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Your search keyword '"T. D. Phan"' showing total 6 results
Start Over Author "T. D. Phan" Journal space science reviews
6 results on '"T. D. Phan"'

1. The Space Physics Environment Data Analysis System (SPEDAS)

Author

V. Angelopoulos, P. Cruce, A. Drozdov, E. W. Grimes, N. Hatzigeorgiu, D. A. King, D. Larson, J. W. Lewis, J. M. McTiernan, D. A. Roberts, C. L. Russell, T. Hori, Y. Kasahara, A. Kumamoto, A. Matsuoka, Y. Miyashita, Y. Miyoshi, I. Shinohara, M. Teramoto, J. B. Faden, A. J. Halford, M. McCarthy, R. M. Millan, J. G. Sample, D. M. Smith, L. A. Woodger, A. Masson, A. A. Narock, K. Asamura, T. F. Chang, C.-Y. Chiang, Y. Kazama, K. Keika, S. Matsuda, T. Segawa, K. Seki, M. Shoji, S. W. Y. Tam, N. Umemura, B.-J. Wang, S.-Y. Wang, R. Redmon, J. V. Rodriguez, H. J. Singer, J. Vandegriff, S. Abe, M. Nose, A. Shinbori, Y.-M. Tanaka, S. UeNo, L. Andersson, P. Dunn, C. Fowler, J. S. Halekas, T. Hara, Y. Harada, C. O. Lee, R. Lillis, D. L. Mitchell, M. R. Argall, K. Bromund, J. L. Burch, I. J. Cohen, M. Galloy, B. Giles, A. N. Jaynes, O. Le Contel, M. Oka, T. D. Phan, B. M. Walsh, J. Westlake, F. D. Wilder, S. D. Bale, R. Livi, M. Pulupa, P. Whittlesey, A. DeWolfe, B. Harter, E. Lucas, U. Auster, J. W. Bonnell, C. M. Cully, E. Donovan, R. E. Ergun, H. U. Frey, B. Jackel, A. Keiling, H. Korth, J. P. McFadden, Y. Nishimura, F. Plaschke, P. Robert, D. L. Turner, J. M. Weygand, R. M. Candey, R. C. Johnson, T. Kovalick, M. H. Liu, R. E. McGuire, A. Breneman, K. Kersten, and P. Schroeder

Published
2019
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3. The Space Physics Environment Data Analysis System (SPEDAS)

Author

Tomonori Segawa, Aaron Breneman, M. H. Liu, Matthew D. McCarthy, Kunihiro Keika, David M. Smith, R. C. Johnson, S. Matsuda, Kanako Seki, Arnaud Masson, Christopher M. Fowler, Drew Turner, Ian J. Cohen, Atsuki Shinbori, Jasper Halekas, Robert E. Ergun, E. Lucas, Alexa Halford, Brian Walsh, Allison Jaynes, Eric Grimes, Marc Pulupa, Jeremy Faden, D. A. King, David L. Mitchell, P. Cruce, Sunny W. Y. Tam, Eric Donovan, R. E. McGuire, Joseph Westlake, James L. Burch, A. DeWolfe, Yuki Harada, U. Auster, James W. Lewis, Matthew R. Argall, Ferdinand Plaschke, Yoichi Kazama, Ayako Matsuoka, Phyllis Whittlesey, Alexander Drozdov, Roberto Livi, Robyn Millan, Michael Galloy, Mariko Teramoto, C. L. Russell, Frederick Wilder, Haje Korth, Juan V. Rodriguez, A. A. Narock, Norio Umemura, Atsushi Kumamoto, Kenneth R. Bromund, Christopher Cully, C. Y. Chiang, P. Robert, T. F. Chang, L. A. Woodger, Yoshizumi Miyoshi, J. P. McFadden, A. Keiling, L. Andersson, Davin Larson, I. Shinohara, B. J. Wang, Christina O. Lee, Masafumi Shoji, P. Dunn, T. D. Phan, T. Kovalick, Stuart D. Bale, John Sample, Kris Kersten, S. UeNo, J. M. McTiernan, S. Abe, P. Schroeder, Takuya Hara, Tomoaki Hori, Jon Vandegriff, Harald U. Frey, Robert J. Redmon, Yoshiya Kasahara, Robert Lillis, Masahito Nose, Robert M. Candey, Yukitoshi Nishimura, Howard J. Singer, James M. Weygand, Vassilis Angelopoulos, Mitsuo Oka, O. Le Contel, Shiang-Yu Wang, Brian Jackel, Yoshimasa Tanaka, Kazushi Asamura, Yukinaga Miyashita, John W. Bonnell, Bryan Harter, D. A. Roberts, N. Hatzigeorgiu, Barbara L. Giles, Laboratoire de Physique des Plasmas (LPP), Université Paris-Saclay-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-École polytechnique (X)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)

