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Journal articleYamauchi M, Brandt PC, Ebihara Y, et al., 2006,
Source location of the wedge-like dispersed ring current in the morning sector during a substorm
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 111, ISSN: 2169-9380- Author Web Link
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- Citations: 22
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Journal articleTakada T, Nakamura R, Baumjohann W, et al., 2006,
Do BBFs contribute to inner magnetosphere dipolarizations:: Concurrent Cluster and Double Star observations
, GEOPHYSICAL RESEARCH LETTERS, Vol: 33, ISSN: 0094-8276- Author Web Link
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- Citations: 52
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Journal articleParenti S, Buchlin E, Cargill PJ, et al., 2006,
Modeling the radiative signatures of turbulent heating in coronal loops
, ASTROPHYSICAL JOURNAL, Vol: 651, Pages: 1219-1228, ISSN: 0004-637X- Author Web Link
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- Citations: 39
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Journal articleJones GH, Krupp N, Krueger H, et al., 2006,
Formation of Saturn's ring spokes by lightning-induced electron beams
, GEOPHYSICAL RESEARCH LETTERS, Vol: 33, ISSN: 0094-8276- Author Web Link
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- Citations: 23
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Journal articleWeygand JM, Kivelson MG, Khurana KK, et al., 2006,
Non-self-similar scaling of plasma sheet and solar wind probability distribution functions of magnetic field fluctuations
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 111, ISSN: 2169-9380- Author Web Link
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- Citations: 15
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Journal articleNakamura R, Baumjohann W, Asano Y, et al., 2006,
Dynamics of thin current sheets associated with magnetotail reconnection
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 111, ISSN: 2169-9380- Author Web Link
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- Citations: 101
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Journal articleGaland M, Yelle RV, Coates AJ, et al., 2006,
Electron temperature of Titan's sunlit ionosphere
, GEOPHYSICAL RESEARCH LETTERS, Vol: 33, ISSN: 0094-8276- Author Web Link
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- Citations: 61
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Journal articleBradshaw SJ, Cargill PJ, 2006,
Explosive heating of low-density coronal plasma
, ASTRONOMY & ASTROPHYSICS, Vol: 458, Pages: 987-995, ISSN: 0004-6361- Author Web Link
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- Citations: 78
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Journal articleMuller-Wodarg ICF, Forbes JM, Keating GM, 2006,
The thermosphere of Venus and its exploration by a Venus Express Accelerometer Experiment
, PLANETARY AND SPACE SCIENCE, Vol: 54, Pages: 1415-1424, ISSN: 0032-0633- Author Web Link
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- Citations: 10
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Journal articleZhang TL, Baumjohann W, Delva M, et al., 2006,
Magnetic field investigation of the Venus plasma environment:: Expected new results from Venus Express
, PLANETARY AND SPACE SCIENCE, Vol: 54, Pages: 1336-1343, ISSN: 0032-0633- Author Web Link
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- Citations: 205
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Journal articleBrindley HE, Russell JE, 2006,
Improving GERB scene identification using SEVIRI: Infrared dust detection strategy
, REMOTE SENSING OF ENVIRONMENT, Vol: 104, Pages: 426-446, ISSN: 0034-4257- Author Web Link
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- Citations: 29
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Journal articleKokorowski M, Sample JG, Holzworth RH, et al., 2006,
Rapid fluctuations of stratospheric electric field following a solar energetic particle event
, GEOPHYSICAL RESEARCH LETTERS, Vol: 33, ISSN: 0094-8276- Author Web Link
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- Citations: 25
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Journal articleRees A, Balogh A, Horbury TS, 2006,
Small-scale solitary wave pulses observed by the Ulysses magnetic field experiment
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 111, ISSN: 2169-9380- Author Web Link
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- Citations: 9
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Journal articleNeubauer FM, Backes H, Dougherty MK, et al., 2006,
Titan's near magnetotail from magnetic field and electron plasma observations and modeling: Cassini flybys TA, TB, and T3
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 111, ISSN: 2169-9380- Author Web Link
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- Citations: 79
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Conference paperCarr CM, Horbury TS, Balogh A, et al., 2006,
A magnetometer for the Solar Orbiter Mission
, ISSN: 0379-6566The magnetometer is a key instrument to the Solar Orbiter mission. The magnetic field is a fundamental parameter in any plasma: a precise and accurate measurement of the field is essential for understanding almost all aspects of plasma dynamics such as shocks and stream-stream interactions. Many of Solar Orbiter's mission goals are focussed around the links between the Sun and space. A combination of in situ measurements by the magnetometer, remote measurements of solar magnetic fields and global modelling is required to determine this link and hence how the Sun affects interplanetary space. The magnetic field is typically one of the most precisely measured plasma parameters and is therefore the most commonly used measurement for studies of waves, turbulence and other small scale phenomena. It is also related to the coronal magnetic field which cannot be measured directly. Accurate knowledge of the magnetic field is essential for the calculation of fundamental plasma parameters such as the plasma beta, Alfven speed and gyroperiod. We describe here the objectives and context of magnetic field measurements on Solar Orbiter and an instrument that fulfils those objectives as defined by the scientific requirements for the mission.
