Werner Schmutz
Werner Schmutz
Senior scientist PMOD/WRC
Bestätigte E-Mail-Adresse bei - Startseite
Zitiert von
Zitiert von
Spectral analysis of 30 Wolf-Rayet stars
W Schmutz, WR Hamann, U Wessolowski
Astronomy and Astrophysics 210 (1-2), 236-248, 1989
A new approach to the long-term reconstruction of the solar irradiance leads to large historical solar forcing
AI Shapiro, W Schmutz, E Rozanov, M Schoell, M Haberreiter, AV Shapiro, ...
Astronomy & Astrophysics 529, A67, 2011
Nominal values for selected solar and planetary quantities: IAU 2015 resolution B3
A Prša, P Harmanec, G Torres, E Mamajek, M Asplund, N Capitaine, ...
The Astronomical Journal 152 (2), 41, 2016
Recent variability of the solar spectral irradiance and its impact on climate modelling
I Ermolli, K Matthes, T Dudok de Wit, NA Krivova, K Tourpali, M Weber, ...
Atmospheric Chemistry and Physics 13 (8), 3945-3977, 2013
The solar orbiter EUI instrument: the extreme ultraviolet imager
P Rochus, F Auchere, D Berghmans, L Harra, W Schmutz, U Schühle, ...
Astronomy & Astrophysics 642, A8, 2020
A database for galaxy evolution modeling
C Leitherer, D Alloin, UFV Alvensleben, JS Gallagher, JP Huchra, ...
Publications of the Astronomical Society of the Pacific 108 (729), 996, 1996
Fundamental parameters of Wolf-Rayet stars. III. The evolutionary status of WNL stars.
PA Crowther, LJ Smith, DJ Hillier, W Schmutz
Astronomy and Astrophysics, Vol. 293, p. 427-445 (1995) 293, 427-445, 1995
Theoretical continuum energy distributions for Wolf-Rayet stars
W Schmutz, C Leitherer, R Gruenwald
Publications of the Astronomical Society of the Pacific 104 (682), 1164, 1992
Influence of the precipitating energetic particles on atmospheric chemistry and climate
E Rozanov, M Calisto, T Egorova, T Peter, W Schmutz
Surveys in geophysics 33, 483-501, 2012
The PMIP4 contribution to CMIP6 – Part 3: The last millennium, scientific objective, and experimental design for the PMIP4 past1000 simulations
JH Jungclaus, E Bard, M Baroni, P Braconnot, J Cao, LP Chini, T Egorova, ...
Geoscientific Model Development 10 (11), 4005-4033, 2017
Photon loss from the helium Lyalpha line-the key to the acceleration of Wolf-Rayet winds.
W Schmutz
Astronomy and Astrophysics, v. 321, p. 268-287 321, 268-287, 1997
Solar surface magnetism and irradiance on time scales from days to the 11-year cycle
V Domingo, I Ermolli, P Fox, C Fröhlich, M Haberreiter, N Krivova, G Kopp, ...
Space Science Reviews 145, 337-380, 2009
Chemical and dynamical response to the 11‐year variability of the solar irradiance simulated with a chemistry‐climate model
T Egorova, E Rozanov, E Manzini, M Haberreiter, W Schmutz, V Zubov, ...
Geophysical Research Letters 31 (6), 2004
Near-infrared spectroscopy of Galactic Wolf-Rayet stars
ID Howarth, W Schmutz
Astronomy and Astrophysics (ISSN 0004-6361), vol. 261, no. 2, p. 503-522 …, 1992
Hydrodynamic atmosphere models for hot luminous stars
D Schaerer, W Schmutz
Astronomy and Astrophysics (ISSN 0004-6361), vol. 288, no. 1, p. 231-254 288 …, 1994
Chemistry-climate model SOCOL: a validation of the present-day climatology
T Egorova, E Rozanov, V Zubov, E Manzini, W Schmutz, T Peter
Atmospheric Chemistry and Physics 5 (6), 1557-1576, 2005
The Solar Orbiter SPICE instrument-An extreme UV imaging spectrometer
M Anderson, T Appourchaux, F Auchère, RA Cuadrado, J Barbay, ...
Astronomy & Astrophysics 642, A14, 2020
Long-term spectroscopic monitoring of the Luminous Blue Variable AG Carinae
O Stahl, I Jankovics, J Kovács, B Wolf, W Schmutz, A Kaufer, T Rivinius, ...
Astronomy & Astrophysics 375 (1), 54-69, 2001
Chemistry-climate model SOCOL: version 2.0 with improved transport and chemistry/microphysics schemes
M Schraner, E Rozanov, C Schnadt Poberaj, P Kenzelmann, AM Fischer, ...
Atmospheric Chemistry and Physics 8 (19), 5957-5974, 2008
Variability of Sun-like stars: reproducing observed photometric trends
AI Shapiro, SK Solanki, NA Krivova, WK Schmutz, WT Ball, R Knaack, ...
Astronomy & Astrophysics 569, A38, 2014
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