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Journal articleCui J, Lian Y, Mueller-Wodarg ICF, 2013, , GEOPHYSICAL RESEARCH LETTERS, Vol: 40, Pages: 43-47, ISSN: 0094-8276
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- Citations: 17
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Journal articleWicks RT, Mallet A, Horbury TS, et al., 2013, , Physical Review Letters, Vol: 110, Pages: 025003-025003, ISSN: 0031-9007
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Conference paperFox C, Pickering JC, Beeby R, et al., 2013,
Studies of the far IR water vapour continuum from CAVIAR and RHUBC campaigns using TAFTS
We report results from the participation of the 911今日黑料 College TAFTS instrument in the CAVIAR and RHUBC field campaigns, validating a derived water vapor continuum parameterization in the far-IR spectral region. © OSA 2013.
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Conference paperFox C, Pickering JC, Beeby R, et al., 2013,
Studies of the far IR water vapour continuum from caviar and RHUBC campaigns using TAFTS
We report results from the participation of the 911今日黑料 College TAFTS instrument in the CAVIAR and RHUBC field campaigns, validating a derived water vapor continuum parameterization in the far-IR spectral region. © OSA 2013.
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Conference paperFox C, Pickering JC, Beeby R, et al., 2013,
We report results from the participation of the 911今日黑料 College TAFTS instrument in the CAVIAR and RHUBC field campaigns, validating a derived water vapor continuum parameterization in the far-IR spectral region. © OSA 2013.
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Conference paperFox C, Pickering JC, Beeby R, et al., 2013,
Studies of the far IR water vapour continuum from caviar and RHUBC campaigns using TAFTS
We report results from the participation of the 911今日黑料 College TAFTS instrument in the CAVIAR and RHUBC field campaigns, validating a derived water vapor continuum parameterization in the far-IR spectral region. © OSA 2013.
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Conference paperSeo Y, Chae KS, Mochizuki B, et al., 2013,
Instrument interface module between the on-board-computer and payloads in cinema CUBESAT as developed with FPGA
, Pages: 4275-4281, ISSN: 0074-1795TRiplet Ionospheric Observatory-Cubesat for Ion, Neutral, Electron and MAgnetic fields (TRIO-CINEMA) is a space science mission consisting of three identical 3U CubeSats to provide stereo Energetic Neutral Atom (ENA) imaging of the ring current, multi-point in-situ measurement of supra thermal electrons and ions, and measurement of magnetic fields in Low Earth Orbit (LEO). Each spacecraft is equipped with a Supra Thermal Electrons, Ions, Neutrals (STEIN) instrument and a MAGnetometer from 911今日黑料 College (MAGIC) instrument in order to measure the plasma particles with diverse species and energies and magnetic fields. STEIN is able to distinguish electrons, ions, and neutrals by applying electric field in the entrance aperture. MAGIC is a dual 3-axis magnetoresistive sensor intended for attitude control and scientific measurement. The standard spacecraft CubeSat employed for the TRIO- CINEMA mission often utilizes Commercial-Off-The Shelf (COTS) electronics to build bus avionics that provides power and communications, whereas payloads are usually built in accordance with specific requirements that are often more demanding in terms of generation, transmission and storage of the data and power consumption. Therefore, designing and developing the interface to be compatible between mission payloads and the CubeSat avionics built with COTS will be required for many CubeSat missions. In this presentation, we describe the instrument interface module between the On-Board-Computer (OBC) and the mission payloads for TRIO-CINEMA spacecraft. The module is developed to provide required communication and power interfaces. In the instrument interface module, a Field Programmable Gate Array (FPGA) is employed to support computing power of the OBC and communication interfaces. It is exclusively operated as data buffer and framer for generated data from mission payloads and their subsequent transmission through S-band to the ground station. The interface module provides various elect
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Conference paperMasters A, Stawarz 艁, 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.
