Published May 1995
| Version v1
Journal article
Determination of the energy of the proton beam formed in a solar flare on the basis of spectropolarimetric data
- 1. St. Petersburg State Univ. (Russian Federation)
- 2. Russian Institute of Solar and Earth Physics, Irkutsk (Russian Federation)
Description
Energy contributions of proton beams to the chromospheric region of a solar flare are determined by the spectropolarimetry technique under the assumption of an impact character of the observed Hα hydrogen line emission. 10 refs., 6 figs., 3 tabs
Additional details
Publishing Information
- Journal Title
- Optics and Spectroscopy
- Journal Volume
- 78
- Journal Issue
- 5
- Journal Page Range
- p. 655-662.
- ISSN
- 0030-400X
- CODEN
- OPSUA3
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 27016992
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Resource subtype / Literary indicator
- Translation
- Descriptors DEI
- CHROMOSPHERE; EMISSION SPECTRA; ENERGY TRANSFER; HYDROGEN; POLARIMETRY; PROTON BEAMS; SCATTERING AMPLITUDES; SOLAR FLARES
- Descriptors DEC
- AMPLITUDES; ATMOSPHERES; BEAMS; ELEMENTS; NONMETALS; NUCLEON BEAMS; PARTICLE BEAMS; SOLAR ACTIVITY; SOLAR ATMOSPHERE; SPECTRA; STELLAR ACTIVITY; STELLAR ATMOSPHERES; STELLAR FLARES
Optional Information
- Notes
- Cover-to-cover Translation of Optika i Spektroskopiya (USSR); Translated from Optika i Spektroskopiya; 78: No. 5, 729-737(1995).