Publications
111 results found
Campagnola S, Boutonnet A, Martens W, et al., 2015, Mission design for the exploration of Neptune and Triton, IEEE Aerospace and Electronic Systems Magazine, Vol: 30, Pages: 6-17, ISSN: 0885-8985
Masters A, 2015, The dayside reconnection voltage applied to Saturn's magnetosphere, GEOPHYSICAL RESEARCH LETTERS, Vol: 42, Pages: 2577-2585, ISSN: 0094-8276
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- Citations: 18
Delamere PA, Bagenal F, Paranicas C, et al., 2015, Solar Wind and Internally Driven Dynamics: Influences on Magnetodiscs and Auroral Responses, SPACE SCIENCE REVIEWS, Vol: 187, Pages: 51-97, ISSN: 0038-6308
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- Citations: 40
Pisa D, Hospodarsky GB, Kurth WS, et al., 2015, Statistics of Langmuir wave amplitudes observed inside Saturn's foreshock by the Cassini spacecraft, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 120, Pages: 2531-2542, ISSN: 2169-9380
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- Citations: 8
Kimura T, Badman SV, Tao C, et al., 2015, Transient internally driven aurora at Jupiter discovered by Hisaki and the Hubble Space Telescope, GEOPHYSICAL RESEARCH LETTERS, Vol: 42, Pages: 1662-1668, ISSN: 0094-8276
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- Citations: 50
Masters A, 2015, Magnetic reconnection at Neptune's magnetopause, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 120, Pages: 479-493, ISSN: 2169-9380
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- Citations: 18
Arridge CS, Achilleos N, Agarwal J, et al., 2014, The science case for an orbital mission to Uranus: Exploring the origins and evolution of ice giant planets, PLANETARY AND SPACE SCIENCE, Vol: 104, Pages: 122-140, ISSN: 0032-0633
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- Citations: 48
Masters A, Achilleos N, Agnor CB, et al., 2014, Neptune and Triton: Essential pieces of the Solar System puzzle, PLANETARY AND SPACE SCIENCE, Vol: 104, Pages: 108-121, ISSN: 0032-0633
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- Citations: 27
Slavin JA, DiBraccio GA, Gershman DJ, et al., 2014, MESSENGER observations of Mercury's dayside magnetosphere under extreme solar wind conditions, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 119, Pages: 8087-8116, ISSN: 2169-9380
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- Citations: 113
Masters A, 2014, Magnetic reconnection at Uranus' magnetopause, Journal of Geophysical Research: Space Physics, Vol: 119, Pages: 5520-5538, ISSN: 2169-9380
The magnetosphere of Uranus has barely been explored by spacecraft but is distinct from other solar system magnetospheres in many respects. Determining how this magnetosphere is coupled to the solar wind is central to understanding energy flow through the system. Here we assess how the solar wind interacts with the Uranian magnetosphere via magnetic reconnection. Analytical models of conditions at the magnetopause are combined with current understanding of reconnection onset to predict where reconnection may occur on the boundary. The results suggest that conditions at Uranus' magnetopause are generally less favorable for reconnection than those at the magnetopause of any planet closer to the Sun, as a result of how typical solar wind parameters vary with heliocentric distance. The location of reconnection sites on the Uranian magnetopause is likely to be highly dependent on not only the interplanetary magnetic field orientation but also planetary longitude and season. Solar wind–magnetosphere coupling via magnetic reconnection may be stronger under near‐solstice conditions than under near‐equinox conditions. We discuss the typical reconnection electric field strength at Uranus' magnetopause and suggest that the typical reconnection voltage is considerably less than 40 kV. Complimentary assessments of other means of coupling to the solar wind (e.g., via a “viscous‐like” interaction) are needed to establish the overall nature of solar wind–magnetosphere coupling at Uranus.
