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Journal articleKanani SJ, Arridge CS, Jones GH, et al., 2010,
A new form of Saturn's magnetopause using a dynamic pressure balance model, based on in situ, multi-instrument Cassini measurements
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 115, ISSN: 2169-9380- Author Web Link
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- Citations: 139
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Journal articleOmidi N, Eastwood JP, Sibeck DG, 2010,
Foreshock bubbles and their global magnetospheric impacts
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 115, ISSN: 2169-9380- Author Web Link
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- Citations: 110
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Conference paperLyons JR, Stark G, Blackie D, et al., 2010,
High-resolution <SUP>x</SUP>SO<sub>2</sub> spectra, and sulfur MIF due to SO<sub>2</sub> photolysis
, Conference on Goldschmidt 2010 - Earth, Energy, and the Environment, Publisher: PERGAMON-ELSEVIER SCIENCE LTD, Pages: A648-A648, ISSN: 0016-7037- Author Web Link
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- Citations: 1
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Journal articlePauluis O, Czaja A, Korty R, 2010,
The Global Atmospheric Circulation in Moist Isentropic Coordinates
, JOURNAL OF CLIMATE, Vol: 23, Pages: 3077-3093, ISSN: 0894-8755- Author Web Link
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- Citations: 79
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Journal articleEgedal J, Le A, Zhu Y, et al., 2010,
Cause of super-thermal electron heating during magnetotail reconnection
, GEOPHYSICAL RESEARCH LETTERS, Vol: 37, ISSN: 0094-8276- Author Web Link
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- Citations: 35
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Journal articleEastwood JP, Shay MA, Phan TD, et al., 2010,
Asymmetry of the Ion Diffusion Region Hall Electric and Magnetic Fields during Guide Field Reconnection: Observations and Comparison with Simulations
, PHYSICAL REVIEW LETTERS, Vol: 104, ISSN: 0031-9007- Author Web Link
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- Citations: 84
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Journal articleOwens MJ, Horbury TS, Arge CN, 2010,
PROBING THE LARGE-SCALE TOPOLOGY OF THE HELIOSPHERIC MAGNETIC FIELD USING JOVIAN ELECTRONS
, ASTROPHYSICAL JOURNAL, Vol: 714, Pages: 1617-1623, ISSN: 0004-637X- Author Web Link
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- Citations: 6
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Journal articleJia Y-D, Russell CT, Khurana KK, et al., 2010,
Time-varying magnetospheric environment near Enceladus as seen by the Cassini magnetometer
, GEOPHYSICAL RESEARCH LETTERS, Vol: 37, ISSN: 0094-8276- Author Web Link
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- Citations: 18
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Journal articleClarke KE, Andrews DJ, Coates AJ, et al., 2010,
Magnetospheric period oscillations of Saturn's bow shock
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 115, ISSN: 2169-9380- Author Web Link
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- Citations: 32
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Journal articleKopf AJ, Gurnett DA, Menietti JD, et al., 2010,
Electron beams as the source of whistler-mode auroral hiss at Saturn
, GEOPHYSICAL RESEARCH LETTERS, Vol: 37, ISSN: 0094-8276- Author Web Link
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- Citations: 27
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Journal articlePerri S, Balogh A, 2010,
STATIONARITY IN SOLAR WIND FLOWS
, ASTROPHYSICAL JOURNAL, Vol: 714, Pages: 937-943, ISSN: 0004-637X- Author Web Link
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- Citations: 32
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Journal articleSavani NP, Owens MJ, Rouillard AP, et al., 2010,
OBSERVATIONAL EVIDENCE OF A CORONAL MASS EJECTION DISTORTION DIRECTLY ATTRIBUTABLE TO A STRUCTURED SOLAR WIND
, ASTROPHYSICAL JOURNAL LETTERS, Vol: 714, Pages: L128-L132, ISSN: 2041-8205- Author Web Link
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- Citations: 83
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Journal articleBalogh A, 2010,
Planetary Magnetic Field Measurements: Missions and Instrumentation
, SPACE SCIENCE REVIEWS, Vol: 152, Pages: 23-97, ISSN: 0038-6308- Author Web Link
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- Citations: 54
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Journal articleSator N, Hietala H, 2010,
Damage in impact fragmentation
, INTERNATIONAL JOURNAL OF FRACTURE, Vol: 163, Pages: 101-108, ISSN: 0376-9429- Author Web Link
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- Citations: 20
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Journal articleRussell CT, Dougherty MK, 2010,
Magnetic Fields of the Outer Planets
, SPACE SCIENCE REVIEWS, Vol: 152, Pages: 251-269, ISSN: 0038-6308- Author Web Link
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- Citations: 41
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Journal articleWang L, Lin RP, Parks GK, et al., 2010,
Energetic, ∼5-90 keV neutral atom imaging of a weak substorm with STEREO/STE
, GEOPHYSICAL RESEARCH LETTERS, Vol: 37, ISSN: 0094-8276- Author Web Link
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- Citations: 6
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Journal articlePulupa MP, Bale SD, Kasper JC, 2010,
Langmuir waves upstream of interplanetary shocks: Dependence on shock and plasma parameters
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 115, ISSN: 2169-9380- Author Web Link
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- Citations: 28
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Journal articleSmith CW, Stawarz JE, Vasquez BJ, et al., 2010,
Comment on "Turbulent Cascade at 1 AU in High Cross-Helicity Flows'' Reply
