Solar Surface Magnetism [E-Book] / edited by Robert J. Rutten, Carolus J. Schrijver.
Observations of the solar magnetic field are largely confined to the radiation emitted from the photosphere, the thin layer of the solar atmosphere which we call "the solar surface". It is from solar surface observations that we must infer the internal structure and the internal magnetohyd...
Saved in:
Full text |
|
Personal Name(s): | Rutten, Robert J., editor |
Schrijver, Carolus J., editor | |
Imprint: |
Dordrecht :
Springer,
1994
|
Physical Description: |
XI, 538 p. online resource. |
Note: |
englisch |
ISBN: |
9789401111881 |
DOI: |
10.1007/978-94-011-1188-1 |
Series Title: |
/* Depending on the record driver, $field may either be an array with
"name" and "number" keys or a flat string containing only the series
name. We should account for both cases to maximize compatibility. */?>
NATO ASI Series, Series C: Mathematical and Physical Sciences ;
433 |
Subject (LOC): |
- I. Context
- The Sun among the stars
- II. Techniques
- Recipes for solar polarimetry
- Some aspects of polarimetry with LEST
- Speckle techniques for spectroscopic observations
- The Fe I 10265 Å line as an excellent tool for magnetic field measurements
- III. Magnetic elements
- Properties of small magnetic elements
- Dynamics of small magnetic elements in a growing active region
- The upper photosphere and lower chromosphere of small-scale magnetic features
- Vector spectropolarimetry with the Advanced Stokes Polarimeter (ASP) for quantitative solar magnetometry
- Preliminary properties of pores derived from 1.56 micron lines
- The magnetic chromosphere
- Fine structures of the solar chromospheres
- Non-linearities of chromospheric oscillations
- Chromospheric oscillations
- Modelling umbrae
- Sunspot temperatures
- Interpretation of sunspot oscillations
- Dynamics of the Evershed effect
- The cause of the Evershed effect in sunspots: flows or waves?
- An analytical model for fluted sunspots and a new interpretation of Evershed flow
- Some consequences of an uncombed and inhomogeneous penumbra
- IV. Magnetic patterns
- On photospheric flows and chromospheric corks
- Large-scale photospheric motions: first results from an extraordinary eleven-hour granulation observation
- Solar magnetic fields and percolation theory
- Scaling properties of photospheric magnetic fields
- Magnetoconvective patterns
- Average east-west inclinations of surface magnetic field lines
- Magnetic field configurations basic to filament channels and filaments
- An observational and conceptual model of the magnetic field of a filament
- The solar magnetic cycle
- Cycle patterns of the axisymmetric magnetic field
- Returning to the random walk
- V. Theory of magnetoconvection
- The solar dynamo
- Dynamics of erupting magnetic flux tubes
- Theory of passive magnetic field transport
- Dynamic interaction of convection with magnetic flux sheets: first results of a new MHD code
- Magnetoconvection and magnetoturbulence
- VI. Prospects
- Solar surface magnetism: quests for observations
- The THEMIS telescope
- THEMIS polarimetry
- SOHO: science objectives and capabilities
- Author index
- Citation index.