Dawn-Dusk Asymmetries in Planetary Plasma Environments / Geophysical Monograph Series Bd.1 (PDF)
(Sprache: Englisch)
Dawn-Dusk Asymmetries in Planetary Plasma Environments
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...
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...
sofort als Download lieferbar
eBook (pdf)
176.99 €
- Lastschrift, Kreditkarte, Paypal, Rechnung
- Kostenloser tolino webreader
Produktdetails
Produktinformationen zu „Dawn-Dusk Asymmetries in Planetary Plasma Environments / Geophysical Monograph Series Bd.1 (PDF)“
Dawn-Dusk Asymmetries in Planetary Plasma Environments
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
Covering both observational and theoretical aspects of dawn dusk asymmetries, Dawn--Dusk Asymmetries in Planetary Plasma Environments will be a valuable resource for academic researchers in space physics, planetary science, astrophysics, physics, geophysics and earth science.
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
Covering both observational and theoretical aspects of dawn dusk asymmetries, Dawn--Dusk Asymmetries in Planetary Plasma Environments will be a valuable resource for academic researchers in space physics, planetary science, astrophysics, physics, geophysics and earth science.
Autoren-Porträt
Stein Haaland, University of Bergen, NorwayAndrei Runov, University of California, Los Angeles, USA
Colin Forsyth, University College London, UK
Bibliographische Angaben
- 2017, 1. Auflage, 376 Seiten, Englisch
- Herausgegeben: Stein Haaland, Andrei Runov, Colin Forsyth
- Verlag: John Wiley & Sons
- ISBN-10: 1119216516
- ISBN-13: 9781119216513
- Erscheinungsdatum: 04.10.2017
Abhängig von Bildschirmgröße und eingestellter Schriftgröße kann die Seitenzahl auf Ihrem Lesegerät variieren.
eBook Informationen
- Dateiformat: PDF
- Größe: 50 MB
- Mit Kopierschutz
Sprache:
Englisch
Kopierschutz
Dieses eBook können Sie uneingeschränkt auf allen Geräten der tolino Familie lesen. Zum Lesen auf sonstigen eReadern und am PC benötigen Sie eine Adobe ID.
Kommentar zu "Dawn-Dusk Asymmetries in Planetary Plasma Environments / Geophysical Monograph Series Bd.1"
0 Gebrauchte Artikel zu „Dawn-Dusk Asymmetries in Planetary Plasma Environments / Geophysical Monograph Series Bd.1“
Zustand | Preis | Porto | Zahlung | Verkäufer | Rating |
---|
Schreiben Sie einen Kommentar zu "Dawn-Dusk Asymmetries in Planetary Plasma Environments / Geophysical Monograph Series Bd.1".
Kommentar verfassen