%TOC% ---+ Conventions * All angles or coordinates are stored internally in *radians* * All angles or coordinates mostly are presented to the user in *degrees* (sexagesimal format for stars) * double must be used as storage ---+ Use cases ---++ Observability of a source (or list of sources) for a given interferometer |Inputs| User format | internal format | |Star coordinate | anything valid (name or any std coords) | RAJ2000,DEJ2000 | |Observing site location | selection of one supported observatory | [[http://jmmc.fr/~upsa/oischema/http___www.jmmc.fr_aspro-oi_0.1/complexType/InterferometerDescription.html][observatory reference]] | |Date of observation ( or period of time )|like DDMMYYYYHHMM| (Modified) Julian Day ( precise up to the second )| Plot outputs: TODO : How to represent the observability of a list of star onto multi-telescope ---+++ Is the source visible in the sky ? ---++++ Is the source over the horizon ? |outputs|Internal/User| Format | | celestial coordinates | Internal | HA / delta ?? units TBC TBD | | over the horizon | User | boolean | ---++++ What is the AirMass value ? |Inputs| User format | internal format | | Seeing | choice or value ? | TBD | | Humidity / Temperature... | choice or value ? | TBD | |outputs|Internal/User| Format | | AirMass | User | double | What is the best method to get the airmass value? ---++++ Where are the sun / moon ? |Inputs| User format | internal format | | twilight constraints | angle degrees <br/> GM: est-ce que ASTRO/NAVAL/CIVIL sont des valeurs discrites qui parlent ? | double radians | |outputs|Internal/User| Format | | sunrise sunset moonrise moonset | User | DateTime couples | Est-ce qu'il faut gerer d'autre planetes sources lumineuses ??? Quelles doit etre la precision pour les ephemerides? ---++++ Is the star still visible given to a shadowing ??? |Inputs| User format | internal format | | environment shadowing ( telescopes, mountains, building ....)| angle d'obstruction ( de 0 a 90 degres) en fonction de l'azimuth (repere a definir) | couples of Altitude / Azimuth points ( pointer ver la specification (a faire) ) | | telescope(s) min elevation | angle degree | angle radians | |outputs|Internal/User| Format | | | | | ---+++ What is the formulae of the observability given to the whole previous results? A-t'on besoin de calculer l'AirMass par station? Est-ce que la voute celeste est la meme pour toutes les stations a un meme moment? S'arrete-ton des le premier critere mauvais ou doit on faire un bilan de pertes...( par ex: une mauvaise airmass compensee par un configuration optique avec moins de pertes) Comment gere-t'on l'observalité d'une liste d'etoiles? Est simplement la juxtaposition des resultats independants ou y-a t'il des contraintes de gestion par groupe? ---++ Modelling of a source from a given interferometer TBD ---+ Various informations ---++ Station Coordinates The software handles station coordinates as described in the OIFITS (see OI_ARRAY table description). ---+++ VLTI configuration Eso defines the coordinates in an propriatary maner. The right way to get the right informations is to read the data from an AMBER oifits ( may be generated by ASPRO ). ---+++ CHARA configuration Chara expresses the station coordinates in the same format as OIFITS : TBD find URL ---++ Java astronomy libraries [[http://www.dartmouth.edu/~physics/faculty/skycalc/flyer.html][JSkyCalc = Java version of skycalc]]<br/> [[http://mhuss.com/AstroLib.html][AstroLib]] [[(URL to be defined)][PAL projet astrogrid (utilisé par APES et topcat)]] Verifier : conversion coordonnees et ephemerid (au moins soleil et lune) ---++ Various libraries * http://jas.freehep.org/jas3/
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Topic revision: r5 - 2009-09-29 - GuillaumeMella
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