Zobrazeno 1 - 10
of 18
pro vyhledávání: '"Schmutz, W. K."'
The solar brightness varies on timescales from minutes to decades. Determining the sources of such variations, often referred to as solar noise, is of importance for multiple reasons: a) it is the background that limits the detection of solar oscilla
Externí odkaz:
http://arxiv.org/abs/1711.04156
Regular spaceborne measurements have revealed that solar brightness varies on multiple timescales, variations on timescales greater than a day being attributed to surface magnetic field. Independently, ground-based and spaceborne measurements suggest
Externí odkaz:
http://arxiv.org/abs/1602.04447
The solar brightness varies on timescales from minutes to decades. A clear identification of the physical processes behind such variations is needed for developing and improving physics-based models of solar brightness variability and reconstructing
Externí odkaz:
http://arxiv.org/abs/1507.05437
Autor:
Shapiro, A. I., Solanki, S. K., Krivova, N. A., Schmutz, W. K., Ball, W. T., Knaack, R., Rozanov, E. V., Unruh, Y. C.
The Sun and stars with low magnetic activity levels, become photometrically brighter when their activity increases. Magnetically more active stars display the opposite behaviour and get fainter when their activity increases. We reproduce the observed
Externí odkaz:
http://arxiv.org/abs/1406.2383
Autor:
Kopp, G., Dudok de Wit, Thierry, Ball, W. T., Finsterle, W., Frohlich, C., Kokkonen, K., Meftah, Mustapha, Schmutz, W. K.
Publikováno v:
American Geophysical Union, Fall Meeting 2018
American Geophysical Union, Fall Meeting 2018, Dec 2018, Washington, United States
American Geophysical Union, Fall Meeting 2018, Dec 2018, Washington, United States
International audience; We present a new total solar irradiance (TSI) composite based on the methodology of Dudok de Wit et al (2017). This new composite has been vetted by the TSI community as that recommended for use by solar and climate researcher
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::c5c6654dde2e7f98b5affed58564e919
https://hal-insu.archives-ouvertes.fr/insu-02089437
https://hal-insu.archives-ouvertes.fr/insu-02089437
Autor:
Anet J. G., Rozanov E. V., Muthers S., Peter T., Brönnimann S., Arfeuille F., Beer J., Shapiro A. I., Raible C. C., Steinhilber F., Schmutz W. K.
Publikováno v:
GEOPHYSICAL RESEARCH LETTERS
Anet, J. G.; Rozanov, E. V.; Muthers, Stefan; Peter, T.; Brönnimann, Stefan; Arfeuille, Florian Xavier; Beer, J.; Shapiro, A. I.; Raible, Christoph; Steinhilber, F.; Schmutz, W. K. (2013). Impact of a potential 21st century “grand solar minimum” on surface temperatures and stratospheric ozone. Geophysical Research Letters, 40(16), pp. 4420-4425. Wiley 10.1002/grl.50806
Geophysical Research Letters
Anet, J. G.; Rozanov, E. V.; Muthers, Stefan; Peter, T.; Brönnimann, Stefan; Arfeuille, Florian Xavier; Beer, J.; Shapiro, A. I.; Raible, Christoph; Steinhilber, F.; Schmutz, W. K. (2013). Impact of a potential 21st century “grand solar minimum” on surface temperatures and stratospheric ozone. Geophysical Research Letters, 40(16), pp. 4420-4425. Wiley 10.1002/grl.50806
Geophysical Research Letters
©2013. American Geophysical Union. All Rights Reserved We investigate the effects of a recently proposed 21st century Dalton minimum like decline of solar activity on the evolution of Earth's climate and ozone layer. Three sets of two member ensembl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::e8009702984009716c32a786237a6236
https://hdl.handle.net/11475/8844
https://hdl.handle.net/11475/8844
Autor:
Shapiro, A., Schmutz, W. K., Thuillier, Gérard, Rozanov, E., Haberreiter, M., Schoell, M., Nyeki, S.
Publikováno v:
American Geophysical Union Fall Meeting 2010
American Geophysical Union Fall Meeting 2010, Dec 2010, San Francisco California, United States. pp.abstract id.GC21B-0875
American Geophysical Union Fall Meeting 2010, Dec 2010, San Francisco California, United States. pp.abstract id.GC21B-0875
International audience; We have developed and published the COde for Solar Irradiance (COSI) which allows us to calculate the entire solar spectrum. COSI reproduces the spectral irradiance measured by SOLSTICE (up to 320 nm) and SIM (from 320 nm onwa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2417::67695ad92d80750b316acd2d7a0ae96e
https://hal.science/hal-04115179
https://hal.science/hal-04115179
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