The meteor year can be divided in two, a half with low meteor activity and one with high activity. The transition between high and low activity usually takes place in mid to late January and extends into June. Still rates seem to be holding up fairly well though we may see only half as many detections by the time February starts.
Obs Date(UT) Time TOT SPO ANT COM NCC XUM GUM ECV SAL 2014-01-20 12h 22m 22 20 1 0 0 0 1 0 SAL 2014-01-19 12h 19m 23 20 0 1 0 2 0 SAL - SALSA3 camera in Tucson (Carl Hergenrother) VIS - Visual observations from Tucson (Carl Hergenrother) Time - Total amount of time each camera looked for meteors TOT - Total number of meteors detected SPO - Sporadics (meteors not affiliated with any particular meteor shower) ANT - Antihelions COM - Coma Berenicids GUM - Gamma Ursae Minorids NCC - Northern Delta Cancrids XUM - January Xi Ursae Majorids ECV - Eta Corvids
The Transient Sky - Comets, Asteroids, Meteors 