Two dimensional maps of the Sun at 164 MHz, obtained with the Nancay Radioheliograph from April to August 1984 are presented. The quiet sun emission and the slowly varying component far from sunspots are studied. The association of local emissions with the chromospheric calcium plages is pointed out and interpreted. The altitude of the radio sources is estimated. The comparison of the location of the sources with K-corona observations confirms previous results obtained for the minimum of the cycle. The brightness temperature of the coronal plateau, which is the radio counterpart of the coronal plasma sheet, is given.
机构:
Aalto Univ, Dept Comp Sci, POB 15400, Aalto 00076, Finland
KTH Royal Inst Technol, NORDITA, Hannes Alfvens Vag 12, S-10691 Stockholm, Sweden
Stockholm Univ, Hannes Alfvens Vag 12, S-10691 Stockholm, SwedenAalto Univ, Dept Comp Sci, POB 15400, Aalto 00076, Finland
Korpi-Lagg, M. J.
Korpi-Lagg, A.
论文数: 0引用数: 0
h-index: 0
机构:
Aalto Univ, Dept Comp Sci, POB 15400, Aalto 00076, Finland
Max Planck Inst Solar Syst Res, Justus von Liebig Weg 3, D-37077 Gottingen, GermanyAalto Univ, Dept Comp Sci, POB 15400, Aalto 00076, Finland
Korpi-Lagg, A.
Olspert, N.
论文数: 0引用数: 0
h-index: 0
机构:
Aalto Univ, Dept Comp Sci, POB 15400, Aalto 00076, FinlandAalto Univ, Dept Comp Sci, POB 15400, Aalto 00076, Finland
Olspert, N.
Truong, H-L
论文数: 0引用数: 0
h-index: 0
机构:
Aalto Univ, Dept Comp Sci, POB 15400, Aalto 00076, FinlandAalto Univ, Dept Comp Sci, POB 15400, Aalto 00076, Finland