例文 | 共起表現 |
「Θ」の共起表現一覧(1語右で並び替え)
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ahedra, and then rotating each by an equal angle | θ about a separate axis passing through the centre |
f is semiconjugate to the irrational rotation by | θ, and the semiconjugating map h of degree 1 is co |
ion (also in other sections α, β, γ, δ, ε, ζ, η, | θ) and in particular the arguments offered by the |
The law of cosines for | θ and θ′ states |
Let the angles formed between a and d be | θ and θ′ where θ includes b and θ′ includes c. |
The sequence cn( | θ) is the signature of θ, and it is a fractal sequ |
the origin of the coordinate system that defines | θ and ω to the point of interest. |
Theta Andromedae ( | θ And, θ Andromedae) is a binary star in the const |
As | θ approaches zero, none of the energy is transferr |
The maximum amount of energy is transferred when | θ approaches 180 degrees. |
Theta Apodis ( | θ Aps, θ Apodis) is a star in the constellation Ap |
Theta Aquilae ( | θ Aql, θ Aquilae) is a binary star in the constell |
Theta Aquarii ( | θ Aqr, θ Aquarii) is a star in the constellation A |
Theta Arae ( | θ Ara, θ Arae) is a star in the constellation Ara. |
pronouncing it as a sharp, dental /s̪/, or even | /θ/ as in English "thing". |
Theta Aurigae ( | θ Aur, θ Aurigae) is a binary star in the constell |
Stars α Aur (Capella), β Aur, | θ Aur, ι Aur, and ε Aur form the charioteer's head |
A third star, the 11th magnitude | θ Aurigae C, is 49 arcseconds away, and is an opti |
The primary, | θ Aurigae A, is a white A-type main sequence dwarf |
Its companion, | θ Aurigae B, is a yellow G-type main sequence dwar |
Let | θ be the angle between m and d and θ′ the angle be |
Let | θ be the angle subtended by the arc s at the centr |
n of supersymmetry, depend only on the variables | θ but not their conjugates. |
θ Cancri is classified as an orange K-type giant w | |
rom studying its light curve during occultation, | θ Cancri is shown to be a close binary, consisting |
It corresponds to γ, δ and | θ Cancri, in the Cancer (constellation). |
Theta Cassiopeiae ( | θ Cas, θ Cassiopeiae) is a star in the constellati |
θ Cassiopeiae is a white A-type main sequence dwar | |
Theta Centauri ( | θ Cen, θ Centauri) is a star in the constellation |
The bright stars of this constellation (α Cen, | θ Cen, ε Cen and η Cen) are seen in Chinese sky, e |
Theta Cephei ( | θ Cep, θ Cephei) is a Class A7, fourth-magnitude s |
Theta Cancri ( | θ Cnc, θ Cancri) is a binary star in the constella |
e length of the chord corresponding to an arc of | θ degrees is |
the electrolyte, A denotes the surface area and | Θ denotes the fraction of the R and O species pres |
the baby from a line of charging hyenas (ι Dra, | θ Dra, η Dra, and ζ Dra). |
s that our geodesics must converge in a caustic ( | θ goes to minus infinity) within a proper time of |
Theta Herculis ( | θ Her, θ Herculis) is a fourth-magnitude star in t |
σaθb(R) selects all those tuples in R for which | θ holds between the a and the b attribute. |
notes expected value over the distribution P(x | | θ), i.e. averaging over all possible observations |
Sine, cosine, and versine of | θ in terms of a unit circle, centered at O |
For each unit vector | θ in S⊥, the orthogonal complement of S, let Sθ de |
there is no dependence on the unknown parameter | θ in the expression for SURE above. |
(pictured), for a certain intermediate value of | θ in which 24 of the triangles form coplanar pairs |
he octahedra have been rotated by the same angle | θ in the opposite direction, yields the compound o |
ation, which says that in order to prove φ → ∃ x | θ intuitionistically, one must create a function t |
s 2θ R2, where R is the radius of the sphere and | θ is the dihedral angle between the two half great |
In mathematics, a cardinal λ < | Θ is a Suslin cardinal if there exists a set P ⊂ 2 |
Ch is the correction of height due to slope, | θ is the angle formed by the slope line oriented f |
ctions where their path-length difference 2d sin | θ is equal to an integer multiple of the wavelengt |
Assume that φ → ∃ x | θ is provable. |
