[1] [1] ROESLER F L,HARLANDER J.Spatial heterodyne spectroscopy:interferometric performance at any wavelength without scanning[J].SPIE,1990,1318:234-243.

[2] [2] HARLANDER J.Spatial heterodyne spectroscopy:interferometric performance at any wavelength without scaning[D].USA:University of Wisconsin-Madison,1991.

[3] [3] HARLANDER J,ROESLER F.Spatial heterodyne spectroscopy:a novel interferometric technique for ground-based and space astronomy[J].SPIE,1990,1235:622-633.

[4] [4] WATCHORN S,ROESLE F L,HARLANDER J,et al.Development of the spatial heterodyne spectrometer for VUV remote sensing of the interstellar medium[J].SPIE,2001,4498:284-295.

[5] [5] MIERKIEWICZ E J,ROESLER F L,HARLANDER J,et al.First light performance of a near-UV spatial heterodyne spectrometer for interstellar emission line studies[J].SPIE,2004,5492:751-766.

[6] [6] ROESLER F L,HARLANDER J.Spatial heterodyne spectroscopy for atmospheric remote sensing[J].SPIE,1999,3756:337-345.

[7] [7] LIN Y L,SHEPHERD G,SOLHEIM B,et al.Introduction to spatial heterodyne observations of water (SHOW) project and its instrument development[C].ITSC-ⅩⅣ Proc.Beijing (Poster),China,2005.