Published 1972 | Version v1
Report

Gyrosynchrotron radiation formulae

Creators

  • 1. Ohio State Univ., Columbus

Description

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, one must distinguish 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. (U.S.)

Additional details

Publishing Information

Imprint Title
High energy phenomena on the sun
Imprint Pagination
p. 198-206.
Report number
N--74-21440

Conference

Title
Proceedings on high energy phenomena on the sun.
Dates
28 Sep 1972.
Place
Greenbelt, Maryland, USA.

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
7223025
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ELECTRONS; EMISSIVITY; GYROFREQUENCY; MAGNETIC FIELDS; MATHEMATICAL MODELS; PLASMA; SYNCHROTRON RADIATION
Descriptors DEC
BREMSSTRAHLUNG; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; LEPTONS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; SURFACE PROPERTIES