「longitude.」の共起表現一覧(1語右で並び替え)
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Longitude: about 78.533 (78°32'0") W | |
r use the moon's position to determine their | longitude accurately. |
The | Longitude Act was an Act of Parliament of the United K |
ented to Westminster Palace in May 1714, the | Longitude Act was passed in July 1714. |
Only one packet encodes latitude and | longitude, altitude, direction, and speed (full positi |
Current location - current latitude, | longitude, altitude, direction, and speed of the phone |
ricane slowly turned to the north along 83°W | Longitude, and it steadily intensified on October 17. |
the island where they have to determine the | longitude and latitude of the island, create a radio f |
graphic position being 24°51'12”-26°13'52” E | longitude and 43°55'31”-44°49'32” N latitude. |
tion in right ascension, but not in ecliptic | longitude and vice versa. |
s on a sphere given angular positions (e.g., | longitude and latitude). |
section with the Meridian of 57 degrees West | Longitude and the shoreline of the southwest coast, lo |
public lecture, as did Dava Sobel, author of | Longitude, and Sir Arnold Wolfendale, the 14th Astrono |
translational position (typically latitude, | longitude and altitude) over a period of time. |
ublished in his lifetime, but left papers on | longitude and the moons of Jupiter that were published |
irty U-boats, is marked only by latitude and | longitude, and has no name by which it will be remembe |
Princeton's | longitude and latitude coordinates |
Lansing's | longitude and latitude coordinates |
e and North Branches, at approximately 94.1W | longitude, and 44.5N latitude. |
of Venus with the sun, and thus finding its | longitude and latitude, while other stars could at any |
situated at 12'41'30" latitude and 74'58'00" | longitude and 28m elevated from M.S.L. |
West | Longitude and is 16 kilometers across. |
West | Longitude and is 15 kilometers across. |
West | Longitude and is 18 kilometers across. |
West | Longitude and is 17 kilometers across. |
surface, discovered the Moon's libration in | longitude, and published his results in Selenographia, |
West | Longitude, and is 15.4 kilometers across. |
West | Longitude, and is 9 kilometers across. |
West | Longitude, and is ten kilometers across. |
cated at 9.8° south latitude and 193.2° west | longitude and is 85.9 km in diameter. |
W. | longitude, and has an area of 4.4 km2. |
West | Longitude and is approximately 132 kilometres long. |
The website provides the best known | longitude and latitude (sometimes only accurate to wit |
West | Longitude and is approximately 20 kilometers across. |
West | Longitude and is approximately 15 kilometers across. |
West | Longitude and is approximately 201 kilometers long. |
The | longitude and latitude of its center are 311.6° |
Keokuk's | longitude and latitude coordinates in decimal form are |
West | Longitude and is approximately 311 km across. |
he title indicates that specific time, date, | longitude, and latitude. |
ts name indicate, respectively, the galactic | longitude and latitude, and velocity towards Earth in |
It reaches 17″ in | longitude and 9″ in obliquity. |
It established the Board of | Longitude and offered a monetary reward (Longitude Pri |
ands in the south Pacific that they knew the | longitude and latitude. |
located at 63.1° North Latitude, 16.9° West | Longitude and is 34 kilometers across. |
is a transparent circular grid with lines of | longitude and latitude that which can overlay a solar |
e village is situated at 38 º 27 'N, 6 º 00' | longitude and an altitude of 481 m. |
It was positioned at 82ºW | longitude, and operated by Telesat Canada. |
This arctic sea is located at 82° north | longitude and 21° west latitude. |
It will be positioned at 111° West | longitude, and is expected to operate for 15 years. |
The 3D position (latitude, | longitude and elevation) of each theodolite is known. |
in one direction or with similar ecliptical | longitude) and to opposition (both sun and moon observ |
intersection of the Meridian of 57o30' West | Longitude and the southern shoreline |
tion of the drop, indicated by the latitude, | longitude, and Marsden Square. |
orrected so that its pixels are aligned with | longitude and latitude lines, and have a narrowly defi |
yne hired him as a computer for the board of | longitude, and two of his mathematical papers were pre |
located at 57.2° North Latitude, 12.0° West | Longitude and is 35 kilometers across. |
e aircraft's identifier, position (latitude, | longitude, and altitude), date and time, flight level, |
usually reported at intervals of 10 degrees | longitude and are used primarily by airline class airc |
he exact time of midday there (an adjunct of | longitude), and became for a while the arbiter of time |
hin the geographical limit of 78o15'-78o45'E | longitude and 11o44'-12o08'N latitude. |
hroat Island, Frenchman´s Creek, Shaka Zulu, | Longitude, and Wives and Daughters. |
Their appearance and | longitude are irregular due to a lack of synchonizatio |
on, supergalactic latitude and supergalactic | longitude are usually denoted by SGB and SGL, respecti |
int must be defined from which the angles of | longitude are measured. |
Their appearance and | longitude are irregular due to a lack of synchonizatio |
