Titlebook: Solar-Terrestrial Physics/1970; Proceedings of the I E. R. Dyer Conference proceedings 1972 Springer Nature B.V. 1972 cosmic ray.ionosphere

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Solar Radiobursts The main reason is that the radiowaves are generally emitted by energetic electrons, which can not be studied by many other means. Moreover, these bursts are often emitted high in the corona, where no other possibility exists up to now to detect solar activity.

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0067-0057 Leningrad, U.S.S.R., 11-19 May 1970. The Symposium may be regarded as the most recent member of a series of inter­ national symposia - for instance, the Symposium on Solar-Terrestrial Physics, Belgrade (1966), the Joint IQSY-COSPAR Symposium on Solar-Terrestrial Physics, London (1967), and the Symp

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Large-Scale Magnetic Fields and Activity Patterns on the Suns of such large-scale features are given: (a) . (super-supergranules) are probably the largest elements in the hierarchy of solar convective cells, which can be defined in the solar atmosphere for example, by magnetic field patterns, faculae, calcium flocculi, and the organization of active regions,

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Local Magnetic Fields on the Sunabout the magnetism of these principal sources. At sufficiently large distances from a spot the magnetic field can, apparently, be well approximated as that of a dipole submerged below the solar photosphere, (classical Mt. Wilson observations of Hale, 1919; Bumba, 1960; Severny, 1964). However, a mo

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Properties of Solar Active Regionsa. These ‘active’ phenomena are: (1) structures such as spots, plages, filaments, flares and coronal condensations; (2) gradual and impulsive enhancements of radiation in the EUV, X-ray and radio region of the solar spectrum; (3) motions and ejections of solar plasma and the acceleration of fast ele

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Permanent Sources of Particle Emission from the Sunr in interplanetary space with a recurrence of 27 days over many solar rotations. It is argued that the particles are of solar origin..For the majority of cases, one may relate particle events with active regions on the sun, even during solar minimum. We thus reject the hypothesis of acceleration of

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Solar Discrete Particle Events particle emission of some kind; relations of the flare capability of particle emission to properties of associated active regions; differences in the size of proton events and the reasons for them; our improving knowledge of electron events, pure electron and proton events, and the possibility of t

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Solar Radioburstsvisible light, UV and X-rays. However the emission of radio bursts accompanying solar activity is a very important phenomenon for the solar physicist. The main reason is that the radiowaves are generally emitted by energetic electrons, which can not be studied by many other means. Moreover, these bu