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

ULTRAVIOLET CONTINUUM ABSORPTION ( <OU= 1000 A) ABOVE THE QUIET SUN TRANSITION REGIONDOSCHEK GA; FELDMAN U.1982; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1982; VOL. 254; NO 1; PART. 1; PP. 371-375; BIBL. 31 REF.Article

EUV SPECTRA FROM SKYLAB (1175-1940 A): MASS MOTIONS IN THE TRANSITION ZONE IN REGIONS OF SOLAR ACTIVITYDOSCHEK GA; FELDMAN U.1978; ASTR. AND ASTROPHYS.; DEU; DA. 1978; VOL. 69; NO 1; PP. 11-21; BIBL. 13 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

Is it justified to assume that Everywhere in the Sun's photosphere-corona domain the electric conductivity is high ? Or, what drives the solar upper atmosphere ?FELDMAN, U.The Astrophysical journal. 1993, Vol 411, Num 2, pp 896-908, issn 0004-637X, 1Article

Transitions from metastable levels emitted during short-duration bursts : how valid are their calculated intensities ?FELDMAN, U.The Astrophysical journal. 1992, Vol 385, Num 2, pp 758-762, issn 0004-637X, p.1Article

Estimating open pack ice parameters using wind field and remotely sensed dataFELDMAN, U.J.G.R. Journal of geophysical research. Part C, Oceans and atmospheres. 1986, Vol 91, Num 2, pp 2503-2509Article

On the unresolved fine structures of the solar atmosphere in the 3×10⁴-2×10⁵K temperature regionFELDMAN, U.The Astrophysical journal. 1983, Vol 275, Num 1, pp 367-373, issn 0004-637XArticle

EMISSION-LINE SPECTRA OF TWO ACTIVE REGIONS ON THE SOLAR LIMB: 1175-1940 AFELDMAN U; DOSCHEK GA.1978; ASTROPHYS. J., SUPPL. SER.; USA; DA. 1978; VOL. 37; NO 4; PP. 443-458; BIBL. 23 REF.Article

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