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periodic celestial event comparison table |
Subject | has discoverer | has rate | has discovery date | has definition | occurs on | has location | has parent object | is a kind of | has radiant | has duration | is an instance of | has observer location | has period |
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active Sun | The Sun during its 11-year cycle of activity when spots, flares, prominences, and variations in radiofrequency radiation are at a maximum. | Sun | solar event | 11 years | |||||||||
equinox | Either of the two points on the celestial sphere at which the ecliptic intersects the celestial equator; also the time at which the Sun passes through either of these intersection points; i.e., when the apparent longitude (see apparent place; celestial longitude) of the Sun is 0° or 180°. (See catalog equinox; dynamical equinox for precise usage.) | periodic celestial event | 1 year | ||||||||||
Forbush decrease | Forbush | 1954 | A decrease in cosmic-ray intensity during active Sun. | Sun | solar event | 11 years | |||||||
location dependent periodic celestial event | Periodic celestial event which depends on the observers location on the planet | periodic celestial event | |||||||||||
meteor shower | the number of meteors observed in a given interval from the observers location | temporary increase in the rate at which meteors are observed when the target runs into a swarm of meteoroids that share a common orbit | which depends on the observer's location on the planet, is it facing the correct direction | the object from which the meteroids originate | periodic celestial event | a location on the sky from which meteor showers seem to originate | a few hours | one year | |||||
orbital event | Periodic celestial event in the orbit of a celestial body | periodic celestial event | 1 orbital period | ||||||||||
solar cycle | The 11-year period between maxima (or minima) of solar activity. Every 11 years the magnetic field of the Sun reverses polarity; hence the more basic period may be 22 years. | Sun | solar event | 11 years | |||||||||
solstice | One of the two points on the ecliptic at which the Sun appears to be farthest away from the celestial equator (representing therefore mid-summer or mid-winter). | periodic celestial event | 1 year |
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