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相关论文: Reconstructed and measured total solar irradiance:…

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A gap in the total solar irradiance (TSI) measurements between ACRIM-1 and ACRIM-2 led to the ongoing debate on the presence or not of a secular trend between the minima preceding cycles 22 (in 1986) and 23 (1996). It was recently proposed…

太阳与恒星天体物理 · 物理学 2014-11-20 N. A. Krivova , S. K. Solanki , T. Wenzler

The variation of total solar irradiance (TSI) has been measured since 1978 and that of the spectral irradiance for an even shorter amount of time. Semi-empirical models are now available that reproduce over 80% of the measured irradiance…

太阳与恒星天体物理 · 物理学 2013-03-11 N. A. Krivova , S. K. Solanki , Y. C. Unruh

Herein I discuss and propose updated satellite composites of the total solar irradiance covering the period 1978-2008. The composites are compiled from measurements made with the three ACRIM experiments. Measurements from the NIMBUS7/ERB…

太阳与恒星天体物理 · 物理学 2010-05-31 Nicola Scafetta

We present a reconstruction of total solar irradiance since 1610 to the present based on variations of the surface distribution of the solar magnetic field. The latter is calculated from the historical record of the Group sunspot number…

天体物理学 · 物理学 2008-11-26 L. Balmaceda , N. A. Krivova , S. K. Solanki

Total and spectral solar irradiance are key parameters in the assessment of solar influence on changes in the Earth's climate. We present a reconstruction of daily solar irradiance obtained using the SATIRE-S model spanning 1974 to 2013…

太阳与恒星天体物理 · 物理学 2015-07-07 K. L. Yeo , N. A. Krivova , S. K. Solanki , K. H. Glassmeier

Context: The study of variations in total solar irradiance (TSI) is important for understanding how the Sun affects the Earth's climate. Aims: Full-disk continuum images and magnetograms are now available for three full solar cycles. We…

太阳与恒星天体物理 · 物理学 2015-06-04 W. T. Ball , Y. C. Unruh , N. A. Krivova , S. Solanki , T. Wenzler , D. J. Mortlock , A. H. Jaffe

Total solar irradiance variations, about 0.1% between solar activity maximum and minimum, are available from accurate satellite measurements since 1978 and thus do not provide useful information on longer-term secular trends. Recently,…

太阳与恒星天体物理 · 物理学 2012-05-23 S. Sello

Solar irradiance measurements are limited to the last few decades, requiring reconstructions to assess solar variability on longer timescales and its impact on Earth's climate. We present the first physics-based reconstruction of total…

太阳与恒星天体物理 · 物理学 2026-05-22 D. Temaj , N. A. Krivova , S. K. Solanki , I. G. Usoskin , T. Chatzistergos

The apparently unusual behaviour of the TSI during the most recent minimum of solar activity has been interpreted as evidence against solar surface magnetism as the main driver of the secular change in the TSI. We test claims that the…

太阳与恒星天体物理 · 物理学 2015-05-27 N. A. Krivova , S. K. Solanki , W. Schmutz

The total solar irradiance (TSI) varies on timescales of minute to centuries. On short timescales it varies due to the superposition of intensity fluctuations produced by turbulent convection and acoustic oscillations. On longer scale…

太阳与恒星天体物理 · 物理学 2022-10-12 V. Penza , F. Berrilli , L. Bertello , M. Cantoresi , S. Criscuoli , P. Giobbi

Total solar irradiance (TSI) has been monitored from space since 1978. The measurements show a prominent variability in phase with the solar cycle, as well as fluctuations on timescales shorter than a few days. However, the measurements…

太阳与恒星天体物理 · 物理学 2020-08-26 Theodosios Chatzistergos , Ilaria Ermolli , Fabrizio Giorgi , Natalie A. Krivova , Cosmin Constantin Puiu

Solar irradiance variations across various timescales, from minutes to centuries, represents a potential natural driver of past regional and global climate cold phases. To accurately assess the Sun's effect on climate, particularly during…

The current cycle minimum appears to be deeper and broader than recent cycle minima, and this minimum appears similar to the minima in the early 1900s. With the best-ever solar irradiance measurements from several different satellite…

太阳与恒星天体物理 · 物理学 2010-03-25 Thomas N. Woods

Herein we adopt a multi-scale dynamical spectral analysis technique to compare and study the dynamical evolution of the harmonic components of the overlapping ACRIMSAT/ACRIM3, SOHO/VIRGO and SORCE/TIM total solar irradiance (TSI) records…

综合物理 · 物理学 2013-11-28 Nicola Scafetta , Richard C. Willson

Solar irradiance models that assume solar irradiance variations to be due to changes in the solar surface magnetic flux have been successfully used to reconstruct total solar irradiance on rotational as well as cyclical and secular time…

太阳与恒星天体物理 · 物理学 2015-06-03 Yvonne C. Unruh , Will T. Ball , Natalie A. Krivova

The Sun is the main energy source to Earth, and understanding its variability is of direct relevance to climate studies. Measurements of total solar irradiance exist since 1978, but this is too short compared to climate-relevant time…

太阳与恒星天体物理 · 物理学 2023-10-17 Theodosios Chatzistergos , Natalie A. Krivova , Kok Leng Yeo

Variations of the solar UV irradiance are an important driver of chemical and physical processes in the Earth's upper atmosphere and may also influence global climate. Here we reconstruct solar UV irradiance in the range 115-400 nm over the…

太阳与恒星天体物理 · 物理学 2009-11-23 N. A. Krivova , S. K. Solanki , T. Wenzler , B. Podlipnik

Accurate information on long-term variations in solar irradiance, important for understanding the solar influence on Earth's climate, cannot be derived from direct irradiance measurements due to the comparatively short lifetimes of…

太阳与恒星天体物理 · 物理学 2025-04-23 Theodosios Chatzistergos , Natalie A. Krivova , Sami K. Solanki , Kok Leng Yeo

The correlation between solar irradiance and the 11-year solar activity cycle is evident in the body of measurements made from space, which extend over the past four decades. Models relating variation in solar irradiance to photospheric…

太阳与恒星天体物理 · 物理学 2015-07-07 K. L. Yeo , N. A. Krivova , S. K. Solanki

Measurements from the Solar Irradiance Monitor (SIM) onboard the SORCE mission indicate that solar spectral irradiance at Visible and IR wavelengths varies in counter phase with the solar activity cycle. The sign of these variations is not…

太阳与恒星天体物理 · 物理学 2015-06-19 Serena Criscuoli , Han Uitenbroek
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