#1
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Surprised
I thought members of this ng would find it moderatly interesting how much
atmosphere they were actually looking through. Based on the feedback I got aparently not. www.HaimannOnline.com/Distance -- Author of Dipperbase (www.HaimannOnline.com/DipperBase) A Astronomy Image database, which allows upload to the web. Currently in alpha-testing. |
#2
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Surprised
Cool, it looks like a lot at 75 Deg.
"Terry A. Haimann" wrote in message news I thought members of this ng would find it moderatly interesting how much atmosphere they were actually looking through. Based on the feedback I got aparently not. www.HaimannOnline.com/Distance -- Author of Dipperbase (www.HaimannOnline.com/DipperBase) A Astronomy Image database, which allows upload to the web. Currently in alpha-testing. |
#3
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Surprised
Cool, it looks like a lot at 75 Deg.
"Terry A. Haimann" wrote in message news I thought members of this ng would find it moderatly interesting how much atmosphere they were actually looking through. Based on the feedback I got aparently not. www.HaimannOnline.com/Distance -- Author of Dipperbase (www.HaimannOnline.com/DipperBase) A Astronomy Image database, which allows upload to the web. Currently in alpha-testing. |
#4
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Surprised
Terry A. Haimann wrote:
I thought members of this ng would find it moderatly interesting how much atmosphere they were actually looking through. Based on the feedback I got aparently not. www.HaimannOnline.com/Distance Whoa, whoa, whoa...! You might try checking your web logs to see how many people loaded the page. I checked the page out, but didn't offer any feedback because I had none to offer. Doesn't mean I wasn't interested. One thing that was a bit unclear on the first read-through was whether you had taken into account the inhomogeneity of the atmosphere--that it's denser at the bottom and thins out exponentially toward the top. I'll take a second look... Brian Tung The Astronomy Corner at http://astro.isi.edu/ Unofficial C5+ Home Page at http://astro.isi.edu/c5plus/ The PleiadAtlas Home Page at http://astro.isi.edu/pleiadatlas/ My Own Personal FAQ (SAA) at http://astro.isi.edu/reference/faq.txt |
#5
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Surprised
Terry A. Haimann wrote:
I thought members of this ng would find it moderatly interesting how much atmosphere they were actually looking through. Based on the feedback I got aparently not. www.HaimannOnline.com/Distance Whoa, whoa, whoa...! You might try checking your web logs to see how many people loaded the page. I checked the page out, but didn't offer any feedback because I had none to offer. Doesn't mean I wasn't interested. One thing that was a bit unclear on the first read-through was whether you had taken into account the inhomogeneity of the atmosphere--that it's denser at the bottom and thins out exponentially toward the top. I'll take a second look... Brian Tung The Astronomy Corner at http://astro.isi.edu/ Unofficial C5+ Home Page at http://astro.isi.edu/c5plus/ The PleiadAtlas Home Page at http://astro.isi.edu/pleiadatlas/ My Own Personal FAQ (SAA) at http://astro.isi.edu/reference/faq.txt |
#6
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Surprised
No I didn't. I'm not knowlegable on the diffrent layers of our
atmosphere. I did this purely out of curiosity. Once you have the edges of the layers, it wouldn't be that dificult to program that in. It occurs to me that the layers could vary though, depending on weather conditions. Terry On Mon, 16 Feb 2004 16:27:20 +0000, Brian Tung wrote: One thing that was a bit unclear on the first read-through was whether you had taken into account the inhomogeneity of the atmosphere--that it's denser at the bottom and thins out exponentially toward the top. I'll take a second look... -- Author of Dipperbase (www.HaimannOnline.com/DipperBase) A Astronomy Image database, which allows upload to the web. Currently in alpha-testing. |
#7
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Surprised
No I didn't. I'm not knowlegable on the diffrent layers of our
atmosphere. I did this purely out of curiosity. Once you have the edges of the layers, it wouldn't be that dificult to program that in. It occurs to me that the layers could vary though, depending on weather conditions. Terry On Mon, 16 Feb 2004 16:27:20 +0000, Brian Tung wrote: One thing that was a bit unclear on the first read-through was whether you had taken into account the inhomogeneity of the atmosphere--that it's denser at the bottom and thins out exponentially toward the top. I'll take a second look... -- Author of Dipperbase (www.HaimannOnline.com/DipperBase) A Astronomy Image database, which allows upload to the web. Currently in alpha-testing. |
#8
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Surprised
Terry A. Haimann wrote:
No I didn't. I'm not knowlegable on the diffrent layers of our atmosphere. I did this purely out of curiosity. You might find this useful. Astronomers use a unit called "airmass" to describe how much air they are looking through. This value is 1.0 at the zenith and increases toward the horizon. Somewhere around a zenith distance of 60 degrees the airmass reaches 2, where you are looking through twice as mush air. Here is the simple formula (which bears some resemblance to your own work): Airmass = 1.0/sin(alt) A more rigorous formula is also available: Define A = 1.0/sin(alt) Airmass = A*(1.0-0.0012*(A*A-1.0)) Whe alt = altitude above horizon * denotes multiplication Have fun. Greg -- Greg Crinklaw Astronomical Software Developer Cloudcroft, New Mexico, USA (33N, 106W, 2700m) SkyTools Software for the Observer: http://www.skyhound.com/cs.html Skyhound Observing Pages: http://www.skyhound.com/sh/skyhound.html To reply remove spleen |
#9
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Surprised
Terry A. Haimann wrote:
No I didn't. I'm not knowlegable on the diffrent layers of our atmosphere. I did this purely out of curiosity. You might find this useful. Astronomers use a unit called "airmass" to describe how much air they are looking through. This value is 1.0 at the zenith and increases toward the horizon. Somewhere around a zenith distance of 60 degrees the airmass reaches 2, where you are looking through twice as mush air. Here is the simple formula (which bears some resemblance to your own work): Airmass = 1.0/sin(alt) A more rigorous formula is also available: Define A = 1.0/sin(alt) Airmass = A*(1.0-0.0012*(A*A-1.0)) Whe alt = altitude above horizon * denotes multiplication Have fun. Greg -- Greg Crinklaw Astronomical Software Developer Cloudcroft, New Mexico, USA (33N, 106W, 2700m) SkyTools Software for the Observer: http://www.skyhound.com/cs.html Skyhound Observing Pages: http://www.skyhound.com/sh/skyhound.html To reply remove spleen |
#10
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Surprised
Greg Crinklaw wrote: Terry A. Haimann wrote: No I didn't. I'm not knowlegable on the diffrent layers of our atmosphere. I did this purely out of curiosity. You might find this useful. Astronomers use a unit called "airmass" to describe how much air they are looking through. This value is 1.0 at the zenith and increases toward the horizon. Somewhere around a zenith distance of 60 degrees the airmass reaches 2, where you are looking through twice as mush air. ^^^^^ Freudian slip? -- ------ Rick S. http://users.rcn.com/rflrs |
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