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I<br />
I<br />
I<br />
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fii) between fwem- ofa aurwy.<br />
tnm nwridlan-A kvm used !0 distinguish the<br />
gmst circle through fhs gsogmphbaf @se trom<br />
MsPtk Metiin, oompsss nreridii, or grid<br />
meridian.<br />
tN@ nori.h-(JCS) The direcibn fnwn sn<br />
observer’s @fiin to the geognrphii North<br />
Pole. Ths north dimdon d any @oun@c<br />
meridiin. ~ term was origiity ep@ied to<br />
aatronomlc narth to daingubfr it frmm<br />
magnetic north.]<br />
true placa-S ee two position.<br />
~No poaftfon-lhe poaifian of a eels.stiaf bdy<br />
sfrer all krmwn mrrect”mns including precoasion<br />
and ntrtefien have bsan rneda. Atso @Jed true<br />
place.<br />
~NO prfmo vertbakl%e vertical circhr<br />
through ths true asat and w- points at the<br />
horizon, es disfinguiahad from magnetic or gfi<br />
prime verficsl through the magnetic or grid esst<br />
end west points, respedhty.<br />
truo sidereal tlms-See ●pparent<br />
●Idoroal tima.<br />
true solar time-See ●pparent solar<br />
tlms.<br />
true sun-See apparent sun.<br />
true vahIe-Thst value of quantii whwh is<br />
=K@Et* f- ftOM arrera. Since lhe errors to<br />
whiih physical measurements are sbjwf<br />
cennof be knewn exscffy, it fotlows thst the true<br />
vafue of a qusntity mvmaf be known with<br />
mactness. In survey ti, ths most probable<br />
vafue ts used es best representing the true<br />
velue of the quantity.<br />
true-to. scale-A cendtiien where map<br />
tW.9sUr~~ts em in exad agreemenf wilh the<br />
afaled msp scale. Stnm atl map projadii<br />
invoke ecxns scale chsnge, the scale b rmt true<br />
at ell @aces on a’ msp.<br />
true-l. Ffefsted to true north as opposed to<br />
ms9~t~ north. 2. Actual, as contrsstad ~h<br />
Wiimua, as true Sun. 3. Related to a freed<br />
point, eitfww on the Emth or in spaca. ss trua<br />
wind; in cOntmSl wilh relat’we, Wlch & retsl~ to<br />
a moving point. 4. Corrected, as true effitude,<br />
S. One of two alternsta velues (TrueJFalse)<br />
MIL-HDBK-850<br />
269<br />
used in 6odeen bgii.<br />
turning point (TP~ poiti on vhii beth a<br />
minus sighl (icmsighf) ad a pfus Sigfd<br />
~) are taken on a &ne 0( dwOd bveta.<br />
Abe, in tcfqmphii Surveys, any point m Whldl<br />
fhelodie heldwhiletfre” ImtNmmtb movedto<br />
emthar 6idon. Thaee turing pohfe are often<br />
msrkedfor futlxaues aetieorcfreok points.<br />
turning point pin-A deal pin about one foot<br />
brig. In Ievefing Operstbrs, the tumhg polnf Is<br />
driwen info the ground where it is neceaaery to<br />
eababfkhapointthetw iUb asiaMe in elevation<br />
fsrasfrod perfodoftlme. Whenkfusaervedtfs<br />
Usefulness at one pokd. if is nanoved and<br />
canied by the rcdrrrm for subaequad reuse.<br />
turret grmrer-A acriing instrument wlrfch<br />
permits the use of points of several weights<br />
intsrchsngeebfy without the inoonvenlence of<br />
intenupfing the acriing 10 rt@ece pdnts. The<br />
turret head ia revolved to position tb cfeafmd<br />
poht, and a.cribhg is resumed.<br />
tumhe-An ink for dmftirrg printing amss on<br />
Iithagraphiipfates.<br />
tuschhrg-llw operst”wn of adding wefk to the<br />
image on o prsas plate, mrrecting Iinaa and<br />
Ietfetfng, and addii aotids by means 01 tuschs.<br />
Also cslled lithographic dmttlng.<br />
two-base mathod-A t=hnlque of<br />
bsmmetrb fevating ufifiing ffrrw berornefera.<br />
TW bsromatera, one high ssfabtii over a<br />
known elavatbn, and me bw estebJbhsd wet<br />
a known elevation, and a roving bemmetw<br />
operating betwaen the two fmown poslficms.<br />
High end low barometers are reed and<br />
recorded, hith tempemture, evety fwe minutes.<br />
The roving barometer and terrperafum ere reed<br />
and recorded at each ststion omupbed. Osta are<br />
reduced to position end elevstion by offlx<br />
~mP@f~n. The only bsmrnatrb leveling<br />
methad sble to consistently pmdum emxs fees<br />
Ihsn *1 meter. See afso fly-by-method;<br />
Ioapfrog method.<br />
twebody orbit-llre nrotien of e point msas<br />
in the prssence of the gravitational attraction, of<br />
another point ~, and in lhe absence of any<br />
other forces. Thii wbii is usualfy an eftipse, but<br />
msy be a psrsbola or hyperbola,<br />
two-body problenr-That problem in celastial<br />
mechanics which tr,sats of the relative motion or<br />
of two-peint msssss under their mutusl