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1 локальная
F-локальнаяlocal F-coronaмаксимальная локальнаяmaximum corona (in period of maximum solar activity)минимальная локальнаяminimum corona (in period of minimum solar activity)монохроматическая локальнаяmonochromatic coronaнепрерывная локальнаяcontinuum coronaполярная локальнаяpolar crown (of solar filaments)промежуточная локальнаяintermediate corona (of the Sun)протяженная локальнаяbroad haloпылевая локальнаяdust coronaрадио-локальнаяradio corona (of the Sun)рентгеновская локальнаяX-ray coronaсолнечная локальная1.solar corona 2.heliosphereсредняя локальнаяmiddle coronaультрафиолетовая локальнаяEUV coronaфраунгоферова локальнаяF-corona (of the Sun)электронная локальнаяelectron coronaэмиссионная линейчатая локальнаяemission line corona
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Solar variation — Solar variations are changes in the amount of solar radiation emitted by the Sun. There are periodic components to these variations, the principal one being the 11 year solar cycle (or sunspot cycle), as well as aperiodic fluctuations. Solar… … Wikipedia
Solar minimum — is the period of least solar activity in the solar cycle of the sun. During this time, sunspot and solar flare activity diminishes, and often does not occur for days at a time. The date of the minimum is described by a smoothed average over 12… … Wikipedia
Solar maximum — or solar max is the period of greatest solar activity in the solar cycle of the sun. During solar maximum, sunspots appear.Solar maximum is contrasted with solar minimum. Solar maximum is the period when the sun s magnetic field lines are the… … Wikipedia
Solar wind — For other uses, see Solar wind (disambiguation). The solar wind is a stream of charged particles ejected from the upper atmosphere of the Sun. It mostly consists of electrons and protons with energies usually between 1.5 and 10 keV. The stream of … Wikipedia
solar cycle — n. a period of time, averaging c. 11 years, during which certain phenomena, as maximum sunspot activity, recur on the sun … English World dictionary
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
Solar and Heliospheric Observatory — Infobox Space telescope name = Solar and Heliospheric Observatory (SOHO) caption = organization = ESA / NASA alt names = nssdc id = location = L1 orbit type = height = 1.5×106 km (heliocentric) period = 1 Earth year velocity = accel gravity =… … Wikipedia
Solar flare — A solar flare is a violent explosion in a star s (like the Sun s) atmosphere releasing as much energy as 6 times; 1025 Joules.cite journal last=Kopp first=G. coauthors=Lawrence, G and Rottman, G. year=2005… … Wikipedia
Solar Max — can be an abbreviation of two things: * The solar maximum period of greatest activity of the Sun * The Solar Maximum Mission satellite to investigate solar phenomena … Wikipedia
Solar power satellite — A solar power satellite, or SPS or Powersat, as originally proposed would be a satellite built in high Earth orbit that uses microwave power transmission to beam solar power to a very large antenna on Earth. Advantages of placing the solar… … Wikipedia
Modern Maximum — History of sunspot number observations showing the recent elevated activity. The Modern Maximum refers to the ongoing period of relatively high solar activity that began circa 1900.[1] This period is a natural example of solar variation, and one… … Wikipedia