ISSN:
1572-946X
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
Abstract Radio noise continuum emissions observed in metric and deca-metric wave frequencies are, in general, associated with actively varying sunspot groups accompanied by the S-component of microwave radio emissions. It is known that these continuum emission sources, often called type I storm sources, are often associated with type III burst storm activity from metric to hectometric wave frequencies. This storm activity is, therefore, closely connected with the development of these continuum emission sources. It is shown that the S-component emission in microwave frequencies generally precedes by several days the emission of these noise continuum storms of lower frequencies. In order for these storms to develop, the growth of sunspot groups into complex types is very important with the increase of the average magnetic field intensity and area of these groups. In particular, the types of these groups such as βγ and γ are very important on the generation of noise continuum storm sources and sharp increase of the flux of these continuum emissions. This fact suggests that sunspot magnetic configuration and its variation, both space and time, are very effective on the growth of the sources for these noise continuum emissions. Although we have not known yet the true mechanism of these emissions, it is very likely that energetic electrons, 10 to 100 keV, accelerated in association with the variation of sunspot magnetic fields, are responsible as the sources of those radio emissions. Furthermore it seems that these electrons are contributing to the emission of type III burst storms, which are associated with the noise continuum storm sources. In explaining the origin of these storms, some plasma processes must be taken into consideration. Furthermore, it should be remarked that the storage mechanism of the electrons mentioned above plays an important role in generating both the noise continuum emissions and type III burst storms, because ‘on-fringe’ type III bursts are all generated above these noise continuum storms sources. After reviewing the theories of these noise continuum storm emissions, a model is briefly considered to explain the relation between these continuums and type III bursts, and a discussion is given on the role of energetic electrons on these two emissions. It is pointed out that instabilities associated with these electrons and their relation to their own stabilizing effects are important in interpreting both of these storm emissions.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF01225964
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