New DIS Slits. [Best read in fixed width font.] We have received new aluminized quartz slits for DIS. The slit widths have been measured using the measuring engine at the Solar Observatory, with mean values of: 211 (+- 4) and 274 (+- 7) microns (both N = 3, small samples) or 1.24 and 1.61 arcsec. The goal was to obtain slits with widths of 2.1 and 3.0 arcsec. The slits were manufactured from and replace the previous (0.47 and 0.87 arcsec) quartz slits. They were produced by Don Loomis using wire-shadow fixtures made earlier by Mike Carr and the aluminizing was done by a sub-contractor. APO supplied the fine piano wires. It is believed that the undersized slits were the result of the aluminizing setup at the subcontractor; the ballistic trajectories of the Al probably were not all near normal to the quartz plates, quite likely if the subcontractor had several jobs in the vacuum chamber. I regret that we did not obtain a 2 arcsec slit this time. I suspect, however, that at least the 1.61 arcsec slit will see service straight away. We are pursuing other sources (including our own aluminizing at the Solar Observatory) for additional slits. ------------------------------------------------------------------------------- For the record, here are some quantitative and qualitative observations of the new slits (which I will call the "1.2 arcsec" and "1.6 arcsec" slits): Provisional Name "1.2 arcsec" "1.6 arcsec" Mean slit width, s 211 microns = 1.24 arcsec 274 microns = 1.61 arcsec Standard dev (N = 3) 4 microns 7 microns Quartz plate w x h 1.860 x 2.995 inches 1.865 x 2.996 inches 4.724 x 7.607 cm 4.737 x 7.610 cm Thickness of plate 0.0624 to 0.638 inch (Not measured, assumed same) Curvature of slit, 17 microns approx. 14 microns approx. (peak displacement of slit from straight line in the central 5 cm of slit length) Edge irregularities Clean, nothing obvious Clean, nothing obvious Edge sharpness No "penumbra" observed in transmission, both slits I guesstimate the accuracy of a single measurement with the engine at around 6 microns. ------------------------------------------------------------------------------- Steve Knapp 11 June 1996 <sknapp@galileo.apo.nmsu.edu> APO APO APO APO APO Apache Point Observatory 3.5m APO APO APO APO APO This is message 18 in the apo35-dis archive. You can find APO the archive on http://www.astro.princeton.edu/APO/apo35-dis/INDEX.html APO To join/leave the list, send mail to apo35-request@astro.princeton.edu APO To post a message, mail it to apo35-dis@astro.princeton.edu APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO