「electromagnetic」の共起表現一覧(1語左が「the」)
該当件数 : 132件
"Sharpening the | Electromagnetic Arrow(s) of Time." |
On the Moon, the | electromagnetic machine is assembled. |
xwell publishes A Dynamical Theory of the | Electromagnetic Field. |
ment of the microwave radio region of the | electromagnetic spectrum. |
th the visible and invisible parts of the | electromagnetic spectrum. |
oduces a characteristic absorption in the | electromagnetic spectrum of the compound involved. |
The V band (vee-band) of the | electromagnetic spectrum ranges from 50 to 75 GHz. |
of practical dimensions that imitated the | electromagnetic response of natural dielectric solids. |
ompilation contains information about the | electromagnetic scattering by spherical particles, releva |
In microwave physics, the | electromagnetic properties of matter at microwave frequen |
He was the inventor of the | electromagnetic transmission and a pioneer in the early a |
rpose of this experiment was to study the | electromagnetic reflective properties of the lunar surfac |
ompilation contains information about the | electromagnetic scattering by cylindrical particles, rele |
e of the experiment consists in using the | electromagnetic propagation through the cometary interior |
It generalizes the | electromagnetic potential but it has two indices instead |
Most meters measure the | electromagnetic radiation flux density (DC fields) or the |
Manticore was still alive, thanks to the | electromagnetic field, so she attempted to finish things |
The Q band of the microwave part of the | electromagnetic spectrum and ranges from 33 to 50 GHz. |
frequencies from 60 GHz to 100 GHz in the | electromagnetic spectrum. |
can refer to two different regions of the | electromagnetic spectrum, in the radio and near-infrared. |
designed to allow for measurements of the | electromagnetic interference existing on the power line. |
f immense amounts of energy, spanning the | electromagnetic spectrum, with the surroundings. |
analog of the vector potential A for the | electromagnetic field. |
thin the ultra high frequency part of the | electromagnetic spectrum. |
and outer space in various regions of the | electromagnetic spectrum, and |
isible and the near infrared parts of the | electromagnetic spectrum is observed. |
infrared, and water vapor regions of the | electromagnetic spectrum. |
ss is conserved during the strong and the | electromagnetic interactions, but not during the weak int |
ithin the very high frequency part of the | electromagnetic spectrum. |
requencies from 110 GHz to 170 GHz in the | electromagnetic spectrum. |
ithin the very high frequency part of the | electromagnetic spectrum. |
or at least the public disclosure) of the | electromagnetic digital computer. |
ntinuum and line-emission portions of the | electromagnetic spectrum of Mkn 590 are highly variable. |
o frequencies from 8 GHz to 10 GHz in the | electromagnetic spectrum. |
network management) and management of the | electromagnetic spectrum. |
field equations, can be thought of as the | electromagnetic laws of attraction and repulsion. |
First of all the total energy of the | electromagnetic field is finite and the electric field is |
frequencies from 90 GHz to 140 GHz in the | electromagnetic spectrum. |
io frequencies from 2 GHz to 3 GHz in the | electromagnetic spectrum. |
k sorceress, who uses Rogue to battle the | electromagnetic demon Magnus. |
requencies from 250 MHz to 500 MHz in the | electromagnetic spectrum. |
visible and near infrared regions of the | electromagnetic spectrum. |
they do not interact with matter via the | electromagnetic or gravitational forces, it is extremely |
can refer to two different regions of the | electromagnetic spectrum, in the radio and near-infrared. |
frequencies from 10 GHz to 20 GHz in the | electromagnetic spectrum. |
of material that minimally attenuates the | electromagnetic signal transmitted or received by the ant |
dio, X-ray, and gamma ray portions of the | electromagnetic spectrum. |
of radio frequencies up to 250 MHz in the | electromagnetic spectrum. |
spective", The new astronomy: opening the | electromagnetic window and expanding our view of planet e |
Originally, the | electromagnetic radiation emitted by X-ray tubes had a lo |
s an instrument for rapidly measuring the | electromagnetic permeability of samples of iron or steel |
slo he has also studied properties of the | electromagnetic field produced by accelerated electric ch |
ion (about 30 - 150 µm wavelength) of the | electromagnetic spectrum. |
monitors the changes in the phase of the | electromagnetic field surrounding a signal being applied |
n two of the four fundamental forces, the | electromagnetic interaction and the strong interaction. |
That is, the | electromagnetic field has infinitely more degrees of free |
t say that the phase space offered by the | electromagnetic field is infinitely larger than that offe |
e the radiation pressure follows from the | electromagnetic theory. |
ed 'wake-fields' (a strong warping of the | electromagnetic field of the beam) that can interact with |
ity measurements showed an anomaly in the | electromagnetic signature that it was thought might be ca |
g three out of four forces of nature: the | electromagnetic force, the strong force, and the weak for |
are spread out because the carrier of the | electromagnetic force, the photon, does not interact with |
output to move towards the red end of the | electromagnetic spectrum. |
ss, and among the first papers to use the | electromagnetic telegraph. |
of the galaxy in the radio portion of the | electromagnetic spectrum show two jets protruding in oppo |
in the X-ray and Gamma ray regions of the | electromagnetic spectrum. |
onary orbit locations and portions of the | electromagnetic spectrum. |
