Results
- Showing results for:
- Reset all filters
Search results
-
Journal articleZhang H, Zong Q-G, Fritz TA, et al., 2008,
Cluster observations of collisionless Hall reconnection at high-latitude magnetopause
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 113, ISSN: 2169-9380- Author Web Link
- Cite
- Citations: 18
-
Journal articleJones GH, Roussos E, Krupp N, et al., 2008,
The dust halo of Saturn's largest icy moon, Rhea
, SCIENCE, Vol: 319, Pages: 1380-1384, ISSN: 0036-8075- Author Web Link
- Cite
- Citations: 49
-
Journal articleLazaridis M, Dzumbova L, Kopanakis I, et al., 2008,
PM<sub>10</sub> and PM<sub>2.5</sub> levels in the eastern Mediterranean (Akrotiri research station, Crete, Greece)
, WATER AIR AND SOIL POLLUTION, Vol: 189, Pages: 85-101, ISSN: 0049-6979- Author Web Link
- Cite
- Citations: 53
-
Journal articleSimon S, Motschmann U, Kleindienst G, et al., 2008,
Titan's magnetic field signature during the Cassini T34 flyby: Comparison between hybrid simulations and MAG data
, GEOPHYSICAL RESEARCH LETTERS, Vol: 35, ISSN: 0094-8276- Author Web Link
- Cite
- Citations: 14
-
Journal articleBunce EJ, Arridge CS, Cowley SWH, et al., 2008,
Magnetic field structure of Saturn's dayside magnetosphere and its mapping to the ionosphere: Results from ring current modeling
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 113, ISSN: 2169-9380- Author Web Link
- Cite
- Citations: 59
-
Journal articleBranduardi-Raymont G, Elsner RF, Galand M, et al., 2008,
Spectral morphology of the X-ray emission from Jupiter's aurorae
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 113, ISSN: 2169-9380- Author Web Link
- Cite
- Citations: 66
-
Journal articleStallard T, Miller S, Lystrup M, et al., 2008,
Dusk-brightening event in Saturn's H<sub>3</sub><SUP>+</SUP> aurora
, ASTROPHYSICAL JOURNAL LETTERS, Vol: 673, Pages: L203-L206, ISSN: 2041-8205- Author Web Link
- Cite
- Citations: 5
-
Journal articleKhurana KK, Russell CT, Dougherty MK, 2008,
Magnetic portraits of Tethys and Rhea
, ICARUS, Vol: 193, Pages: 465-474, ISSN: 0019-1035- Author Web Link
- Cite
- Citations: 54
-
Journal articleHill TW, Thomsen MF, Henderson MG, et al., 2008,
Plasmoids in Saturn's magnetotail
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 113, ISSN: 2169-9380- Author Web Link
- Cite
- Citations: 83
-
Journal articleZong Q-G, Zhang H, Fritz TA, et al., 2008,
Multiple cusps during an extended northward IMF period with a significant <i>B<sub>y</sub></i> component
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 113, ISSN: 2169-9380- Author Web Link
- Cite
- Citations: 13
-
Journal articleEastwood JP, Brain DA, Halekas JS, et al., 2008,
Evidence for collisionless magnetic reconnection at Mars
, GEOPHYSICAL RESEARCH LETTERS, Vol: 35, ISSN: 0094-8276- Author Web Link
- Open Access Link
- Cite
- Citations: 88
-
Journal articleCattell C, Wygant JR, Goetz K, et al., 2008,
Discovery of very large amplitude whistler-mode waves in Earth's radiation belts
, GEOPHYSICAL RESEARCH LETTERS, Vol: 35, ISSN: 0094-8276- Author Web Link
- Cite
- Citations: 229
-
Journal articleMasters A, Arridge CS, Dougherty MK, et al., 2008,
Cassini encounters with hot flow anomaly-like phenomena at Saturn’s bow shock
, \grl, Vol: 35, Pages: L02202-L02202 -
Journal articleCosta JES, Kepler SO, Winget DE, et al., 2008,
The pulsation modes of the pre-white dwarf PG 1159-035
, ASTRONOMY & ASTROPHYSICS, Vol: 477, Pages: 627-640, ISSN: 1432-0746- Author Web Link
- Cite
- Citations: 39
-
Journal articleZhong W, Hogan RJ, Haigh JD, 2008,
Three-dimensional radiative transfer in midlatitude cirrus clouds
, QUARTERLY JOURNAL OF THE ROYAL METEOROLOGICAL SOCIETY, Vol: 134, Pages: 199-215, ISSN: 0035-9009- Author Web Link
- Cite
- Citations: 9
-
Journal articleMasood W, Schwartz SJ, 2008,
