  We present the polarization images in the $J$, $H$, & $Ks$ bands of the Orion
Molecular Cloud 1 South region. The polarization images clearly show at least
six infrared reflection nebulae (IRNe) which are barely seen or invisible in
the intensity images. Our polarization vector images also identify the
illuminating sources of the nebulae: IRN 1 & 2, IRN 3, 4, & 5, and IRN 6 are
illuminated by three IR sources, Source 144-351, Source 145-356, and Source
136-355, respectively. Moreover, our polarization images suggest the candidate
driving sources of the optical Herbig-Haro objects for the first time; HH529, a
pair of HH202 and HH528 or HH 203/204, HH 530 and HH269 are originated from
Source 144-351, Source 145-356, and Source 136-355, respectively.
