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Solar Prominences

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Cover of 'Solar Prominences'

Table of Contents

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    Book Overview
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    Chapter 1 Historical Background and Introduction
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    Chapter 2 Description and Classification of Prominences
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    Chapter 3 Spectral Diagnostics of Cool Prominence and PCTR Optically Thin Plasmas
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    Chapter 4 Derivations and Observations of Prominence Bulk Motions and Mass
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    Chapter 5 Radiative Transfer in Solar Prominences
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    Chapter 6 Derivation of the Major Properties of Prominences Using NLTE Modelling
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    Chapter 7 Energy Balance
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    Chapter 8 Magnetometry of Prominences
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    Chapter 9 The Magnetic Field Structure of Prominences from Direct and Indirect Observations
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    Chapter 10 Plasma Structure and Dynamics
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    Chapter 11 Magnetism and Dynamics of Prominences: MHD Waves
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    Chapter 12 MHD Equilibria and Triggers for Prominence Eruption
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    Chapter 13 Coronal Cavities: Observations and Implications for the Magnetic Environment of Prominences
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    Chapter 14 Formation and Large-Scale Patterns of Filament Channels and Filaments
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    Chapter 15 The dynamics of eruptive prominences
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    Chapter 16 Eruptive Prominences and Their Association with Coronal Mass Ejections
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    Chapter 17 Eruptive Prominences and Their Impact on the Earth and Our Life
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    Chapter 18 Stellar Activity and CMEs: Important Factors of Planetary Evolution
Attention for Chapter 6: Derivation of the Major Properties of Prominences Using NLTE Modelling
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Chapter title
Derivation of the Major Properties of Prominences Using NLTE Modelling
Chapter number 6
Book title
Solar Prominences
Published in
ADS, January 2015
DOI 10.1007/978-3-319-10416-4_6
Book ISBNs
978-3-31-910415-7, 978-3-31-910416-4
Authors

Nicolas Labrosse

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Mendeley readers

The data shown below were compiled from readership statistics for 1 Mendeley reader of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Unknown 1 100%

Demographic breakdown

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

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