Description Usage Arguments Value Author(s) References See Also Examples
The astronomical refraction is determined using the inverse of Sinclair's formula. This formula is based on the International Standard Atmosphere (ISA: which by the way does not mean the 'average' atmosphere;-). Due to the uncertainties aorund the atmsopheric condition of the Boundary Layers, the calcuated refractions will not be very accurate (say with 0.5deg). Below a Topocentric altitude of -3.5deg, the Apparent altitude is made equal.
1 2 | AppAltfromTopoAlt(TopoAlt, TempE = TempDefault,
PresE = PressureDefault)
|
TopoAlt |
the Topocentric altitude (deg), double |
TempE |
Temperature at height eyes (C, default=15C), double |
PresE |
Airpressure at height eyes (mbar, default=1013.25mbar), double |
AppAlt de Apparent altitude (deg), double
Victor Reijs, lists@archaeocosmology.org
Bennett, G.G. 1982. 'The calculation of astronomical refraction in marine navigation', Journal of Inst. navigation, Vol 35: pp. 255-59.
http://www.archaeocosmology.org/eng/refract.htm
1 2 3 4 5 | AppAltfromTopoAlt(0,15,1013.25)
#0.4721438916
AppAltfromTopoAlt(c(-4,-0.5,0,2,20))
#-4.00000000000 0.04956607457 0.47214389159 2.27870879488 20.04373829337
|
Add the following code to your website.
For more information on customizing the embed code, read Embedding Snippets.