Published November 1979 | Version v1
Book

A synthetic explanation on solar, interplanetary, and terrestrial phenomena by means of the two-hemisphere model

  • 1. Tohoku Univ., Sendai (Japan)

Description

Three our papers on the heliomagnetosphere that were published within these four months are reviewed. Antipodal relation found in both solar M-regions and coronal hole tongues substantiates our two-hemisphere model on the three-dimensional structure of the heliomagnetosphere. Characteristics on reversals and excursions of the heliomagnetic dipole are discussed on the basis of an analysis of the K-corona, dark filament, and photospheric magnetic field. An application of the two-hemisphere model to the 27-day recurrence time patterns of the sector polarity and B sub(Z)-component of IMF, diurnal amplitude of cosmic ray intensity, geomagnetic C9 index, and geomagnetic Pc3 pulsation index enables us to explain synthetically the relations among these interplanetary and terrestrial phenomena. (author)

Additional details

Additional titles

Original title (no language)
IMS shinpojiumu.

Publishing Information

Publisher
Tokyo Univ., Inst. of Space and Aeronautical Science.
Imprint Place
Tokyo
Imprint Title
IMS (International Magnetosphere Study) symposium, 1979
Journal Page Range
p. 214-221.

Conference

Title
IMS (International Magnetosphere Study) symposium.
Dates
12 - 14 Nov 1979.
Place
Tokyo, Japan.

INIS

Country of Publication
Japan
Country of Input or Organization
Japan
INIS RN
12595372
Subject category
S58: GEOSCIENCES;
Resource subtype / Literary indicator
Conference
Descriptors DEI
INTERPLANETARY MAGNETIC FIELDS; INTERPLANETARY SPACE; SOLAR CORONA; STAR MODELS
Descriptors DEC
MAGNETIC FIELDS; MATHEMATICAL MODELS; SPACE

Optional Information

Notes
Imprint:IMS shinpojiumu.