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dleplacsrment; Illt displacement; xdlsplacement;<br />

y-displacement.<br />

display—The graphic presentation of the<br />

output data 01 any device on system.<br />

dlmolve-(digifal) The process of removing<br />

shared common attributes by eliminating the<br />

shard boumtarias when merging two or mora<br />

polygons.<br />

dletanca sangle-An angle In a ttiangle<br />

ofWOstie a side used as a basa in the solution<br />

01 the Mangle, or a side whose length is to be<br />

computed.<br />

dltstenco measuring ●quipment (DME)-<br />

See electronic distance measuring<br />

equipment.<br />

dkstance prorate rule-A method of<br />

bel.ancing a survey. A rule for holding angles to<br />

their racorded values and pforatlng the lengths<br />

of the lines In the traverse; oparaled by locating<br />

the beartngs to a wnvanlenl meridian,<br />

preferably the cbsing fine of the traverse, and<br />

prorating the dimensions through a<br />

trigonometric precess.<br />

distance-lhe spalial separation of two<br />

poims, measured by the length of a line joining<br />

them. Sea also ●ngular dlatanm; double<br />

merldlan d18tance; double zenith<br />

dlstanca; ecllptlc polar dlatence;<br />

electrical distance; external dletstnce;<br />

felllng; front focal distance; great-circle<br />

distance; grid length; ground distance;<br />

hyperfocal distance; Interocular<br />

dlatance; lunar dietance; merldlan<br />

distance: marldlonal distance; plus<br />

dletance; potar dlatance; prhtclpal<br />

dletance; projection dlatance; relatlve<br />

distance; rhumb Ilne distance; slant<br />

range; Sun-zenith distance: tangent<br />

dletence; time dletance; zenith<br />

dlatance.<br />

dlatant polnte-Similar to tie poinls but which<br />

appaar only on the obllques lacing outward on<br />

the perimeter of a mmpilation. Distant points<br />

unfte the sets of a sfrlp Into a flight unit; bul,<br />

unlike tie poima, do not serve to join several<br />

flight strips together.<br />

dletortlon compenaatlon—<br />

(photogrammstry) In a double projection direct<br />

viewing pbffer sysfem, that corracflon applied to<br />

offset the effect of radial distortion introduced in<br />

MIL-HDBK-850<br />

74<br />

an original negative by the objective tens of an<br />

aerial camera.<br />

diatortlon curve-A curve represeming the<br />

finaar distoflion charactarbtka of a tens; ii is<br />

plotted with image radial dislance from the lens<br />

axie es abscissae and Image radial<br />

dbplacements as ordinatas.<br />

dlatortlon-Lens aberrations affecting the<br />

posltbne of Images from their true relative<br />

poaitiirrs. See also aberration, detinftiorr 2;<br />

angular dlstortlon, definl!ion 2; dllferentlal<br />

distortion; flim dlaforllon; Image<br />

dlstortlon; Image motion Compenaetlon<br />

dlatortlon; lane dletortlon; linear<br />

dlstorflon; panorsmlc dlsitortlon; radial<br />

dlatortlon; seen poeltlonel dlstonlon:<br />

tangantlal dlatotllon; tfpped panoramic<br />

dtatortlon.<br />

distributed data baaa-A data basa with<br />

unique mmponents in geographically dispersed<br />

locations finked through a telemmmunications<br />

netwok<br />

dlstrlbutlon map-A map which shows the<br />

geographic arrangement of a specific product,<br />

commodity, or formation.<br />

dleturblng tunctlon—Sse dlaturblng<br />

poientlal, definition 2.<br />

Uiaturblng potential—l. (geodesy) The<br />

difference betwean the gravity potarrtial of the<br />

actual Earth and the potential function of tha<br />

normal gravity. Also called potantlaf<br />

dleturbance; potential of disturbing<br />

maaaes; potantlal 01 random maaeaa. 2.<br />

(astronomy) The diffarerrca bafwaen the total<br />

gravitational potential and the pofemial<br />

petlaining to a spherbel mass dbfr~}on. Abo<br />

called disturbing function,<br />

diurnal aberration-Aberration reaufring horn<br />

the rotation of me Earth on Rs asis. The value of<br />

diurnal SberfafiOn varies with the latitude Of the<br />

observer and ranges trom zem at the poles to<br />

0.32 second of arc al the Equator. A correction<br />

tor dlumal aberration Is applied to astronomic<br />

ObSeNatlOflS for longitude and azimuth. Also<br />

called daily aberration.<br />

diurnal age—Sae aga ot diurnal<br />

Irrequaflly.<br />

dfurnaf arc—See aetronomlc arc.

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