{"product_id":"dawn-dusk-asymmetries-in-planetary-plasma-environments-isbn-9781119216322","title":"Dawn-Dusk Asymmetries in Planetary Plasma Environments","description":"\u003cp\u003e\u003cb\u003eDawn­Dusk Asymmetries in Planetary Plasma Environments\u003c\/b\u003e\u003c\/p\u003e \u003cp\u003eDawn-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.\u003c\/p\u003e \u003cp\u003eVolume highlights include:\u003c\/p\u003e \u003cul\u003e \u003cli\u003eA 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\u003c\/li\u003e \u003cli\u003eValuable contributions from internationally recognized experts, covering both observations, simulations and theories discussing all important aspects of dawn-dusk asymmetries\u003c\/li\u003e \u003cli\u003eSpace 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\u003c\/li\u003e \u003c\/ul\u003e \u003cp\u003eCovering both observational and theoretical aspects of dawn dusk asymmetries, \u003ci\u003eDawn­-Dusk Asymmetries in Planetary Plasma Environments\u003c\/i\u003e will be a valuable resource for academic researchers in space physics, planetary science, astrophysics, physics, geophysics and earth science.\u003c\/p\u003e \u003cp\u003eContributors vii\u003c\/p\u003e \u003cp\u003ePreface xi\u003c\/p\u003e \u003cp\u003eAcknowledgments xiii\u003c\/p\u003e \u003cp\u003eAcronyms xv\u003c\/p\u003e \u003cp\u003e\u003cb\u003ePart I: External Contributions to Dawn-Dusk Asymmetries\u003c\/b\u003e\u003c\/p\u003e \u003cp\u003e1 The Magnetosphere of the Earth under Sub-Alfvenic Solar Wind Conditions as Observed on 24 and 25 May 2002\u003cbr\u003e\u003ci\u003eEmmanuel Chane, Joachim Saur, Joachim Raeder, Fritz M  Neubauer, Kristofor M  Maynard, and Stefaan Poedts  3\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e2 Dayside Magnetosphere Response to Solar Wind Dynamic Pressure Changes: Propagation Geometry and Speed\u003cbr\u003e\u003ci\u003eBrian J  Jackel and Konstantin Kabin    15\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e3 Magnetopause Plasma Parameters and Asymmetries in Solar Wind–Magnetosphere Coupling\u003cbr\u003e\u003ci\u003eBrian M  Walsh  29\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e4 Large-Scale Simulations of Solar Wind Ion Entry and Dayside Precipitation: Dawn-Dusk Asymmetry\u003cbr\u003e\u003ci\u003eJean Berchem, Robert L  Richard, C  Philippe Escoubet, Simon Wing, and Frederic Pitout    41\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e5 Dawn-Dusk Asymmetries of the Earth’s Dayside Magnetosheath in the Magnetosheath Interplanetary Medium Reference Frame\u003cbr\u003e\u003ci\u003eA  P  Dimmock, K  Nykyri, A  Osmane, H  Karimabadi, and T  I  Pulkkinen  49\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e6 Dawn-Dusk Asymmetries at the Terrestrial Magnetopause: Observations\u003cbr\u003e\u003ci\u003eStein Haaland, Hiroshi Hasegawa, Johan De Keyser, and Lukas Maes 73\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e7 Magnetopause Thickness at the Dawn and Dusk Flanks\u003cbr\u003e\u003ci\u003eJohan De Keyser, Lukas Maes, Romain Maggiolo, and Stein Haaland  85\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e8 On IMF By-Induced Dawn-Dusk Asymmetries in Earthward Convective Fast Flows\u003cbr\u003e\u003ci\u003eTimo Pitkanen, Maria Hamrin, Tomas Karlsson, Hans Nilsson, and Anita Kullen  95\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e9 Time-Dependence of Dawn-Dusk Asymmetries in the Terrestrial Ionospheric Convection Pattern\u003cbr\u003e\u003ci\u003eAdrian Grocott  107\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e10 The Role of the Upper Atmosphere for Dawn-Dusk Differences in the Coupled Magnetosphere-Ionosphere-Thermosphere System\u003cbr\u003e\u003ci\u003eMatthias Forster, Eelco Doornbos, and Stein Haaland 125\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e11 Surveys of 557    7\/630    0 nm Dayside Auroral Emissions in\u003cbr\u003e\u003ci\u003eNy\u003c\/i\u003e\u003ci\u003e-\u003c\/i\u003e\u003ci\u003eÅ\u003c\/i\u003e\u003ci\u003elesund, Svalbard, and South Pole Station Ze\u003c\/i\u003e\u003ci\u003e-\u003c\/i\u003e\u003ci\u003eJun Hu, Hui\u003c\/i\u003e\u003ci\u003e-\u003c\/i\u003e\u003ci\u003eGen Yang, Yusuke Ebihara, Hong\u003c\/i\u003e\u003ci\u003e-\u003c\/i\u003e\u003ci\u003eQiao Hu, and Bei\u003c\/i\u003e\u003ci\u003e-\u003c\/i\u003e\u003ci\u003eChen Zhang 143\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e\u003cb\u003ePart II: Internal Contributions to Dawn-Dusk Asymmetries\u003c\/b\u003e\u003c\/p\u003e \u003cp\u003e12 Aspects of the Morning\/Afternoon Asymmetry of Geomagnetic Fluctuations at Middle and Low Frequencies\u003cbr\u003e\u003ci\u003eUmberto Villante 157\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e13 Premidnight Preponderance of Dispersionless Ion and Electron Injections\u003cbr\u003e\u003ci\u003eChristine Gabrielse, Andrei Runov, Vassilis Angelopoulos, Emma Spanswick, and Drew L  Turner 171\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e14 Dawn-Dusk Asymmetries