Pascal and Francis Bibliographic Databases

Help

Search results

Your search

kw.\*:("OPTICALLY THICK PLASMA")

Publication Year[py]

A-Z Z-A Frequency ↓ Frequency ↑
Export in CSV

Discipline (document) [di]

A-Z Z-A Frequency ↓ Frequency ↑
Export in CSV

Language

A-Z Z-A Frequency ↓ Frequency ↑
Export in CSV

Author Country

A-Z Z-A Frequency ↓ Frequency ↑
Export in CSV

Results 1 to 25 of 65

  • Page / 3
Export

Selection :

  • and

METHODES APPROCHEES DE RESOLUTION DES PROBLEMES DE TRANSFERT RADIATIF DANS UN PLASMA FROID FORTEMENT MAGNETISEKAMINKER AD; PAVLOV GG; SILANT'EV NA et al.1982; ASTROFIZIKA; ISSN 0571-7132; SUN; DA. 1982; VOL. 18; NO 2; PP. 283-299; ABS. ENG; BIBL. 22 REF.Article

ETUDE DES RAIES DE L'ALUMINIUM REDUITES A UNE COUCHE MINCE DANS LES CONDITIONS DU PLASMA OPTIQUEMENT DENSEFISHMAN IS; SALAKHOV M KH; SARANDAEV EV et al.1981; OPT. SPEKTROSK.; ISSN 0030-4034; SUN; DA. 1981; VOL. 51; NO 5; PP. 785-793; BIBL. 14 REF.Article

Optically thick plasmas: a summary of contributed papersMASON, K. O.Physica scripta. T. 1984, Vol 7, pp 187-189, issn 0281-1847Article

DIRECT SOLUTION OF THE EQUATION OF TRANSFER USING FREQUENCY AND ANGLE-AVERAGED PHOTON ESCAPE PROBABILITIES WITH APPLICATION TO A MULTISTAGE MULTIVEL ALUMINIUM PLASMAAPRUZESE JP; DAVIS J; DUSTON D et al.1980; J. QUANT. SPECTROSC. RAD. TRANSFER; GBR; DA. 1980; VOL. 23; NO 5; PP. 479-487; BIBL. 9 REF.Article

RAYONNEMENT THERMIQUE PROVENANT DE PLASMA OPTIQUEMENT EPAIS AVEC UN FORT CHAMP MAGNETIQUEPAVLOV GG; SHIBANOV YU A.1978; ASTR. ZH.; S.S.S.R.; DA. 1978; VOL. 55; NO 2; PP. 373-389; BIBL. 21 REF.Article

METHODE DE MESURE DE LA POPULATION DES NIVEAUX DE RESONANCE DANS UNE SOURCE A SYMETRIE AXIALEGOLUBOVSKIJ YU B; RYKOV VI.1977; ZH. PRIKL. SPEKTROSK., BELORUS. S.S.R.; S.S.S.R.; DA. 1977; VOL. 26; NO 5; PP. 895-899; BIBL. 6 REF.Article

POPULATION INVERSION IN OPTICALLY THICK, RECOMBINING HYDROGEN PLASMASFURUKANE U; YOKOTA T; KAWASAKI K et al.1982; JOURNAL OF QUANTITATIVE SPECTROSCOPY AND RADIATIVE TRANSFER; ISSN 0022-4073; GBR; DA. 1982; VOL. 29; NO 1; PP. 75-79; BIBL. 9 REF.Article

PRESSURE DETERMINATION OF MERCURY DISCHARGES FROM SELF-REVERSED SPECTRAL LINESKARABOURNIOTIS D; DAMELINCOURT JJ.1982; J. APPL. PHYS.; ISSN 0021-8979; USA; DA. 1982; VOL. 53; NO 4; PP. 2965-2970; BIBL. 23 REF.Article

EQUILIBRE D'UNE DECHARGE A COURANT INTENSE CONTRACTEE DANS UN PLASMA DENSE OPTIQUEMENT OPAQUEGRISHIN YU M; KOZLOV NP; MOSIN AA et al.1980; Z. TEH. FIZ.; ISSN 0044-4642; SUN; DA. 1980; VOL. 50; NO 4; PP. 685-692; BIBL. 6 REF.Article

DIAGNOSTIC LOCALISE D'UN PLASMA ASYMETRIQUE OPTIQUEMENT DENSEMEL'NIKOVA TS; PIKALOV VV; PREOBRAZHENSKIJ NG et al.1980; OPT. I SPEKTROSK., SBOR. STATEJ; SUN; DA. 1980; VOL. 48; NO 3; PP. 474-479; BIBL. 15 REF.Article

THEORIE DES DECHARGES INTENSES A COURANT INVERSEALEKSANDROV AF; RESHETNYAK SA.1976; VEST. MOSKOV. UNIV., 3; S.S.S.R.; DA. 1976; VOL. 31; NO 4; PP. 466-474; BIBL. 11 REF.Article

