Physics
Scientific paper
Apr 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978soph...57..423m&link_type=abstract
Solar Physics, vol. 57, Apr. 1978, p. 423-428.
Physics
1
Density Distribution, Solar Corona, Stellar Structure, Type 3 Bursts, Radial Distribution, Solar Limb, Solar X-Rays, Synoptic Measurement
Scientific paper
Using Mercier and Rosenberg's (1974) set of data on Type III bursts at 169 MHz, Leblanc and de la Noe (1977) showed that, in 75 percent of cases, the active regions responsible for Type III bursts are associated with low-density coronal structures and occur in low-density regions. In the present paper, Leblanc and de la Noe's methods and conclusions are critically analyzed, and certain inconsistencies are pointed out. Specifically, the use of white light and X-ray data and their relevance to the relationship between Type III bursts and coronal structures are questioned, along with the use of the radial hypothesis. It is seen that the density values deduced from the derived heights of Type III bursts do not support the relationship established between Type III bursts and coronal low-density structures.
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