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PREDICTION OF TRANSPIRED TURBULENT BOUNDARY LAYERS.PLETCHER RH.1974; J. HEAT TRANSFER; U.S.A.; DA. 1974; VOL. 96; NO 1; PP. 89-94; BIBL. 20 REF.Article

THE EFFECTS OF DIFFERENCES IN COMPOSITION, EQUATION OF STATE, AND MIXING LENGTH UPON THE STRUCTURE OF WHITE-DWARF CONVECTION ZONES.FONTAINE G; VAN HORN HM; BOHM KH et al.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 193; NO 1 PART. 1; PP. 205-211; BIBL. 22 REF.Article

A VARIABLE MIXING-LENGTH RATIO FOR CONVECTION THEORYCHAN KL; WOLFF CL; SOFIA S et al.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 244; NO 2; PART. 1; PP. 582-586; BIBL. 22 REF.Article

MODELS OF THE SOLAR CONVECTIVE ZONE. THE INFLUENCE OF FREE PARAMETERS IN MIXING LENGHT THEORIES.STAUDE J.1976; BULL. ASTR. INST. CZECHOSL.; CZECHOSL.; DA. 1976; VOL. 27; NO 6; PP. 365-374; ABS. RUSSE; BIBL. 31 REF.Article

SUR LES ECHELLES LINEAIRES DE LA TURBULENCE DANS LA THEORIE SEMI EMPIRIQUEAKATNOV NI.1974; IZVEST. AKAD. NAUK S.S.S.R., MEKH. ZHIDKOSTI GAZA; S.S.S.R.; DA. 1974; NO 3; PP. 53-57; BIBL. 19 REF.Article

THE PATTERN OF CONVECTION IN THE SUN.WEISS NO.1976; INTERNATION. ASTR. UN., SYMP.; NETHERL.; DA. 1976; NO 71; PP. 229-242; BIBL. 1 P. 1/2; (BASIC MECH. SOL. ACT. SYMP.; PRAGUE, CZECHOSL.; 1975)Conference Paper

ZONES CONVECTIVES ET EPUISEMENT DU LITHIUM DANS LES ETOILES DU TYPE SOLAIREEHRGMA EH; PAMYATNYKH AA.1971; ASTR. SOVET AKAD. NAUK S.S.S.R., NAUCH. INFORM.; S.S.S.R.; DA. 1971; NO 20; PP. 71-85; ABS. ANGL.; BIBL. 1P.Serial Issue

ANOTHER FUNDAMENTAL, BUT CORRECTABLE, INCONSISTENCY OF THE LOCAL MIXING-LENGHT THEORYDEUPREE RG.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 234; NO 1 PART. 1; PP. 228-231; BIBL. 16 REF.Article

THE INFLUENCE OF THE OPACITY VALUES AND MINING LENGTH ON THE EVOLUTION OF POPULATION II MAIN SEQUENCE STARS.STABELL R.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 44; NO 2; PP. 315-319; BIBL. 12 REF.Article

CHEMICAL COMPOSITION AND AGE OF ALPHA CEN SYSTEM AND MIXING LENGTH.SAIO H; SHIBATA Y.1974; SCI. REP. TOHOKU UNIV., 1; JAP.; DA. 1974; VOL. 57; NO 3; PP. 87-96; BIBL. 20 REF.Article

THE ROLE OF TURBULENT PRESSURE IN MIXING LONGTH CONVECTION.STELLINGWERF RF.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 206; NO 2 PART. 1; PP. 543-547; BIBL. 10 REF.Article

EDDY VISCOSITY AND ENTRAINMENT IN EQUILIBRIUM BOUNDARY LAYERS.HEAD MR; MCDGALBRAITH RA.1975; AERONAUT. QUART.; G.B.; DA. 1975; VOL. 26; NO 4; PP. 229-242; BIBL. 1 P.Article

