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[vsnet-chat 5095] Airmass, extinction and seeing at moderate altitude (h) above the horizon
- Date: Fri, 15 Feb 2002 19:17:50 +0100
- To: vsnet chat <vsnet-chat@kusastro.kyoto-u.ac.jp>
- From: Gianluca Masi <gianmasi@fr.flashnet.it>
- Subject: [vsnet-chat 5095] Airmass, extinction and seeing at moderate altitude (h) above the horizon
- Delivered-To: vsnet-chat@kusastro.kyoto-u.ac.jp
- Organization: Bellatrix Astronomical Observatory
- Sender: owner-vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp
Dear All,
I've been trying to find a description of the problems encoutered
observing lower than 45° above the horizon (h<45°)ccd, particularly the
effect of the airmass in limiting the fantest observable stars with an
unfiltered CCD. As a general rule, I have reviewed (in an old message to
this list) the formula:
X = sec(Z) = 1 / cos(Z)
for zenith distance (Z) less than 60 degrees. As I would like to extend
this formula to reach h=25°, is there a large deviation from it in this
range? Also, is the 0.25mag loss per airmass still valid?
Also, it is of interest to me to know if there is any formula/comment
describing the effect on the seeing of these quite low altitudes; in
other words, if at the zenith I have a 1" seeing, what value I can
expect looking at h=30°?
Any comments, personal experiences would be very appreciated.
Thank you very much,
Gianluca
--
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* Gianluca Masi "Two things fill the soul *
* Via Madonna de Loco, 47 with awe and reverence [...]: *
* 03023 Ceccano (FR) the starry sky above me and *
* ITALY the moral law within me" *
* e-mail: gianmasi@fr.flashnet.it *
* web: http://vsnet.bellatrixobservatory.org I. Kant *
* Minor Planet Center Obs. Code: 470 - Ceccano *
* Center for Backyard Astrophysics - Italy *
* VSNET Collaboration Team member *
* CCD-astrometry-photometry@egroup.com mailing-list moderator *
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