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1 факел
faculaфакел со вспышкойflare-like faculaполярные факелыpolar faculaeсолнечные факелыsolar faculaeфотосферные факелыphotospheric faculaeхромосферные факелы1.chromospheric faculae 2.flocculi -
2 фотосферные факелы
Makarov: photospheric faculaeУниверсальный русско-английский словарь > фотосферные факелы
См. также в других словарях:
Corona — This article is about the astronomical term. For other uses, see Corona (disambiguation). During a total solar eclipse, the solar corona can be seen with the naked eye. A corona is a type of plasma atmosphere of the Sun or other celestial body,… … Wikipedia
facula — facular, adj. /fak yeuh leuh/, n., pl. faculae / lee /. Astron. an irregular, unusually bright patch on the sun s surface. [1700 10; < L: little torch, equiv. to fac (s. of fax) torch + ula ULE] * * * ▪ astronomy in astronomy, bright… … Universalium
Plage (astronomy) — A plage is a bright region in the chromosphere of the Sun, typically found in regions of the chromosphere near sunspots. The term itself is poetically taken from the French word for beach. The plage regions map closely to the faculae in the… … Wikipedia
Sun — This article is about the star. For other uses, see Sun (disambiguation). The Sun … Wikipedia
Solar cycle — The solar cycle, or the solar magnetic activity cycle, is the main source of periodic variation of all solar phenomena driving variations in space weather. [ [http://www7.nationalacademies.org/ssb/SSB Space weather97.pdf Space Weather: A Research … Wikipedia
Limb darkening — refers to the diminishing of intensity in the image of a star as one moves from the center of the image to the edge or limb of the image. Limb darkening occurs as the result of two effects:* The density of the star diminishes as the distance from … Wikipedia
Coronal radiative losses — In astronomy and in astrophysics, for radiative losses of the solar corona, it is meant the energy flux irradiated from the external atmosphere of the Sun (traditionally divided into chromosphere, transition region and corona), and, in particular … Wikipedia
Nanoflares — A nanoflare is a very small solar flare which happens in the corona, the external atmosphere of the Sun. The hypothesis of microflares as a possible explanation of the coronal heating was first suggested by Gold [1] and then later developed by… … Wikipedia