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528 XVII. Origin of turbulence I1<br />
IIICIII, \vitJ~ tncn~~~rctr~r~~l~~.<br />
This (::~n l)c infcrrotl very clearly from the pictures of snch<br />
'l':~.ylor vorl,icc,s ol)t:ainotl I J I?. ~ Schultz-(lrnnow and 11. IIein [204], several of whicll<br />
hnvo I1t:t:n rq~rotlnrcti in I'ig. 17.333. In their cxperimcntal arrangement in which the<br />
pip 11:t.tI I.lw tlimc~~sion or d .= 4 mm, and the inner radius was R, -- 21 mm, the<br />
vcwl.it~r.s :i.pp~:~~:d ;LI> :L ~wril)hcrnl vclority, I/(, which corrcspontls to n lboynoltls<br />
n~~tnlwr R (Ii d/v : .: !)4.5, Fig. 17.33:~. It, is t~ol~cworl,l~y t,h;~I, t,l~t: flnw rctn:iint:tI<br />
lihtni~t:ir :I(, L11t' IIIII(:~ I~igl~t:r ~bt:ynohIs I I I I I I I I ) ~ of ~ ~ R r--- 322 (T, --= 141) a11t1 R -:= 8(i8<br />
(T, =- M7), IGgs. 17.33 IJ, c. 'l'urbulcnt flow did not bccomc tlevelopctl until a Rcynoltls<br />
rli~mlm R -= :l!)fiO (T, = 1715) had bcct~ mncl~ctl, Pig. 17.33tl. It, should I)c sl,rcsscd<br />
rn~pl~n~.ir:~lly LhnL tshc first nppcnmncc of ncutral vortices n.t thc limit of stnl~ility<br />
in nocortlnncc wit,h cqn. (17.20) and thc pcrsistcnce of arnpliIict1 vorticos at higher<br />
Tnylor numl)rrs tlors not in any way imply that thc flow has bccome turbulent. On<br />
t.lw contrary, cvcn if the limit of st,ahility is exceeded by a large margin, the flow<br />
rcmains wt,Il ortlrrcd nntl Inminnr. Turbulent flow does not bccome developed until<br />
'I'nylor, ant1 t.l~rrcfort:, ltryr~oltls numbers vastly cxccctling the limit of st.al)ilit,y<br />
:~rr nl hit~ctl.<br />
.I. '1'. Sh~nrl, 12181 s~tc:c:twlcd in con~puting thc flow pattern of the unstal)lc<br />
Intnin:~r Ilow in l.11~ prcscnrc of Taylor vorticcs nntl with thc non-lincnr terms in<br />
(.llr r(luat.iot~ of' mo(,ion rctninctl. Ilc disrovnretl the sxist,once of equilibrium bctwccn<br />
Kg. 17.34. I'low hot\rsc:cn t.wo conoentxic rylintlrr.q: tor+io cocflicicnt for inner cylinder in t,rrms<br />
of t.hr 'I'nglor nnml)cr, T,,.<br />
f. Stability of a bo~inclary layer in Lho proscnm of tl~rcc-di~ncnniotlrbl tlisl,t~rl~:inws 52!)<br />
the transfcr of energy from the base flow to the sccondnry flow ant1 t.11~ viscous<br />
energy dissipation in t>hc secondary flow. The t,ransfcr of cncrgy fron~ the Onsc<br />
flow t,o thc secondary flow causes a Inrgc incrcnsc in thn torqrtc rcq~~irrd to roht,c<br />
t.l~(! inner cylinder. 7'hc diagram in Fig. 17.34 cotitair~s n compnrison I)ct,wrcn Ihc<br />
t.l~rorrt.icn.lly dcrivctl :inti thr cxpcrirntwt.ally mcns~trrcl v:~l~~rs of 1 h t.orcj~tc, roc*f'L<br />
ricnl, C,,. '1'11t- I:~l.tvr is clcfinwl as<br />
Xi<br />
C, = ------- - . - . . (17.21)<br />
R,~ 1' '<br />
-4- n ~ ( 2<br />
wit,l~ 1~ as tthc l~cight, of I,hc cylintlcr. '1'11~ 1inc:tr l,l~(:or~l wil,l~ SLII:LII rrhtivt: g;111s,<br />
(//I(,, yields<br />
In :tcldit.ion to the? txtrvc wllic:h (:orrt~spot~l~ 10 IJiis lint.:t.r t.lt(!ory, IIII(I wl1i(41 I(-:I.(IH<br />
lo :L Ior(11tc t;ot:l'fit~it:t~l, (,'M . - 047/T,, Sor d/11', O.OW, lht* (li~~pxtn (:o~~t,;~it~:+<br />
t,Iit:<br />
cllrvc provitlc:d 11y .J. '1'. SI,~~nrt,'s ~IOII-lirtwr t1~:or.y as wcll ILS on(: givt:tt l),y ;L I.Iwory<br />
lor turl)ulcnt flow; thc Intber leads to tho formul;~ tlial. Cnr - T,,-".2. 111 all, wt: may<br />
tlisccrn t,hrcc rcgirncs of Ilow, cnch circ:umscril)c:tl I)y 1.h~ 'l':~ylor r~~~rnltc:r in tho<br />
li)llowing way:<br />
T, < 41.3: laminar Coucttc flow,<br />
41.3 < T, < 400 : laminar llow with 'I'nylor vorl,ic:os,<br />
T, > 400 : lurl~tllor~t Ilow.<br />
Agrccmcnt bctwccn theory and cx~wrimrnt is cxecllrnt in thc first I.wo rangost.<br />
An extension of Taylor's thoory can bc found in a study hy Ii. Iiirchgarssner [IOG].<br />
A detailed experimental investigation of Couettc Row, particularly in transition,<br />
was carried out in 1965 by 1) Colcs [291<br />
Ekct of an axinl velocity: The preceding stability calculations have been<br />
extended by 13. Ludwieg [I 32, 1331 to includc the case when the two ryl~ntlct s arc<br />
also axially displaced with respect to each other. Let u(r) denote the tangential<br />
velocity, and let w(r) denotc the axial velocity. If we now introduce the dimensionless<br />
velocity gradients<br />
- r dzl r dw<br />
u=-- and GI=--,<br />
u dr u dr<br />
wc can writc the stability criterion for n non-viscous fl~tid in the form<br />
t l'lic cxperirner~tnl msulkq displnycd in Fig. 17.34 dernonstrntc furtl~or that an increase in the<br />
Taylor number, that is, that an increase in tho lteynolrls number at a constant value of d/.R,,<br />
cansen n trflnnition from cellular to tnrhulcnt flow. Whcn thc flnw is tc~rI)nlcnt (1, > 400),<br />
wo have CM - Td-0.2. and I~cncc, nt constnnt d/Rt al~o CM w ((I, dlv)-o.Z - R (1 2. 'l'lm sarno<br />
~(:RIIIL WIW discov(:red IIY {I. It~it:J~nrtlI, ((201 in Cl~np. XI X) WIICII 110 ~t.ndi(:~I I h I:ILH(: or I~III::~~<br />
Couette flow between flat parallol walls. It is remarkable that ll~c same dependence of the<br />
torqm coefficient on Iteynolds number exists for a disk rotating in a llnid at rcst, eqn. (21 30).