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Conference paperKrasnoselskikh V, Abbett WP, Hudson H, et al., 2012, , Workshop on Waves and Instabilities in Space and Astrophysical Plasmas, Publisher: AMER INST PHYSICS, Pages: 42-62, ISSN: 0094-243X
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Journal articleBorg AL, Taylor MGGT, Eastwood JP, 2012, , ANNALES GEOPHYSICAE, Vol: 30, Pages: 109-117, ISSN: 0992-7689
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- Citations: 6
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Journal articleSun WJ, Shi QQ, Fu SY, et al., 2012, , ANNALES GEOPHYSICAE, Vol: 30, Pages: 583-595, ISSN: 0992-7689
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- Citations: 74
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Journal articleMitchell JJ, Schwartz SJ, Auster U, 2012, , ANNALES GEOPHYSICAE, Vol: 30, Pages: 503-513, ISSN: 0992-7689
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- Citations: 14
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Journal articleNewman SM, Green PD, Ptashnik IV, et al., 2012, , Phil. Trans. R. Soc. A, Vol: 370
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Journal articleBorg AL, Taylor MGGT, Eastwood JP, 2012, , ANNALES GEOPHYSICAE, Vol: 30, Pages: 761-773, ISSN: 0992-7689
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- Citations: 45
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Journal articleTaylor MGGT, Hasegawa H, Lavraud B, et al., 2012, , ANNALES GEOPHYSICAE, Vol: 30, Pages: 1025-1035, ISSN: 0992-7689
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- Citations: 65
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Journal articleMushtaq S, Steers EBM, Pickering JC, et al., 2012, , JOURNAL OF ANALYTICAL ATOMIC SPECTROMETRY, Vol: 27, Pages: 1264-1273, ISSN: 0267-9477
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- Citations: 13
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Journal articleMueller-Wodarg ICFM, Moore L, Galand M, et al., 2012, , Icarus, Vol: 221, Pages: 481 - 494-481 - 494, ISSN: 0019-1035
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Journal articleField RD, Risi C, Schmidt GA, et al., 2012, , Atmos. Chem. Phys., Vol: 12, Pages: 10485-10504
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ReportNorth GR, Baker DN, Bradley RS, et al., 2012,
The Effects of Solar Variability on Earth's Climate: A Workshop Report.
, Washington DC, Publisher: National Academies Press -
Journal articleDai L, Wygant JR, Cattell C, et al., 2011, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 116, ISSN: 2169-9380
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- Citations: 29
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Journal articleLi LY, Cao JB, Zhou GC, et al., 2011, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 116, ISSN: 2169-9380
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- Citations: 29
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Journal articleChandran BDG, Dennis TJ, Quataert E, et al., 2011, , ASTROPHYSICAL JOURNAL, Vol: 743, ISSN: 0004-637X
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- Citations: 188
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Journal articleLazio TJW, MacDowall RJ, Burns JO, et al., 2011, , ADVANCES IN SPACE RESEARCH, Vol: 48, Pages: 1942-1957, ISSN: 0273-1177
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- Citations: 27
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Journal articleArridge CS, Andr茅 N, McAndrews HJ, et al., 2011, , Space Science Reviews, Vol: 164, Pages: 1-83, ISSN: 0038-6308
Saturn's rich magnetospheric environment is unique in the solar system, with a large number of active magnetospheric processes and phenomena. Observations of this environment from the Cassini spacecraft has enabled the study of a magnetospheric system which strongly interacts with other components of the saturnian system: the planet, its rings, numerous satellites (icy moons and Titan) and various dust, neutral and plasma populations. Understanding these regions, their dynamics and equilibria, and how they interact with the rest of the system via the exchange of mass, momentum and energy is important in understanding the system as a whole. Such an understanding represents a challenge to theorists, modellers and observers. Studies of Saturn's magnetosphere based on Cassini data have revealed a system which is highly variable which has made understanding the physics of Saturn's magnetosphere all the more difficult. Cassini's combination of a comprehensive suite of magnetospheric fields and particles instruments with excellent orbital coverage of the saturnian system offers a unique opportunity for an in-depth study of the saturnian plasma and fields environment. In this paper knowledge of Saturn's equatorial magnetosphere will be presented and synthesised into a global picture. Data from the Cassini magnetometer, low-energy plasma spectrometers, energetic particle detectors, radio and plasma wave instrumentation, cosmic dust detectors, and the results of theory and modelling are combined to provide a multi-instrumental identification and characterisation of equatorial magnetospheric regions at Saturn. This work emphasises the physical processes at work in each region and at their boundaries. The result of this study is a map of Saturn's near equatorial magnetosphere, which represents a synthesis of our current understanding at the end of the Cassini Prime Mission of the global configuration of the equatorial magnetosphere. © 2011 Springer Science+Business Media B
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Conference paperRuffoni M, Pickering JC, Thorne AP, et al., 2011,
New atomic data for astrophysics by high resolution fourier transform spectrometry
New measurements, by high resolution IR-VUV Fourier Transform spectrometry, of accurate atomic data (wavelengths, energy levels, transition probabilities) for astrophysics applications are presented. © 2011 Optical Society of America.
