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LINE FORMATION IN A JOVIAN ATMOSPHEREHUNT GE.sdIN: CONF. ATMOS. RADIAT. PREPR. FORT COLLINS, COLO, 1972,; BOSTON; AM. METEOROL. SOC.; DA. S.D.; PP. 45-46; BIBL. 15REF.Conference Paper

NON-ISOTROPIC REDISTRIBUTION EFFECTS ON SPECTRAL LINE FORMATION.VARDAVAS JM.1976; J. QUANT. SPECTROSC. RAD. TRANSFER; G.B.; DA. 1976; VOL. 16; NO 1; PP. 1-13; BIBL. 18 REF.Article

THEORETICAL QUASAR EMISSION LINE RATIOS. I: TRANSFER AND ESCAPE OF RADIATIONCANFIELD RC; PUETTER RC.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 243; NO 2; PART. 1; PP. 381-389; BIBL. 39 REF.Article

LA PROFONDEUR DE FORMATION DES RAIES DE LA MOLECULE CN DANS L'ATMOSPHERE DU SOLEILPORFIR'EVA GA.1975; ASTR. ZH.; S.S.S.R.; DA. 1975; VOL. 52; NO 3; PP. 593-598; BIBL. 21 REF.Article

L'INFLUENCE DES PARAMETRES ATOMIQUES SUR LA PROFONDEUR DE FORMATION DES RAIES DE FRAUNHOFER FAIBLESGURTOVENKO EH A; RATNIKOVA VA.1974; ASTR. ZH.; S.S.S.R.; DA. 1974; VOL. 51; NO 5; PP. 1032-1035; ABS. ANGL.; BIBL. 3 REF.Article

SOLUTIONS TO RADIATIVE TRANSFER PROBLEMS USING APPROXIMATE LAMBDA OPERATORSSCHARMER GB.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 249; NO 2; PART. 1; PP. 720-730; BIBL. 17 REF.Article

LINE FORMATION IN TURBULENT MEDIA: COMPARISON BETWEEN CONTINUOUS AND DISCONTINUOUS VELOCITY FIELDS.GAIL HP; SEDLMAYR E; TRAVING G et al.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 46; NO 3; PP. 441-445; BIBL. 8 REF.Article

EFFECTS OF TURBULENT VELOCITIES ON NASER LINES.GAIL HP; KEGEL WH; SEDLMAYR E et al.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 42; NO 1; PP. 81-84; BIBL. 8 REF.Article

HEIGHTS OF FORMATION OF NON-MAGNETIC SOLAR LINES SUITABLE FOR VELOCITY STUDIES.ALTROCK RC; NOVEMBER LJ; SIMON GW et al.1975; SOLAR PHYS.; NETHERL.; DA. 1975; VOL. 43; NO 1; PP. 33-37; BIBL. 13 REF.Article

ON SPATIAL VARIATIONS IN THE INTENSITY OF CHROMOSPHERIC HALPHA .GEBBIE KB; STEINITZ R.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 188; NO 2 PART. 1; PP. 399-406; H.T. 5; BIBL. 30 REF.Article

EVALUATION DE LA HAUTEUR DE FORMATION DES RAIES D'EMISSION H ET K CAII DANS LES OMBRES DES TACHES SOLAIRESTEPLITSKAYA RB; EHFENDIEVA SA.1974; SOLNECH. DANNYE, BJULL.; S.S.S.R.; DA. 1974; NO 11; PP. 66-71; ABS. ANGL.; BIBL. 11 REF.Article

QUANTUM THEORY OF LINE FORMATION IN A MAGNETIC FIELDLANDI DEGL'INNOCENTI E; LANDI DEGLI'INNOCENTI M.1972; SOLAR PHYS.; NETHERL.; DA. 1972; VOL. 27; NO 2; PP. 319-329; BIBL. 14REF.Serial Issue