s from the intersection of this latitude and | longitude are protected under the provisions of Histor |
e 1m-class optical telescopes distributed in | longitude around the southern hemisphere in order to p |
the highest mean annual temperature at each | longitude around the globe. |
for the Moon to return to the same ecliptic | longitude as the Sun: the synodic month. |
The Board of | Longitude asked Kendall to copy and develop John Harri |
of a series of experiments used to determine | longitude at sea. |
West | Longitude, at the base of the continental slope of Nor |
Branchville has a latitude at 31.15 and a | longitude at -84.315. |
way of enabling mariners to determine their | longitude at sea. |
onometer for precise clocks designed to find | longitude at sea. |
es corresponding to 30 degrees difference in | longitude, at different latitudes |
els a sun-synchronous orbit, passing a given | longitude at 10:30 AM local time. |
This brought the problem of measuring | longitude at sea into sharp focus once more. |
allowed navigators to successfully calculate | longitude at sea. |
solutions were proposed for how to determine | longitude at the end of an exploratory sea voyage and |
e wide range of estimates of the distance in | longitude between Toledo and Rome. |
new land at 62° south lattitude and 60° west | longitude, but did not land on it. |
Longitude, but no Richter Scale magnitude can be asses | |
r ring, the other on a method of determining | longitude by means of lunar eclipses. |
The Method of Finding the | Longitude by Timekeepers (1794) |
atellites and on the mode of determining the | longitude by these means (1810) |
inclination and the ascending node, the true | longitude can tell us the precise direction from the c |
alk rate - the rate at which the areocentric | longitude changed with each orbit, and the periapsis w |
ies and districts for which the latitude and | longitude coordinates are included below, may be seen |
Latitude and | longitude coordinates are provided for many National R |
ies and districts for which the latitude and | longitude coordinates are included below, may be seen |
Register district for which the latitude and | longitude coordinates are included below, may be seen |
ies and districts for which the latitude and | longitude coordinates are included below, may be seen |
gister properties for which the latitude and | longitude coordinates are included below, may be seen |
ies and districts for which the latitude and | longitude coordinates are included below, may be seen |
Latitude and | longitude coordinates are provided for many National R |
above sea level and is located at latitude - | longitude coordinates of N 36.829028 |
ies and districts for which the latitude and | longitude coordinates are included below may be seen i |
Turtle Mound is located at the latitude and | longitude coordinates of N 28.93082 and W -80.827 |
l properties and districts with latitude and | longitude coordinates in the table below. |
ricts (at least for all showing latitude and | longitude coordinates below) may be seen in a Google m |
imal place of one second of the latitude and | longitude coordinates). |
The latitude | longitude cordinates for Christopher Nagar is 8°11'14" |
nd RootsMagic are supported for latitude and | longitude data. |
A | longitude describes the location of a place on Earth e |
o obtain a location could input latitude and | longitude details to see how far away other online use |
t this would eventually solve the problem of | longitude determination for ocean navigators. |
ne chronometer, thereby allowing for precise | longitude determination while at sea. |
He believed he could improve the accuracy of | longitude determination, particularly at sea, by obser |
he meridian of Jerusalem, corresponding to a | longitude difference of 8°55'. |
rt to redetermine with greater precision the | longitude difference between London and Paris. |
etween England and France - this would allow | longitude differences to be measured very accurately, |
le can be expressed in terms of latitude and | longitude differences dlat,dlong, using only cosines, |
ed at the crossing of Latitude N 23 -50` and | Longitude E 91-17`, covering 3 km² during that period. |
this region is divided into 12 signs of 30° | longitude each. |
Supports GEDCOM 5.5.1 draft's Latitude and | Longitude extensions. |
Character pairs encode | longitude first, and then latitude. |
stward to its intersection with the 21° east | longitude, follows this degree of longitude northward |
d Arnold were granted awards by the Board of | Longitude for their improvements to chronometers; Earn |
ension and declination are like latitude and | longitude for astronomy). |
had been working on the problem of measuring | longitude for a long time. |
Mary Croarken (2002), "Providing | Longitude for All", Journal of Maritime Research (Nati |
useful at sea; particularly for deducing the | longitude from lunar distance, and the latitude from t |
in latitude from 41° 20' to 42° 40' N and in | longitude from 109° 50' to 111° 25' E. |
e 9-1-1 center is provided with latitude and | longitude from the radio's GPS receiver. |
s in latitude from 27° 50'-29° 16' N, and in | longitude from 103° 36'-105° 20' E, stretching 153 kil |
teroids and comets and on the measurement of | longitude, improving the accuracy of the Connaissance |
