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diff --git a/doc/kmoon/carlosmail b/doc/kmoon/carlosmail new file mode 100644 index 0000000..760845b --- /dev/null +++ b/doc/kmoon/carlosmail @@ -0,0 +1,74 @@ +From [email protected] Fri Oct 20 23:12:11 2000 +Return-Path: <[email protected]> +Delivered-To: [email protected] +Received: (qmail 22568 invoked by uid 1055); 20 Oct 2000 21:12:11 -0000 +Delivered-To: [email protected] +Received: (qmail 22489 invoked from network); 20 Oct 2000 21:12:07 -0000 +Received: from nova.ov.ufrj.br ([email protected]) + by max.tat.physik.uni-tuebingen.de with SMTP; 20 Oct 2000 21:12:07 -0000 +Received: from localhost (localhost [[UNIX: localhost]]) + by nova.ov.ufrj.br (8.9.3/8.9.3) id TAA09140 + for [email protected]; Fri, 20 Oct 2000 19:14:00 -0200 +From: Carlos Roberto Raba<E7>a <[email protected]> +Reply-To: [email protected] +Organization: Observatorio do Valongo - UFRJ +To: Stephan Kulow <[email protected]> +Subject: Re: Moon tool +Date: Fri, 20 Oct 2000 17:10:39 -0200 +X-Mailer: KMail [version 1.0.29] +Content-Type: text/plain +References: <[email protected]> <[email protected]> +In-Reply-To: <[email protected]> +MIME-Version: 1.0 +Message-Id: <[email protected]> +Content-Transfer-Encoding: 8bit +Status: O +X-Status: + +Stephan, + +> In KDE2 I implemented free choice view angle, so I could also slide +> it some degrees off to see it like I see it here :) + +It is nice to hear that! Unfortunately, I still use KDE 1.1.2.... By the way, +when is the final release o 2.0? + +> But if you're an expert, I would like your advise on the correct +> terms. Where on the earth you see the moon in the the default view +> you can see on web pages etc.? + +As you know, the moon keeps always the same face turned to earth (the so called +near side). This is a composition of its period of orbital motion and rotation: +they are approximately the same. The moon's orbit is inclined with respect to +the equator by (only) 5 degrees, and for our purposes, keeps the polar +orientation in the sky unchanged. This means that the angle that you +see the moon in the sky changes by a composition of two factors only: 1) +latitude of the observer, and 2) time of the day that you look at the moon. If +you look at the moon over many hours, the change of orientation in the sky is +moon's orbital plane is close to the equator (as I said before) the discussion +of orientation looses any meaning. At these positions, the passage by the +meridian happens very close to the top of your head. So, I can be facing east +and move my head up to see the moon, or I can be facing west and move my head +up. Which rotation should I addopt? That is why I told you to use 0 or 180 +degrees. Otherwise, you would need to incorporate in your code many otherif he +relations, including the latitude of the observer.he will see the first quarter +moon as a C and the last quater moon as a D (see +> The current kmoon uses the pictures of this site:l) when the moon is over +> http://timbeauchamp.tripod.com/moon/, but a (german) colleague ofes over his +> yours pointed out that the images are mirrored horizontally, son is reversed. +> we corrected that (the larger craters appear on the left ontor. Since the +> the moon I see in the sky, while they are right on the web). + +My colleague is correct. The east-west sides in the pictures are wrong, so you +should flip them sideways. For an observer in the northern hemisthere this is +all you need to do. For an observer in the southern hemisphere, you need to +rotate this new set of images by 180 degrees. Keep in mind that in the sky if +north is up east is to the left, if south is up east is to the right. You can +easily see this if you lay down ;-/ on the floor with you head/legs pointing to +the north/south line. Now, try to point your left arm to the geographic +east while facing up. + +I hope this helps you. If you like more info, it will be a pleasure to +help. Best wishes, + +Carlos |