Sulaiman AH, Masters A, Dougherty MK, et al., 2014, The magnetic structure of Saturn's magnetosheath, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 119, Pages: 5651-5661, ISSN: 2169-9380
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- Citations: 20
Pilkington NM, Achilleos N, Arridge CS, et al., 2014, Polar confinement of Saturn's magnetosphere revealed by in situ Cassini observations, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 119, Pages: 2858-2875, ISSN: 2169-9380
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- Citations: 20
Fuselier SA, Frahm R, Lewis WS, et al., 2014, The location of magnetic reconnection at Saturn's magnetopause: A comparison with Earth, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 119, Pages: 2563-2578, ISSN: 2169-9380
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- Citations: 51
Masters A, Fujimoto M, Hasegawa H, et al., 2014, Can magnetopause reconnection drive Saturn's magnetosphere?, GEOPHYSICAL RESEARCH LETTERS, Vol: 41, Pages: 1862-1868, ISSN: 0094-8276
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- Citations: 22
Mistry R, Dougherty MK, Masters A, et al., 2014, Separating drivers of Saturnian magnetopause motion, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 119, Pages: 1514-1522, ISSN: 2169-9380
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- Citations: 5
Collinson GA, Sibeck DG, Masters A, et al., 2014, A survey of hot flow anomalies at Venus, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 119, Pages: 978-991, ISSN: 2169-9380
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- Citations: 18
Masters A, Phan TD, Badman SV, et al., 2014, The plasma depletion layer in Saturn's magnetosheath, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 119, Pages: 121-130, ISSN: 2169-9380
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- Citations: 15
Ghavamian P, Schwartz SJ, Mitchell J, et al., 2014, Electron-Ion Temperature Equilibration in Collisionless Shocks: The Supernova Remnant-Solar Wind Connection, MICROPHYSICS OF COSMIC PLASMAS, Editors: Balogh, Bykov, Cargill, Dendy, DeWit, Raymond, Publisher: SPRINGER, Pages: 557-587, ISBN: 978-1-4899-7412-9
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- Citations: 3
Eastwood JP, Phan TD, Oieroset M, et al., 2013, Influence of asymmetries and guide fields on the magnetic reconnection diffusion region in collisionless space plasmas, PLASMA PHYSICS AND CONTROLLED FUSION, Vol: 55, ISSN: 0741-3335
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- Citations: 42
Masters A, Stawarz L, Fujimoto M, et al., 2013, <i>In situ</i> observations of high-Mach number collisionless shocks in space plasmas, PLASMA PHYSICS AND CONTROLLED FUSION, Vol: 55, ISSN: 0741-3335
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- Citations: 7
Ghavamian P, Schwartz SJ, Mitchell J, et al., 2013, Electron-Ion Temperature Equilibration in Collisionless Shocks: The Supernova Remnant-Solar Wind Connection, SPACE SCIENCE REVIEWS, Vol: 178, Pages: 633-663, ISSN: 0038-6308
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- Citations: 71
Masters A, Slavin JA, DiBraccio GA, et al., 2013, A comparison of magnetic overshoots at the bow shocks of Mercury and Saturn, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 118, Pages: 4381-4390, ISSN: 2169-9380
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- Citations: 15
Walsh AP, Arridge CS, Masters A, et al., 2013, An indication of the existence of a solar wind strahl at 10AU, GEOPHYSICAL RESEARCH LETTERS, Vol: 40, Pages: 2495-2499, ISSN: 0094-8276
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- Citations: 9
Branduardi-Raymont G, Ford PG, Hansen KC, et al., 2013, Search for Saturn's X-ray aurorae at the arrival of a solar wind shock, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 118, Pages: 2145-2156, ISSN: 2169-9380
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- Citations: 12
Sergis N, Jackman CM, Masters A, et al., 2013, Particle and magnetic field properties of the Saturnian magnetosheath: Presence and upstream escape of hot magnetospheric plasma, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 118, Pages: 1620-1634, ISSN: 2169-9380
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- Citations: 34
Badman SV, Masters A, Hasegawa H, et al., 2013, Bursty magnetic reconnection at Saturn's magnetopause, GEOPHYSICAL RESEARCH LETTERS, Vol: 40, Pages: 1027-1031, ISSN: 0094-8276
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- Citations: 72
Masters A, Stawarz L, Fujimoto M, et al., 2013, Electron acceleration to relativistic energies at a strong quasi-parallel shock wave, NATURE PHYSICS, Vol: 9, Pages: 164-167, ISSN: 1745-2473
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- Citations: 63
Masters A, Stawarz Ł, Fujimoto M, et al., 2013, Electron acceleration to relativistic energies at a strong quasi-parallel shock wave
Electrons can be accelerated to ultrarelativistic energies at strong (high-Mach number) collisionless shock waves that form when stellar debris rapidly expands after a supernova [4, 2, 19]. Collisionless shock waves also form in the flow of particles from the Sun (the solar wind), and extensive spacecraft observations have established that electron acceleration at these shocks is effectively absent whenever the upstream magnetic field is roughly parallel to the shock surface normal (quasi-parallel conditions) [16, 8, 10, 17, 14]. However, it is unclear whether this magnetic dependence of electron acceleration also applies to the far stronger shocks around young supernova remnants, where local magnetic conditions are poorly understood. Here we present Cassini spacecraft observations of an unusually strong solar system shock wave (Saturn’s bow shock) where significant local electron acceleration has been confirmed under quasi- parallel magnetic conditions for the first time, contradicting the established magnetic dependence of electron acceleration at solar system shocks [16, 8, 10, 17, 14]. Furthermore, the acceleration led to electrons at relativistic energies (∼ MeV), comparable to the highest energies ever attributed to shock-acceleration in the solar wind [16]. These observations suggest that at high-Mach numbers, like those of young supernova remnant shocks, quasi-parallel shocks become considerably more effective electron accelerators. For full details please see: Nature Physics, Volume 9, Issue 3, pp. 164-167.
Kasahara S, Kronberg EA, Kimura T, et al., 2013, Asymmetric distribution of reconnection jet fronts in the Jovian nightside magnetosphere, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 118, Pages: 375-384, ISSN: 2169-9380
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- Citations: 42
Volwerk M, Andre N, Arridge CS, et al., 2013, Comparative magnetotail flapping: an overview of selected events at Earth, Jupiter and Saturn, ANNALES GEOPHYSICAE, Vol: 31, Pages: 817-833, ISSN: 0992-7689
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- Citations: 32
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