
%0 Journal Article
%A Reynolds, RJ 
%A Tufte, SL 
%A Percival, JW 
%A jaehnig, K 
%A Haffner, LM 
%T The Wisconsin Halpha Mapper (WHAM): A Brief Review of Performance Characteristics and Early Scientific Results
%J Publications of the Astronomical Society of Australia
%D 1998/04/01
%V 15
%N 1
%P 14-18
%K 
%R https://doi.org/10.1071/AS98014
%U https://www.publish.csiro.au/paper/AS98014 
%X The Wisconsin Halpha Mapper (WHAM) is a recently completed facility for the detection and study of faint optical emission lines from diffuse ionised gas in the disk and halo of the Galaxy. WHAM consists of a 15 cm diameter Fabry-Perot spectrometer coupled to a 0.6 m `telescope', which provide a 1° diameter beam on the sky and produce a 12 km s^-1 resolution spectrum within a 200 km s^-1 spectral window. This facility is now located at Kitt Peak in Arizona and operated remotely from Madison, Wisconsin, 2400 km distant. Early results include a velocity-resolved Halpha map of a 70° x 100° region of the sky near the Galactic anticentre, the first detections of Halpha emission from the M I and A high velocity clouds, and the first detections of [O I] lambda6300 and other faint 'diagnostic' lines from the warm ionised medium. Through the summer of 1998, WHAM will be devoted almost exclusively to a survey of the northern sky, which will provide maps of the distribution and kinematics of the diffuse HII through the optical Halpha line in a manner that is analogous to earlier sky surveys of the HI made through the 21 cm line. 
