
| 2005WPO | Jan | Feb | Mar* | Apr | May | Jun | Jul | Aug | Sept | Oct | Nov | Dec | Totals |
| daily obs | got PST | - | 5 | 15 | 9 | 18 | 20 | 22 | 23 | 22 | 18 | 12 | 164 days |
| pics/month | - | - | 15 | 30 | 21 | 51 | 57 | 54 | 49 | 77 | 56 | 27 | 437 pics |
| % days clear | - | - | 36%* | 50% | 29% | 60% | 65% | 71% | 77% | 71% | 60% | 38% | Ave=56% |
The sun is very dynamic and whenever possible
warrants close attention - you may see something unique. The dark
filament [2005 May 16 below] appeared immediately after a bright flare
near a sunspot and both faded away within about 20 minutes. Images
below via Minolta Dimage 7.



























































Straight out of the box - the sun put on a fine display with two large eruptive looped prominences over a large sunspot on the western limb that were seen to change in almost real-time over an hour. Two quiet prominences near the north pole, bright active regions around sunspots and long dark filaments [prominences silhouetted against the disk] also seen. Viewing in comfort from the shaded conditions indoors seems to increase contrast without obvious loss of image quality through double glazing. Outdoors a simple clock-drive keeps the sun centred and 'static' from a seated position.Early attempts on a low winter sun to capture images via afocal and Barlow projection into a Canon 300D DSLR camera don't do the PST justice. Projected image 14mm diameter @ f/40 image onto sensor's 7.4 micron pixels. Image scale ~1 arcsec/pixel - 40mm OG res ~ 3"arc sampled by 3x3pixels.