Dawn?dusk asymmetries in the coupled solar wind?magnetosphere?ionosphere system: a review

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F14%3A00431936" target="_blank" >RIV/68378289:_____/14:00431936 - isvavai.cz</a>

Výsledek na webu

<a href="http://dx.doi.org/10.5194/angeo-32-705-2014" target="_blank" >http://dx.doi.org/10.5194/angeo-32-705-2014</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.5194/angeo-32-705-2014" target="_blank" >10.5194/angeo-32-705-2014</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Dawn?dusk asymmetries in the coupled solar wind?magnetosphere?ionosphere system: a review

Popis výsledku v původním jazyce

Dawn?dusk asymmetries are ubiquitous features of the coupled solar-wind?magnetosphere?ionosphere system. During the last decades, increasing availability of satellite and ground-based measurements has made it possible to study these phenomena in more detail. Numerous publications have documented the existence of persistent asymmetries in processes, properties and topology of plasma structures in various regions of geospace. In this paper, we present a review of our present knowledge of some of the mostpronounced dawn?dusk asymmetries. We focus on four key aspects: (1) the role of external influences such as the solar wind and its interaction with the Earth?s magnetosphere; (2) properties of the magnetosphere itself; (3) the role of the ionosphere and(4) feedback and coupling between regions. We have also identified potential inconsistencies and gaps in our understanding of dawn?dusk asymmetries in the Earth?s magnetosphere and ionosphere.

Název v anglickém jazyce

Dawn?dusk asymmetries in the coupled solar wind?magnetosphere?ionosphere system: a review

Popis výsledku anglicky

Dawn?dusk asymmetries are ubiquitous features of the coupled solar-wind?magnetosphere?ionosphere system. During the last decades, increasing availability of satellite and ground-based measurements has made it possible to study these phenomena in more detail. Numerous publications have documented the existence of persistent asymmetries in processes, properties and topology of plasma structures in various regions of geospace. In this paper, we present a review of our present knowledge of some of the mostpronounced dawn?dusk asymmetries. We focus on four key aspects: (1) the role of external influences such as the solar wind and its interaction with the Earth?s magnetosphere; (2) properties of the magnetosphere itself; (3) the role of the ionosphere and(4) feedback and coupling between regions. We have also identified potential inconsistencies and gaps in our understanding of dawn?dusk asymmetries in the Earth?s magnetosphere and ionosphere.

Druh

J_x - Nezařazeno - Článek v odborném periodiku (Jimp, Jsc a Jost)

CEP obor

BN - Astronomie a nebeská mechanika, astrofyzika

OECD FORD obor

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Projekt

<a href="/cs/project/GAP209%2F12%2F2394" target="_blank" >GAP209/12/2394: Úloha nízkofrekvenčních plazmových vln v globální dynamice planetárních magnetosfér</a><br>

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2014

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Annales Geophysicae

ISSN

0992-7689

e-ISSN

—

Svazek periodika

32

Číslo periodika v rámci svazku

7

Stát vydavatele periodika

DE - Spolková republika Německo

Počet stran výsledku

33

Strana od-do

705-737

Kód UT WoS článku

000339938200001

EID výsledku v databázi Scopus

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