Solar irradiance during the last 1200 years based on cosmogenic nuclides

By E. Bard, G. Raisbeck, Françise Yiou, J. Jouzel. 2000

589 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/b7261b7f264169d89a1d3107392477fe2b34ddce

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. S. Solanki
2. M. Lockwood
3. N. Krivova
4. I. Usoskin
5. C. Fröhlich
6. L. Vieira
7. J. Lean
8. F. Joos

In Atmospheric Science

1. M. Lockwood
2. I. Usoskin
3. F. Joos
4. S. Solanki
5. Jochem Marotzke
6. N. Krivova
7. Johann Jungclaus
8. A. Timmermann

In Molecular Biology

1. I. Usoskin
2. M. Lockwood
3. S. Solanki
4. N. Krivova
5. F. Joos
6. J. Lean
7. L. Vieira
8. M. Vonmoos

Citations in the corpus

• Solar activity during the last 1000 yr inferred from radionuclide records (2007, background): “The differences between the 10Be records from Greenland and Antarctica for the period after 1950 AD have led to strongly differing conclusions about solar activity in the past (Bard et al., 2000; Usoskin et al., 2003).”
• Climate change and solar variability: what's new under the sun? (2006, background): “The black line is based on sunspots [10] and the grey line on cosmogenic nuclides [45].”
• What caused Earths temperature variations during the last 800,000 years? Data-based evidences on radiative forcing and constraints on climate sensitivity (2009, background): “…reconstructions, total irradiance during the last millenniumwas estimated to be 0.15–0.65% (radiative forcing about "0.36 to "1.55 Wm"2) below the present day-mean (e.g. Bard et al., 2000), whereas other work suggest a reduction of only about 0.1% in solar energy output (e.g. Wang et al., 2005).”
• A reconstruction of radiocarbon production and total solar irradiance from the Holocene 14 C and CO 2 records: implications of data and model uncertainties (2013, unknown): “This is also reflected in the large spread in past and recent reconstructions of TSI variability on multi-decadal to centennial timescales (e.g.Bard et al., 2000; Lean, 2000; Wang et al., 2005; Steinhilber et al., 2009; Steinhilber et al., 2012; Shapiro et al., 2011; Schrijver et al., 2011).”
• El Niño as a mediator of the solar influence on climate (2007, methodology): “We therefore apply the linear scaling of Bard et al. [2000] : The reference scale PA3210 EMILE-GEAY ET AL.: SOLAR-MODULATED ENSO”
• Evidence for solar forcing on the Indian monsoon during the last millennium (2002, methodology): “Recently, the TSI reconstruction has been extended to 843 AD based on a quantitative estimate of common variations in the production rates of 14C and 10Be [11].”
• The influence of volcanic, solar and CO2 forcing on the temperatures in the Dalton Minimum (1790–1830): a model study (2005, methodology): “The difference in the total solar irradiance between present values and the LMM is 0.30% (with a peak change of 0.35%), which is well within the range of other different solar reconstructions (cf. Bard et al. 2000 ).”
• Solar radiative output and its variability: evidence and mechanisms (2004, background): “…variability are magnetic active regions near the surface of the sun, cosmogenic isotopes variations occur because the extended solar atmosphere in interplanetary space modulates the ux of galactic cosmic rays that reaches the Earth's atmosphere (Bard et al., 2000; Webber and Higbie, 2003).”
• SOLAR INFLUENCES ON CLIMATE (2010, unknown): “…sunspot maps [Lockwood, 2004]; p mode amplitudes (estimated from R) [Bhatnagar et al., 2002]; cosmogenic isotopes deposited in terrestrial reservoirs [Bard et al., 2000; Steinhilber et al., 2009]; and the open magnetic flux of the Sun derived from geomagnetic activity data [Lockwood, 2002].”
• Large variations in Holocene solar activity: Constraints from 10Be in the Greenland Ice Core Project ice core (2006, background): “reconstructions of solar activity for the last millennium or the entire Holocene are based on them, so in terms of total solar irradiance [Bard et al., 2000] and sunspots [Solanki et al.”
• An Antarctic view of Beryllium-10 and solar activity for the past millennium (2011, background): “In this regard, the central Antarctic Plateau combines two advantages: (i) (10)Be deposition is very sensitive to solar activity and much less so to geomagnetism, (ii) and (10)Be deposition is arguably more stable than anywhere else (see discussion in Bard et al. 1997). We discuss both points in Sec”
• Evidence for solar forcing of sea-surface temperature on the North Icelandic Shelf during the late Holocene (2005, methodology): “Accordingly, daily insolation values for 678N at summer solstice (after Berger, 1978) were calculated by using the irradiance values (Bard et al., 2000) as input.”
• Solar Influence on Global and Regional Climates (2012, background): “The abundances of these isotopes are routinely used in paleoclimate studies as a proxy indicator of solar irradiance (Bard et al. 2000).”
• Climate and carbon-cycle variability over the last millennium (2010, methodology): “The TSI series used for the E2 ensemble is based on another compilation of 14C and10Be production rates (Bard et al., 2000) from which an annual data set was derived (Ammann et al.”
• Are there connections between the Earth's magnetic field and climate? (2007, background): “[26]; (3) Greenhouse gases; and (4) Tropospheric aerosols (figure adapted from Crowley [25]).”
• Internal and forced climate variability during the last millennium: a model-data comparison using ensemble simulations (2005, background): “The evolution of solar irradiance follows the reconstruction of Lean et al. (1995) extended back in time by Bard et al. (2000) .”