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Conference paperLee Y, Jin H, Seon J, et al., 2011,
Development of CubeSat for space science mission: Cinema
, Pages: 3658-3662We are developing three identical cubesats for space science mission called TRIO-CINEMA(TRiplet Ionospheric Observatory-Cubesat for Ion, Neutral, Electron, and MAgnetic fields). Three institutes participate in the CINEMA: School of Space 91桃色 at Kyung Hee University, Space Science Laboratory at University of California, Berkeley, and 91桃色. CINEMA has a 3U cubesat platform; the volume is 100 x 100 x 340.5 mm. The mass is about 3 kg, and power is 3 W. The three CINEMA cubesats each carry a suprathermal electron, ion, neutral (STEIN) instrument to provide stereo Energetic Neutral Atom (ENA) imaging of the ring current and multi-point in situ measurements of suprathermal electrons and ions, and dual 3-axis magnetometers of magnetoresistive sensors, one at the end of 1-m long stacer boom, to measure magnetic fields and, the other within the spacecraft to measure the fields for attitude control. STEIN uses an array of silicon detectors, with heritage from the STEREO mission, behind an electrostatuic deflection system, to detect ∼ 2 to 200 keV electrons, ions, and ENAs. CINEMA consists of communication modules, avionics bus, solar panels, and the scientific instruments. The spacecraft is spin-stabilized at a spin rate of 4 RPM. The attitude information is derived by two sun sensors and inboard magnetometer. The spacecraft sends the data through S-band transmitter and receives commands from the ground station via UHF receiver. In this paper, we introduce the system design and the qualification model for CINEMA. Copyright ©2011 by the International Astronautical Federation. All rights reserved.
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Journal articleSibeck DG, Angelopoulos V, Brain DA, et al., 2011, , SPACE SCIENCE REVIEWS, Vol: 165, Pages: 59-91, ISSN: 0038-6308
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- Citations: 54
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Journal articleTeh W-L, Nakamura R, Sonnerup BUO, et al., 2011, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 116, ISSN: 2169-9380
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- Citations: 18
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Journal articleCui J, Yelle RV, Mueller-Wodarg ICF, et al., 2011, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 116, ISSN: 2169-9380
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- Citations: 26
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Journal articleSchwartz SJ, Henley E, Mitchell J, et al., 2011, , PHYSICAL REVIEW LETTERS, Vol: 107, ISSN: 0031-9007
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- Citations: 83
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Journal articleMaruca BA, Kasper JC, Bale SD, 2011, , PHYSICAL REVIEW LETTERS, Vol: 107, ISSN: 0031-9007
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- Citations: 142
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Journal articleArridge CS, Andre N, Khurana KK, et al., 2011, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 116, ISSN: 2169-9380
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- Citations: 84
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Journal articleIneson S, Scaife AA, Knight JR, et al., 2011, , NATURE GEOSCIENCE, Vol: 4, Pages: 753-757, ISSN: 1752-0894
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- Citations: 291
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Journal articleMasters A, Schwartz SJ, Henley EM, et al., 2011, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 116, ISSN: 2169-9380
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- Citations: 43
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Journal articleOka M, Phan T-D, Eastwood JP, et al., 2011, , GEOPHYSICAL RESEARCH LETTERS, Vol: 38, ISSN: 0094-8276
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- Citations: 32
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Journal articleKriegel H, Simon S, Motschmann U, et al., 2011, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 116, ISSN: 2169-9380
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- Citations: 62
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Journal articleDelamere PA, Wilson RJ, Masters A, 2011, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 116, ISSN: 2169-9380
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- Citations: 33
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Journal articleCutler JC, Dougherty MK, Lucek E, et al., 2011, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 116, ISSN: 2169-9380
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- Citations: 14
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