「Radii」の共起表現一覧(2語右で並び替え)
該当件数 : 56件
s estimated to have a radius around 0.13 solar | radii, and a mass of around 0.085 solar masses, or a |
t a very large and bloated radius of 370 solar | radii and a high luminosity, 7,000 times higher than |
rs in the values of Mars' polar and equatorial | radii gives a considerably different result). |
It has a radius of 30 solar | radii, and a luminosity of 269 suns. |
osities of 18 and 13 times solar respectively, | radii of about twice solar and also masses of roughl |
A putative radius of 0.0157 Earth | radii is also inferred. |
ve indices n1 and n2 and the core and cladding | radii a and b. |
for other transition metals with similar ionic | radii (Fe2+ and Mg2+). |
sons find that models underpredict the stellar | radii by approximately 5%. |
s estimated to have a radius around 0.12 solar | radii, or around 20% larger than Jupiter's, and a ma |
ular diameter and a linear radius of 450 Solar | radii have been measured in three colors by lunar oc |
upergiants of spectral class F6 - K2 and their | radii change by (~25% for the longer-period l Car) m |
lane, are narrow, or have curves with tighter | radii or cambers. |
nd Simeonov's characterization in terms of the | radii of circles within each of four triangles |
e two surfaces of the reflector have different | radii to correct the aberration of the spherical mir |
: Point lights, spotlights (both with editable | radii), and directional lights |
Beyond 5 | radii, the discontinuous debris is considered distal |
r unlike the standard layout that Moscow Metro | radii, which follow a more or less tangental path to |
P. Rami - Quibus geodesiam adjecimus per usum | radii geometrici, Frankfurt: 1600. |
onal imaging at 2000-3000 A and up to 24 Solar | radii distance from Solar disk; |
onalised by the smaller size of gallium (ionic | radii of Ga(III) 62 pm, In(III) 80 pm). |
n, geostationary satellites orbit at 5.6 Earth | radii and GPS satellites orbit at 3.17 Earth radii f |
This application exploits the similar ionic | radii and hydrophilicity of perchlorate and iodide. |
ction: 0.713 by 0.535 in (18 by 14 mm); corner | radii: 0.143 in (3.6 mm) |
ions give linear scaling behaviour, and as the | radii are increased tend to the exact result. |
If the arcs have equal | radii, it is called a symmetric lens. |
radius of the primary is estimated at 60 solar | radii, and its mass is estimated to be between one a |
The radius of this star is 20 solar | radii and its surface temperature is 7200 kelvins. |
-> 349,000 and found the number of 4.89 Jovian | radii (71398 km) which would make a distance of 349, |
are typically assumed to be compactified with | radii much larger than the traditional Planck length |
um separation at periastron is about 1.1 solar | radii; the maximum separation at apastron is 4.8 sol |
nowhere on the circle page is it stated that | radii are nonzero.Grabba (talk) 19:37, 4 March 2010 |
and the perfectly-formed, tangentially-blended | radii formed on edges, which improves high- and low- |
Similar atomic | radii (15% or less difference) |
e van der Waals surface as given by the atomic | radii is shown in red. |
ctral type G star, about 1.16 solar masses and | radii greater than our Sun, and only 200 Kelvins hot |
helices with opposite directions but identical | radii, implying that the ratios differ only in sign; |
on, the heavier rare earths have smaller ionic | radii than the lighter ones. |
ful information was transmitted was 42.3 Earth | radii, and the local time at this point was 2200 h. |
net's orbit thereby defined the lengths of the | radii of the inner and outer limits of its celestial |
falls within 1 crater radius of the rim, or 2 | radii from the center of the crater. |
teric conflicts arising from the van der Waals | radii of the divergent atoms between target and temp |
own glass with spherical surfaces of different | radii with the reflective coating on the shallower r |
-anion distance determined by the sum of ionic | radii and the coordination number (C.N.) by the radi |
ing a domain of area F. Let r and R denote the | radii of the incircle and the circumcircle. |
The dusty arms extend 6 times the | radii of the starry arms of the galaxy, and is shown |
at 15:35 UTC on March 31, 2004 (or 2.02 Earth | radii from the centre of the Earth.) |
g south via the Serpukhovky and Zamoskvoretsky | radii to the district of Biryulyovo before continuin |
It is 0.72344 Earth | radii from the rotation axis and +0.68811 Earth radi |
Several Virrat crater | radii to the north are the craters Koga and Nhill. |
where rA and rB denote the atomic | radii of the two atoms. |
90% of the debris falls within approximately 5 | radii of the center of the crater. |
tational axis of the Earth, and +0.55040 Earth | radii above the equatorial plane. |
The above equations give the | radii of the Moon and Sun entirely in terms of obser |
t, whose centre was the Grand Hotel, and whose | radii were traced by a fan-work of avenues shaded wi |
At large | radii, radial velocity dispersion exhibit strange be |
こんにちは ゲスト さん
ログイン |
Weblio会員(無料)になると 検索履歴を保存できる! 語彙力診断の実施回数増加! |
こんにちは ゲスト さん
ログイン |
Weblio会員(無料)になると 検索履歴を保存できる! 語彙力診断の実施回数増加! |