Magnetic field strength estimation in synchrotron radiation sources
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/BF00627086.pdf
Reference8 articles.
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2. Batchelor D.A., Benz, A.O. and Wiehl, H.J.: 1984,Astrophys. J. 280, 879.
3. Dulk, G.A. and Marsh, K.A.: 1982,Astrophys. J. 259, 350.
4. Dulk, G.A.: 1985,Ann. Rev. Astron. Astrophys. 23, 169.
5. Gary, D.: 1985,Astrophys. J. 297, 799.
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1. Harmonic Structures of Gyrosynchrotron Radiation and Cyclotron Maser Instability;Chinese Journal of Astronomy and Astrophysics;2001-08
2. Diagnostics of Magnetic Field Strength in Gyrosynchrotron Radiation Regions for the Case of Transverse Propagation;Chinese Physics Letters;2000-12-01
3. Diagnostics of magnetic field strength for gyrosynchrotron radiation regions of the lower harmonics;Chinese Science Bulletin;1998-07
4. Two sets of improved approximate expressions of the gyrosynchrotron radiation;Solar Physics;1998
5. Improved formula of coronal magnetic field strength diagnostic;Chinese Science Bulletin;1997-02
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