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I<br />

I<br />

I<br />

I<br />

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

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