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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

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