Published 1972 | Version v1
Report Metadata-only

Further results on cooling mechanisms for soft x-ray flares

Creators

  • 1. University Coll., London

Description

Two solar events with discontinuous temperature decays are analyzed. Temperatures and emission measures for both flares are derived. Cooling via radiation, conduction to chromospheric regions, and the collisional process are considered and three possibilities to explain the temperature decay are cited. (U.S.)

Additional details

Publishing Information

Imprint Title
High energy phenomena on the sun
Imprint Pagination
p. 276-282.
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
7222891
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
COLLISIONAL HEATING; COOLING; EMISSION; RADIATION HEATING; SOFT X RADIATION; SOLAR FLARES; TEMPERATURE MEASUREMENT; THERMAL CONDUCTIVITY; ULTRAHIGH TEMPERATURE
Descriptors DEC
ELECTROMAGNETIC RADIATION; HEATING; HIGH-FREQUENCY HEATING; IONIZING RADIATIONS; MAGNETIC-PUMPING HEATING; PHYSICAL PROPERTIES; PLASMA HEATING; RADIATIONS; SOLAR ACTIVITY; THERMODYNAMIC PROPERTIES; X RADIATION