Subjects
010504 meteorology & atmospheric sciences, Solar wind, Ionospheric physics, Planetary magnetospheres, ASCII, 01 natural sciences, Article, Space exploration, Software, Heliophysics, Data retrieval, [PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph], 0103 physical sciences, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, computer.programming_language, Graphical user interface, Geospace science, business.industry, Software development, Astronomy and Astrophysics, Python (programming language), Space and Planetary Science, Magnetospheric physics, Space plasmas, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Software engineering, business, computer
Abstract

著者人数: 102名（所属. 宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS): 松岡, 彩子; 篠原, 育; 浅村, 和史), Accepted: 2018-12-29, 資料番号: SA1180350000

Published
2019
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4. Magnetopause Processes

Author

Laurence Rezeau, Rudolf A. Treumann, Andris Vaivads, David Attié, T. D. Phan, Goetz Paschmann, Barrett Rogers, Bengt U. Ö. Sonnerup, S. A. Fuselier, C. P. Escoubet, Space Sciences Laboratory [Berkeley] (SSL), University of California [Berkeley], University of California-University of California, Space Science Department of ESA, European Space Research and Technology Centre (ESTEC), European Space Agency (ESA)-European Space Agency (ESA), Centre d'étude des environnements terrestre et planétaires (CETP), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Max-Planck-Institut für Extraterrestrische Physik (MPE), Swedish Institute of Space Physics [Kiruna] (IRF), International Space Science Institute [Bern] (ISSI), Lockheed Martin Advanced Technology Laboratories (ATL), Lockheed Martin Advanced Technology Laboratories, Department of Physics and Astronomy [Hanover], Dartmouth College [Hanover], and Thayer School of Engineering

Subjects
Physics, 010504 meteorology & atmospheric sciences, [PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], Astronomy and Astrophysics, Geophysics, 01 natural sciences, [PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph], Space and Planetary Science, 0103 physical sciences, Magnetopause, 010303 astronomy & astrophysics, ComputingMilieux_MISCELLANEOUS, 0105 earth and related environmental sciences
Abstract

International audience; Not Available

Published
2005
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5. Critical Issues on Magnetic Reconnection in Space Plasmas

Author

G. S. Lakhina, Yan Song, Masatoshi Yamauchi, Tsugunobu Nagai, Rudolf A. Treumann, Rickard Lundin, L. M. Zelenyi, T. D. Phan, M. Roth, Anthony T. Y. Lui, Zuyin Pu, and Christian Jacquey

Subjects
Physics, Classical mechanics, Flux tube, Magnetic energy, Space and Planetary Science, Field line, Physics::Space Physics, Magnetosphere, Magnetopause, Astronomy and Astrophysics, Magnetic reconnection, Magnetohydrodynamics, Magnetic flux
Abstract

The idea of expedient energy transformation by magnetic reconnection (MR) has generated much enthusiasm in the space plasma community. The early concept of MR, which was envisioned for the solar flare phenomenon in a simple two-dimensional (2D) steady-state situation, is in dire need for extension to encompass three-dimensional (3D) non-steady-state phenomena prevalent in space plasmas in nature like in the magnetosphere. A workshop was organized to address this and related critical issues on MR. The essential outcome of this workshop is summarized in this review. After a brief evaluation on the pros and cons of existing definitions of MR, we propose essentially a working definition that can be used to identify MR in transient and spatially localized phenomena. The word “essentially” reflects a slight diversity in the opinion on how transient and localized 3D MR process might be defined. MR is defined here as a process with the following characteristics: (1) there is a plasma bulk flow across a boundary separating regions with topologically different magnetic field lines if projected on the plane of MR, thereby converting magnetic energy into kinetic particle energy, (2) there can be an out-of-the-plane magnetic field component (the so-called guide field) present such that the reconnected magnetic flux tubes are twisted to form flux ropes, and (3) the region exhibiting non-ideal MHD conditions should be localized to a scale comparable to the ion inertial length in the direction of the plasma inflow velocity. This definition captures the most important 3D aspects and preserves many essential characteristics of the 2D case. It may be considered as the first step in the generalization of the traditional 2D concept. As a demonstration on the utility of this definition, we apply it to identify MR associated with plasma phenomena in the dayside magnetopause and nightside magnetotail of the Earth’s magnetosphere. How MR may be distinguished from other competing mechanisms for these magnetospheric phenomena are then discussed.

Published
2005
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6. [Untitled]

Author

W. Lennartsson, David G. Sibeck, M. Roth, T. D. Phan, K. Stasiewicz, G. Paschmann, K. W. Ogilvie, Terrance Onsager, Manfred Scholer, N. Sckopke, Rudolf A. Treumann, S. A. Fuselier, Masatoshi Yamauchi, Mike Lockwood, and Rickard Lundin

Subjects
Physics, Space and Planetary Science, Magnetopause, Astronomy and Astrophysics, Mechanics, Plasma
Published
1999
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