io frequencies from 4 GHz to 6 GHz in the | electromagnetic spectrum. |
tube of a solid cylinder, and models the | electromagnetic and gravitational fields inside the beam, |
rates in the low frequency portion of the | electromagnetic spectrum from 90 to 110 Kilohertz. |
unt for the coupling between them and the | electromagnetic field. |
ation emitted in the infrared part of the | electromagnetic spectrum. |
in the low (or far) infrared range of the | electromagnetic spectrum. |
he four forces of nature-the weak and the | electromagnetic forces-under the same set of equations. |
Changing the | electromagnetic radiation used to detect, discover, and o |
itz and Heinz London, who showed that the | electromagnetic free energy in a superconductor is minimi |
ure of the object as well, by mapping the | electromagnetic scattering coefficient onto a two-dimensi |
As with any wave, the | electromagnetic wave transports energy, thus the total en |
, citing the physiological effects of the | electromagnetic field from transmission lines. |
e some form of bioluminescence within the | electromagnetic spectrum, but most are neither visible no |
ions in the far-ultraviolet region of the | electromagnetic spectrum. |
thin the ultra high frequency part of the | electromagnetic spectrum. |
he super high frequency (SHF) part of the | electromagnetic spectrum. |
EMP is that all of the components of the | electromagnetic pulse are generated outside of the weapon |
devices which strengthen and maintain the | electromagnetic field which defines her humanoid form. |
ation utilizing conventional bands of the | electromagnetic spectrum (i.e. |
ultraviolet and infrared portions of the | electromagnetic spectrum. |
e ultraviolet to the radar regions of the | electromagnetic spectrum. |
After most of the | electromagnetic pulse measurements on Starfish Prime had |
gents, and was also badly affected by the | electromagnetic fields of TVs, radios and even human bein |
sical nongravitational fields such as the | electromagnetic field. |
d state, there are many ways in which the | electromagnetic field may go from the ground state to a o |
the flares have been detected across the | electromagnetic spectrum as high as the X-ray band. |
ar gravitational field in addition to the | electromagnetic field potential Aμ in an attempt to creat |
for large changes in the intensity of the | electromagnetic field. |
rovide intense focused light spanning the | electromagnetic spectrum from the infrared through x-rays |
n this happens due to the presence of the | electromagnetic field from a photon, a photon is released |
sorbance in the ultraviolet region of the | electromagnetic spectrum, which is useful for laboratory |
ow, the only two wavelength ranges of the | electromagnetic spectrum that are not severely attenuated |
nt of energy due to inefficiencies in the | electromagnetic accelerators and decelerators in the towe |
enkov emission in the radio regime of the | electromagnetic spectrum from the interaction of high ene |
y frequencies, or frequency bands, in the | electromagnetic spectrum for use in systems or equipment. |
hey are often divided into two types: the | electromagnetic calorimeter that specializes in absorbing |
cance: it ensures the universality of the | electromagnetic interaction." |
d, or in any other frequency range of the | electromagnetic radiation). |
It is even possible to monitor the | electromagnetic emissions of computer displays or keyboar |
portion to the current carried due to the | electromagnetic field. |
o not interact with matter via either the | electromagnetic, the strong nuclear, or gravitational for |
round field is a classical version of the | electromagnetic ZPF of QED, though in SED literature the |
nate the electric field shown as E in the | electromagnetic wave equation which can be derived from M |
steresis as the magnetic component of the | electromagnetic field repeatedly distorts the crystalline |
the end of the 1980s, the topology of the | electromagnetic field was studied in detail and a topolog |
ts), that operate in the same part of the | electromagnetic spectrum as radar guns. |
like charged particles are sources of the | electromagnetic field. |
stronomical objects at wavelengths of the | electromagnetic spectrum that cannot penetrate the Earth' |
ion of the radio frequency portion of the | electromagnetic spectrum (also known as spectrum manageme |
astrophysics, and observations across the | electromagnetic spectrum have contributed much to our cur |
ity in the fundamental fields such as the | electromagnetic potential A. For example, in an SU(N) Yan |
incident is particularly notable for the | electromagnetic interference effects observed upon aircra |
rk Maxwell in 1873, is the physics of the | electromagnetic field; a field encompassing all of space |
etric tensor and the antisymmetric to the | electromagnetic field tensor. |
ell into the far infrared portions of the | electromagnetic spectrum. |
rk Maxwell's mathematical theories of the | electromagnetic field during the late 1870s and all of th |
ons are in the ultraviolet portion of the | electromagnetic spectrum of the hydrogen atom and immedia |
views the very high energy density of the | electromagnetic vacuum as propagating waves, which must n |
ounds, called susceptors, that absorb the | electromagnetic energy from the induction coil, become ho |
The change in velocity of the | electromagnetic wave induced by propagation through the c |
ifference is related to the fact that the | electromagnetic potential is integrated over one-dimensio |
so observations in these portions of the | electromagnetic spectrum are best carried out from a loca |
, which characterizes the strength of the | electromagnetic interaction, is dimensionless. |
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