Published December 1, 1974
| Version v1
Journal article
Interplanetary sector structure: 1970--1972
Description
IMP-3 i n t h e l a t t e r half of 1965 are discussed with r e l a t i o n t o previQus s a t e l l i t e observations of t h e interplanetary f i e l d . The seetor property remains a prominent feature of the observations, with t h e average f i e l d d i r e c t i o n a t t h e Archimedes spiral angle. The sector p a t t e r n has a 27-day recurrence period from 1962 t o 1964, and during the year 1964 the p a t t e r n appears t o be quasi-stable. I n 1965 the recurrence period is about 28 days, and the evolution of t h e p a t t e r n is more rapid, with new sectors appearing and expanding.
Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Geophysical Research
- Journal Volume
- 79
- Journal Issue
- 34
- Series
- J. Geophys. Res.
- Journal Page Range
- 5089-5094
- ISSN
- 0148-0227
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 6188846
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- INTERPLANETARY MAGNETIC FIELDS; SOLAR CYCLE; ZONES
- Descriptors DEC
- MAGNETIC FIELDS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent