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