Fragmented Energy Release in Sun and Stars The Interface between MHD and Plasma Physics
Magnetic energy release plays an important role in a wide variety of cosmic objects such as the Sun, stellar coronae, stellar and galactic accretion disks and pulsars. The observed radio, X-ray and gamma-ray emission often directly results from magnetic `flares', implying that these processes a...
| Other Authors: | |
|---|---|
| Format: | eBook |
| Language: | English |
| Published: |
Dordrecht
Springer Netherlands
1994, 1994
|
| Edition: | 1st ed. 1994 |
| Subjects: | |
| Online Access: | |
| Collection: | Springer Book Archives -2004 - Collection details see MPG.ReNa |
Table of Contents:
- Studies of Anomalous Potential Drops Due to Ion Density Inhomogeneities
- 2 Fragmented Solar Emission
- Observations of Fragmented Energy Release
- Imaging Diagnostics of Solar Non-Thermal Particles
- Cyclotron Masers and Solar Spike Bursts
- Chaos Theory and Radio Emission
- On Deterministic Chaos, Stationarity Periodicity and Intermittency in Coronal Bursts and Flares
- Periodic or Random Acceleration in Solar Flares?
- Radio Emission from Quasi-parallel Shock Waves in the Corona
- Microwave Bursts of November 17, 1991: Evidence of Fragmented Particle Injection into a Coronal Loop
- Evidence for a Common Source of Fragmented Decimeter Emission and Meter Wave Type II Bursts in Some Solar Type IV Bursts
- Thermal and Nonthermal Flare Emission Observed with the Nobeyama Radio Heliograph
- Thermal Cyclotron Radiation from aHot Coronal Loop with Helical Magnetic Field
- Fine Scale Temporal Structures in Solar Hard X-ray Bursts Observed by PHEBUS
- Modelling Particle Transport with Stochastic Simulations
- Transition Radio Emission of Mildly Relativistic Particles
- Analysis of Solar Spike Events by Means of Symbolic Dynamics Methods
- Multiple Frequency Spike Emission During Solar Flares
- Radio Evidence of Long Lasting Release of Nonthermal Energy in the Solar Corona
- SSRT: First Results of Millisecond Spike Observations
- Discrete Energy Release in Microwave Emission in the Preflare Stage
- Microwave Spectrum Analysis as Solar Energy Release Diagnostics
- 3 Stars
- Stellar Flares
- Radiation-Driven Diskons: an Overview
- First Millimetric Detections of AE Aquarii
- Variability and Origin of Permanent Radio Emission in RS CVn and Algol Type Binaries
- 4 Stellar and Galactic Accretion Disks
- Energy Release in Stellar Magnetospheres
- Magnetic Energy Release near Accreting Black Holes
- Dissipation of Magnetic Fields in Active Galactic Nuclei
- Distribution and Flow of Magnetic Energy in an Accretion Disk
- 1 Energy Release Processes
- Coronal Heating by Dissipation of Magnetic Structure
- Reconnective Release of Magnetic Energy in Astrophysical Plasmas
- Energy Release in Double Layers
- Theory of Fragmented Energy Release in the Sun
- Alfvén Wave Heating
- Low Frequency Turbulence and Energy Dissipation in the Solar Wind
- Dynamic Behavior and Topology of 3D Magnetic Fields
- Detailed Magnetic Structure and Stochastic Threshold
- Current Dissipation within the Chromosphere-Corona Transition
- Spatial Fragmentation of Solar Flare Plasma and Beams
- Nanoflares and Current Sheet Dissipation
- 3D Nonlinear Wave Heating of Coronal Loops
- Nonlinear Dust Alfvén Modes
- The Role of Vorticity in 3D Magnetic Field Annihilation
- Particle Orbits near a Neutral Point
- Electron Beam Propagation in the Solar Corona
- MHD Waves in Coronal Flux Tubes
- Heating of the Solar Corona by Alfvén Wave Envelopes
- Observational Support of Reconnection in Solar Flares
- Slender Fluxtubes in Accretion Disks
- A Magnetic Explanation for the Rapid Burster
- 5 Pulsars
- Electric Gaps in Pulsar Magnetospheres
- Radiative Properties of Pulsar Magnetospheres
- Pulsar Radio Emission
- Pair Creation in Double Layers
- Linear Acceleration Emission in a Strong Electric Field
- Closing Lecture
- Closing Address
- Author index