, PHYSICAL REVIEW LETTERS, Vol: 104, ISSN: 0031-9007- Author Web Link
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- Citations: 8
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Journal articleAndrews DJ, Cowley SWH, Dougherty MK, et al., 2010,
Magnetic field oscillations near the planetary period in Saturn's equatorial magnetosphere: Variation of amplitude and phase with radial distance and local time
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 115, ISSN: 2169-9380- Author Web Link
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- Citations: 73
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Journal articleStawarz JE, Smith CW, Vasquez BJ, et al., 2010,
THE TURBULENT CASCADE FOR HIGH CROSS-HELICITY STATES AT 1 AU
, ASTROPHYSICAL JOURNAL, Vol: 713, Pages: 920-934, ISSN: 0004-637X- Author Web Link
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- Citations: 45
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Journal articleRouillard AP, Davies JA, Lavraud B, et al., 2010,
Intermittent release of transients in the slow solar wind: 1. Remote sensing observations
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 115, ISSN: 2169-9380- Author Web Link
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- Citations: 94
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Journal articleRouillard AP, Lavraud B, Davies JA, et al., 2010,
Intermittent release of transients in the slow solar wind: 2. In situ evidence
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 115, ISSN: 2169-9380- Author Web Link
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- Citations: 63
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Journal articleBebesi Z, Szego K, Balogh A, et al., 2010,
Slow-mode shock candidate in the Jovian magnetosheath
, PLANETARY AND SPACE SCIENCE, Vol: 58, Pages: 807-813, ISSN: 0032-0633- Author Web Link
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- Citations: 4
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Journal articleCox CV, Harries JE, Taylor JP, et al., 2010,
Measurement and simulation of mid- and far-infrared spectra in the presence of cirrus
, QUARTERLY JOURNAL OF THE ROYAL METEOROLOGICAL SOCIETY, Vol: 136, Pages: 718-739, ISSN: 0035-9009- Author Web Link
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- Citations: 29
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Journal articlePanchenko M, Rucker HO, Kaiser ML, et al., 2010,
New periodicity in Jovian decametric radio emission
, GEOPHYSICAL RESEARCH LETTERS, Vol: 37, ISSN: 0094-8276- Author Web Link
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- Citations: 6
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Journal articleMalaspina DM, Kellogg PJ, Bale SD, et al., 2010,
MEASUREMENTS OF RAPID DENSITY FLUCTUATIONS IN THE SOLAR WIND
, ASTROPHYSICAL JOURNAL, Vol: 711, Pages: 322-327, ISSN: 0004-637X- Author Web Link
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- Citations: 13
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Journal articleWei HY, Russell CT, Zhang TL, et al., 2010,
Comparison study of magnetic flux ropes in the ionospheres of Venus, Mars and Titan
, ICARUS, Vol: 206, Pages: 174-181, ISSN: 0019-1035- Author Web Link
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- Citations: 21
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Journal articlePerri S, Balogh A, 2010,
CHARACTERIZATION OF TRANSITIONS IN THE SOLAR WIND PARAMETERS
, ASTROPHYSICAL JOURNAL, Vol: 710, Pages: 1286-1294, ISSN: 0004-637X- Author Web Link
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- Citations: 8
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Journal articleChen CHK, Wicks RT, Horbury TS, et al., 2010,
Interpreting Power Anisotropy Measurements in Plasma Turbulence
, The Astrophysical Journal Letters, Vol: 711, Pages: L79-L83, ISSN: 2041-8205A relationship is derived between power anisotropy and wavevector anisotropy in turbulent fluctuations. This can be used to interpret plasma turbulence measurements, for example, in the solar wind. If fluctuations are spatially anisotropic, then the ion gyroscale break point in measured spectra in the directions parallel and perpendicular to the magnetic field would not occur at the same frequency, and similarly for the electron gyroscale break point. This is an important consideration when interpreting solar wind measurements in terms of anisotropic turbulence theories. Model magnetic field power spectra are presented assuming a cascade of critically balanced Alfvén waves in the inertial range and kinetic Alfvén waves in the dissipation range. The variation of power anisotropy with scale is compared to existing solar wind measurements, and the similarities and differences are discussed.
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Journal articleWicks RT, Owens MJ, Horbury TS, 2010,
The Variation of SolarWind Correlation Lengths OverThree Solar Cycles
, Solar Physics, Vol: 262, Pages: 191-198, ISSN: 0038-0938We present the results of a study of solar wind velocity and magnetic field correlation lengths over the last 35 years. The correlation length of the magnetic field magnitude λ|B| increases on average by a factor of two at solar maxima compared to solar minima. The correlation lengths of the components of the magnetic field λBXYZ and of the velocity λVYZ do not show this change and have similar values, indicating a continual turbulent correlation length of around 1.4 × 106 km. We conclude that a linear relation between λ|B|, VB2, and Kp suggests that the former is related to the total magnetic energy in the solar wind and an estimate of the average size of geoeffective structures, which is, in turn, proportionalto VB2. By looking at the distribution of daily correlation lengths we show that the solarminimum values of λ|B| correspond to the turbulent outer scale. A tail of larger λ|B| values is present at solar maximum causing the increase in mean value.
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