al., 2008,

  Spectroscopic <i>Hinode</i> Observables from Turbulent Heating and Cooling of Coronal Loops

  , Workshop on First Results from Hinode, Publisher: ASTRONOMICAL SOC PACIFIC, Pages: 83-+
  • Cite
• Conference paper
  Culhane JL, Hara H, Watanabe T, Matsuzaki K, Harra LK, Cargill P, Mariska JT, Doschek GAet al., 2008,

  Long Duration Flare Observed with <i>Hinode</i> EIS

  , Workshop on First Results from Hinode, Publisher: ASTRONOMICAL SOC PACIFIC, Pages: 121-+
  • Cite
  • Citations: 1
• Journal article
  Huttunen KEJ, Bale SD, Salem C, 2008,
  , ANNALES GEOPHYSICAE, Vol: 26, Pages: 2701-2710, ISSN: 0992-7689
  • Cite
  • Citations: 14
• Journal article
  Roussos E, Mueller J, Simon S, Boesswetter A, Motschmann U, Krupp N, Fraenz M, Woch J, Khurana KK, Dougherty MKet al., 2008,
  , ANNALES GEOPHYSICAE, Vol: 26, Pages: 619-637, ISSN: 0992-7689
  • Cite
  • Citations: 49
• Journal article
  Billingham L, Schwartz SJ, Sibeck DG, 2008,

  The statistics of foreshock cavities: results of a Cluster survey

  , Annales Geophysicae, Vol: 26, Pages: 3653-3667

  We use Cluster magnetic field, thermal ion, and energetic particle observations upstream of the Earth's bow shock to investigate the occurrence patterns of foreshock cavities. Such cavities are thought to form when bundles of magnetic field connect to the quasi-parallel bow shock. Shock-processed suprathermal ions can then stream along the field, back against the flow of the solar wind. These suprathermals enhance the pressure on shock-connected field lines causing them to expand into the surrounding ambient solar wind plasma. Foreshock cavities exhibit depressions in magnetic field magnitude and thermal ion density, associated with enhanced fluxes of energetic ions. We find typical cavity duration to be few minutes with interior densities and magnetic field magnitudes dropping to ~60% of those in the surrounding solar wind. Cavities are found to occur preferentially in fast, moderate magnetic field strength solar wind streams. Cavities are observed in all parts of the Cluster orbit upstream of the bow shock. When localised in a coordinate system organised by the underlying physical processes in the foreshock, there is a systematic change in foreshock cavity location with IMF cone angle. At low (high) cone angles foreshock cavities are observed outside (inside) the expected upstream boundary of the intermediate ion foreshock.

  • Abstract
  • Cite
• Journal article
  Russell CT, Khurana KK, Arridge CS, Dougherty MKet al., 2008,
  , ADVANCES IN SPACE RESEARCH, Vol: 41, Pages: 1310-1318, ISSN: 0273-1177
  • Cite
  • Citations: 5
• Journal article
  Volwerk M, Nakamura R, Baumjohann W, Uozumi T, Yumoto K, Balogh Aet al., 2008,
  , ANNALES GEOPHYSICAE, Vol: 26, Pages: 4023-4030, ISSN: 0992-7689
  • Cite
  • Citations: 8
• Journal article
  Snowden D, Winglee R, Bertucci C, Dougherty Met al., 2007,
  , J GEOPHYS RES-SPACE, Vol: 112
  • Cite
• Journal article
  Southwood DJ, Kivelson MG, 2007,
  , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 112, ISSN: 2169-9380
  • Cite
  • Citations: 123
• Journal article
  Phan TD, Drake JF, Shay MA, Mozer FS, Eastwood JPet al., 2007,
  , PHYSICAL REVIEW LETTERS, Vol: 99, ISSN: 0031-9007
  • Cite
  • Citations: 156
• Journal article
  Haigh JD, 2007,
  , LIVING REVIEWS IN SOLAR PHYSICS, Vol: 4, ISSN: 2367-3648
  • Cite
  • Citations: 177
• Journal article
  Cox CV, Murray JE, Taylor JP, Green PD, Pickering JC, Harries JE, Last AEet al., 2007,
  , QUARTERLY JOURNAL OF THE ROYAL METEOROLOGICAL SOCIETY, Vol: 133, Pages: 273-283, ISSN: 0035-9009
  • Cite
  • Citations: 15
• Journal article
  Zhang TL, Delva M, Baumjohann W, Auster H-U, Carr C, Russell CT, Barabash S, Balikhin M, Kudela K, Berghofer G, Biernat HK, Lammer H, Lichtenegger H, Magnes W, Nakamura R, Schwingenschuh K, Volwerk M, Voros Z, Zambelli W, Fornacon K-H, Glassmeier K-H, Richter I, Balogh A, Schwarzl H, Pope SA, Shi JK, Wang C, Motschmann U, Lebreton J-Pet al., 2007,
  , NATURE, Vol: 450, Pages: 654-656, ISSN: 0028-0836
  • Cite
  • Citations: 76
• Journal article
  Stallard T, Smith C, Miller S, Melin H, Lystrup M, Aylward A, Achilleos N, Dougherty Met al., 2007,
  , ICARUS, Vol: 191, Pages: 678-690, ISSN: 0019-1035
  • Cite
  • Citations: 26
• Journal article
  Bertucci C, Neubauer FM, Szego K, Wahlund J-E, Coates AJ, Dougherty MK, Young DT, Kurth WSet al., 2007,
  , GEOPHYSICAL RESEARCH LETTERS, Vol: 34, ISSN: 0094-8276
  • Cite
  • Citations: 31
• Journal article
  Wei HY, Russell CT, Wahlund J-E, Dougherty MK, Bertucci C, Modolo R, Ma YJ, Neubauer FMet al., 2007,
  , GEOPHYSICAL RESEARCH LETTERS, Vol: 34, ISSN: 0094-8276
  • Cite
  • Citations: 25
• Journal article
  O'Brien H, Brown P, Beek T, Carr C, Cupido E, Oddy Tet al., 2007,
  , MEASUREMENT SCIENCE AND TECHNOLOGY, Vol: 18, Pages: 3645-3650, ISSN: 0957-0233
  • Cite
  • Citations: 26
• Journal article
  Wei XH, Cao JB, Zhou GC, Santolik O, Reme H, Dandouras I, Cornilleau-Wehrlin N, Lucek E, Carr CM, Fazakerley Aet al., 2007,
  , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 112, ISSN: 2169-9380
  • Cite
  • Citations: 104
• Journal article
  Petrukovich AA, Baumjohann W, Nakamura R, Runov A, Balogh A, Reme Het al., 2007,
  , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 112, ISSN: 2169-9380
  • Cite
  • Citations: 75
• Journal article
  Pu ZY, Zhang XG, Wang XG, Wang J, Zhou X-Z, Dunlop MW, Xie L, Xiao CJ, Zong QG, Fu SY, Liu ZX, Carr C, Ma ZW, Shen C, Lucek E, Reme H, Escoubet Pet al., 2007,
  , GEOPHYSICAL RESEARCH LETTERS, Vol: 34, ISSN: 0094-8276
  • Cite
  • Citations: 66
• Journal article
  Simon S, Kleindienst G, Boesswetter A, Bagdonat T, Motschmann U, Glassmeier K-H, Schuele J, Bertucci C, Dougherty MKet al., 2007,
  , GEOPHYSICAL RESEARCH LETTERS, Vol: 34, ISSN: 0094-8276
  • Cite
  • Citations: 30
• Journal article
  Bunce EJ, Cowley SWH, Alexeev II, Arridge CS, Dougherty MK, Nichols JD, Russell CTet al., 2007,
  , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 112, ISSN: 2169-9380
  • Cite
  • Citations: 112
• Journal article
  Haigh JD, 2007,

