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ON THE INTERPRETATION OF OPTICALLY THIN SYNCHROTRON SPECTRAPINEAULT S.1982; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1982; VOL. 114; NO 1; PP. 177-181; BIBL. 16 REF.Article

PHYSICAL CONDITIONS IN AN OPTICALLY THIN RELATIVISTIC GAS IRRADIATED BY GAMMA -RAYSKOVNER Z; MILGROM M.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 100; NO 2; PP. 271-276; BIBL. 18 REF.Article

SPECTRAL POLARIZATION PROPERTIES OF OPTICALLY THIN SYNCHROTRON RADIATIONBJOERNSSON CI; BLUMENTHAL GR.1982; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1982; VOL. 259; NO 2; PART. 1; PP. 805-819; BIBL. 13 REF.Article

THE ROLE OF DIRECT IONIZATION-EXCITATION IN POPULATING HE II EXCITED STATES IN OPTICALLY THIN PLASMASSRIVASTAVA HC; GHOSH PK.1980; PHYSICA B+C; ISSN 0378-4363; NLD; DA. 1980; VOL. 101; NO 1; PP. 120-124; BIBL. 6 REF.Article

EXTREME ULTRAVIOLET SPECTRUM OF A HOT INTERSTELLAR PLASMASTERN R; WANG E; BOWYER S et al.1978; ASTROPHYS. J., SUPPL. SER.; USA; DA. 1978; VOL. 37; NO 2; PP. 195-222; BIBL. 92 REF.Article

SIMULATION NUMERIQUE DE L'HYDRODYNAMIQUE D'UN PLASMA TRANSPARENT LORS DE SON ECHAUFFEMENT IMPULSIONNEL PAR DES ELECTRONS A SPECTRE DE PUISSANCESPEKTOR AR.1979; TRUDY FIZ. INST. P.N. LEBEDEVA, MOSKVA; SUN; DA. 1979; VOL. 110; PP. 95-105; BIBL. 6 REF.Article

RESONANCE LINE SCATTERING FROM OPTICALLY THIN STRUCTURES LOCATED ABOVE THE SOLAR LIMB.CRAM LE; VARDAVAS IM.1978; SOLAR PHYS.; NLD; DA. 1978; VOL. 57; NO 1; PP. 27-36; BIBL. 10 REF.Article

ZWEI VERFAHREN ZUR LOESUNG DER ABELSCHEN INTEGRALGLEICHUNG UND ZUR BERECHNUNG DER RADIALEN VOLUMENSTRAHLDICHTE = DEUX METHODES POUR LA RESOLUTION DE L'EQUATION INTEGRALE D'ABEL ET LE CALCUL DE LA DENSITE DE RAYONNEMENT EN VOLUME RADIALEVALENTINI HB.1978; BEITR. PLASMAPHYS.; DDR; DA. 1978; VOL. 18; NO 2; PP. 125-129; ABS. ENG; BIBL. 14 REF.Article

SYSTEMATIC TRENDS IN THE RADIATIVE EMISSION RATES FOR LOW- AND MEDIUM-Z ELEMENTS IN HIGH-TEMPERATURE PLASMASDAVIS J; JACOBS VL.1980; J. QUANT. SPECTROSC. RADIAT. TRANSFER; ISSN 0022-4073; GBR; DA. 1980; VOL. 24; NO 4; PP. 283-288; BIBL. 15 REF.Article

THEORIE STATISTIQUE QUANTIQUE DU CONTINUUM DE RECOMBINAISON D'UN PLASMA D'HYDROGENE OPTIQUEMENT MINCEGINZBURG MD; PARGAMANIK L EH.1979; UKRAIN. FIZ. ZH.; UKR; DA. 1979; VOL. 24; NO 6; PP. 749-757; ABS. ENG; BIBL. 27 REF.Article

SOFT X-RAY SPECTRUM OF A HOT PLASMA.RAYMOND JC; SMITH BW.1977; ASTROPHYS. J., SUPPL. SER.; U.S.A.; DA. 1977; VOL. 35; NO 4; PP. 419-439; BIBL. 97 REF.Article

HYDRODYNAMIQUE DU PLASMA OPTIQUEMENT TRANSPARENT AVEC UNE SOURCE DE CHAUFFAGE REPARTISOMOV BV; SPEKTOR AR; SYROVATSKIJ SI et al.1979; TRUDY FIZ. INST. P.N. LEBEDEVA, MOSKVA; SUN; DA. 1979; VOL. 110; PP. 73-94; BIBL. 36 REF.Article

