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I<br />
radm range atatiina. Also called redlo facility<br />
chart.<br />
en:lty node-A primitive used to represent<br />
featurea thal are truly zam dimenabnal. Entity<br />
nodes are Iopobgically linked 10 their containing<br />
face when tecee are praeam.<br />
OnIffy point-Pointe used to represent<br />
teeturee that are zem-ctimeneional (such ae<br />
survey points). Enliy poims may be<br />
topobgicaliy finked 10 a containing face.<br />
.trtlty Set-An attribute table or group of<br />
attributes.<br />
entrance pupil—The image of the aperture<br />
atop formed by all the lens elements on the<br />
object aIda of the aperture stop,<br />
entrance ellt-slit through which energy<br />
emera a spactroec4plc Inswument.<br />
entrance window—The image of me tield<br />
stop formed by all the Iena elements on the<br />
object side of the fietd atop.<br />
Ebtv6s correcrlon-Component of .uncorrected<br />
observed gravity obtained on a<br />
rrwving ptatform thal is attributed to Ihe easlwest<br />
comporram of the velocity that either<br />
increases or decreasee ihe effect of the<br />
centrifugal force caused by the Earth’s rotation,<br />
The formula for the correction usually includes<br />
the term for the secondary vebcity correction,<br />
E6tv6s effect—A vertical torte experienced<br />
by a t=zdy movin~ in an east-west direction on<br />
the rotating Eafth. In gravity measurements, a<br />
posfriie correcfiin is apptied if moving eastward,<br />
and a negatfve correction if moving westward.<br />
E6tv6a unft—The unit of gravitational gradient<br />
10-9 meters par second per second per meter.<br />
ephemerle time-The uniform meaaure of<br />
time defined by the laws of dynamics and<br />
determined in principal fmm the orbital motions<br />
Of the planete, specifically in the orbital motion<br />
of the Earth aa represented by Newcomb’s<br />
Tables of tha Sun.- Ephemaris fima for close-<br />
Earth Salelliles, or more cmrectty the llme<br />
associated wfih satellite ephemerides, Is<br />
observation dependem. For example, It the<br />
observaflona were made In universal lime (UTJ,<br />
the ephemetis time is UT; ff the obsewations<br />
were made in imemafional atomic time (IAT),<br />
MIL-HDBK-850<br />
84<br />
the ephemeris time is in IAT.<br />
ephamerla—(JCS) A publication giving the<br />
computed places of lha celestial bodies lor each<br />
day of the year, or tor olher regutar intervata. [A<br />
publication giving similar krformettin in a iomr<br />
suitable for use by a nevlgator la catted an<br />
almanac. An ephemeris la also a statement,<br />
not necessarily In a pubtiiation, presenting a<br />
correlation of time ard position of caleslial<br />
bodies or man-made satellites. A short<br />
ephemeris of future focation/time of salelfite is<br />
known as a set of alerts.] See also<br />
broadcast ephemarle; precise<br />
ephemerle.<br />
eplpolar plane-( photogrammetry) Any plane<br />
which mntakrs fhe eplpoles, therefore, any<br />
plane comaining the air base. Also called basal<br />
plene.<br />
eplpolar ray —’The tine on the plane 01 a<br />
photograph joining the epipole and the image of<br />
an object. Also expressed as the trace of an<br />
epipolar plane on a photograph.<br />
epfpolee—in tha perspective setup of Iwo<br />
prolographs (IWO perspective projections), I he<br />
points cm the planes o: the photographs whara<br />
they ara cut by the air base (astended line<br />
joining the IWO perspective centers). In the case<br />
of a pair of truly verlical photographs, the<br />
epipoles ara intiniiety distant from the principal<br />
points,<br />
epoch—1. A particular instant for which cerlain<br />
data are given. 2. A given period of time during<br />
which a series of related acts or events takes<br />
place. 3. An arbitrary moment in time to whjch<br />
measurements of position for a body or<br />
orientation for an orbit are referred.<br />
Equel &c Second Baeter Qhart/Map<br />
[ARC)-A rectangular coordinate and<br />
projection system at any scale for the<br />
entire elfipsoid based on the World Geodetic<br />
System 1984 (WGSG4). The ARC syslem<br />
divides the eltipaoid surface into 18 overtapping<br />
latitudinal band acafed zones.<br />
equal energy—Spectral distribution<br />
characterized by equal ftux per untt wavelength<br />
imervai.<br />
equal-altltude obaervatlona of the<br />
Sun—Azimuth Observalbns that consial of<br />
measuring horizontal angles from a southerly<br />
reference ooinf to the Sun’s timbs at an identiial