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Solar journey: The significance of our galactic environment for the heliosphere and earth

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Cover of 'Solar journey: The significance of our galactic environment for the heliosphere and earth'

Table of Contents

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    Book Overview
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    Chapter 1 Introduction: Paleoheliosphere versus PaleoLISM
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    Chapter 2 Heliospheric Variation in Response to Changing Interstellar Environments
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    Chapter 3 The Influence of the Interstellar Magnetic Field on the Heliospheric Interface
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    Chapter 4 Interstellar Conditions and Planetary Magnetospheres
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    Chapter 5 Long-term Variations in the Galactic Environment of the Sun
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    Chapter 6 Short-term Variations in the Galactic Environment of the Sun
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    Chapter 7 Variations of the Interstellar Dust Distribution in the Heliosphere
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    Chapter 8 Effects in the Inner Heliosphere Caused by Changing Conditions in the Galactic Environment
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    Chapter 9 Variable Terrestrial Particle Environments During the Galactic Orbit of the Sun
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    Chapter 10 The Galactic Cosmic Ray Intensity in the Heliosphere in Response to Variable Interstellar Environments
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    Chapter 11 Accretion of Interstellar Material into the Heliosphere and onto Earth
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    Chapter 12 Variations of Galactic Cosmic Rays and the Earth's Climate
Attention for Chapter 10: The Galactic Cosmic Ray Intensity in the Heliosphere in Response to Variable Interstellar Environments
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Chapter title
The Galactic Cosmic Ray Intensity in the Heliosphere in Response to Variable Interstellar Environments
Chapter number 10
Book title
Solar journey: The significance of our galactic environment for the heliosphere and earth
Published in
ADS, January 2006
DOI 10.1007/1-4020-4557-3_10
Book ISBNs
978-1-4020-4397-0, 978-1-4020-4557-8
Authors

Vladimir Florinski, Gary P. Zank, Florinski, Vladimir, Zank, Gary P.

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Mendeley readers

Mendeley readers

The data shown below were compiled from readership statistics for 2 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Unknown 2 100%

Demographic breakdown

Readers by professional status Count As %
Professor 1 50%
Researcher 1 50%
Readers by discipline Count As %
Physics and Astronomy 2 100%

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