TRIP 1, A TIME-DEPENDENT RECOMBINATION IONISATION PACKAGEMAGILL J.1978; COMPUTER PHYS. COMMUNIC.; NLD; DA. 1978 PUBL. 1979; VOL. 16; NO 1; PP. 129-137; BIBL. 6 REF.Article

HOMOLOGIE ET SENSIBILITE A LA CONCENTRATION LORS D'UNE EXCITATION D'EQUILIBRESERAPINAS PD; SHALKAUSKAS YU S.1976; ZH. PRIKL. SPEKTROSK., BELORUSS. S.S.R.; S.S.S.R.; DA. 1976; VOL. 25; NO 6; PP. 978-983; BIBL. 8 REF.Article

THE X-RAY SPECTRUM OF A HOT INTERSTELLAR PLASMASHULL JM.1981; ASTROPHYS. J., SUPPL. SER.; ISSN 0067-0049; USA; DA. 1981; VOL. 46; NO 1; PP. 27-40; BIBL. 27 REF.Article

ANNIHILATION SPECTRUM OF RELATIVISTIC PLASMAZDZIARSKI AA.1980; ACTA ASTRON.; ISSN 0001-5237; POL; DA. 1980; VOL. 30; NO 4; PP. 371-391; BIBL. 20 REF.Article

ENERGY TRANSFER IN MAGNETIZED PLASMASNOCERA L.1982; JOURNAL OF PLASMA PHYSICS; ISSN 0022-3778; GBR; DA. 1982; VOL. 28; NO 3; PP. 565-573; BIBL. 12 REF.Article

TRANSPORT ET DEPOT D'ENERGIE DES PARTICULES ALPHA, TRAITEMENT DE L'EQUATION DE FOKKER-PLANCK = ALPHA PARTICLE ENERGY TRANSPORT AND DEPOSITION, STUDY OF FOKKER-PLANCK EQUATIONBESNARD D.1982; ; FRA; DA. 1982; CEA-N/2338; 127 P.; 30 CMReport

CALCULATED X-RADIATION FROM OPTICALLY THIN PLASMAS. III. ABUNDANCE EFFECTS ON CONTINUUM EMISSION.GRONEN SCHILD EHBM; MEWE R.1978; ASTR. AND ASTROPHYS., SUPPL. SER.; GERM.; DA. 1978; VOL. 32; NO 2; PP. 283-305; BIBL. 33 REF.Article

Peculiarities of entropy and magnetosonic waves in optically thin cosmic plasmaSOMOV, B. V; DZHALILOV, N. S; STAUDE, J et al.Astronomy letters (Print). 2007, Vol 33, Num 5, pp 309-318, issn 1063-7737, 10 p.Article

THE STABILITY OF OPTICALLY THIN REACTING PLASMAS: EFFECTS OF THE BULK VISCOSITYIBANEZ S., Miguel H.The Astrophysical journal. 2009, Vol 695, Num 1, pp 479-487, issn 0004-637X, 9 p., 1Article

X-ray and EUV emission from optically thin plasmaLANDINI, M; MONSIGNORI FOSSI, B. C.Physica scripta. T. 1984, Vol 7, pp 53-55, issn 0281-1847Article

THE SPECTROSCOPY OF PLASMAS CARRYING SOUND WAVES. II. SPECTRAL LINE PROFILES.BYERLEY A; MCWHIRTER RWP; WILSON R et al.1978; J. PHYS. B; G.B.; DA. 1978; VOL. 11; NO 4; PP. 613-621; BIBL. 7 REF.Article

DISTRIBUTION RADIALE DE QUELQUES PARAMETRES DANS UN PLASMA DE DECHARGE D'ARC OPTIQUEMENT MINCEAVECHKYIN GV; SANDRYGAJLA LE.1977; VESCI AKAD. NAVUK B.S.S.R., FIZ.-MAT. NAVUK; S.S.S.R.; DA. 1977; NO 2; PP. 92-96; BIBL. 12 REF.Article

POPULATION PROBABILITIES OF THE EXCITED LEVELS OF IONS IN A STEADY-STATE PLASMA. I: BASIC EQUATIONS AND RESULTSSALZMANN D.1979; PHYS. REV. A; ISSN 0556-2791; USA; DA. 1979; VOL. 20; NO 4; PP. 1704-1712; BIBL. 8 REF.Article

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