My Astro Images
Venus 05.02.2014

Venus 19.05.2012
Venus; f/10; Baader IR-Pass and silicon window (deep IR); 18:52, 19:04 UT:



Venus 28.04.2012
Night side with 1000 nm longpass filter (18:34 UT):


Venus 17.04.2012
Venus ~18:40 UT; UV, IR (Baader IR-pass), IR (1000 nm longpass):




- RAW Stacks (ZIP)
Venus 09.04.2012
Fused Silica Barlow; ~f/24,5; Channels: infrared deepest (silicon window), infrared deep (1000 nm longpass), UV (Astrodon UVenus); color - IR/IR/UV; 18:30 - 18:40:







Venus 11.02.2012
Venus in false colors: L1000-#47-UVenus:





Venus 06.01.2011
RG1000 at 4:46 UTC:




Venus 05.01.2011
Venus f/10, Ir-RGB 6:18 UTC. No much of detail in visual range:

UV filtr is BG39+UG1 Schott glass
Venus f/10, infrared channel, RG850 filter, f/10, 6:18 UTC


Silicon window is a polished piece of pure silicon (Si) that looks like a filter. It starts transmiting somewhere between 1000-1100 and by default it's not designed for CCDs that go blind at ~1100 nm ;) I was trying to catch Venus night side with it (as I did with RG1000) but today I didn't got any signs of the night side. I'll try tomorrow with RG1000 and Si side by side. The phase of day side may be to big.
Venus f/28, ProPlanet 742, 5:49 UTC:
Venus 17.12.2010
Venus, f/15, Pro Planet 807 and RG1000. 6:13 and 6:09

Venus 26.11.2010
RG-1000, f/10, 5:29 UTC:



Night side of Venus, thermal emition at 1010 nm (RG1000):
