「precession」の共起表現(1語右で並び替え) - Weblio英語共起表現検索


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Weblio 辞書 > 英和辞典・和英辞典 > precessionの意味・解説 > precessionに関連した共起表現

「precession」の共起表現一覧(1語右で並び替え)

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shift can also be discerned, (the planetary precession, along the instantaneous equator, which resu
This apsidal precession also causes the full moon cycle, which can b
* The theories of precession and nutation have advanced since 1976, and t
The difference between de Sitter precession and Lense-Thirring precession (frame draggin
nalysing the Earth's rotation, including its precession and nutation, and using observations to supp
ough cyclical & Zodiacal stages based on the precession, and that myths which encode this astronomic
The difference between de Sitter precession and the Lense-Thirring effect is that the de
0° for the epoch 1950 of the Earth's orbital precession and proper motions at the dynamical equinox
Earth's axis completes one full cycle of precession approximately every 26,000 years (25771.4
anomalistic precession as distinct from equinoctial precession), sh
To derive the precession, assume the system is in a rotating Schwarzs
This nodal precession causes that the time for the Sun to return t
a force in the horizontal plane that, due to precession, causes the gyro and its gimbal to rotate ab
pear to come into alignment, and every year, precession causes a slight shift in the Sun's position
Further, precession changes the date of first helical rise: Alth
This apsidal precession completes one rotation in the same time as t
Le Verrier postulated that the excess precession could be explained by the presence of a smal
ere are approximately two such lunar apsidal precession cycles in a Saros cycle.
As at AD2000 precession epoch, the rule would be: "From Polaris, go
is number against the applied frequency, the precession frequency can be determined.
The precession frequency is measured using the Ramsey separ
precess about the magnetic field axis at the precession frequency; after a period of ~100s, another
ad been known to the ancient Greeks, gradual precession had lowered them below the European horizon
yr is the mathematical abstraction of Thomas precession into an operator called Thomas gyration and
Due to precession, Iota Carinae will be the South Star in abou
The total precession is calculated by combining the de Sitter pre
In the case of Earth, this type of precession is also known as the precession of the equin
Larmor precession is important in nuclear magnetic resonance,
Precession is the rotation of a plane (or its associate
This orbital precession is in the opposite sense to the gyroscopic m
ite in a prograde orbit about the Earth, the precession is westward (nodal regression), the node and
This precession is a process purely due to contact forces an
intuitive, but the torque exerted due to the precession is several orders of magnitude greater than
Axial precession is the movement of the rotational axis of an
Starting with some value of the angle, the precession is replaced by libration around 90° or 270°,
eginning now because the secular decrease in precession is beginning to cross a resonance in Earth's
ample he wrote works on comets, Gravitation, Precession, Kinematics and statistics of stars etc.).
A few centuries later, when precession made the orientations obsolete, the temples
ons, a twisted accretion disk, in retrograde precession, modulates the X-rays illuminating HZ Her an
Precession, nutation, polar motion
For precession of orbiting bodies, see de Sitter precession
This phenomenon is called the precession of the equinoxes.
This article is about precession of orbiting bodies.
Secular resonances occur when the precession of two orbits is synchronised (a precession
astronomy, trepidation is oscillation in the precession of the equinoxes.
Due to the precession of the equinoxes, Polaris will not always be
dars attempt to track) is shorter due to the precession of Earth's rotational axis, the two forms of
ished in 1943, clearly showed the perihelion precession of Mercury predicted by the general theory o
tion orbits, the perturbations result in the precession of the argument of pericenter.
Due to precession of the equinoxes, it will become the pole st
ligned with the constellation because of the precession of the equinoxes.
n the parallax of Venus, and he measured the precession of the Earth's rotational axis.
The spin precession of electron in an external electromagnetic f
has published a new table, corrected for the precession of the Earth's orbit, which changes the sign
This discovery of the relativistic precession of the electron spin led to the understandin
irection of the orbital motion (relativistic precession of periastron).
will change after some centuries due to the precession of the equinoxes.
ry year equinoxes slide by 50 seconds due to precession of equinoxes, giving birth to Ayanamsha and
celestial pole is moving away from it due to precession of the equinoxes.
can also be applied to a particular secular precession of astronomical orbits, equivalent to the ro
Because of a phenomenon known as the precession of the equinoxes, the poles trace out circle
m a late (Ptolemaic) age, supposedly records precession of the equinoxes (Tompkins 1971).
Due to precession of the equinoxes, it will be the closest bri
The discovery of the precession of the equinoxes in the west is attributed t
Ptolemy used these observations to confirm precession of the equinoxes, a phenomenon that had been
that demonstrated ancient man understood the precession of equinoxes and solstices.
ears, which corresponds to the period of the precession of the Earth's axis.
shorter than a sidereal year because of the precession of the nodes.
ate of December 21, 2012, is associated with precession of the equinoxes and therefore can provide a
The difference is caused by the precession of the equinoxes, and means that over long p
a 35-day period believed associated with the precession of the accretion disk.
Effects of apsidal precession on the seasons
,000 years, the same as the constants of the precession p of the equinoxes (although not of the prec
(Due to precession R.A. of the stars has been shifted since 395
is the precession rate (rad/s)
A good approximation of the precession rate is
rbation analysis (spacecraft) gives that the precession rate of an orbit around an oblate planet is
The orbital precession rate may be derived using this radial effect
be a fairly simple matter to plot the rough precession rate.
ppears to be stable, as the eccentricity and precession rates are such that it avoids close encounte
named) ancient astrologers believed that the precession, rather than being a steady unending motion,
xed among the stars but due to the lunisolar precession slowly shifting westwards over the ecliptic
lowly over the centuries, due to the Earth's precession, so the directions of these cairn pairs can
tivity, particularly in the area of geodetic precession, the phenomena of precession of a freely fal
Due to Precession, the celestial pole moves in a circle around
Because of this precession, the stars appear to move around the Earth i
as used in former centuries when, because of precession, the star Polaris was much further from the
In precession, the equinoxes appear to move slowly through
n any case, if the ancient Egyptians knew of precession, their knowledge is not recorded in survivin
ly running into what appears to be a funeral precession, they uncover the deadly truth of the town's
left-threaded on the left-hand crank so that precession tightens the pedal rather than loosening it.
uch planet was ever found, and the anomalous precession was eventually explained by general relativi
Similar claims have been made that precession was known in Ancient Egypt prior to the time
nce of ferromagnetic resonance of the Larmor precession, which was independently verified in experim
Precession will be greater than p+ by the small amount
                                                                                                    


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