I’ve observed these two comets (whose cometary features was discovered by members of the T3 project at the end of December) on 2011, Jan. 02 and their activity now is well visible, especially for P/2002 VP94 (LINEAR).

It exhibits a tail at least 60″ long in PA 214°.
P/2010 WK (LINEAR) has no tail, but a round coma 30″ wide. Its strong central condensation has a FWHM of 4.4″, compared to 3.1″ of stars: