  We describe Very Large Array observations of the extreme carbon star
IRC+10216 at 8.4, 14.9, and 22.5 GHz made over a two year period. We find
possible variability correlated with the infrared phase and a cm- to
sub-millimeter wavelength spectral index very close to 2. The variability,
observed flux densities, and upper limit on the size are consistent with the
emission arising from the stellar photosphere or a slightly larger radio
photosphere.
