Theoretical Stokes profiles for magnetic stars. I: Rotation, line asymmetries and crossoverSTIFT, M. J.Monthly Notices of the Royal Astronomical Society. 1985, Vol 217, Num 1, pp 55-68, issn 0035-8711Article

Simple formulae for estimating Stark widths and shifts of neutral atom linesDIMITRIJEVIC, M. S; KONJEVIC, N.Astronomy and astrophysics (Berlin. Print). 1986, Vol 163, Num 1-2, pp 297-300, issn 0004-6361Article

Spatial and temporal variation of circular Zeeman Profiles in isolated solar Ca⁺K structuresWIEHR, E.Astronomy and astrophysics (Berlin. Print). 1985, Vol 149, Num 1, pp 217-220, issn 0004-6361Article

Changement du profil de la raie spectrale solaire λ5123,7 @ entre le centre et le bordBABIJ, B. T; KOKHAN, E. K; KOVAL'CHUK, M. M et al.Astrometriâ i astrofizika. 1984, Num 53, pp 10-14, issn 0582-8198Article

Variations of the asymmetry of disk-integrated solar line profilesBRUNING, D. H; LABONTE, B.Solar physics. 1985, Vol 97, Num 1, pp 1-7, issn 0038-0938Article

Observations of photometric profiles of two planetary nebulaeLOUISE, R; KHEROUS, A.Astrophysics and space science. 1991, Vol 176, Num 1, pp 149-162, issn 0004-640X, 14 p.Article

Importance de certains paramètres dans la synthèse du spectre solaire non ETL du potassium neutre KI. III: TempératureSHUKINA, N. G.Solnečnye dannye. 1985, Num 2, pp 84-87, issn 0552-5829Article

On the theories of cyclotron resonance line shapeARGYRES, P. N.Solid state communications. 1984, Vol 50, Num 3, pp 279-281, issn 0038-1098Article

Stark broadening in non-LTE stellar atmospheres: effects on occupation numbers and line profilesWERNER, K.Astronomy and astrophysics (Berlin. Print). 1984, Vol 139, Num 1, pp 237-239, issn 0004-6361Article

The influences of penumbral fine structures on line profilesWIEHR, E; KOCH, A; KNÖLKER, M et al.Astronomy and astrophysics (Berlin. Print). 1984, Vol 140, Num 2, pp 352-356, issn 0004-6361Article

Expected and observed profiles of CO and CS in cometary spectraKRISHNA SWAMY, K. S.Moon and the planets. 1983, Vol 29, Num 2, pp 191-193, issn 0165-0807Article

Etude des «flashes d'ombre» en divers points du disque solaire, et structure fine des ombres de taches solairesTEPLITSKAYA, R. B; TUROVA, I. P.Solnečnye dannye. 1983, Num 8, pp 102-112, issn 0552-5829Article

LINE PROFILES AND MAGNETIC INTENSIFICATION IN MAGNETIC STARS.HAVNES O; MOE OK.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 42; NO 2; PP. 269-272; BIBL. 9 REF.Article

MESURE DES CONTOURS DE RAIES PAR LES TECHNIQUES DE TELEVISION.FEHRENBACH C; VIN A.1975; ASTROPHYS. SPACE SCI. LIBRARY; NETHERL.; DA. 1975; VOL. 54; PP. 109-116; (IMAGE PROCESS. TECH. ASTRON. PROC. CONF.; UTRECHT; 1975)Conference Paper

SOLAR LINE PROFILES OF HE I 584 A AND HE II 304 A.CUSHMAN GW; FARWELL L; GODDEN G et al.1975; J. GEOPHYS. RES.; U.S.A.; DA. 1975; VOL. 80; NO 4; PP. 482-486; BIBL. 11 REF.Article

DISTRIBUTION DES DEMI-LARGEURS DES PROFILS DES RAIES CORONALESTETRUASHVILI EH I.1975; ABASTUMAN. ASTROFIZ. OBS., BJULL.; S.S.S.R.; DA. 1975; NO 46; PP. 185-188; ABS. GEORGIEN ANGL.; BIBL. 5 REF.Article

POSSIBILITES ET RESTRICTIONS DE LA METHODE DE "CARTOGRAPHIE" DE LA SURFACE DES ETOILES AP D'APRES LES PROFILS DES RAIES SPECTRALESKHOKHLOVA VL.1975; ASTR. ZH.; S.S.S.R.; DA. 1975; VOL. 52; NO 5; PP. 950-955; BIBL. 7 REF.Article

THE HELIUM 10830 A LINE IN EARLY-TYPE STARS; AN ATLAS OF FABRY-PEROT SCANSMEISEL DD; SAUNDERS BA; FRANK ZA et al.1982; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1982; VOL. 263; NO 2; PART. 1; PP. 759-776; BIBL. 63 REF.Article

A MECHANISM FOR THE PRODUCTION OF LIGHT AND DARK CONTRASTS IN RADIATIVELY CONTROLLED LINESGEBBIE KB; STEINITZ R.1973; SOLAR PHYS.; NETHERL.; DA. 1973; VOL. 29; NO 1; PP. 3-15; BIBL. 4 REF.Serial Issue

OBSERVATIONS OF SHIFTS OF HYDROGEN LINESBENGTSON RD; CHESTER GR.1972; ASTROPHYS. J.,; U.S.A.; DA. 1972; VOL. 178; NO 2PART1; PP. 565-569; BIBL. 13REF.Serial Issue

PROFILS ET LARGEURS A MI HAUTEUR DES RAIES TELLURIQUESKOZHEVNIKOV NI; SITNIK GF; KHLYSTOV AI et al.1972; SOOBSHCH. GOS. ASTR. INST. P.K. SHTERNBERGA; S.S.S.R.; DA. 1972; NO 180; PP. 3-19; ABS. ANGL; BIBL. 15REF.Serial Issue

Gated peak integration versus peak detection in white noiseVOIGTMAN, E.Applied spectroscopy. 1991, Vol 45, Num 2, pp 237-241, issn 0003-7028Article

Particularités physiques et morphologiques de l'émergence d'un filament actifFERRO RAMOS, I.Solnečnye dannye. 1986, Num 7, pp 50-57, issn 0552-5829Article

The hydrocarbon ring C₃H₂ is ubiquitous in the GalaxyMATTHEWS, H. E; IRVINE, W. M.The Astrophysical journal. 1985, Vol 298, Num 2, pp L61-L65, issn 0004-637XArticle

Simultaneous H and K CaII, h and k MgII, Lα and Lβ HI profiles of the April 15, 1978 solar flare observed with the oso-8/L.P.S.P. experimentLEMAIRE, P; CHOUCQ-BRUSTON, M; VIAL, J.-C et al.Solar physics. 1984, Vol 90, Num 1, pp 63-82, issn 0038-0938Article