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・ Urstromtaler
・ Ursu
・ Urs Schönenberger
・ Urs Sonderegger
・ Urs Steinmann
・ Urs Suter
・ Urs Vercoli
・ Urs Vescoli
・ Urs von Wartburg
・ Urs Widmer
・ Urs Zimmermann
・ Urs, Ariège
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・ Ursa
・ Ursa (comics)
Ursa (Finland)
・ Ursa (spider)
・ Ursa constellation
・ Ursa Dwarf
・ Ursa ibn al-Zubayr
・ Ursa Major
・ Ursa Major (album)
・ Ursa Major (Chinese astronomy)
・ Ursa Major (comics)
・ Ursa Major (disambiguation)
・ Ursa Major (excavator)
・ Ursa Major (sculpture)
・ Ursa Major Cluster
・ Ursa Major Dwarf
・ Ursa Major I Dwarf


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Ursa (Finland) : ウィキペディア英語版
Ursa (Finland)

Ursa Astronomical Association ((フィンランド語:Tähtitieteellinen yhdistys Ursa ry)) is the largest astronomical association in Finland. Ursa was founded on 2 November 1921. Founding members include a renowned Finnish astronomer Yrjö Väisälä. In 1926 Ursa established the Ursa Observatory in Kaivopuisto district of Helsinki. In 2007 the Tähtikallio Observatory & Education Center was established in Artjärvi, its current equipment includes an Astrofox 36" Folded Newtonian Open tube telescope, an Alluna 16" Ritchey-Chrétien telescope, a Meade 16" LX200GPS Schmidt-Cassegrain telescope, a Sky-Watcher ED 120mm refractor telescope fitted with a Baader AstroSolar Solar Filter and a piggybacked Coronado SolarMax 40 H-Alpha telescope. Ursa's primary functions include advancing amateur astronomy and astronomical education. They have also published a magazine ''Tähdet ja avaruus'' since 1971. Anyone interested in astronomy can join the 17,500-member organization.
==Sections==
The organization has thirteen sections specialized in different aspects of amateur astronomy (and meteorology):
* Solar section
* Halo section
* Instrument section
* Atmospheric optical phenomena section
* Clubs and organization
* Lunar, planetary and cometary section
* Mathematics and information technology section
* Meteor section
* Storm chasing section
* Minor planet and occultation section
* Aurora section
* Deep sky section
* Satellite section
In addition, Ursa has two loosely organized hobby groups:
* Variable stars
* Observation conditions

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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