Sunspot oscillations: where is the corona?
 3 minute oscillations are a chromospheric phenomenon:
should not occur in the corona
 At high frequencies (> 15 GHz), surfaces never get very
high, so not unexpected
At lower frequencies where gyroresonance surfaces are
higher in the corona, expect to see effects at edges where
surfaces drop into chromosphere, or in o mode which is 2nd
harmonic, hence lower
 Observations at 5 GHz show oscillations at edges (Nindos et
al. 2002)
 Observations that 8 GHz V oscillations are anticorrelated
with I oscillations consistent: 2nd harmonic o mode TB varies,
3rd harmonic x mode does not, so V decreases as o mode TB
and hence I increases