THE USE OF SPECTRAL EMISSION LINES IN THE DIAGNOSTICS OF HOT SOLAR PLASMASFELDMAN U.1981; PHYS. SCR.; ISSN 0031-8949; SWE; DA. 1981; VOL. 24; NO 4; PP. 681-711; BIBL. 121 REF.Article

SPECTROSCOPY FROM LASER-PRODUCED PLASMAS AT FLARE TEMPERATURES.FELDMAN U.1976; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1976; VOL. 41; NO 1; PP. 155-181; BIBL. 25 REF.Article

The beam-driven chromospheric evaporation model of solar flares : a model not supported by observations from nonimpulsive large flaresFELDMAN, U.The Astrophysical journal. 1990, Vol 364, Num 1, pp 322-325, issn 0004-637X, 4 p., p.1Article

HIGH-RESOLUTION SPECTRA OF THE SOLAR MG II H AND K LINES FROM SKYLAB.DOSCHEK GA; FELDMAN U.1977; ASTROPHYS. J., SUPPL. SER.; U.S.A.; DA. 1977; VOL. 35; NO 4; PP. 471-482; H.T. 1; BIBL. 16 REF.Article

THE EMISSION SPECTRUM OF THE HYDROGEN BALMER SERIES OBSERVED ABOVE THE SOLAR LIMB FROM SKYLAB. II. ACTIVE REGIONS.FELDMAN U; DOSCHEIK GA.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 212; NO 3 PART. 1; PP. 913-922; BIBL. 13 REF.Article

SOLAR CORONAL LINE PROFILES IN THE EXTREME-ULTRAVIOLET.FELDMAN U; BEHRING WE.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 189; NO 1 PART. 2; PP. 45-46; BIBL. 6 REF.Article

ON THE PROBLEM OF DENSITY DIAGNOSTICS FOR THE EUV SPECTRUM OF THE SOLAR TRANSITION ZONE.DOSCHEK GA; FELDMAN U.1977; ASTR. AND ASTROPHYS.; GERM.; DA. 1977; VOL. 58; NO 1-2; PP. L13-L15; BIBL. 17 REF.Article

THE CORONAL TEMPERATURE AND NONTHERMAL MOTIONS IN A CORONAL HOLE COMPARED WITH OTHER SOLAR REGIONS.DOSCHEK GA; FELDMAN U.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 212; NO 3 PART. 2; PP. L143-L146; BIBL. 24 REF.Article

THE SOLAR SPECTRUM IN THE VINICITY OF THE SI IV LINES AT 1122 AND 1128 A.FELDMAN U; DOSCHEK GA.1977; ASTR. AND ASTROPHYS.; GERM.; DA. 1977; VOL. 61; NO 2; PP. 295-296; BIBL. 7 REF.Article

On the unresolved fine structures of the solar atmosphere. II: The temperature region 2 X 10⁵-5 X10⁵ KFELDMAN, U.The Astrophysical journal. 1987, Vol 320, Num 1, pp 426-429, issn 0004-637X, 1Article

A SEARCH FOR A TURBULENT FREE REGION IN THE SOLAR TRANSITION ZONE.FELDMAN U; DOSCHEK GA.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 216; NO 3 PART. 2; PP. L119-L121; BIBL. 16 REF.Article

METEOROLOGICAL CONDITIONS NEAR THE WISE OBSERVATORY, ISRAEL.VIDAL NV; FELDMAN U.1974; QUART. J.R. ASTR. SOC.; G.B.; DA. 1974; VOL. 15; NO 4; PP. 462-472; BIBL. 8 REF.Article

ON IONIZATION EQUILIBRIUM IN SOLAR FLARES AS DETERMINED FROM X-RAY EMISSION LINES OF CA XVIII AND CA XIXDOSCHEK GA; FELDMAN U.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 251; NO 2; PP. 792-796; BIBL. 24 REF.Article

