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Chromospheric Fine Structure
Overview of attention for book
Table of Contents
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Book Overview
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Chapter 1
Spicules and Their Surroundings
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Chapter 2
Radiation Pressure in Stellar Atmospheres with Application to Solar Spicules
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Chapter 3
Chromospheric Fine Structures near the Solar Limb in H α
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Chapter 4
Recent Developments in Improving Daytime Angular Resolution from the Ground
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Chapter 5
Spatial and Spectral Structure of Chromospheric Lines
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Chapter 6
Why the Chromosphere has Its Discrete Fine Structure
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Chapter 7
Properties of the Solar Filigree Structure
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Chapter 8
Spicules are Bright and Dark
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Chapter 9
High Resolution Spectroscopy of the Disk Chromosphere
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Chapter 10
Comparison of H α and Ca ii H and K Spectro-heliograms as a Diagnostic Probe
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Chapter 11
Fine Structure of the Sun at Centimeter Wavelengths
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Chapter 12
Fine Structure of the Upper Chromosphere
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Chapter 13
Further Observations of the Structure of the Chromosphere-Corona Transition Region from Limb and Disk Intensities
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Chapter 14
Non-Static Structure of the Chromosphere-Corona Transition Region
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Chapter 15
On the Design of Chromospheric Models
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Chapter 16
Motions of Chromospheric Fine Structures
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Chapter 17
Waves and Oscillations in the Chromosphere in Active and Quiet Regions
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Chapter 18
Chromospheric Oscillations in Plages
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Chapter 19
Trapped Oscillations in the Chromosphere in the Presence of a Magnetic Field
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Chapter 20
The Magnetic Structure of Plages
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Chapter 21
On Facular Models
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Chapter 22
A Facula Model and Its Application to Facula Fine Structures
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Chapter 23
The Relation between Chromospheric and Photospheric Structures in Sunspot Groups
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Chapter 24
The Structure of the Prominence-Corona Interface
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Chapter 25
Helical Field Lines in an Erupting Filament
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Chapter 26
Streaming Magnetic Features near Sunspots
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Chapter 27
On the Relation between Moving Magnetic Features and the Decay Rates of Sunspots
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Chapter 28
A Theoretical Model for the Convection of Magnetic Flux in and near Sunspots
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Chapter 29
Evolution of Chromospheric Fine Structures on the Disk
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Chapter 30
Evolution of Structures in the Bright H α Network
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Chapter 31
H α Fine Structure and the Dynamics of the Solar Atmosphere
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Chapter 32
The Chromospheric Energy Balance
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Chapter 33
Ray Trapping in Stellar Envelopes, Pulsational Instabilities and Heating of External Layers
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Chapter 34
A Magnetic Model of the Chromosphere-Corona Transition Region
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Chapter 35
Excess Heating of Corona and Chromosphere above Magnetic Regions by Non-Linear Alfvén Waves
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Chapter 36
The Stability of a Magnetic Flux Rope and Its Relation to Sunspots, Faculae and Flares
Overall attention for this book and its chapters
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Mentioned by
syllabi
1
institution with syllabi
Citations
dimensions_citation
30
Dimensions
Book overview
1. Spicules and Their Surroundings
2. Radiation Pressure in Stellar Atmospheres with Application to Solar Spicules
3. Chromospheric Fine Structures near the Solar Limb in H α
4. Recent Developments in Improving Daytime Angular Resolution from the Ground
5. Spatial and Spectral Structure of Chromospheric Lines
6. Why the Chromosphere has Its Discrete Fine Structure
7. Properties of the Solar Filigree Structure
8. Spicules are Bright and Dark
9. High Resolution Spectroscopy of the Disk Chromosphere
10. Comparison of H α and Ca ii H and K Spectro-heliograms as a Diagnostic Probe
11. Fine Structure of the Sun at Centimeter Wavelengths
12. Fine Structure of the Upper Chromosphere
13. Further Observations of the Structure of the Chromosphere-Corona Transition Region from Limb and Disk Intensities
14. Non-Static Structure of the Chromosphere-Corona Transition Region
15. On the Design of Chromospheric Models
16. Motions of Chromospheric Fine Structures
17. Waves and Oscillations in the Chromosphere in Active and Quiet Regions
18. Chromospheric Oscillations in Plages
19. Trapped Oscillations in the Chromosphere in the Presence of a Magnetic Field
20. The Magnetic Structure of Plages
21. On Facular Models
22. A Facula Model and Its Application to Facula Fine Structures
23. The Relation between Chromospheric and Photospheric Structures in Sunspot Groups
24. The Structure of the Prominence-Corona Interface
25. Helical Field Lines in an Erupting Filament
26. Streaming Magnetic Features near Sunspots
27. On the Relation between Moving Magnetic Features and the Decay Rates of Sunspots
28. A Theoretical Model for the Convection of Magnetic Flux in and near Sunspots
29. Evolution of Chromospheric Fine Structures on the Disk
30. Evolution of Structures in the Bright H α Network
31. H α Fine Structure and the Dynamics of the Solar Atmosphere
32. The Chromospheric Energy Balance
33. Ray Trapping in Stellar Envelopes, Pulsational Instabilities and Heating of External Layers
34. A Magnetic Model of the Chromosphere-Corona Transition Region
35. Excess Heating of Corona and Chromosphere above Magnetic Regions by Non-Linear Alfvén Waves
36. The Stability of a Magnetic Flux Rope and Its Relation to Sunspots, Faculae and Flares
Summary
Syllabi
Dimensions citations
This data is correct as of December 2015 - for more up to date information, please visit
https://opensyllabus.org/
So far, Altmetric has seen this research output assigned in
1
syllabus from an institution on Open Syllabus Project.
Institution
Syllabi count
Course subject areas covered
Utrecht University
1
Unknown