THE FORMATION OF MGI 4571 A IN THE SOLAR ATMOSPHERE. I. A MODEL ANALYSIS OF A ONE-DIMENSIONAL STATIC ATMOSPHEREALTROCK RC; CANNON CJ.1972; SOLAR PHYS.; NETHERL.; DA. 1972; VOL. 26; NO 1; PP. 21-29; BIBL. 15 REF.Serial Issue

TRANSFER OF RESONANCE-LINE RADIATION IN DIFFERENTIALLY EXPANDING ATMOSPHERES. I. GENERAL CONSIDERATIONS AND MONTE CARLO CALCULATIONSCAROFF LJ; NOERDLINGER PD; SCARGLE JD et al.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 176; NO 2, PART 1; PP. 439-461; BIBL. 30REF.Serial Issue

ELECTRON SCATTERING BY HOT GAS IN QSOS.SHIELDS GA; MCKEE CF.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 246; NO 2; PART. 2; PP. L57-L60; BIBL. 14 REF.Article

FORMATION DES RAIES SPECTRALES ET OSCILLATIONS DANS LA CHROMOSPHERE SOLAIREGOUTTEBROZE PIERRE.1980; ; FRA; DA. 1980; 206 P.; 30 CM; BIBL. 13 P.; TH.: SCI. PHYS./PARIS 7/1980Thesis

FORMATION OF COUPLED SPECTRAL LINES IN A PLANETARY ATMOSPHERE.CHAMBERLAIN JW; WALLACE L.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 190; NO 2 PART. 1; PP. 487-495; BIBL. 6 REF.Article

RESOLUTION DE L'EQUATION DE TRANSFERT EN PRESENCE D'UN CHAMP DE VITESSESSIMONNEAU E.1972; C.R. ACAD. SCI., B; FR.; DA. 1972; VOL. 275; NO 3; PP. 169-172; BIBL. 2REF.Serial Issue

ANGLE-AVERAGED REDISTRIBUTION FUNCTION IN THE LABORATORY FRAMESEITZ M; BASCHEK B; WEHRSE R et al.1982; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1982; VOL. 109; NO 1; PP. 10-16; BIBL. 23 REF.Article

REDISTRIBUTION OF RADIATION FOR THE WINGS OF LYMAN-ALPHAYELNIK JB; BURNETT K; COOPER J et al.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 248; NO 2; PART. 1; PP. 705-716; BIBL. 29 REF.Article

EFFECT OF WEAK TURBULENCE ON SPECTRAL LINE FORMATION.RYBICKI G.1976; IN: PHYS. MOUVEMENTS ATMOS. STELLAIRES. COLLOQ. INT. C.N.R.S.; NICE; 1975; PARIS; C.N.R.S.; DA. 1976; PP. 189-204; ABS. FR.; BIBL. 9 REF.Conference Paper

AN ANALYTIC SOLUTION FOR THE LINE FORMATION IN A MAGNETIC FIELD I.SIDLICHOVSKY M.1976; BULL. ASTR. INST. CZECHOSL.; CZECHOSL.; DA. 1976; VOL. 27; NO 2; PP. 71-74; ABS. RUSSE; BIBL. 9 REF.Article

KINETIC EQUILIBRIUM AND LINE FORMATION OF NAI IN THE SOLAR ATMOSPHERE.GEHREN T.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 38; NO 2; PP. 289-302; BIBL. 40 REF.Article

THE LINE RESPONSE FUNCTION OF STELLAR ATMOSPHERES AND THE EFFECTIVE DEPTH OF LINE FORMATION.BECKERS JM; MILKEY RW.1975; SOLAR PHYS.; NETHERL.; DA. 1975; VOL. 43; NO 2; PP. 289-292; BIBL. 3 REF.Article

THE USE OF VARIABLE QUADRATURE WEIGHTS.FRANDSEN S.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 40; NO 1-2; PP. 213-216; BIBL. 8 REF.Article

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