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Conference paperHorbury T, 2006,
Turbulence in the Solar wind - Prospects for Solar Orbiter
, ISSN: 0379-6566Solar Orbiter will, among many other advances, provide us with unique measurements of waves and turbulence in the inner heliosphere. We discuss expectations of conditions over the orbit of the spacecraft that are relevant to turbulence studies, such as solar wind speeds and Alfven Mach number, based on earlier Helios data. We describe some of the topics within solar wind turbulence research that the mission will address, as well as some of the challenges that will be faced.
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Journal articleMatteini L, Landi S, Hellinger P, et al., 2006,
Parallel proton fire hose instability in the expanding solar wind: Hybrid simulations
, Journal of Geophysical Research: Space Physics, Vol: 111, ISSN: 0148-0227<jats:p>We report a study of the properties of the parallel proton fire hose instability comparing the results obtained by the linear analysis, from one‐dimensional (1‐D) standard hybrid simulations and 1‐D hybrid expanding box simulations. The three different approaches converge toward the same instability threshold condition which is in good agreement with in situ observations, suggesting that such instability is relevant in the solar wind context. We investigate also the effect of the wave‐particle interactions on shaping the proton distribution function and on the evolution of the spectrum of the magnetic fluctuations during the expansion. We find that the resonant interaction can provide the proton distribution function to depart from the bi‐Maxwellian form.</jats:p>
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Journal articleMoullard O, Burgess D, Horbury TS, et al., 2006,
Ripples observed on the surface of the Earth's quasi-perpendicular bow shock
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 111, ISSN: 2169-9380- Author Web Link
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- Citations: 43
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Journal articleCattaneo MBB, Marcucci MF, Retino A, et al., 2006,
Kinetic signatures during a quasi-continuous lobe reconnection event:: Cluster Ion Spectrometer (CIS) observations
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 111, ISSN: 2169-9380- Author Web Link
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- Citations: 14
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Journal articleOsborne DR, Vassilicos JC, Sung K, et al., 2006,
Fundamentals of pair diffusion in kinematic simulations of turbulence
, PHYSICAL REVIEW E, Vol: 74, ISSN: 2470-0045- Author Web Link
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- Citations: 28
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Journal articleGaland M, Chakrabarti S, 2006,
Proton aurora observed from the ground
, JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, Vol: 68, Pages: 1488-1501, ISSN: 1364-6826- Author Web Link
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- Citations: 20
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Journal articleBlyth E, Evans J, Finch J, et al., 2006,
Spatial variability of the English agricultural landscape and its effect on evaporation
, Agricultural and Forest Meteorology, Vol: 138, Pages: 19-28The variability of leaf area index, canopy height and albedo is measured across an agricultural landscape in lowland Britain. The dependency of the variability with spatial sampling is quantified and the sensitivity of modelled evaporation to the variability is assessed. From this study, it appears that the leaf area index can display significant variability between fields of growing crops as their plant and harvest times may differ by the order of a month. In addition the albedo variability is high. Both these quantities have an influence on the resulting evaporation (between 1% and 40% depending on assumptions) and need to be accounted for. Although the crop height varies considerably, it does not have a big impact on evaporation (less than 4%).
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Journal articleHull AJ, Larson DE, Wilber M, et al., 2006,
Large-amplitude electrostatic waves associated with magnetic ramp substructure at Earth's bow shock
, GEOPHYSICAL RESEARCH LETTERS, Vol: 33, ISSN: 0094-8276- Author Web Link
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- Citations: 32
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Journal articleKrueger H, Graps AL, Hamilton DP, et al., 2006,
Ulysses jovian latitude scan of high-velocity dust streams originating from the jovian system
, PLANETARY AND SPACE SCIENCE, Vol: 54, Pages: 919-931, ISSN: 0032-0633- Author Web Link
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- Citations: 21
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Journal articleJaritz N, Windholz L, Zaheer U, et al., 2006,
Investigation of the hyperfine structure of TaI lines (X)
, PHYSICA SCRIPTA, Vol: 74, Pages: 211-217, ISSN: 0031-8949- Author Web Link
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- Citations: 5
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Journal articleRoth I, Bale SD, 2006,
Heliospheric ion energization due to emerging CME shocks
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 111, ISSN: 2169-9380- Author Web Link
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- Citations: 2
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Journal articleKellogg PJ, Bale SD, Mozer FS, et al., 2006,
Solar wind electric fields in the ion cyclotron frequency range
, ASTROPHYSICAL JOURNAL, Vol: 645, Pages: 704-710, ISSN: 0004-637X- Author Web Link
- Open Access Link
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- Citations: 22
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Journal articleXiao CJ, Wang XG, Pu ZY, et al., 2006,
<i>In situ</i> evidence for the structure of the magnetic null in a 3D reconnection event in the Earth'smagnetotail
, NATURE PHYSICS, Vol: 2, Pages: 478-483, ISSN: 1745-2473- Author Web Link
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- Citations: 108
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Journal articleBrindley HE, Ignatov A, 2006,
Retrieval of mineral aerosol optical depth and size information from Meteosat Second Generation SEVIRI solar reflectance bands
, REMOTE SENSING OF ENVIRONMENT, Vol: 102, Pages: 344-363, ISSN: 0034-4257- Author Web Link
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- Citations: 31
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Journal articleGosling JT, Eriksson S, Skoug RM, et al., 2006,
Petschek-type reconnection exhausts in the solar wind well beyond 1 AU:: <i>ULYSSES</i>
, ASTROPHYSICAL JOURNAL, Vol: 644, Pages: 613-621, ISSN: 0004-637X- Author Web Link
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- Citations: 65
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