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Results 1 to 25 of 1254

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Biases in Ion Transmission Through an Electrospray Ionization-Mass Spectrometry Capillary InletPAGE, Jason S; MARGINEAN, Ioan; BAKER, Erin S et al.Journal of the American Society for Mass Spectrometry. 2009, Vol 20, Num 12, pp 2265-2272, issn 1044-0305, 8 p.Article

Explicit expression for the intensity tensor for 3/2-1/2 transitions and solution of the ambiguity problem in Mössbauer spectroscopySZYMANSKI, K.Journal of physics. Condensed matter (Print). 2000, Vol 12, Num 33, pp 7495-7507, issn 0953-8984Article

The Jovian sodium nebula : two years of ground-based observations : Variable phenomena in Jovian planetary systems. IIFLYNN, B; MENDILLO, M; BAUMGARDNER, J et al.Journal of geophysical research. 1994, Vol 99, Num E4, pp 8403-8409, issn 0148-0227Article

Detection of Lyman-α-emitting galaxies at redshift 4.55HU, E. M; MCMAHON, R. G.Nature (London). 1996, Vol 382, Num 6588, pp 231-233, issn 0028-0836Article

Faint Object Spectrograph spectra of the UV emission lines in NGC 5548 : detection of strong narrow componentsCRENSHAW, D. M; BOGGESS, A; CHI-CHAO WU et al.The Astrophysical journal. 1993, Vol 416, Num 2, pp L67-L70, issn 0004-637X, 2Article

Solar magnetic field studies using the 12 micron emission lines. II: Stokes profiles and vector field samples in sunspotsHEWAGAMA, T; DEMING, D; JENNINGS, D. E et al.The Astrophysical journal. Supplement series. 1993, Vol 86, Num 1, pp 313-332, issn 0067-0049Article

The infrared (3.2-3.6 μm) spectrum of comet P/Swift-Tuttle: detection of methanol and other organicsDAVIES, J. K; MUMMA, M. J; REUTER, D. C et al.Monthly Notices of the Royal Astronomical Society. 1993, Vol 265, Num 4, pp 1022-1026, issn 0035-8711Article

The calculation of monatomic spectral lines' intensities and composition in plasma out of thermal equilibrium; evaluation of thermal disequilibrium in ICP torchesANDRE, P; ONDET, J; PELLET, R et al.Journal of physics. D, Applied physics (Print). 1997, Vol 30, Num 14, pp 2043-2055, issn 0022-3727Article

Substantial outgassing of CO from comet Hale-Bopp at large heliocentric distanceBIVER, N; RAUER, H; DESPOIS, D et al.Nature (London). 1996, Vol 380, Num 6570, pp 137-139, issn 0028-0836Article

How bright is the [Si X] 1431 nm coronal emission line?PENN, M. J; KUHN, J. R.Solar physics. 1994, Vol 151, Num 1, pp 51-56, issn 0038-0938Article

Helium-like iron line temperature diagnostics in clusters of galaxiesSWARTZ, D. A; SULKANEN, M. E.The Astrophysical journal. 1993, Vol 417, Num 2, pp 487-493, issn 0004-637X, 1Article

Variation of lunar sodium emission intensity with phase anglePOTTER, A. E; MORGAN, T. H.Geophysical research letters. 1994, Vol 21, Num 21, pp 2263-2266, issn 0094-8276Article

An unsolved problem in the spectrum of quasars: the FeII emission linesJOLY, M.Annales de physique (Imprimé). 1993, Vol 18, Num 3, pp 241-267, issn 0003-4169Article

Oxygen abundance determination in H II regions: The strong line intensities-abundance calibration revisitedPILYUGIN, Leonid S; THUAN, Trinh X.The Astrophysical journal. 2005, Vol 631, Num 1, pp 231-243, issn 0004-637X, 13 p., 1Article

Effect of Coster-Kronig transitions and incident photon energy on the L subshell X-ray intensity ratios of 4F transition elementsALLAWADHI, K. L; ARORA, S. K; SINGH, N et al.Radiation physics and chemistry (1993). 1998, Vol 51, Num 4-6, issn 0969-806X, p. 347Conference Paper

Effect of the luminol signal enhancer on the chemiluminescence intensity and kineticsLIANG, Yan-Li; YU FEI; YU, Song-Cheng et al.Journal of luminescence. 2012, Vol 132, Num 4, pp 1021-1024, issn 0022-2313, 4 p.Article

Charge order as seen by resonant (elastic) X-ray scatteringLORENZO, J. E; JOLY, Y; MANNIX, D et al.The European physical journal. Special topics. 2012, Vol 208, pp 121-127, issn 1951-6355, 7 p.Article

Study of an atmospheric pressure flowing afterglow in N2/NO mixture and its application to the measurement of N2(A) concentrationPOINTU, A. M; MINTUSOV, E; FROMY, P et al.Plasma sources science & technology (Print). 2010, Vol 19, Num 1, issn 0963-0252, 015018.1-015018.10Article

The O+ and O++ emission lines near 834 Å in the quiet sun solar spectrumDOSCHEK, G. A.Geophysical research letters. 2002, Vol 29, Num 7, pp 63.1-63.4, issn 0094-8276Article

Fluorescence intensity fluctuations of single atoms, molecules and nanoparticlesBASCHE, T.Journal of luminescence. 1998, Vol 76-77, pp 263-269, issn 0022-2313Conference Paper

Cosmological baryon density derived from the deuterium abundance at redshift z = 3.57TYTLER, D; FAN, X.-M; BURLES, S et al.Nature (London). 1996, Vol 381, Num 6579, pp 207-209, issn 0028-0836Article

Measurement of the opacity of ionized helium in the intergalactic mediumDAVIDSEN, A. F; KRISS, G. A; ZHENG, W et al.Nature (London). 1996, Vol 380, Num 6569, pp 47-49, issn 0028-0836Article

Near-IR emissions in the upper Jovian atmosphere after SL-9 impact: indications of possible northern counterparts : The collision of comet Shoemaker-Levy 9 with Jupiter. IIISCHULZ, R; ENCRENAZ, T; STÜWE, J. A et al.Geophysical research letters. 1995, Vol 22, Num 17, pp 2421-2424, issn 0094-8276Article

Contribution à l'interprétation des spectres de raies d'émission dans les nébuleuses ionisées = Contribution to the interpretation of emission-line spectra in ionised nebulaeRola, Claudia; Stasinska, G.1995, 193 p.Thesis

Accurate measurement of Mg and AlKα1,2 X-ray energy profilesSCHWEPPE, J; DESLATTES, R. D; MOONEY, T et al.Journal of electron spectroscopy and related phenomena. 1994, Vol 67, Num 3, pp 463-478, issn 0368-2048Article

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