「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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