Search Results - "Schmutz, W. K."

Impact of a potential 21st century "grand solar minimum" on surface temperatures and stratospheric ozone by 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.

“…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…”
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The nature of solar brightness variations by Shapiro, A. I., Solanki, S. K., Krivova, N. A., Cameron, R. H., Yeo, K. L., Schmutz, W. K.

“…Determining the sources of solar brightness variations 1 , 2 , often referred to as solar noise 3 , is important because solar noise limits the detection of…”
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Traceable radiometry underpinning terrestrial- and helio-studies (TRUTHS) by Fox, N., Aiken, J., Barnett, J.J., Briottet, X., Carvell, R., Frohlich, C., Groom, S.B., Hagolle, O., Haigh, J.D., Kieffer, H.H., Lean, J., Pollock, D.B., Quinn, T., Sandford, M.C.W., Schaepman, M., Shine, K.P., Schmutz, W.K., Teillet, P.M., Thome, K.J., Verstraete, M.M., Zalewski, E.

“…The Traceable Radiometry Underpinning Terrestrial- and Helio- Studies (TRUTHS) mission offers a novel approach to the provision of key scientific data with…”
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Solar-Blind Diamond Detectors for Lyra, the Solar VUV Radiometer on Board Proba II by Benmoussa, A, Hochedez, J-F, Schmutz, W K, SchUehle, U, NeslAdek, M, Stockman, Y, Kroth, U, Richter, M, Theissen, A, Remes, Z, Haenen, K, Mortet, V, Koller, S, Halain, J P, Petersen, R, Dominique, M, D'Olieslaeger, M

“…Fabrication, packaging and experimental results on the calibration of metal-semiconductor-metal (MSM) photodetectors made on diamond are reported. LYRA…”
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Influence of solar wind on ozone and circulation in the middle atmosphere: A model study by Zubov, V A, Rozanov, E V, Shirochkov, A V, Makarova, L N, Egorova, T A, Kiselev, A A, Ozolin, YuE, Karol, IL, Schmutz, W K

“…A study investigated the influence of solar wind on ozone and circulation in the middle atmosphere. During the warm half of the year (from May to September),…”
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Are solar brightness variations faculae- or spot-dominated? by Shapiro, A. I, Solanki, S. K, Krivova, N. A, Yeo, K. L, Schmutz, W. K

“…Regular spaceborne measurements have revealed that solar brightness varies on multiple timescales, variations on timescales greater than a day being attributed…”
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The role of the Fraunhofer lines in solar brightness variability by Shapiro, A. I, Solanki, S. K, Krivova, N. A, Tagirov, R. V, Schmutz, W. K

“…The solar brightness varies on timescales from minutes to decades. A clear identification of the physical processes behind such variations is needed for…”
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The variability of Sun-like stars: reproducing observed photometric trends by 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…”
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The nature of solar brightness variations by Shapiro, A. I, Solanki, S. K, Krivova, N. A, Cameron, R. H, Yeo, K. L, 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…”
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