pHinds answered, here are some extras in case you or anyone else wants them
Solar system speed relative to CMB rest frame is around 370 km/s in direction of constellation Leo (a spring constellation).
the opposite direction, i.e. BEHIND us, is Aquarius constellation (a fall constellation, Sept. Oct Nov evenings)
good web resource is what Ned Wright has to say. He was part of a team that made one of first accurate measurements of the CMB dipole
(dipole = doppler hot spot in Leo, cold spot in Aquarius, )
google "CMB dipole" and scroll down to ...ucla.edu/wright... link, which is:
http://www.astro.ucla.edu/~wright/CMB-DT.html
Don't get bogged in Wright's technicalities. He is a scientist and his specialty is cosmology, especially CMB. Notice he says 368 km/s and average temp 2.725 Kelvin, and
doppler hotspot 0.00335 Kelvin hotter, coldspot 0.00335 Kelvin colder
He gives coordinates of the dipole, but he doesn't say what constellation it is in and what time of year you can spot the direction the solar system is going.
Notice that 0.00335/2.725 is the same fraction that 368 km/s is of the speed of light. The temperature is doppler raised by the same fraction as the speed is of the speed of light.
they measure the sky temperature with a horn radio antenna because the heat glow is down in the infrared/microwave.
http://Earth'sky.org/constellations/aquarius-heres-your-constellation
http://Earth'sky.org/constellations/leo-heres-your-constellation
http://stardate.org/nightsky/constellations/leo
This popular nontechnical account mentions the two constellations that mark the directions of the solar system speed in the sky
http://astronomy.swin.edu.au/cosmos/C/Cosmic+Microwave+Background+Dipole
It also points out that the solar system speed is due IN PART to the motion of our galaxy, and it is also the result of our solar system circulating WITHIN the galaxy. The galaxy is whizzing one way and the sun and planets are whizzing another way and they partly cancel and the result is this 368 km/s I've been talking about. That is what we measure, by the doppler effect.