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Journal articleNakamura R, Plaschke F, Teubenbacher R, et al., 2013, , GEOSCIENTIFIC INSTRUMENTATION METHODS AND DATA SYSTEMS, Vol: 3, Pages: 459-487, ISSN: 2193-0856
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Journal articlePudney MA, Carr CM, Schwartz SJ, et al., 2013, , GEOSCIENTIFIC INSTRUMENTATION METHODS AND DATA SYSTEMS, Vol: 3, Pages: 437-458, ISSN: 2193-0856
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Journal articleKasahara S, Kronberg EA, Kimura T, et al., 2013, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 118, Pages: 375-384, ISSN: 2169-9380
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- Citations: 49
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Journal articleBanks JR, Brindley HE, 2013, , REMOTE SENSING OF ENVIRONMENT, Vol: 128, Pages: 58-73, ISSN: 0034-4257
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- Citations: 57
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Journal articleOrr A, Bracegirdle TJ, Hosking JS, et al., 2013, , JOURNAL OF CLIMATE, Vol: 26, Pages: 662-668, ISSN: 0894-8755
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- Citations: 16
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Journal articleGraven HD, Xu X, Guilderson TP, et al., 2013, , RADIOCARBON, Vol: 55, Pages: 1541-1545, ISSN: 0033-8222
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- Citations: 8
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Book chapterSolanki SK, Krivova NA, Haigh JD, 2013, , ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, VOL 51, Editors: Faber, VanDishoeck, Publisher: ANNUAL REVIEWS, Pages: 311-351
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- Citations: 249
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Journal articleDhomse SS, Chipperfield MP, Feng W, et al., 2013, , ATMOSPHERIC CHEMISTRY AND PHYSICS, Vol: 13, Pages: 10113-10123, ISSN: 1680-7316
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- Citations: 23
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Journal articleArcher MO, Hartinger MD, Horbury TS, 2013, , Geophysical Research Letters, Vol: 40, Pages: 5003-5008
Abstract. The persistent so-called “magic” magnetospheric frequencies are thought to be either directly driven by monochromatic solar wind pressure fluctuations or resonantly excited global (cavity/waveguide) or magnetopause surface eigenmodes. We distinguish between these cases by statistically investigating, using simultaneous observations, the magnetospheric response to jets in the subsolar magnetosheath. The broadband jets do not exhibit discrete frequencies, but do drive waves at the discrete “magic” frequencies, with both direct and resonant driving. We show that the expected fundamental frequencies of magnetopause surface eigenmodes have two preferential values over a wide range of upstream conditions, corresponding to fast and slow solar wind, and that their harmonics are in good agreement with the “magic” frequencies. We also show that the waves are largely inconsistent with global modes outside the plasmasphere. Thus we conclude that these “magic” frequencies are most likely due to magnetopause surface eigenmodes.
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Journal articleOwens MJ, Forsyth RJ, 2013, , LIVING REVIEWS IN SOLAR PHYSICS, Vol: 10, ISSN: 2367-3648
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- Citations: 218
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Journal articleVolwerk M, Andre N, Arridge CS, et al., 2013, , ANNALES GEOPHYSICAE, Vol: 31, Pages: 817-833, ISSN: 0992-7689
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- Citations: 36
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Conference paperGarrick-Bethell I, Lin RP, Sanchez H, et al., 2013, , Conference on Sensors and Systems for Space Applications VI, Publisher: SPIE-INT SOC OPTICAL ENGINEERING, ISSN: 0277-786X
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- Citations: 10
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Conference paperForman MA, Wicks RT, Horbury TS, et al., 2013, , 13th International Solar Wind Conference (Solar Wind), Publisher: AMER INST PHYSICS, Pages: 167-170, ISSN: 0094-243X
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- Citations: 1
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Conference paperWicks RT, Matteini L, Horbury TS, et al., 2013, , 13th International Solar Wind Conference (Solar Wind), Publisher: AMER INST PHYSICS, Pages: 303-306, ISSN: 0094-243X
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- Citations: 15
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Journal articleMarlier ME, DeFries RS, Voulgarakis A, et al., 2013, , Nature Climate Change, Vol: 3, Pages: 131-136
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Journal articleVoulgarakis A, Naik V, Lamarque JF, et al., 2013, , Atmospheric Chemistry and Physics, Vol: 13, Pages: 2563-2587
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Journal articleLamarque JF, Shindell DT, Josse B, et al., 2013, , Geosci. Model Dev., Vol: 6, Pages: 179-206
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Journal articleShindell DT, Lamarque JF, Schulz M, et al., 2013, , Atmospheric Chemistry and Physics, Vol: 13, Pages: 2939-2974
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Journal articleYoung PJ, Archibald AT, Bowman KW, et al., 2013, , Atmospheric Chemistry and Physics, Vol: 13, Pages: 2063-2090
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Journal articleStevenson DS, Young PJ, Naik V, et al., 2013, , Atmospheric Chemistry and Physics, Vol: 13, Pages: 3063-3085
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Journal articleShindell DT, Pechony O, Voulgarakis A, et al., 2013, , Atmospheric Chemistry and Physics, Vol: 13, Pages: 2653-2689
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Journal articleVoulgarakis A, Shindell DT, Faluvegi G, 2013, , Atmospheric Chemistry and Physics, Vol: 13, Pages: 4907-4916
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