Hostname: page-component-745bb68f8f-cphqk Total loading time: 0 Render date: 2025-02-03T09:12:57.642Z Has data issue: false hasContentIssue false
  • English
  • Français

Classification and Investigation of Solar Flare Situations Conformably to Interplanetary and Magnetospheric Disturbances

Published online by Cambridge University Press:  14 August 2015

K. G. Ivanov ,
N. V. Mikerina  and
L. V. Evdokimova
K. G. Ivanov
Affiliation:
Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation Academy of Sciences Moscow Region, Troytsk, USSR
N. V. Mikerina
Affiliation:
Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation Academy of Sciences Moscow Region, Troytsk, USSR
L. V. Evdokimova
Affiliation:
Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation Academy of Sciences Moscow Region, Troytsk, USSR

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A new classification of large solar flares is presented. If the time spacings between the flares are over 2.5 days, the flares and the corresponding interplanetary streams are classified as isolated ones. The concepts of the nearest, intermediate and distant flare zones (N, I and D zones) are introduced. The limits of the zones are determined at 30° longitude intervals and at 15° latitude ones. The classification is applied to the flares of 1966-1974 (Ivanov et al., 1979). It allows one to study the interplanetary and the magnetospherical disturbances more systematically.

Type
Part V. Coronal and Interplanetary Responses to Short Time Scale Phenomena: - Observations
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 421 - 424
Copyright
Copyright © Reidel 1980 

References

Ivanov, K. G., Mikerina, N. V., Zovoykina, A. I., and Treschotkina, V. M., Catalogue of Flare Situations of 1966-1974, IZMIRAN, Moscow, 1979.Google Scholar