Published October 1984 | Version v1
Report Restricted

Study of the solar corona using radio and space observations

Creators

Description

The physics of coronal transients, the characteristics of radiation and accelerated particles at the time of flares, and the density/temperature structure of the transition region and corona and the coronal magnetic field are investigated

Availability note (English)

MF available from INIS under the Report Number; Available from NTIS, PC A03/MF A01.

Files

Restricted

The record is publicly accessible, but files are restricted to users with access.

Additional details

Publishing Information

Imprint Pagination
37 p.
Report number
N--85-11963

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
16069549
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ABSTRACTS; ASTROPHYSICS; FLUX DENSITY; MAGNETIC FIELDS; MAPS; MASERS; SOLAR CORONA; SOLAR FLARES; STAR MODELS
Descriptors DEC
AMPLIFIERS; ATMOSPHERES; ELECTRONIC EQUIPMENT; EQUIPMENT; MATHEMATICAL MODELS; MICROWAVE AMPLIFIERS; MICROWAVE EQUIPMENT; SOLAR ACTIVITY; SOLAR ATMOSPHERE; STELLAR ACTIVITY; STELLAR ATMOSPHERES; STELLAR CORONAE; STELLAR FLARES

Optional Information

Secondary number(s)
NASA-CR--174034.