1 - NGA
1 - NGA
1 - NGA
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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.