DETERMINATION DE LA LIMITE QUASI STATIQUE DES ELECTRONS D'APRES L'ASYMETRIE DU PROFIL DES RAIES SPECTRALES SATELLITES DE L'HYDROGENEOKS EA; SHOLIN GV.1972; OPT. I SPEKTROSK.; S.S.S.R.; DA. 1972; VOL. 33; NO 3; PP. 401-404; BIBL. 11 REF.Serial Issue

NON-THERMAL BROADENING OF WEAK LINES.GURTOVENKO EA; DE JAGER C; LINDENBERGH A et al.1976; IN: PHYS. MOUVEMENTS ATMOS. STELLAIRES. COLLOQ. INT. C.N.R.S.; NICE; 1975; PARIS; C.N.R.S.; DA. 1976; PP. 331-336; ABS. FR.; BIBL. 7 REF.Conference Paper

ON THE BROADENING AND SHIFT OF SPECTRAL LINES.VAN RENSBERGEN W; DE DONCKER E; DERIDDER G et al.1975; SOLAR PHYS.; NETHERL.; DA. 1975; VOL. 40; NO 2; PP. 303-315; BIBL. 32 REF.Article

HOLTSMARK'S 5/2 POWER LAW FOR THE WINGS OF STARK-BROADENED HYDROGEN LINESGRIEM HR.1972; COMMENTS ATOM. MOLEC. PHYS.; G.B.; DA. 1972; VOL. 3; NO 4; PP. 121-126; BIBL. 19 REF.Serial Issue

SOME CONSEQUENCES OF A RAPID DOPPLER WIDTH VARIATION ON THE FORMATION OF STELLAR CHROMOSPHERIC LINES.MAGNAN C.1974; ASTR. AND ASTROPHYS.; GERM.; DA. 1974; VOL. 33; NO 1; PP. 139-141; BIBL. 6 REF.Article

THE WIDTH OF SPECTRAL LINES.PEACH G.1975; CONTEMPOR. PHYS.; G.B.; DA. 1975; VOL. 16; NO 1; PP. 17-34; BIBL. 1 P.Article

INFLUENCE DES ELECTRONS SUR L'ELARGISSEMENT DES RAIES DE L'HYDROGENEANTIPOVA LI.1978; ASTR. SOVET AKAD. NAUK S.S.S.R., NAUCH. INFORM.; SUN; DA. 1978; NO 42; PP. 3-20; ABS. ENG; BIBL. 17 REF.Article

EFFECTS OF TIME ORDERING ON PLASMA-BROADENED HYDROGEN PROFILES.ROSZMAN LJ.1975; PHYS. REV. LETTERS; U.S.A.; DA. 1975; VOL. 34; NO 13; PP. 785-788; BIBL. 29 REF.Article

QUANTUM MECHANICAL CALCULATIONS FOR THE ELECTRON IMPACT BROADENING AND SHIFT OF SOME LINES OF NEUTRAL HELIUM IN A HOT PLASMA.BASSALO JM; CATTANI M.1975; CANAD. J. PHYS.; CANADA; DA. 1975; VOL. 53; NO 20; PP. 2285-2288; ABS. FR.; BIBL. 9 REF.Article

DEPLACEMENT ET ELARGISSEMENT THERMIQUES DES RAIES DE LUMINESCENCE ET D'ABSORPTION DE L'ION ND³⁺ DANS LES CRISTAUX DE FLUORAPATITEMINKOV BI; OSTROVSKAYA EM; SAZONOVA SA et al.1976; OPT. I. SPEKTROSK.; S.S.S.R.; DA. 1976; VOL. 40; NO 4; PP. 713-718; BIBL. 18 REF.Article

APPLICATIONS OF FOURIER ANALYSIS TO BROADENING OF STELLAR LINE PROFILES. III. SOLAR MICROTURBULENCE AND MACROTURBULENCE FROM IRON LINES.SMITH MA; TESTERMAN L; EVANS JC et al.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 207; NO 1 PART. 1; PP. 308-324; BIBL. 31 REF.Article

STARK BROADENING AND DISPLACEMENT OF ISOLATED HE I LINES.DIATTA CS; FLEURIER C; CHAPELLE J et al.1974; PHYS. LETTERS, A; NETHERL.; DA. 1974; VOL. 49; NO 6; PP. 450-452; BIBL. 10 REF.Article

