-
1 chromospheric line
-
2 хромосферная линия
-
3 интенсивность
1.intensity 2.strengthинтенсивность источника излученияsource strengthинтенсивность космических лучейcosmic ray intensityинтенсивность падающего излученияincident (radiation) intensityинтенсивность поглощенияabsorption strengthинтенсивность полярного сиянияauroral intensityинтенсивность светаlight intensityинтенсивность скачка уплотненияshock-wave strengthинтенсивность спектральной линии1.intensity of spectral line 2.line strengthинтенсивность хромосферной активностиchromospheric intensityинтегральная интенсивностьintegrated intensityспектральная интенсивностьspectral intensity -
4 intensity
@intensity of spectral lineинтенсивность спектральной линии@intensity of terrestrial magnetismнапряженность магнитного поля Земли@auroral intensityинтенсивность полярного сияния@chromospheric intensityинтенсивность хромосферной активности@cosmic ray intensityинтенсивность космических лучей@horizontal intensityгоризонтальная составляющая напряженности геомагнитного поля@
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
Coronal loop — Typical coronal loops observed by TRACE Coronal loops form the basic structure of the lower corona and transition region of the Sun. These highly structured and elegant loops are a direct consequence of the twisted solar magnetic flux within the… … Wikipedia
Tau Ceti — Starbox begin name=Tau Ceti Starbox image caption=Tau Ceti (highlighted center) in the southern part of the constellation Cetus. Starbox observe epoch=J2000 constell=Cetus ra=RA|01|44|04.0829cite web url=http://simbad3.u strasbg.fr/sim… … Wikipedia
sun — sunlike, adj. /sun/, n., v., sunned, sunning. n. 1. (often cap.) the star that is the central body of the solar system, around which the planets revolve and from which they receive light and heat: its mean distance from the earth is about 93… … Universalium
List of radio propagation topics — This is a list of radio propagation terms. NOTOC A a index A index aa index active prominence active prominence region (APR) active region active surge region (ASR) active dark filament (ADF) AE index Air Force Geophysics Laboratory (AFGL) arch… … Wikipedia
Capella (star) — For other uses, see Capella (disambiguation). Capella Aa/Ab Capella is the brightest star in Auriga Observation data Epoch J2000.0 … Wikipedia
61 Cygni — Not be confused with 16 Cygni, a more distant system containing two G type stars harboring the gas giant planet 16 Cygni Bb. Starbox begin name=61 CygniStarbox image caption=Expanded view of the star field around 61 Cygni. This system is located… … Wikipedia
Proxima Centauri — Coordinates: 14h 29m … Wikipedia
Upsilon Andromedae — Starbox begin name = Upsilon Andromedae Starbox observe epoch = J2000.0 constell = Andromeda ra = 01h 36m 47.8s dec = +41° 24 20 appmag v =4.09 Starbox character class = F8V r i = 0.30 v r = 0.30 b v = 0.54 u b = 0.06 variable = Starbox… … Wikipedia
Meghnad Saha — মেঘনাদ সাহা Meghnad Saha in Berlin Born 6 October 1893( … 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