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On Thu, 10 Jun 2004 21:40:24 +0100, Martin Frey
wrote: Problem 4: If I do what Pete says, my head explodes. It was always the tried and trusted way of determining NSEW for the image. A planetarium program or the www tells you where contact 1 will occur for your location so all you have to do is to determine at worst the quadrant where the event is going to occur and at best the ~20 degree arc where things are going to kick off. Now the pressure's off - try it. First find N and S by centering on the Sun and moving the scope up and down (in dec) watching the movement of the Sun through the scope. As you move N, the last limb you see it the one with the highest declination. As you move south, it's the southern most limb. -- Pete Lawrence http://www.pbl33.co.uk Most recent images http://www.pbl33.fast24.co.uk/recent_images.html |
#32
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Pete Lawrence wrote:
Now the pressure's off - try it. First find N and S by centering on the Sun and moving the scope up and down (in dec) watching the movement of the Sun through the scope. As you move N, the last limb you see it the one with the highest declination. As you move south, it's the southern most limb. Pete, thanks. We got it right for all the scopes except the PST and when I try to rinse away the smarty I will have a chance to see what's its optical path actually is, but we sure guessed it wrong. The extraordinary thing is the degree of concentration we bring to these things. I don't know what the apparent field of view of the PST is but magnification is not huge (about 35x on the day) and an image of the whole Sun is sitting there on quite a small portion of your retina.If you are concentrating on one edge of the disc, the Queen could do Riverdance naked on the opposite edge without being noticed. It's not a blind spot thing and I don't have tunnel vision: I suspect we can narrow our area of concentration down on demand when we really want to see a really subtle change. But I will follow your scheme: next time it's sunny, take cover - there may be an explosion. -- Martin Frey http://www.hadastro.org.uk N 51 02 E 0 47 |
#33
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JRS: In article , seen in
news:uk.sci.astronomy, Martin Frey posted at Thu, 10 Jun 2004 21:40:24 : Dr John Stockton wrote: But it usually has spots; the motion from day to day of a spot shows the image orientation, and if compared with a known-orientation image so usually does the spot pattern. AIUI, anyone who can observe transits can observe spots. Therefore, I suggest that during the month or so before the next event diagrams of the Sun should be published, showing the current spots, the direction of their motion, and the predicted path of the event. One just observes the spots beforehand to determine how one's equipment presents the solar image. Probably, if one knew where to look, the current spots are already published on the WWW, in a known orientation; all that need be added is a diagram of the event in the same orientation, with enough publicity to ensure that any blunders will be noticed. Problem 1: there was only the faintest scattering of spots and they were as near as dammit in the centre AIUI, that's unusual; I wasn't suggesting that it could be done for the previous transit. The orientation test for ToV 2012 can be done at any time from now, provided that the observer can correct for moving the equipment to somewhere that the phenomenon is not occulted by the Earth. Of course, if the spots were in the centre on Tuesday, they'd have been only half-way in on Friday evening. Problem 2: they don't show up very well or unambiguously in an H-a scope - there seems to be tons of activity on the surface but not necessarily where the spots are. If the activity is "fixed" to the "surface" and lasts for at least a known minimum time, then the same can be done with an H-a picture in the Web. In fact, a real-time display could be used, with a button for unveiling an overlay of the future track. Problem 3: The new PST looks like a scope with a built in star diagonal - but the light path is clearly more complex than that as the image is reversed top to bottom unlike a normal refractor+diag Given an adequately unsymmetrical pattern, that too would be demonstrated. Problem 4: If I do what Pete says, my head explodes. That's only significant if you can also show that if you do not do what Pete says then your head does not explode. Showing that with an already-exploded head is left as an exercise for the reader ... -- © John Stockton, Surrey, UK. Turnpike v4.00 MIME. © Web URL:http://www.merlyn.demon.co.uk/ - FAQish topics, acronyms, & links. Proper = 4-line sig. separator as above, a line exactly "-- " (SonOfRFC1036) Do not Mail News to me. Before a reply, quote with "" or " " (SonOfRFC1036) |
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Dr John Stockton wrote:
That's only significant if you can also show that if you do not do what Pete says then your head does not explode. Showing that with an already-exploded head is left as an exercise for the reader ... Ooh err -- Martin Frey http://www.hadastro.org.uk N 51 02 E 0 47 |
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