MIXING LENGTH IN LOW REYNOLDS NUMBER COMPRESSIBLE TURBULENT BOUNDARY LAYERS.BUSHNELL DM; CARY AM JR; HOULLEY BB et al.1975; A.I.A.A. J., NEW YORK; U.S.A.; DA. 1975; VOL. 13; NO 8; PP. 1119-1121; BIBL. 23 REF.Article

FORMULA FOR THE MIXING LENGTH IN THE PLANETARY BOUNDARY LAYER.DJOLOV G; SYRAKOV E.1975; KHIDROL. I METEOROL.; BALG.; DA. 1975; VOL. 24; NO 6; PP. 7-14; ABS. RUSSE; BIBL. 10 REF.Article

INFLUENCE OF THE NOZZLE DIAMETRE ON THE HYDRODYNAMIC STRUCTURE OF TURBULENT FREE JETS.MADEJSKI J.1976; BULL. ACAD. POLON. SCI., SCI. TECH.; POLOGNE; DA. 1976; VOL. 24; NO 1; PP. 71-80; ABS. RUSSE; BIBL. 2 REF.Article

ABOUT THE PROPER CHOICE OF THE CHARACTERISTIC LENGTH IN THE CONVECTION THEORY.BOEHM VITENSE E; NELSON GD.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 210; NO 3 PART. 1; PP. 741-749; BIBL. 13 REF.Article

SULLA SCELTA DELLA LUNGHEZZA DI MISCELAMENTO CON RIFERIMENTO AL FATTORE DI ATTRITO. = CHOIX DE LA LONGUEUR DE MELANGE AVEC REFERENCE AU COEFFICIENT DE FROTTEMENTBARSANTI G; FAGGIANI S.1974; TERMOTECNICA; ITAL.; DA. 1974; VOL. 28; NO 8; PP. 427-432; ABS. ANGL.; BIBL. 9 REF.Article

ASYMPTOTIC ANALYSIS OF TURBULENT CHANNEL FLOW FOR MIXING LENGTH THEORY.BUSH WB; FENDELL FE.1974; S.I.A.M. J. APPL. MATH.; U.S.A.; DA. 1974; VOL. 26; NO 2; PP. 413-427; BIBL. 12 REF.Article

AN INSTABILITY DUE TO THE LOCAL MIXING-LENGTH APPROXIMATION.KRUSKAL M; SCHWARZCHILD M; HAERM R et al.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 214; NO 2 PART. 1; PP. 498-501; BIBL. 2 REF.Article

STABILITY OF MEAN TURBULENT FLOWS.AHMADI G.1975; PHYS. OF FLUIDS; U.S.A.; DA. 1975; VOL. 18; NO 11; PP. 1582-1583; BIBL. 6 REF.Article

TURBULENT SEDIMENT TRANSPORT USING MOMENTUM BALANCE, THE STRONG TURBULENCE APPROXIMATION.DREW DA; KOGELMAN S.1975; APPL. SCI. RES.; NETHERL.; DA. 1975; VOL. 30; NO 4; PP. 279-290; BIBL. 4 REF.Article

ON SHALLOW CONVECTIVE ENVELOPESDEUPREE RG.1975; ASTROPHYS. J.; USA; DA. 1975; VOL. 201; NO 1 PART. 1; PP. 183-189; BIBL. 27 REF.Article

POSSIBLE ORIGIN OF PRANDTL'S MIXING-BENGTH THEORY.BRADSHAW P.1974; NATURE; G.B.; DA. 1974; VOL. 249; NO 5453; PP. 135-136; BIBL. 7 REF.Article

MIXING LENGTH IN LOW REYNOLDS NUMBER TURBULENT BOUNDARY LAYERSINMAN PN; BRADSHAW P.1981; AIAA J.; ISSN 0001-1452; USA; DA. 1981; VOL. 19; NO 5; PP. 653-655; BIBL. 13 REF.Article

SOLAR MODELS, HELIUM CONTENT AND MIXING LENGTHMAZZITELLI I.1979; ASTR. AND ASTROPHYS.; DEU; DA. 1979; VOL. 79; NO 1-2; PP. 251-253; BIBL. 16 REF.Article

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