「Radii」の共起表現一覧(1語右で並び替え)
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ve indices n1 and n2 and the core and cladding | radii a and b. |
tational axis of the Earth, and +0.55040 Earth | radii above the equatorial plane. |
ful information was transmitted was 42.3 Earth | radii, and the local time at this point was 2200 h. |
s estimated to have a radius around 0.13 solar | radii, and a mass of around 0.085 solar masses, or a |
radius of the primary is estimated at 60 solar | radii, and its mass is estimated to be between one a |
-anion distance determined by the sum of ionic | radii and the coordination number (C.N.) by the radi |
t a very large and bloated radius of 370 solar | radii and a high luminosity, 7,000 times higher than |
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. |
The radius of this star is 20 solar | radii and its surface temperature is 7200 kelvins. |
It has a radius of 30 solar | radii, and a luminosity of 269 suns. |
: Point lights, spotlights (both with editable | radii), and directional lights |
ions give linear scaling behaviour, and as the | radii are increased tend to the exact result. |
nowhere on the circle page is it stated that | radii are nonzero.Grabba (talk) 19:37, 4 March 2010 |
sons find that models underpredict the stellar | radii by approximately 5%. |
upergiants of spectral class F6 - K2 and their | radii change by (~25% for the longer-period l Car) m |
onal imaging at 2000-3000 A and up to 24 Solar | radii distance from Solar disk; |
and the perfectly-formed, tangentially-blended | radii formed on edges, which improves high- and low- |
falls within 1 crater radius of the rim, or 2 | radii from the center of the crater. |
at 15:35 UTC on March 31, 2004 (or 2.02 Earth | radii from the centre of the Earth.) |
It is 0.72344 Earth | radii from the rotation axis and +0.68811 Earth radi |
P. Rami - Quibus geodesiam adjecimus per usum | radii geometrici, Frankfurt: 1600. |
rs in the values of Mars' polar and equatorial | radii gives a considerably different result). |
ctral type G star, about 1.16 solar masses and | radii greater than our Sun, and only 200 Kelvins hot |
ular diameter and a linear radius of 450 Solar | radii have been measured in three colors by lunar oc |
helices with opposite directions but identical | radii, implying that the ratios differ only in sign; |
A putative radius of 0.0157 Earth | radii is also inferred. |
e van der Waals surface as given by the atomic | radii is shown in red. |
If the arcs have equal | radii, it is called a symmetric lens. |
are typically assumed to be compactified with | radii much larger than the traditional Planck length |
onalised by the smaller size of gallium (ionic | radii of Ga(III) 62 pm, In(III) 80 pm). |
net's orbit thereby defined the lengths of the | radii of the inner and outer limits of its celestial |
s 0.541 nm, calculated from geometry and ionic | radii of 0.074 nm (zinc) and 0.184 nm (sulfide). |
teric conflicts arising from the van der Waals | radii of the divergent atoms between target and temp |
osities of 18 and 13 times solar respectively, | radii of about twice solar and also masses of roughl |
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 |
For bend | radii of 50 times the material thickness of a low ca |
nd Simeonov's characterization in terms of the | radii of circles within each of four triangles |
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. |
The above equations give the | radii of the Moon and Sun entirely in terms of obser |
lane, are narrow, or have curves with tighter | radii or cambers. |
s estimated to have a radius around 0.12 solar | radii, or around 20% larger than Jupiter's, and a ma |
t of 6,500 Suns, and has a radius of 200 solar | radii, or 0.95 times the radius of Earth's orbit, th |
At large | radii, radial velocity dispersion exhibit strange be |
the inner main belt with a of over 100 primary | radii, S/2002 (3749) 1 is the most loosely-bound bin |
on, the heavier rare earths have smaller ionic | radii than the lighter ones. |
Beyond 5 | radii, the discontinuous debris is considered distal |
um separation at periastron is about 1.1 solar | radii; the maximum separation at apastron is 4.8 sol |
g south via the Serpukhovky and Zamoskvoretsky | radii to the district of Biryulyovo before continuin |
Several Virrat crater | radii to the north are the craters Koga and Nhill. |
e two surfaces of the reflector have different | radii to correct the aberration of the spherical mir |
t, whose centre was the Grand Hotel, and whose | radii were traced by a fan-work of avenues shaded wi |
r unlike the standard layout that Moscow Metro | radii, which follow a more or less tangental path to |
own glass with spherical surfaces of different | radii with the reflective coating on the shallower r |
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