«PHOTOSPHERIC»に関連する英語の本
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photosphericの使いかたを見つけましょう。
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1
Principles and Perspectives in Cosmochemistry
4.2 Comparison of Photospheric and Meteoritic Abundances The photospheric
and CI chondrite abundances on the astronomical abundance scale are given in
Table 3. Agreement within 10% for meteoritic and photospheric data exists for 40
...
2
Solar Photosphere: Structure, Convection, and Magnetic ...
FINE STRUCTURE OF PHOTOSPHERIC FACULAE R. MULLER Pic Du Midi
Observatory 65200 Bagneres de Bigorre ABSTRACT Properties of the
photospheric bright points associated with magnetic flux tubes are reviewed both
in faculae ...
3
The Composition of Matter: Symposium honouring Johannes ...
(2005) published modified photospheric abundance values. The photospheric
abundances of Mg and Fe in the Lodders (2003) publication are logMg = 7.55 ±
0.02 and logFe = 7.47 ± 0.03. These values are 0.02 higher than values
published ...
R. von Steiger, G. Gloeckler, G.M. Mason, 2007
4
Physics of the Interstellar and Intergalactic Medium
(2009); see text) Z X (mX)/a.mu SOUI'CG 1 H 1.0080 1 1 2 He 4.0026 9.55 X
1072*“01 3.82 X 1071 Photospheric 3 Li 6.941 2.00 X 1079*“05 1.38 X 1078
Meteoritic 4 Be 9.012 2.19 X 1071115“03 1.97 X 10710 Meteoritic 5 B 10.811
6.76 X ...
5
Plasma Astrophysics, Part II: Reconnection and Flares
and eruption of a long twisted filament along the photospheric neutral line before
the flare (Liu and Zhang 2001; Yan et al. 2001; Zhang et al. 2001). Bearing this
morphological fact in mind, we are going to consider some physical processes in
...
6
The Observation and Analysis of Stellar Photospheres
1.6) have higher luminosity and lower photospheric pressures. Indeed, pressure
effects are often referred to as luminosity effects. Those pressure effects that are
large enough to see at classification dispersion are used to assign the luminosity
...
7
The Century of Space Science
5 10 channel wavelength (Angstrom). ASCA SISO+SIS1 -Algol Ne/Fe L Mg/Ni Fe
K 20 in the (optical) determination of the photospheric abundances of active stars
, and in many cases accurate photospheric abundances are totally lacking.
J. A. M. Bleeker, Johannes Geiss, M. Huber, 2001
tinuum radiated from photospheric levels near r05 = 1. The network becomes
easily observable in photospheric lines and UV continua formed higher in the
photosphere. It is well seen in Fig. 5-2 around the layers of the temperature
minimum.
9
Encyclopedia of the Solar System
Berger with the Swedish Solar Observatory. photospheric temperature of T1⁄4
6400 K at l 1⁄4 5000 A ̊. These few ionized electrons come mostly from less
abundant elements with a low ionization potential, such as magnesium, while ...
Doris Breuer, Torrence Johnson, 2014
10
Issues in Astronomy and Astrophysics: 2013 Edition
According to news reporting originating in Berkeley, California, by VerticalNews
journalists, researchers stated “We show how the build-up of magnetic gradients
in the Sun's corona may be inferred directly from photospheric velocity data.
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Complex Organic and Inorganic Compounds in Shells of Lithium …
This shell would later be detached, specially when the star stops its Li enrichment and a rapid photospheric Li depletion occurs. In order to gain ... «Astrobiology News, 4月 15»
Mattel's View-Master Is Back, and Now It's a Virtual Reality Headset
... to offer virtual reality, augmented reality and “photospheric” images, using a smartphone as the display inside a plastic View-Master casing. «Yahoo Tech, 2月 15»
Hot explosions on the cool sun
The massive photospheric explosions cannot be spotted in visible light, but leave traces in the ultraviolet radiation the Sun emits into space. «Phys.Org, 10月 14»
Solar Explosions inside a Computer: Predicting Solar Flares
Citation: Mendoza M, Kaydul A, de Arcangelis L, Andrade JS, Herrmann HJ: “Modelling the influence of photospheric turbulence on solar flare ... «Scientific Computing, 9月 14»
Supernova Impostors Baffle Astronomers
... a gigantic bubble boiling on its surface and a vast plume of gas being ejected to at least six photospheric radii or roughly the orbit of Neptune. «Forbes, 8月 14»
The Maunder Minimum and sunspots
... dark, sharply defined region on the solar disc – marked by an umbra, dark area, which is 2000 degrees cooler than the effective photospheric temperature. «SunLive, 6月 14»
Observing solar explosions in visible light
The SCFS measurements of chromospheric and photospheric spectral lines, together with the continuum spectra, will be used to study a variety ... «SPIE Newsroom, 12月 13»
New and remarkable details of the sun now available from NJIT's …
The other photospheric photograph is the most precise sunspot image ever taken: A textbook sunspot that looks like a daisy with many petals. «Eureka! Science News, 8月 13»
NRL Leads NASA Team Workshop on "Coronal Mass Ejection …
Second: how can photospheric observations of flux emergence and dynamics be incorporated into coronal CME initiation simulations to ... «U.S. Naval Research Laboratory, 7月 12»
FUSE Detects Xenon and Krypton in White Dwarf Star
Along with krypton and xenon, the team observing RE 0503-289 also detected highly ionized photospheric lines from other trans-iron group ... «Sci-News.com, 7月 12»
