Cosmic Plasma Physics [E-Book] : Proceedings of the Conference on Cosmic Plasma Physics Held at the European Space Research Institute (ESRIN), Frascati, Italy, September 20–24, 1971 / edited by Karl Schindler.
The plan to hold a conference on cosmic plasma physics originated in the Plasma Physics Division of the European Physical Society, whose chairman, B. Lehnert, took the first steps towards its realization. - ESRIN readily adopted this idea, and preliminary contacts with a number of other groups showe...
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Full text |
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Personal Name(s): | Schindler, Karl, editor |
Imprint: |
Boston, MA :
Springer,
1972
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Physical Description: |
XII, 370 p. online resource. |
Note: |
englisch |
ISBN: |
9781461567585 |
DOI: |
10.1007/978-1-4615-6758-5 |
Subject (LOC): |
- Relations between cosmic and laboratory plasma physics (IS)
- Planetary Environments
- Magnetospheric substorms (IS)
- Parametric instabilities generated in the ionosphere by intense radio waves (C)
- Study of a Jovian plasmasphere and the occurrence of Jupiter radiobursts (C)
- Effect of a large amplitude wave packet and second order resonance on the stimulation of VLF emissions (C)
- Universal instability associated with the plasmapause and its role in geomagnetic micropulsations (C)
- Deformation and striation of barium clouds in the ionosphere (C)
- Solar Wind
- Thermal energy transport in the solar wind (IS)
- The solar wind near the sun: the solar envelope (IT)
- Influence of neutral interstellar matter on the expansion of the solar wind (C)
- Hydrogen-helium expansion from the sun (C)
- Heating of the solar wind ions (C)
- On the generation of shock pairs in the solar wind (C)
- Spectral anisotropy of Alfvén waves in the solar wind (C)
- Evidence for waves and/or turbulence in the vicinity of shocks in space (C)
- Solar Wind Interaction with Planets and Comets
- Comets in the solar wind (IT)
- Comet-like interaction of Venus with the solar wind (C)
- Laboratory experiments on the interaction between a plasma and a neutral gas (IT)
- Wave motion in type I comet tails (C)
- Solar Physics
- Divers solar rotations (IS)
- Soft x-ray spectral studies of solar flare plasmas (C)
- Similarities between solar flares and laboratory hot plasma phenomena (C)
- Gyromagnetic radiation from bunched electrons (C)
- Observations of coronal magnetic field strengths and flux tubes and their stability (C)
- Stellar and Interstellar Plasma
- The dynamical behavior of the interstellar gas, fields and cosmic rays (IS)
- Stellar magnetohydrodynamics (IS)
- Plasma turbulent heating and thermal x-ray sources (IS)
- Pulsars
- Radio and optical observations of pulsars (IS)
- Propagation of relativistic electromagnetic waves in a plasma (C)
- A three-dimensional relativistic computation for the pulsar magnetosphere (C)
- On the origin of pulsar radiation (IS)
- Strong magnetic field effects in the pulsar crusts and atmospheres (C)
- General Theory
- Cosmic ray spectrum and plasma turbulence (IS)
- The properties of magnetic neutral sheet systems (IT)
- Field line motion in the presence of finite conductivity (C)
- Shock Waves, Turbulence
- Collisionless shocks (IS)
- Non-linear evolution of firehose-unstable Alfvén waves (C)
- Resonant diffusion in strongly turbulent plasmas (C)
- The structure of the earth’s bow shock (C)
- Experimental study of electron and ion heating in high-? perpendicular collisionless shock waves (C)
- Nonlinear theory of cross-field and two-stream instabilities in the equatorial electrojet (C)
- Cosmic Rays
- Fermi acceleration in interplanetary space (C)
- The galactic cosmic ray diurnal variation as a streaming plasma interaction between galactic and solar corpuscular radiation (C)
- The interplanetary conditions associated with cosmic ray Forbush decreases (C)
- The diurnal effect of cosmic rays and its dependence on the interplanetary magnetic field (C).