Emissivités de surface d'un plasma magnétisé optiquement épais, et luminosités d'étoiles à neutrons en accrétionPAVLOV, G. G; SHIBANOV, YU. A.Astronomičeskij žurnal. 1985, Vol 62, Num 1, pp 43-53, issn 0004-6299Article

An analytic Voigt profile escape probability approximationAPRUZESE, J. P.Journal of quantitative spectroscopy & radiative transfer. 1985, Vol 34, Num 5, pp 447-452, issn 0022-4073Article

Series expansion for the emission intensity of optically thick plasmasVICHARELLI, P. A; REISER, P. A.Physics letters. A. 1987, Vol 125, Num 6-7, pp 326-329, issn 0375-9601Article

DETERMINATION OF SELF-ABSORPTION IN EMISSION LINES FROM SOME OPTICALLY THICK PLASMASPIANAROSA P; GAGNE JM; LARIN G et al.1982; J. OPT. SOC. AM. (1980); ISSN 0030-3941; USA; DA. 1982; VOL. 72; NO 3; PP. 392-394; BIBL. 7 REF.Article

INTENSITES DES SATELLITES BIELECTRONIQUES DE LA RAIE DE RESONANCE DES IONS DU TYPE HE DANS UN PLASMA OPTIQUEMENT EPAISBOJKO VA; MAJOROV SA; PIKUZ SA et al.1982; OPT. SPEKTROSK.; ISSN 0030-4034; SUN; DA. 1982; VOL. 52; NO 3; PP. 433-436; BIBL. 7 REF.Article

PHOTON ESCAPE PROBABILITIES FOR STARK-BROADENED LYMAN SERIES LINESWEISHEIT JC.1979; J. QUANT. SPECTROSC. RAD. TRANSFER; GBR; DA. 1979; VOL. 22; NO 6; PP. 585-588; BIBL. 11 REF.Article

SIMPLE CONVECTION-LOSS DOMINATED MODEL FOR OPTICALLY THICK SF6 ARCSAIREY DR.1978; PROC. INSTIT. ELECTR. ENGRS; GBR; DA. 1978; VOL. 125; NO 8; PP. 770-775; BIBL. 33 REF.Article

DESEXCITATION COLLISIONNELLE DES NIVEAUX METASTABLES ET INTENSITE DES COMPOSANTES DU DOUBLET DE RESONANCE D'IONS HYDROGENOIDES DANS UN PLASMA PRODUIT PAR LASERBEJGMAN IL; BOJKO VA; PIKUZ SA et al.1976; ZH. EKSPER. TEOR. FIZ.; S.S.S.R.; DA. 1976; VOL. 71; NO 3; PP. 975-983; ABS. ANGL.; BIBL. 17 REF.Article

DIAGNOSTIC D'UN PLASMA OPTIQUEMENT EPAIS D'APRES LES INTENSITES RELATIVES DES RAIES SPECTRALES DES IONS A CHARGES MULTIPLESBOJKO VA; VINOGRADOV AV; PIKUZ SA et al.1980; Z. TEH. FIZ.; ISSN 0044-4642; SUN; DA. 1980; VOL. 50; NO 1; PP. 201-203; BIBL. 11 REF.Article

REGENERATION D'ONDES D'APPLITUDE FINIE AU-DELA DE LA BARRIERE D'OPACITEKRASOVSKIJ VL; ORAEVSKIJ VN.1979; FIZ. PLAZMY; SUN; DA. 1979; VOL. 5; NO 5; PP. 1072-1077; BIBL. 7 REF.Article

INTERPRETATION OF THE SPATIAL AND SPECTRAL INTENSITIES OF OPTICALLY THICK RESONANCE LINES EMITTED FROM A SPHERICAL LASER-HEATED PLASMA.APRUZESE JP; DAVIS J; WHITNEY KG et al.1977; J. APPL. PHYS.; U.S.A.; DA. 1977; VOL. 48; NO 2; PP. 667-673; BIBL. 14 REF.Article

PROFILE: A CODE FOR EVALUATING LINE PROFILE SHAPES FOR OPTICALLY THICK EXPANDING PLASMASTALLENTS GJ.1982; COMPUT. PHYS. COMMUN.; ISSN 0010-4655; NLD; DA. 1982; VOL. 25; NO 2; PP. 141-148; BIBL. 17 REF.Article

AN INTERPRETATION OF ANOMALOUS INTENSITY RATIOS WITHIN THE HYDROGEN-LIKE LALPHA DAUBLET IN OPTICALLY THICK LASER PRODUCED PLASMASIRONS FE.1980; AUS. J. PHYS.; ISSN 0004-9506; AUS; DA. 1980; VOL. 33; NO 2A; PP. 283-301; BIBL. 51 REF.Article

AN INVESTIGATION OF THE POTENTIAL OF OPTICALLY THICK LINE PROFILES FOR DETERMINING LASER-PRODUCED PLASMA PARAMETERSTALLENTS GJ.1980; J. PHYS. B; ISSN 0022-3700; GBR; DA. 1980; VOL. 13; NO 15; PP. 3057-3072; BIBL. 34 REF.Article

  • Page / 3