Radio Sun in
Meterwaves
•
•
Thermal emission: optical depth
could be large at low frequencies.
•
•
Direct imaging using free free
emission from
the corona &
CMEs
(Sheridan et al., 1978;
Gopalswamy and Kundu, 1992;
Maia et al.,
2000)
CLRO quiet Sun at 50 MHz; Optical Sun blocked to mimic eclipse