ELARGISSEMENT INHOMOGENE ET DEPLACEMENT DES RAIES SANS PHONON DU SPECTRE DE LUMINESCENCE DE O₂^- DANS KCLFREJBERG AM; REBANE LA.1974; FIZ. TVERD. TELA; S.S.S.R.; DA. 1974; VOL. 16; NO 9; PP. 2626-2632; BIBL. 16 REF.Article

ETUDE EXPERIMENTALE DE L'ELARGISSEMENT PAR EFFET STARK DES RAIES SPECTRALES HEI, LAMBDA =4471.48 A ET HEI, LAMBDA =4470.04 A EMISES PAR UN PLASMA.RAMETTE J.1973; ; S.L.; DA. 1973; PP. 1-161; ABS. ANGL.; BIBL. DISSEM.; (THESE DOCT. 3EME CYCLE, SPEC. PHYS. GAZ PLASMAS; PARIS XI ORSAY)Thesis

ON THE EFFECT OF TIME-ORDERING FOR LYMAN-ALPHA .GREENE RL; COOPER J.1975; J. QUANT. SPECTROSC. RAD. TRANSFER; G.B.; DA. 1975; VOL. 15; NO 11; PP. 991-993; BIBL. 12 REF.Article

CALCUL DES PROFILS DE RAIES DE LA SERIE DE BALMER.STAMM R; VOSLAMBER D.1975; C.R. ACAD. SCI., B; FR.; DA. 1975; VOL. 280; NO 8; PP. 223-226; ABS. ANGL.; BIBL. 8 REF.Article

LINEWIDTHS IN X-RAY PHOTOEMISSION AND X-RAY EMISSION SPECTROSCOPIES: WHAT DO THEY MEASURE.CITRIN PH; EISENBERGER PM; MARRA WC et al.1974; PHYS. REV., B; U.S.A.; DA. 1974; VOL. 10; NO 4; PP. 1762-1765; BIBL. 19 REF.Article

RESONANCE-LINE TRANSFER WITH PARTIAL REDISTRIBUTION. II. THE SOLAR MGII LINES.MILKEY RW; MIHALAS D.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 192; NO 3 PART. 1; PP. 769-776; BIBL. 30 REF.Article

PROFILS DES RAIES SPECTRALES D'UN PLASMA INHOMOGENE POUR UNE AUGMENTATION APPARENTE DE L'EPAISSEUR OPTIQUE (MESURES DE LA TEMPERATURE DU PLASMA)LITSKI YA; SUKEVER SH.1972; INR-1388-VII-XVIII-PP; POL'SKA; DA. 1972; PP. (23 P.); ABS. ANGL. POL.; BIBL. 17 REF.Report

PROFILES OF RADIO RECOMBINATION LINES.HIGGS LA.1975; J.R. ASTR. SOC. CANADA; CANADA; DA. 1975; VOL. 69; NO 6; PP. 289-298; BIBL. 11 REF.Article

SPECTRAL FEATURES TO BE EXPECTED FROM ROTATIONAL AND EXPANSIONAL MOTIONS IN FINE SOLAR STRUCTURES.ROMPOLT B.1975; SOLAR PHYS.; NETHERL.; DA. 1975; VOL. 41; NO 2; PP. 329-348; BIBL. 12 REF.Article

PLASMA POLARIZATION SHIFT FOR MEMBERS OF THE RESONANCE SERIES OF IONIZED HELIUMGABRIEL AH; VOLONTE S.1973; PHYS. LETTERS, A; NETHERL.; DA. 1973; VOL. 43; NO 4; PP. 372-374; BIBL. 9 REF.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

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

COMPARISON OF HALPHA AND CAII H AND K SPECTROHELIOGRAMS AS A DIAGNOSTIC PROBE.GEBBIE KB; STEINITZ R.1974; INTERNATION. ASTR. UN., SYMP.; NETHERL.; DA. 1974; NO 56; PP. 55-307 (14P.); BIBL. 11 REF.; (CHROMOS. FINE STRUCT. SYMP. NO 56; SURFER'S PARADISE, QUEENSL.; 1973)Article