ed its orbit to within 2 arcminutes error in | longitude in his geoheliocentric model when Kepler had |
located at 6° north latitude and 355.5° west | longitude in the Oxia Palus quadrangle. |
To determine | longitude in navigation, Werner proposed determining t |
ts designated orbital slot is 74 degree East | longitude in the Geostationary Orbit. |
e observatory was moved closer to the 82.5°E | longitude in Mirzapur in Uttar Pradesh. |
The satellite was positioned at 4° W | longitude in the geo-stationary orbit. |
It became operational at 74° West | longitude in the geostationary orbit and replaced SBS- |
Longitude incorrectly marked as East rather than West. | |
The | longitude is -97.2W. |
The | longitude is -80.375W. |
In this case, the | longitude is also called the right ascension of the as |
The | longitude is -93.855W). |
The | longitude is -80.976W. |
The | longitude is -81.076W. |
The | longitude is -88.13W. |
The | longitude is -89.49W. |
The | longitude is -73.945W. |
latitude of this place is 29°40'33"N and the | longitude is 80°16'20"E. |
The zero point for supergalactic | longitude is defined by the intersection of this plane |
Its latitude of is 26.784N and its | longitude is -80.037W. |
In astrodynamics true | longitude is the longitude at which an orbiting body c |
Greenough's latitude is at 31.317 and its | longitude is at -84.102. |
Its latitude is 41.2833/41º16'60 N and its | longitude is 1.36667/01º22'0 E. The population in 2003 |
Flint's latitude is at 31.317 and its | longitude is at -84.179. |
latitude of Creighton is 40.587N, while the | longitude is -79.778W. |
Thus, the area between two meridians of | longitude is a lune. |
The latitude of Breed is 45.073N and the | longitude is -88.424W. |
The | longitude is-89.656W. |
of Mars at 48.6° south latitude and 26° west | longitude, It is 129 km in diameter and was named afte |
ree southern latitude and 76 degrees western | longitude, just between the Martian equator and the Va |
oper River was on the corner of East Bay and | Longitude Lane. |
the region along the later-proposed 70º east | longitude line was proposed by the Empire of Japan in |
d border and from east of the 78 degree west | longitude line to just west of Chambersburg, PA. |
cause it lies as far as 30° east of the 180° | longitude line), and thus the first part of the planet |
y Mouse-shaped globe containing latitude and | longitude lines, with the property's name presented in |
e, the stars shift eastwards (increase their | longitude) measured with respect to the equinoxes - in |
ing one degree of latitude and one degree of | longitude, named according to their south western corn |
es were 3°34' north latitude and 56°30' east | longitude, near the edge of the Mare Fecunditatis ("Se |
conjunctions in right ascension and ecliptic | longitude need not to take place on the same date. |
day when the Sun is exactly at the celestial | longitude of 120°. |
day when the Sun is exactly at the celestial | longitude of 240°. |
feet) at a latitude of 7.65°N (7°39'0"N) and | longitude of 124.45°E (124°27'0"E). |
e unexplained fluctuation in the Moon's mean | longitude of the order of 10 arcseconds. |
ard Time Zone at a latitude of 36.248N and a | longitude of -82.545W. |
me at Greenwich by a difference equal to the | longitude of the fictitious mean Sun used for defining |
and | Longitude of 089º56.456. |
day when the Sun is exactly at the celestial | longitude of 195°. |
ts was the determination of the latitude and | longitude of Washington, D.C. in 1846. |
day when the Sun is exactly at the celestial | longitude of 285°. |
day when the Sun is exactly at the celestial | longitude of 30°. |
pradesh with latitude of 28 degree north and | longitude of 95 degree east. |
semi-major axis, eccentricity, inclination, | longitude of periastron, time of periastron, maximum t |
is | longitude of orbit's periapsis, |
day when the Sun is exactly at the celestial | longitude of 150°. |
en DnaG and DnaB is necessary to control the | longitude of Okazaki fragments on the lagging strand. |
fined by two parameters, Inclination (i) and | Longitude of the ascending node (Ω). |
of not implying knowledge of the historical | longitude of continents, which is difficult to determi |
day when the Sun is exactly at the celestial | longitude of 180°. |
eostationary orbit, and will be located at a | longitude of 61.5° West, from where it is intended to |
Bombay, and Canton; as also the Latitude and | Longitude of Point de Galle and the Friar's Hood." |
longitude of the perihelion: 159.079 degree | |
ged in the determination of the latitude and | longitude of prominent capes, bays, etc., and of the m |
longitude of ascending node: 218.993 degree | |
longitude of the ascending node: 41.07311 deg | |
stars, so as to find out the so-much desired | longitude of places for the perfecting the art of navi |
ane of reference are the inclination and the | longitude of the ascending node. |
1 was positioned in geostationary orbit at a | longitude of 104° West for testing and on-orbit storag |
Longitude of the ascending node: 92.24656 degree (equi | |
It will be positioned at a | longitude of 1° West. |
It has a Latitude of 42° 57' 0 North,a | Longitude of 4° 5' 60 West, and an Altitude of 3481 fe |
It begins when the Sun reaches the celestial | longitude of 45° and ends when it reaches the longitud |
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