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A Community Devoted to the Preservation and Practice of Celestial Navigation and Other Methods of Traditional Wayfinding
Re: Basics of computing sunrise/sunset
From: Frank Reed
Date: 2009 Jun 19, 17:16 -0700
From: Frank Reed
Date: 2009 Jun 19, 17:16 -0700
Jim Wilson, you wrote: "Having viewed the last six total solar eclipses, I can now worry about the conditions immediately preceding totality." First of all, I'm jealous. :-) Six total eclipses... very nice! As for worrying, no, I wouldn't. The people who are at risk in those last few dozen seconds before or after totality are people who are unaware that they are looking at an eclipse. It's really very strange to me how long it takes for casual obervers to notice that there is an eclipse in progress (unless the Sun is near the horizon). I remember observing a 99% eclipse in Chicago years ago, and no one that I spoke to noticed anything wrong with the Sun though some did sense the "harshness" and "strangeness" of the sunlight on the landscape. And incidentally, the next time you see a 99% eclipse, consider that you're seeing as much sunlight and the same total brightness for the Sun as you would see on a sunny day from the rings of Saturn (10x further from the Sun, 100x fainter). Now as the eclipse passes from 99% to 99.9% and then totality, quite suddenly casual observers will notice the Sun is "wrong" and they may start staring at it --it's rather spectacular at that point. The catch is that, while the total brightness of the Sun is greatly reduced and does not induce the normal "blink" reflex, the intensity of the light is quite unchanged and staring at it for a dozen or a few dozen seconds will cause permanent damage. Of course, any observer who has been forewarned will not make this mistake. Unfortunately, the media sometimes over-do these warnings and create the impression that an eclipse is beaming evil death rays at the unwary. And you concluded: "We were always advised to never look at the pre-eclipse sun through binoculars, even with shades. But during totality, they're indispensable, allowing us to see local sun activity like sunspots and solar flares. I find that 10x20 are perfect, where the sun fills the field." Looking through 10x binoculars at a 1% spot of the Sun is no different from looking at the full Sun with the unaided eye (except that the glass of the lenses --even without shades-- significantly reduces the UV portion of the spectrum). So for example, if you're looking at the very end of totality through binoculars and you suddenly see Bailly's beads (small bits of the Sun's disk visible through valleys and depressions along the limb of the Moon), you will not harm your eyes so long as you look away within a second or so --just as you would do if you glanced at the full Sun high in the sky without optical aid. Binoculars or telescopes make the image of the Sun LARGER but do not change its surface brightness, in the sense of either energy per square millimeter on the retina or energy per square arcsecond in the visual field. So if you're looking at a 1% bit of the Sun, then magnified by a factor of ten, its area either in square arcseconds, would be the same as the Sun normally. The total brightness of that 1% bit would be just the same as the full Sun with no optical aid. The magnification alone is responsible for this --there's no additional "enhancement" of the energy. -FER --~--~---------~--~----~------------~-------~--~----~ Navigation List archive: www.fer3.com/arc To post, email NavList@fer3.com To , email NavList-@fer3.com -~----------~----~----~----~------~----~------~--~---