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A Community Devoted to the Preservation and Practice of Celestial Navigation and Other Methods of Traditional Wayfinding
Re: Refraction
From: Marcel Tschudin
Date: 2005 Aug 26, 19:41 +0300
From: Marcel Tschudin
Date: 2005 Aug 26, 19:41 +0300
George wrote > I'm pleased that Marcel has followed up my lead to Andrew Young's useful > series, and that Andy has come up with the goods, as I expected he would. Yes, I followed your suggestion, and indeed Andy Young was very helpful in discussing the subject via mail. George asks further > Presumably, Sunset science 4 has references to the previous 3 instalments. > Is it the concluding item in that series, or are there others to follow? > It > would be helpful if Marcel would list references to all the items in this > series for which he has details. No doubt, several listmembers would find > them interesting. The three preceiding papers are indeed mentioned. To make it easier for all those who are interested, I just add the references from NASA ADS by copy/paste at the end of this mail. The abstract can be read at ADS. Unfortunately all these articles can not be downloaded for free. I was not able to find out whether the series will continue or not. Let me just mention the last part of his conclusions: "Refraction within about 5deg of the horizon is so variable that no a priori formula or table can be expected to give accurate values there; the local lapse rate and thickness of the boundary layer above the observer must be known. However, numerical integration using standard lapse rate, matched to the actual temperature and pressure at the observer, should give values good to a minute of arc or so - that is, good enough for telescope pointing - down to 2deg or 3deg apparent altitude. Below that, numerical integrations will give useful values if the actual boundary-layer lapse rate and thickness are known, but only the bottom kilometer or so of the atmosphere needs to be measured, and ordinary balloon soundings are adequate. At and below the astronomical horizon, the refraction depends primarily on atmospheric structure below the observer and varies so much (tens of minutes, or even several degees) that only very crude predictions can be made. The observed time of sunset at a sea horizon often varies by a few minutes from day to day, and the variations increase with height above the sea." That is more or less what also Frank found after having calculated various models using the BAS pocedure, as Andy Young calls it. I hope that Frank's transfer function for calculating refraction as a function of altitude and height receives the appreciation it deserves. Marcel Here now the references: Title: Sunset science. I. The mock mirage Authors: Young, Andrew T.; Kattawar, George W.; Parviainen, Pekka Journal: Applied Optics LP, vol. 36, Issue 12, pp.2689-2700 Publication Date: 04/1997 Origin: AIP; OSA Bibliographic Code: 1997ApOpt..36.2689Y Title: Sunset Science. II. A useful diagram Authors: Young, Andrew T.; Kattawar, George W. Journal: Applied Optics LP, vol. 37, Issue 18, pp.3785-3792 Publication Date: 06/1998 Origin: AIP; OSA Bibliographic Code: 1998ApOpt..37.3785Y Title: Sunset science. III. Visual adaptation and green flashes Authors: Young, Andrew T. Journal: Journal of the Optical Society of America A: Optics, Image Science, and Vision, Volume 17, Issue 12, December 2000, pp.2129-2139 Publication Date: 12/2000 Origin: AIP; OSA Bibliographic Code: 2000OSAJ...17.2129Y Title: Sunset Science. IV. Low-Altitude Refraction Authors: Young, Andrew T. Affiliation: AA(Department of Astronomy, San Diego State University, 5500 Campanile Drive, San Diego, CA 92182-1221 aty@mintaka.sdsu.edu) Journal: The Astronomical Journal, Volume 127, Issue 6, pp. 3622-3637. (AJ Homepage) Publication Date: 06/2004 Origin: UCP AJ Keywords: Atmospheric Effects Abstract Copyright: (c) 2004: The American Astronomical Society DOI: 10.1086/420806 Bibliographic Code: 2004AJ....127.3622Y