Physics of the Solar Corona

reportActive / Technical Report | Accession Number: AD0741000 | Open PDF

Abstract:

Progress for the year included uncompleted analysis of 1966 eclipse plates for evidence of a difference in the chemical content of coronal condensations from that in the corona in general, continued work toward interpretation of the gradient of the emission-line features in the corona, the discovery of a linear relationship between flare productivity and length of the neutral lines in the longitudinal magnetic field in active regions, and the formulation of plans to study the color of the K-corona at the March 7, 1970, eclipse.

Author(s):
Billings, Donald E.
Author Organization(s):
COLORADO UNIV AT BOULDER DEPT OF ASTRO-GEOPHYSICS
Descriptive Note:
Annual summary rept. 31 Aug 1968-31 Aug 1969
Supplementary Note:
See also AD674896. DOI: 10.21236/AD0741000
Pagination:
0007

Security Markings

DOCUMENT & CONTEXTUAL SUMMARY

Distribution:
Approved For Public Release
Distribution Statement:
Approved For Public Release; Distribution Is Unlimited.

RECORD

Collection: TR
Identifying Numbers
Contract/Grant Number(s):
N00014-67-C-0290
Project Number(s):
NR-046-740
Monitor Series:
ONR
 Subject Terms
Joint Capability Areas:
JCA_5.3_Planning; JCA_5_Command and Control; JCA_1.2_Force Preparation; JCA_1_Force Support; JCA_6_Net Centric
Communities of Interest:
No COI(s) Identified
Descriptor(s):
*SOLAR CORONA, IRON, SOLAR FLARES, ISOTOPE AVAILABILITY, SCIENTIFIC RESEARCH, MAGNETOHYDRODYNAMICS, SOLAR SPECTRUM
Field(s)/Group(s):
Astrophysics
Report Date:
1969 Aug 31