THE ELECTRON DENSITY AT 10⁵ K IN DIFFERENT REGIONS OF THE SOLAR ATMOSPHERE DERIVED FROM AN INTERSYSTEM LINE OF OIV.FELDMAN U; DOSCHEK GA.1978; ASTR. AND ASTROPHYS.; GERM.; DA. 1978; VOL. 65; NO 2; PP. 215-222; BIBL. 24 REF.Article

PLASMA DIAGNOSTICS USING HIGH-RESOLUTION SPECTROSCOPIC TECHNIQUES.FELDMAN U; DOSCHEK GA.1977; J. OPT. SOC. AMER.; U.S.A.; DA. 1977; VOL. 67; NO 6; PP. 726-734; BIBL. 34 REF.Article

THE 3S-3P AND 3P-3D LINES OF MG II OBSERVED ABOVE THE SOLAR LIMB FROM SKYLAB.FELDMAN U; DOSCHEK GA.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 212; NO 3 PART. 2; PP. L147-L150; BIBL. 10 REF.Article

EXPLORING PLASMAS - IN THE SUN AND IN THE LABORATORY.DOSCHEK GA; FELDMAN U.1976; ASTRONAUT. AND AERONAUT.; U.S.A.; DA. 1976; VOL. 14; NO 7-8; PP. 24-30Article

HIGH RESOLUTION ROCKET EUV SOLAR SPECTROGRAPH = SPECTROGRAPHE SOLAIRE A UV LOINTAIN, A HAUTE RESOLUTION, POUR FUSEEBEHRING WE; UGIANSKY RJ; FELDMAN U et al.1973; APPL. OPT.; U.S.A.; DA. 1973; VOL. 12; NO 3; PP. 528-532; BIBL. 8 REF.Serial Issue

THE WIDTHS OF THE SOLAR HE I AND HE II LINES AT 584, 537, AND 304 A.DOSCHEK GA; BEHRING WE; FELDMAN U et al.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 190; NO 3 PART. 2; PP. 141-142; BIBL. 13 REF.Article

THE SOLAR SPECTRUM: WAVELENGTHS AND IDENTIFICATIONS FROM 60 TO 385 ANGSTROMSBEHRING WE; COHEN L; FELDMAN U et al.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 175; NO 2, PART 1; PP. 493-523; H.T. 2; BIBL. 1P.Serial Issue

FORBIDDEN LINE EMISSION FROM HIGHLY IONIZED ATOMS IN TOKAMAK PLASMASFELDMAN U; DOSCHEK GA; BHATIA AK et al.1982; JOURNAL OF APPLIED PHYSICS; ISSN 0021-8979; USA; DA. 1982; VOL. 53; NO 12; PP. 8554-8561; BIBL. 25 REF.Article

HIGH RESOLUTION X-RAY SPECTRA OF SOLAR FLARES. V: INTERPRETATION OF INNER-SHELL TRANSITIONS IN FE XX-FE XXIIIDOSCHEK GA; FELDMAN U; COWAN RD et al.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 245; NO 1; PART. 1; PP. 315-327; BIBL. 27 REF.Article

SOLAR OBSERVATIONS AND ATOMIC DATA FOR THE 3S^{2 1}S₀-3S3P ³P₁ TRANSITION IN S VFELDMAN U; DOSCHEK GA; BHATIA AK et al.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 250; NO 2; PART. 1; PP. 799-804; BIBL. 14 REF.Article

WHAT PRODUCES THE HIGH DENSITIES OBSERVED IN SOLAR FLARE PLASMAS.CHUNG CHIEH CHENG; FELDMAN U; DOSCHEK GA et al.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 97; NO 1; PP. 210-212; BIBL. 17 REF.Article

PHYSICAL CONDITIONS IN THE SOLAR ATMOSPHERE ABOVE AN ACTIVE REGIONMARISKA JT; FELDMAN U; DOSCHEK GA et al.1980; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1980; VOL. 240; NO 1; PART. 1; PP. 300-305; BIBL. 26 REF.Article