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| Title: |
Gyrosynchrotron radiation formulae
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| Author(s): |
Ko, H. C.
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| Abstract: |
The wave-normal emissivity and the ray emissivity formulas for an electron moving along a helical path in a magnetoactive medium are presented. Simplified formulas for the case of an isotropic plasma are also given. Because of the helical motion of the electron, a difference exists between the radiated power per unit solid angle and the received power per unit solid angle. The relation between these two quantities in a magnetoactive medium is shown. Results are compared with those obtained by others, and the sources of discrepancies are pointed out.
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| NASA Center: |
NASA (non Center Specific)
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| Publication Date: |
JAN 1, 1973
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| Document Source: |
CASI |
| No Digital Version Available: |
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| Document ID: |
19740013343
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| Accession ID: |
74N21456
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| Publication Information: |
NASA, Washington High Energy Phenomena on the Sun, p 198-206, Number of Pages = 9 |
| Price Code: |
A02 |
| Related Information: |
Sponsored in part by AFCRL |
| Keywords: |
ELECTRON MOBILITY; EMISSION SPECTRA; HIGH ENERGY INTERACTIONS; MAGNETIC FIELDS; PLASMA DYNAMICS; APPLICATIONS OF MATHEMATICS; EQUATIONS OF MOTION; NUMERICAL ANALYSIS; WAVE EQUATIONS;
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| Notes: |
In NASA, Washington High Energy Phenomena on the Sun p 198-206 (SEE N74-21440 12-30) |
| Accessibility: |
Unclassified; No Copyright; Unlimited; Publicly available; |
| Updated/Added to NTRS: |
2006-08-02 |
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