Interplanetary magnetohydrodynamics / L.F. Burlaga.
Material type:![Text](/opac-tmpl/lib/famfamfam/BK.png)
- text
- computer
- online resource
- 1423729285
- 9781423729280
- 1601299451
- 9781601299451
- 9780195084726
- 0195084721
- 523.01/86 22
- QB790 .B79 1995eb
Item type | Home library | Collection | Call number | Materials specified | Status | Date due | Barcode | |
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OPJGU Sonepat- Campus | E-Books EBSCO | Available |
Includes bibliographical references (pages 215-241) and indexes.
1 Introduction; 2 Large-Scale Magnetic Field; 3 Large-Scale Plasma; 4 Pressure Balanced Structures; 5 Shocks; 6 Magnetic Clouds and Force-Free Magnetic Fields; 7 Corotating Streams and Interaction Regions; 8 Merged Interaction Regions; 9 Large-Scale Fluctuations; 10 Heliospheric Vortex Street; References; Author Index; Subject Index.
Data from spacecraft such as Pioneer, Vela and Voyager have revealed the interstellar medium to be a remarkable physical system, which has served as a laboratory for the study of turbulent, supersonic, ideal magnetohydrodynamic (MHD) flows. The results of these studies provided confirmation of many theoretical models of the interstellar medium.
Print version record.
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