  The Sun and the Earth’s Climate

  , Living Reviews in Solar Physics, Vol: 4, ISSN: 1614-4961
  • Cite
• Journal article
  Roscoe HK, Haigh JD, 2007,
  , QUARTERLY JOURNAL OF THE ROYAL METEOROLOGICAL SOCIETY, Vol: 133, Pages: 1855-1864, ISSN: 0035-9009
  • Cite
  • Citations: 62
• Journal article
  Matteini L, Landi S, Hellinger P, Pantellini F, Maksimovic M, Velli M, Goldstein BE, Marsch Eet al., 2007,
  , Geophysical Research Letters, Vol: 34, ISSN: 0094-8276

  <jats:p>We report an analysis of the proton temperature anisotropy evolution from 0.3 to 2.5 AU based on the Helios and Ulysses observations. With increasing distance the fast wind data show a path in the parameter space (<jats:italic>β</jats:italic><jats:sub>∥<jats:italic>p</jats:italic></jats:sub>, <jats:italic>T</jats:italic><jats:sub>⊥<jats:italic>p</jats:italic></jats:sub>/<jats:italic>T</jats:italic><jats:sub>∥<jats:italic>p</jats:italic></jats:sub>). The first part of the trajectory is well described by an anticorrelation between the temperature anisotropy <jats:italic>T</jats:italic><jats:sub>⊥<jats:italic>p</jats:italic></jats:sub>/<jats:italic>T</jats:italic><jats:sub>∥<jats:italic>p</jats:italic></jats:sub> and the proton parallel beta, while after 1 AU the evolution with distance in the parameter space changes and the data result in agreement with the constraints derived by a fire hose instability. The slow wind data show a more irregular behavior, and in general it is not possible to recover a single evolution path. However, on small temporal scale we find that different slow streams populate different regions of the parameter space, and this suggests that when considering single streams also the slow wind follows some possible evolution path.</jats:p>

  • Abstract
  • Cite
• Journal article
  Bertucci C, Achilleos N, Mazelle C, Hospodarsky GB, Thomsen M, Dougherty MK, Kurth Wet al., 2007,
  , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 112, ISSN: 2169-9380
  • Cite
  • Citations: 20
• Journal article
  Brindley HE, 2007,
  , Atmospheric Science Letters, Vol: 8, Pages: 74-79

  This paper presents a methodology for estimating the longwave top-of-atmosphere direct radiative forcing due to Saharan dust aerosol from satellite observations made by the Spinning Enhanced Visible and InfraRed Imager (SEVIRI) and Geostationary Earth Radiation Budget (GERB) instruments. Narrow-band observations from SEVIRI are used to detect dust presence and quantify its loading, while GERB provides an estimate of the dust impact on the total outgoing longwave radiation. Applying the technique to observations made over the Banizoumbou surface station in Niger through March-June 2006 indicates a midday longwave forcing efficiency of 17 ± 5 W m-2 per unit aerosol optical depth.

  • Abstract
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• Journal article
  Eastwood JP, Bale SD, Mozer FS, Hull AJet al., 2007,
  , GEOPHYSICAL RESEARCH LETTERS, Vol: 34, ISSN: 0094-8276
  • Cite
  • Citations: 11

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