Observations of the development of electron temperature anisotropies in Earth’s magnetosheath
, Journal of Geophysical Research (Space Physics), Vol: 113, Pages: A01216-A01216 -
Journal articleRoussos E, Mueller J, Simon S, et al., 2008,
Plasma and fields in the wake of Rhea: 3-D hybrid simulation and comparison with Cassini data
, ANNALES GEOPHYSICAE, Vol: 26, Pages: 619-637, ISSN: 0992-7689- Author Web Link
- Cite
- Citations: 48
-
Conference paperBuchlin E, Cargill PJ, Bradshaw SJ, et 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-+ -
Conference paperIntriligator DS, Sun W, Rees A, et al., 2008,
Three-dimensional simulations of shock propagation in the heliosphere and beyond
, 7th Annual International Astrophysics Conference, Publisher: AMER INST PHYSICS, Pages: 375-+, ISSN: 0094-243X- Author Web Link
- Cite
- Citations: 7
-
Journal articleCowley SWH, Arridge CS, Bunce EJ, et al., 2008,
Auroral current systems in Saturn's magnetosphere:: comparison of theoretical models with Cassini and HST observations
, ANNALES GEOPHYSICAE, Vol: 26, Pages: 2613-2630, ISSN: 0992-7689- Author Web Link
- Cite
- Citations: 58
-
Journal articleRunov A, Voronkov I, Asano Y, et al., 2008,
Structure of the near-Earth plasma sheet during tailward flows
, ANNALES GEOPHYSICAE, Vol: 26, Pages: 709-724, ISSN: 0992-7689- Author Web Link
- Cite
- Citations: 4
-
Journal articleBrown P, Dunlop MW, Balogh A, et al., 2008,
Calibration techniques for magnetometers implementing on-board de-spinning algorithms
, ADVANCES IN SPACE RESEARCH, Vol: 41, Pages: 1571-1578, ISSN: 0273-1177- Author Web Link
- Cite
- Citations: 3
-
Book chapterHorbury TS, Osman KT, 2008,
Multi-Spacecraft Turbulence Analysis Methods
, Multi-Spacecraft Analysis Methods Revisited, Editors: Paschmann, Daly, Noordwijk, Publisher: ESA Communications, Pages: 55-64 -
Journal articleVolwerk M, Zhang TL, Glassmeier KH, et al., 2008,
Study of waves in the magnetotail region with Cluster and DSP
, ADVANCES IN SPACE RESEARCH, Vol: 41, Pages: 1593-1597, ISSN: 0273-1177- Author Web Link
- Cite
- Citations: 8
-
Journal articleTakada T, Nakamura R, Asano Y, et al., 2008,
Plasma sheet oscillations and their relation to substorm development:: Cluster and Double Star TC1 case study
, ADVANCES IN SPACE RESEARCH, Vol: 41, Pages: 1585-1592, ISSN: 0273-1177- Author Web Link
- Cite
- Citations: 4
-
Journal articleTatrallyay M, Erdos G, Balogh A, et al., 2008,
The evolution of mirror type magnetic fluctuations in the magnetosheath based on multipoint observations
, ADVANCES IN SPACE RESEARCH, Vol: 41, Pages: 1537-1544, ISSN: 0273-1177- Author Web Link
- Cite
- Citations: 19
-
Journal articleVolwerk M, Nakamura R, Baumjohann W, et al., 2008,
Tailward propagation of Pi2 waves in the Earth's magnetotail lobe
, ANNALES GEOPHYSICAE, Vol: 26, Pages: 4023-4030, ISSN: 0992-7689- Author Web Link
- Cite
- Citations: 7
-
Journal articleRussell CT, Khurana KK, Arridge CS, et al., 2008,
The magnetospheres of Jupiter and Saturn and their lessons for the Earth
, ADVANCES IN SPACE RESEARCH, Vol: 41, Pages: 1310-1318, ISSN: 0273-1177- Author Web Link
- Cite
- Citations: 5
-
Journal articleBillingham L, Schwartz SJ, Sibeck DG, 2008,
The statistics of foreshock cavities: results of a Cluster survey
, Annales Geophysicae, Vol: 26, Pages: 3653-3667We 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.
-
Journal articleHuttunen KEJ, Bale SD, Salem C, 2008,
Wind observations of low energy particles within a solar wind reconnection region
, ANNALES GEOPHYSICAE, Vol: 26, Pages: 2701-2710, ISSN: 0992-7689- Author Web Link
- Cite
- Citations: 13
This data is extracted from the Web of Science and reproduced under a licence from Thomson Reuters. You may not copy or re-distribute this data in whole or in part without the written consent of the Science business of Thomson Reuters.