Thus ∃ x (φ → | θ) is provable. |
if | θ is measured in degrees, and |
θ is a binary operation in the set | |
If Φ is a tautology, and | Θ is a substitution instance of Φ, then Θ is again |
When | θ is 60 degrees, the more symmetric compound of fo |
When | θ is 45 degrees, the more symmetric compound of si |
Θ is also the supremum of the lengths of all prewe | |
where | θ is the zenith angle (or zenith distance, i.e. th |
where | θ is to be interpreted as polar angle such that it |
When | θ is 45 degrees, the cubes coincide in pairs yield |
When | θ is 60 degrees, the octahedra coincide in pairs y |
When | θ is zero or 60 degrees, the octahedra coincide in |
When | θ is 36 degrees, the antiprisms coincide in pairs |
s (or even if the reals can be wellordered) then | Θ is simply , the cardinal successor of the cardin |
if and only if it is bipartite and the relation | Θ is transitive. |
ed perimeter (2w + 2d) of the Wilhelmy plate and | θ is the contact angle between the liquid phase an |
In cylindrical coordinates, theta, | θ, is almost universally used to represent the azi |
The theta meson ( | θ) is a hypothetical form of quarkonium (i.e. a fl |
where R is the distance to the particle, | θ is the scattering angle, n is the refractive ind |
the porosity (0-1), σ is the surface tension and | θ is the contact angle. |
where, | θ is the absolute value of the angle through which |
Here | Θ is the angle between the asymptotes of the hyper |
On the other hand, a proof of ∃ x (φ → | θ) must first demonstrate a particular x, and then |
e second equation by m, and add to eliminate cos | θ, obtaining |
Not to be confused with the | θ+ of the τ-θ puzzle, which is now identified as ka |
the azimuth is usually denoted by either theta, | θ, or phi, φ. |
reports of a resonance which they interpret as a | Θ+ pentaquark candidate made of two up quarks, two |
Theta Persei ( | θ Per) is a star system 37 light years away from E |
Theta Pictoris ( | θ Pic, HR 1818, HD 35860, SAO 233965, CP -52 718, |
Theta Piscium ( | θ Psc) is a star approximately 159 light years awa |
where ρ and | θ range from negative infinity to positive infinit |
Therefore, 1 − | θ represents the fraction of binding sites that ar |
The variable | θ represents the fraction of binding sites that ar |
Theta Scorpii ( | θ Sco, θ Scorpii) is a star in the constellation S |
θ Scorpii A is a yellow giant of spectral type F1 | |
The Bayer designation Theta Sagittarii ( | θ Sgr, θ Sagittarii) is shared by two star systems |
Here | Θ signifies an asymptotically tight bound. |
2 DNA Pol III enzymes, made up of α, ε and | θ subunits. |
Theta Tauri ( | θ Tau, θ Tauri) is a star system in the constellat |
ill holds, but with Tc replaced by a temperature | Θ that is somewhat higher than the actual Curie te |
ned in terms of the object's actual size, x, and | θ the angular size of the object as viewed from ea |
th of the beam, n being the refractive index and | θ the wedge angle. |
x atoms per volume, λ the electron escape depth, | θ the analyzer angle, T the transmission of the an |
Some authors call | Θ the Weiss constant to distinguish it from the te |
he magnetostrictive expansion at saturation, and | θ the angle between the saturation magnetization a |
treat photon radial geodesic with constant r and | θ, therefore |
For the same value of the solar mixing angle, | θ, this would correspond to a suppression Pee ≈ 60 |
Theta Trianguli Australis ( | θ TrA, θ Trianguli Australis) is a star in the con |
Theta Tucanae ( | θ Tuc, θ Tucanae) is a star in the constellation T |
Theta Ursae Majoris ( | θ UMa, θ Ursae Majoris) is a binary star in the co |
Theta Ursae Minoris ( | θ UMi, θ Ursae Minoris) is a star in the constella |
Writing the trace as | θ, we have |
ltiply the numerator and denominator by (1 - cos | θ), we get |
with the anode wires in the azimuthal direction, | θ, which provides information on the radial coordi |
If confirmed, the | Θ+ would be the first discovered exotic baryon. |
These have no voiceless counterparts (such as /f | θ x/). |
例文 | 共起表現 |
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