Dawn-dusk asymmetries in planetary plasma environments / Stein Haaland, Andrei Runov, Colin Forsyth, editors.

"Dawn-dusk asymmetries are ubiquitous features of the plasma environment of many of the planets in our solar system. They occur when a particular process or feature is more pronounced at one side of a planet than the other. For example, recent observations indicate that Earth's magnetopaus...

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Bibliographic Details
Other Authors: Haaland, Stein (Editor), Runov, Andrei (Editor), Forsyth, Colin (Editor)
Format: Book
Language:English
Published: Washington, D.C. : Hoboken, NJ : American Geophysical Union ; John Wiley & Sons, Inc., 2017.
Series:Geophysical monograph ; 230.
Subjects:

MARC

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245 0 0 |a Dawn-dusk asymmetries in planetary plasma environments /  |c Stein Haaland, Andrei Runov, Colin Forsyth, editors. 
264 1 |a Washington, D.C. :  |b American Geophysical Union ;  |a Hoboken, NJ :  |b John Wiley & Sons, Inc.,  |c 2017. 
300 |a xvi, 360 pages :  |b illustrations ;  |c 29 cm. 
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337 |a unmediated  |b n  |2 rdamedia. 
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490 1 |a Geophysical monograph ;  |v 230. 
500 |a "This work is a co-publication of the American Geophysical Union and John Wiley and Sons, Inc." 
504 |a Includes bibliographical references and index. 
505 0 |a External contributions to dawn-dusk asymmetries. The magnetosphere of the earth under sub-Alfvénic solar wind conditions as observed on 24 and 25 May 2002 / Emmanuel Chané, Joachim Saur, Joachim Raeder, Fritz M. Neubauer, Kristofor M. Maynard, and Stefaan Poedts -- Dayside magnetosphere response to solar wind dynamic pressure changes : propagation geometry and speed / Brian J. Jackel and Konstantin Kabin -- Magnetopause plasma parameters and asymmetries in solar wind-magnetosphere coupling / Brian M. Walsh -- Large-scale simulations of solar wind ion entry and dayside precipitation : dawn-dusk asymmetry / Jean Berchem, Robert L. Richard, C. Philippe Escoubet, Simon Wing, and Frederic Pitout -- Dawn-dusk asymmetries of the earth's dayside magnetosheath in the magnetosheath interplanetary medium reference frame / A.P. Dimmock, K. Nykyri, A. Osmane, H. Karimabadi, and T.I. Pulkkinen -- Dawn-dusk asymmetries at the terrestrial magnetopause : observations / Stein Haaland, Hiroshi Hasegawa, Johan De Keyser, and Lukas Maes -- Magnetopause thickness at the dawn and dusk flanks / Johan De Keyser, Lukas Maes, Romain Maggiolo, and Stein Haaland -- On IMF By-induced dawn-dusk asymmetries in earthward convective fast flows / TImo Pitkänen, Maria Hamrin, Tomas Karlsson, Hans Nilsson, and Anita Kullen -- Time-dependence of dawn-dusk asymmetries in the terrestrial ionospheric convection pattern / Adrian Grocott -- The role of the upper atmosphere for dawn-dusk differences in the coupled magnetosphere-ionosphere-thermosphere system / Matthias Förster, Eelco Doornbos, and Stein Haaland -- Surveys of 557.7/630.0 nm dayside auroral emissions in Ny-Ålesund, Svalbard, and South Pole Station / Ze-Jun Hu, Hui-Gen Yang, Yusuke Ebihara, Hong-Qiao Hu, and Bei-Chen Zhang -- Internal contributions to dawn-dusk asymmetries. Aspects of the morning/afternoon asymmetry of geomagnetic fluctuations / Christine Gabrielse, Andrei Runov, Vassilis Angelopoulos, Emma Spanswick, and Drew L. Turner -- Dawn-dusk asymmetries in ultra-low-frequency waves / I. Jonathan Rae -- Spatial structure and asymmetries of magnetospheric currents inferred from high-resolution empirical geomagnetic field models / Mikhail I. Sitnov, Grant K. Stephens, Nikolai A. Tsyganenko, Aleksandr Y. Ykhorskiy, Simon Wing, Haje Korth, and Brian J. Anderson -- A review of dawn-dusk asymmetries observed using the TWINS mission of opportunity / Amy M. Keesee -- Dawn-dusk asymmetries of solar-wind-magnetosphere coupling in the earth's midtail / Chih-Ping Wang, Xiaoyan Xing, T.K.M. Nakamura, Larry R. Lyons, and Vassilis Angelopoulos -- Dawn-dusk asymmetries in magnetotail transients / Andrei Runov, S. Kiehas, and S.S. Li -- Dawn-dusk asymmetries in the near-earth plasma sheet : ion observations / Elena A. Kronberg, Kun Li, Elena E. Grigorenko, Romain Maggiolo, Stein Haaland, Patrick W. Daly, and Hao Luo -- Dawn-dusk asymmetries in the auroral particle precipitation and their modulations by substorms / Simon Wing, Jay R. Johnson, and Enrico Camporeale -- Dawn-dusk asymmetries of ionospheric outflow / Kun Li, Elena A. Kronberg, Mats André, Patrick W. Daly, Yong Wei, and Stein Haaland -- Conjugate aurora location during a strong IMF By storm / William Longley, Patricia Reiff, Antoun G. Daou, and Marc Hairston -- Dawn-dusk asymmetries in auroral morphology and processes / Tomas Karlsson, Anita Kullen, and Göran Marklund -- Dawn dusk asymmetries in other planets. Dawn-dusk asymmetries in Jupiter's magnetosphere / Benjamin Palmaerts, Marissa F. Vogt, Norbert Krupp, Denis Grodent, and Bertrand Bonfond -- Local time asymmetries in Saturn's magnetosphere / James F. Carbary, Donald G. Mitchell, Abigail M. Rymer, Norbert Krupp, Doug Hamilton, Stamatios M. Krimigis, and Sarah V. Badman -- Dawn-dusk asymmetries in Mercury's magnetosphere / Torbjörn Sundberg. 
520 |a "Dawn-dusk asymmetries are ubiquitous features of the plasma environment of many of the planets in our solar system. They occur when a particular process or feature is more pronounced at one side of a planet than the other. For example, recent observations indicate that Earth's magnetopause is thicker at dawn than at dusk. Likewise, auroral breakups at Earth are more likely to occur in the pre-midnight than post-midnight sectors. Increasing availability of remotely sensed and in situ measurements of planetary ionospheres, magnetospheres and their interfaces to the solar wind have revealed significant and persistent dawn-dusk asymmetries. As yet there is no consensus regarding the source of many of these asymmetries, nor the physical mechanisms by which they are produced and maintained. Volume highlights include: A comprehensive and updated overview of current knowledge about dawn-dusk asymmetries in the plasma environments of planets in our solar system and the mechanisms behind them; Valuable contributions from internationally recognized experts, covering both observations, simulations and theories discussing all important aspects of dawn-dusk asymmetries; Space weather effects are caused by processes in space, mainly the magnetotail, and can be highly localized on ground. Knowing where the source, i.e., where dawn-dusk location is will allow for a better prediction of where the effects on ground will be most pronounced"--Provided by publisher. 
650 0 |a Magnetosphere.  |0 http://id.loc.gov/authorities/subjects/sh85079789. 
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700 1 |a Forsyth, Colin,  |e editor.  |0 http://id.loc.gov/authorities/names/nb2017025772. 
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