We report the results of a rocket-borne observation of [C II] 158µm line and far-infrared continuum emission at 152.5µm toward the high latitude molecular clouds in Ursa Major. We also present the results of a follow-up observation of the millimeter 12 CO J = 1 → 0 line over a selected region observed by the rocket-borne experiment. We have discovered three small CO cloudlets from the follow-up 12 CO observations. We show that these molecular cloudlets, as well as the MBM clouds(MBM 27/28/29/30), are not gravitationally bound. Magnetic pressure and turbulent pressure dominate the dynamic balance of the clouds.