Sight reduction explained
In astronavigation, sight reduction is the process of deriving from a sight (in celestial navigation usually obtained using a sextant) the information needed for establishing a line of position, generally by intercept method.
Sight is defined as the observation of the altitude, and sometimes also the azimuth, of a celestial body for a line of position; or the data obtained by such observation.[1]
The mathematical basis of sight reduction is the circle of equal altitude. The calculation can be done by computer, or by hand via tabular methods and longhand methods.
Algorithm
Given:
, the
latitude (North - positive, South - negative),
the
longitude (East - positive, West - negative), both approximate (assumed);
, the
declination of the body observed;
, the
Greenwich hour angle of the body observed;
, the
local hour angle of the body observed.
First calculate the altitude of the celestial body
using the equation of
circle of equal altitude:
The azimuth
or
(Zn=0 at North, measured eastward) is then calculated by:
These values are contrasted with the observed altitude
.
,
, and
are the three inputs to the
intercept method (Marcq St Hilaire method), which uses the difference in observed and calculated altitudes to ascertain one's relative location to the assumed point.
Tabular sight reduction
The methods included are:
- The Nautical Almanac Sight Reduction (NASR, originally known as Concise Tables for Sight Reduction or Davies, 1984, 22pg)
- Pub. 249 (formerly H.O. 249, Sight Reduction Tables for Air Navigation, A.P. 3270 in the UK, 1947 - 53, 1+2 volumes)[2]
- Pub. 229 (formerly H.O. 229, Sight Reduction Tables for Marine Navigation, H.D. 605/NP 401 in the UK, 1970, 6 volumes.[3]
- The variant of HO-229: Sight Reduction Tables for Small Boat Navigation, known as Schlereth, 1983, 1 volume)
- H.O. 214 (Tables of Computed Altitude and Azimuth, H.D. 486 in the UK, 1936 - 46, 9 vol.)
- H.O. 211 (Dead Reckoning Altitude and Azimuth Table, known as Ageton, 1931, 36pg. And 2 variants of H.O. 211: Compact Sight Reduction Table, also known as Ageton - Bayless, 1980, 9+ pg. S-Table, also known as Pepperday, 1992, 9+ pg.)
- H.O. 208 (Navigation Tables for Mariners and Aviators, known as Dreisonstok, 1928, 113pg.)
Longhand haversine sight reduction
This method is a practical procedure to reduce celestial sights with the needed accuracy, without using electronic tools such as calculator or a computer. And it could serve as a backup in case of malfunction of the positioning system aboard.
Doniol
The first approach of a compact and concise method was published by R. Doniol in 1955[4] and involved haversines. The altitude is derived from
, in which
,
,
a=\operatorname{hav}(LHA)
.
The calculation is: n = cos(Lat − Dec) m = cos(Lat + Dec) a = hav(LHA) Hc = arcsin(n − a ⋅ (m + n))
Ultra compact sight reduction
A practical and friendly method using only haversines was developed between 2014 and 2015,[5] and published in NavList.
A compact expression for the altitude was derived[6] using haversines,
, for all the terms of the equation:
\operatorname{hav}(ZD)=\operatorname{hav}(Lat-Dec)+\left(1-\operatorname{hav}(Lat-Dec)-\operatorname{hav}(Lat+Dec)\right) ⋅ \operatorname{hav}(LHA)
where
is the zenith distance,
is the calculated altitude.
The algorithm if absolute values are used is:For the azimuth a diagram[7] was developed for a faster solution without calculation, and with an accuracy of 1°.This diagram could be used also for star identification.[8]
An ambiguity in the value of azimuth may arise since in the diagram
0\circ\leqslantZ\leqslant90\circ
.
is E↔W as the name of the meridian angle, but the N↕S name is not determined. In most situations azimuth ambiguities are resolved simply by observation.
When there are reasons for doubt or for the purpose of checking the following formula[9] should be used:
\operatorname{hav}(Z)=
\circ\pm\vertDec\vert)-\operatorname{hav}(\vertLat\vert-Hc)}{1-\operatorname{hav}(\vertLat\vert-Hc)-\operatorname{hav}(\vertLat\vert+Hc)}
The algorithm if absolute values are used is:This computation of the altitude and the azimuth needs a haversine table. For a precision of 1 minute of arc, a four figure table is enough.[10] [11]
An example
See also
External links
Notes and References
- The American Practical Navigator (2002)
- https://www.thenauticalalmanac.com/Pub.%20249%20Vol.%201-2020-Dec.pdf Pub. 249 Volume 1. Stars
- https://msi.nga.mil/MSISiteContent/StaticFiles/NAV_PUBS/SRTM/Pub229/Vol_1/Pub229Vol1.pdf Pub. 229 Volume 1. Latitudes 0° to 15°
- Table de point miniature (Hauteur et azimut), by R. Doniol, Navigation IFN Vol. III Nº 10, Avril 1955 Paper
- Ultra compact sight reduction . Greg . Rudzinski . Ix, Hanno . Ocean Navigator . Navigator Publishing LLC . Portland, ME, USA . July 2015 . 227 . 0886-0149 . 42–43 . 2015-11-07.
- Altitude haversine formula by Hanno Ix http://fer3.com/arc/m2.aspx/Longhand-Sight-Reduction-HannoIx-nov-2014-g29121
- Azimuth diagram by Hanno Ix. http://fer3.com/arc/m2.aspx/Gregs-article-havDoniol-Ocean-Navigator-HannoIx-jun-2015-g31689
- Hc by Azimuth Diagram http://fer3.com/arc/m2.aspx/Hc-Azimuth-Diagram-finally-HannoIx-aug-2013-g24772
- Azimuth haversine formula by Lars Bergman http://fer3.com/arc/m2.aspx/Longhand-Sight-Reduction-Bergman-nov-2014-g29441
- Web site: NavList: Re: Longhand Sight Reduction (129172).
- https://yadi.sk/i/4MmOYyXhUshbxA Natural-Haversine 4-place Table