Solar dynamics and its effects on the heliosphere and earth

The SOHO and Cluster missions form a single ESA cornerstone. Yet they observe very different regions in our solar system: the solar atmosphere on one hand and the Earth's magnetosphere on the other. At the same time the Ulysses mission provides observations in the third dimension of the heliosp...

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Egile nagusia: Baker, Delbert, 1947-...., astrophysicien
Beste egile batzuk: Klecker, Bernt (Argitalpenaren zuzendaria), Schwartz, Steven Jay, 1951-...., astrophysicien (Argitalpenaren zuzendaria), Schwenn, Rainer, 1941- (Argitalpenaren zuzendaria), Steiger, Rudolf von, 1957- (Argitalpenaren zuzendaria)
Formatua: Livre numérique
Hizkuntza:Anglais
Argitaratua: New York, NY : Springer New York [20..].
Cham : Springer Nature
Edizioa:1st ed. 2007.
Saila:Space Sciences Series of ISSI 22
Sarrera elektronikoa:Accès sur la plateforme de l'éditeur
Accès sur la plateforme Istex
Accès Université d'Orléans
Accès INSA CVL
Oharra: Archives Springer e-books (Licence nationale)
Archives Springer e-books (Licence nationale)
Autres localisations: Voir dans le Sudoc
Edition sous un autre format:• Solar Dynamics and its Effects on the Heliosphere and Earth, Texte imprimé, 9780387517698
• Solar Dynamics and its Effects on the Heliosphere and Earth, Texte imprimé, 9781441924117
• Solar dynamics and its effects on the heliosphere and earth, edited by D.N. Baker, B. Klecker, S. J. Schwartz... [et al.], Dordrecht, Springer, 2007, 1 vol. (viii-372 p.), Space sciences series of ISSI, 978-0-387-69531-0
• Solar Dynamics and its Effects on the Heliosphere and Earth, Texte imprimé, 9780387517698
• Solar Dynamics and its Effects on the Heliosphere and Earth, Texte imprimé, 9781441924117
• Solar dynamics and its effects on the heliosphere and earth, edited by D.N. Baker, B. Klecker, S. J. Schwartz... [et al.], Dordrecht, Springer, 2007, 1 vol. (viii-372 p.), Space sciences series of ISSI, 978-0-387-69531-0
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100 1 |a Baker, Delbert,  |d 1947-....,  |c astrophysicien. 
245 1 0 |a Solar dynamics and its effects on the heliosphere and earth   |c edited by D. N. Baker, B. Klecker, S. J. Schwartz, R. Schwenn, R. Steiger. 
250 |a 1st ed. 2007. 
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505 1 |a Solar Dynamics Active Region Dynamics Sunspot Structure and Dynamics Coronal Dynamics and the AIA on SDO Wind in the Solar Corona: Dynamics and Composition Solar Wind Chain Solar Wind Sources and Their Variations over the Solar Cycle Heliospheric Physics: Linking the Sun to the Magnetosphere Substorms and Their Solar Wind Causes Modeling of the Magnetospheric Response to the Dynamic Solar Wind Review of Ionospheric Effects of Solar Wind Magnetosphere Coupling in the Context of the Expanding Contracting Polar Cap Boundary Model CME Chain The Evolving Sigmoid: Evidence for Magnetic Flux Ropes in the Corona Before, During, and after CMES Properties of Interplanetary Coronal Mass Ejections Geoeffectivity of Coronal Mass Ejections Ring Current Dynamics Plasmasphere Response: Tutorial and Review of Recent Imaging Results End-to-End Modeling of the Solar Terrestrial System SEP Chain Particle Acceleration by the Sun: Electrons, Hard X-Rays/Gamma-Rays Particle Acceleration in a Three-Dimensional Model of Reconnecting Coronal Magnetic Fields The Seed Population for Energetic Particles Accelerated By CME-Driven Shocks Acceleration of Solar-Energetic Particles by Shocks Solar Energetic Particle Charge States: An Overview Solar Energetic Particle Composition, Energy Spectra, and Space Weather Commonalities Commonalities Between Ionosphere and Chromosphere Shocks: Commonalities in Solar-Terrestrial Chains Theory and Simulation of Reconnection The Localization of Particle Acceleration Sites in Solar Flares and CMEs. 
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520 |a The SOHO and Cluster missions form a single ESA cornerstone. Yet they observe very different regions in our solar system: the solar atmosphere on one hand and the Earth's magnetosphere on the other. At the same time the Ulysses mission provides observations in the third dimension of the heliosphere, and many others add to the picture from the Lagrangian point L1 to the edge of the heliosphere. It is the aim of this ISSI volume to tie these observations together in addressing the topic of Solar Dynamics and its Effects on the Heliosphere and Earth, thus contributing to the International Living With a Star (ILWS) program. The volume starts out with an assessment and description of the reasons for solar dynamics and how it couples into the heliosphere. The three subsequent sections are each devoted to following one chain of events from the Sun all the way to the Earth's magnetosphere and ionosphere: The normal solar wind chain, the chain associated with coronal mass ejections, and the solar energetic particles chain. The final section is devoted to common physical processes occurring both at the Sun and in the magnetosphere such as reconnection, shock acceleration, dipolarisation of magnetic field, and others. 
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700 1 |a Schwartz, Steven Jay,  |d 1951-....,  |c astrophysicien.  |4 pbd 
700 1 |a Schwenn, Rainer,  |d 1941-  |4 pbd 
700 1 |a Steiger, Rudolf von,  |d 1957-  |4 pbd 
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