in Ultra-Low-Frequency Waves\u003cbr\u003e\u003ci\u003eI  Jonathan Rae  187\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e15 Spatial Structure and Asymmetries of Magnetospheric Currents Inferred from High-Resolution Empirical Geomagnetic Field Models\u003cbr\u003e\u003ci\u003eMikhail I  Sitnov, Grant K  Stephens, Nikolai A  Tsyganenko, Aleksandr Y  Ukhorskiy, Simon Wing, Haje Korth, and Brian J  Anderson  199\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e16 A Review of Dawn-Dusk Asymmetries Observed Using the TWINS Mission of Opportunity\u003cbr\u003e\u003ci\u003eAmy M  Keesee  213\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e17 Dawn-Dusk Asymmetries of Solar-Wind–Magnetosphere Coupling in the Earth’s Midtail\u003cbr\u003e\u003ci\u003eChih\u003c\/i\u003e\u003ci\u003e-\u003c\/i\u003e\u003ci\u003ePing Wang, Xiaoyan Xing, T  K  M  Nakamura, Larry R  Lyons, and Vassilis Angelopoulos\u003c\/i\u003e \u003ci\u003e223\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e18 Dawn-Dusk Asymmetries in Magnetotail Transients\u003cbr\u003e\u003ci\u003eAndrei Runov, S  Kiehas, and S  S  Li 233\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e19 Dawn-Dusk Asymmetries in the Near-Earth Plasma Sheet: Ion Observations\u003cbr\u003e\u003ci\u003eElena A  Kronberg, Kun Li, Elena E  Grigorenko, Romain Maggiolo, Stein Haaland, Patrick W\u003c\/i\u003e  \u003ci\u003eDaly, and Hao Luo 243\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e20 Dawn-Dusk Asymmetries in the Auroral Particle Precipitation and Their Modulations by Substorms\u003cbr\u003e\u003ci\u003eSimon Wing, Jay R  Johnson, and Enrico Camporeale  255\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e21 Dawn-Dusk Asymmetries of Ionospheric Outflow\u003cbr\u003e\u003ci\u003eKun Li, Elena A  Kronberg, Mats Andre, Patrick W  Daly, Yong Wei, and Stein Haaland  273\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e22 Conjugate Aurora Location During a Strong IMF By Storm\u003cbr\u003e\u003ci\u003eWilliam Longley, Patricia Reiff, Antoun G  Daou, and Marc Hairston 285\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e23 Dawn-Dusk Asymmetries in Auroral Morphology and Processes\u003cbr\u003e\u003ci\u003eTomas Karlsson, Anita Kullen, and Goran Marklund  295\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e\u003cb\u003ePart III: Dawn Dusk Asymmetries in Other Planets\u003c\/b\u003e\u003c\/p\u003e \u003cp\u003e24 Dawn-Dusk Asymmetries in Jupiter’s Magnetosphere\u003cbr\u003e\u003ci\u003eBenjamin Palmaerts, Marissa F  Vogt, Norbert Krupp, Denis Grodent, and Bertrand Bonfond 309\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e25 Local Time Asymmetries in Saturn’s Magnetosphere\u003cbr\u003e\u003ci\u003eJames F  Carbary, Donald G  Mitchell, Abigail M  Rymer, Norbert Krupp, Doug Hamilton, Stamatios M  Krimigis, and Sarah V  Badman 323\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e26 Dawn-Dusk Asymmetries in Mercury’s Magnetosphere\u003cbr\u003e\u003ci\u003eTorbjorn Sundberg 337\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003eIndex 349\u003c\/p\u003e   \u003cp\u003e\u003cstrong\u003eStein Haaland,\u003c\/strong\u003e\u003cem\u003e University of Bergen, Norway\u003c\/em\u003e\u003cbr\u003e   \u003cstrong\u003eAndrei Runov, \u003c\/strong\u003e\u003cem\u003eUniversity of California, Los Angeles, USA\u003c\/em\u003e\u003cbr\u003e \u003cstrong\u003eColin Forsyth, \u003c\/strong\u003e\u003cem\u003eUniversity College London, UK\u003c\/em\u003e     \u003c\/p\u003e\u003cp\u003e 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.  \u003c\/p\u003e\u003cp\u003e 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.  \u003c\/p\u003e\u003cp\u003e Volume highlights include:  \u003c\/p\u003e\u003cul\u003e \u003cli\u003eA comprehensive overview of mechanisms and current knowledge about dawn-dusk asymmetries in the plasma environments of planets in our solar system\u003c\/li\u003e \u003cli\u003eValuable contributions from internationally recognized experts, covering observations, simulations and theories on all important aspects of dawn-dusk asymmetries\u003c\/li\u003e \u003cli\u003eDiscussions of space weather effects caused by dawn-dusk asymmetries\u003c\/li\u003e \u003c\/ul\u003e \u003cem\u003e\u003cbr\u003e  \u003c\/em\u003e \u003cp\u003e\u003cem\u003e Dawn-Dusk Asymmetries in Planetary Plasma Environments\u003c\/em\u003e is a valuable resource for academic researchers in space physics, planetary science, astrophysics, physics, geophysics, and earth science.\u003c\/p\u003e","brand":"American Geophysical Union","offers":[{"title":"Default Title","offer_id":47989027078373,"sku":"NP9781119216322","price":224.95,"currency_code":"USD","in_stock":false}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/1842\/7735\/files\/9781119216322.jpg?v=1761782496","url":"https:\/\/k12savings.com\/products\/dawn-dusk-asymmetries-in-planetary-plasma-environments-isbn-9781119216322","provider":"K12savings","version":"1.0","type":"link"}