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I<br />
dlroction ●rgla-in lra~ing, the angle<br />
between the mtenna base line and an<br />
hrre@rary line cixmecfing the cenler 01 the base<br />
line with the target .<br />
dlractlon Instrument theodollte-A<br />
tha@oiiie In which the graduated horizontal<br />
C4rcle remains fixed during a 6erfaa of<br />
obaervatbna, the telesco~ being poinlad on a<br />
nurrtiar of signals or objjcfs In succession, and<br />
the cfirectbn of each read on the circle, usual~<br />
by mearra of mlciumeler mlcroecopas. Direction<br />
krstrumenf lhaodoliles are used abrrost<br />
excbaively In first- and eacorxkrrder<br />
Irirmgulafion. Atao called dlrectlon<br />
theodollte; triangulation theodollte.<br />
dlrsctlon method of adjustment—<br />
(trlarrgufstfon and traverse) A melfrod 01<br />
adjustment of observations which determines<br />
Corrections to obsenred directions. The direction<br />
method Is used in the adjustment of first- and<br />
eecxmkrder suwey obsewalions.<br />
dlrecflon method of dotermlnlng<br />
astronomic aslmuth-The determination of<br />
the astronomic azimuth of a line by measuring,<br />
with a dkection theodolite, the horizontal angle”.<br />
between a selecled star and e suitable mark<br />
and applying that ar@e to the azimuth of the<br />
star computed for the epoch 01 the observation.<br />
direction method of meeaurlng<br />
horizontal anQlee—See dlrectlon metfSOd<br />
of obatsrvatlon.<br />
dlrectlon method of obaarvatlon-A<br />
melhod of obsewing angular relationships<br />
wherein fhe graduated circle is hetd in a fixed<br />
position, and the directions of the various<br />
signals are observed around the hortzon. Thus,<br />
directions are poimings whereby angles are<br />
found by the differences in directions. Also<br />
called sflractlon method of maaaurhrg<br />
horizontal anglea.<br />
dlrectlon ot grevlty-See dlrectlon of the<br />
Iorco of gravity.<br />
dlrectlon of relallve movement—The<br />
direction of motion relative to a reference pcint,<br />
Ifeeff uaualfy In motion.<br />
dlrectlon of the force of gravity—Th e<br />
direction indiiated by a plumb line. It is<br />
perpendicular to the surface 01 the geoid. Also<br />
called dlrectlon of gravity.<br />
MIL-HDBK-8S0<br />
73<br />
dlractlon Ot tilt—The direction (azimuth) of<br />
the prtncfpal plane of a phoksgraph. Also, the<br />
direction of Ihe principal line on a photograph.<br />
dlrectlon theodollte-See dlrectlon<br />
Instrument theodollta.<br />
directional radar prediction-(JCS) A<br />
prectktion made for a particular heading.<br />
dlrectlonel reflectance-Reflectance<br />
measured for a specific mode of Irradmtbn and<br />
collecfbn.<br />
dlrectlorr-1. (JCS) A term used by a spotter<br />
Or ObSaWEr In a call tor fire to Indiie the<br />
bearing of the spotting line. 2. The poaftiorr of<br />
one point relative to another without reference<br />
to the dk.lance between them. Direction may be<br />
either twodimensional or three-dimenskwral, the<br />
horizontal being the usual plane 01 the latter.<br />
Direction is usually incketed In terms of Ifs<br />
angular distance tmm a reference diiectlon. See<br />
also gteat-circle direction; grid dlrectlon;<br />
horizontal direction; magnetic direction;<br />
Mercator dlrectlon; reference dlrfrctlon;<br />
reletlve direction; true direction; x.<br />
dlreclion.<br />
discrepancy—A difference betwean results ot<br />
dupliia!e or comparable measures of a quantity.<br />
The difference in computed values of a quantity<br />
obtained by different processes using data from<br />
the same suwey.<br />
diek oparatlng system (DOS)-One of<br />
many operating ayaleme tor computers which<br />
act as an interface between e user end the<br />
computer hardware. DOS was ap.acMcally<br />
designed lor personal comrnstem (PCs).<br />
dlapereton—(oplice) The separetiin 0! tight<br />
Inlo its component cobm by its passage through<br />
a diffraction grating or by refraakm such es that<br />
provided by a prism.<br />
displacement—l. (cartography) The<br />
hortzomal shift of the plotted position of a<br />
topographic feature from Ifs true position,<br />
caused by required adherence to prescribed line<br />
weights and symbol sizes. 2. Any shii in the<br />
position of an image on a photograph which<br />
does not alter the perspective characteristics of<br />
the photograph (I.e., shill due to lilt of the<br />
photograph, scale change in the photograph,<br />
and relief 0! the objects photogrephedj. See<br />
also refraction displacement; relle?