Almucantar
Circle on the celestial sphere parallel to the horizon
title: "Almucantar" type: doc version: 1 created: 2026-02-28 author: "Wikipedia contributors" status: active scope: public tags: ["astronomical-coordinate-systems", "measuring-instruments", "astronomical-instruments", "navigational-equipment", "celestial-navigation", "historical-scientific-instruments"] description: "Circle on the celestial sphere parallel to the horizon" topic_path: "general/astronomical-coordinate-systems" source: "https://en.wikipedia.org/wiki/Almucantar" license: "CC BY-SA 4.0" wikipedia_page_id: 0 wikipedia_revision_id: 0
::summary Circle on the celestial sphere parallel to the horizon ::
::figure[src="https://upload.wikimedia.org/wikipedia/commons/e/ed/Almucantarat_(it).svg" caption="altitude]]."] ::
The term was introduced into European astronomy by monastic astronomer Hermann Contractus of Reichenau, Latinized from the Arabic word ar ("the almucantar, sundial", plural: ar), derived from ar ("arch, bridge")
Almucantar staff
An almucantar staff is an instrument chiefly used to determine the time of sunrise and sunset, in order to find the amplitude and consequently the variations of the compass. Usually made of pear tree or boxwood, with an arch of 15° to 30°, it is an example of a backstaff. ::figure[src="https://upload.wikimedia.org/wikipedia/commons/6/68/Almucantar-staff.png" caption="This is a drawing of an almucantar staff. There are three vanes - the horizon vane (A), the shadow vane (B) and the sighting vane (C)."] ::
The sun casts that shadow of a vane (B in the adjacent image) on a horizon vane (A). The horizon vane has a slit or hole to allow the observer to see the horizon in the distance. The observer aligns the horizon and shadow so they show at the same point on the horizon vane and sets the sighting vane (C) to align his line of sight with the horizon. The altitude of the sun is the angle between the shadow vane and the sighting vane (B-A-C).
Solar almucantar
The almucantar plane that contains the Sun is used to characterize multiple scattering of aerosols. Measurements are carried out rapidly at several angles at both sides of the Sun using a spectroradiometer or a photometer. There are several models to obtain aerosol properties from the solar almucantar. The most relevant were developed by Oleg Dubovik and used in the NASA AERONET network, and by Teruyuki Nakajima (named SkyRad.pack).
References
- Adelaide Observatory: Almucantar graphs of hour angles, Adelaide, R. E. E. Rogers, Govt. printer, 1927.
- Chandler, Seth Carlo, (1846–1913): The almucantar, Cambridge, J. Wilson and Son, 1887.
- Dubovik, O. and M. D. King, 2000: A flexible inversion algorithm for retrieval of aerosol optical properties from Sun and sky radiance measurements," Journal of Geophysical Research, 105, 20 673-20 696 pdf version
- Nakajima T, Tonna G, Rao RZ, et al.:Use of sky brightness measurements from ground for remote sensing of particulate polydispersions, Applied Optics 35 (15), 2672–2686, 1996
References
- {{OED. almucantar
- {{MerriamWebsterDictionary. almucantar
- [[Commander W.E. May. May, William Edward]], ''A History of Marine Navigation'', G. T. Foulis & Co. Ltd., Henley-on-Thames, Oxfordshire, 1973, {{ISBN. 0-85429-143-1
- [http://pen.agbi.tsukuba.ac.jp/~RStiger/hiki2/?Skyrad.pack SkyRad.pack] {{Webarchive. link. (2015-03-12 {{in lang). ja
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