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      Production of cosmogenic isotopes7Be,10Be,14C,22Na, and36Cl in the atmosphere: Altitudinal profiles of yield functions : COSMOGENIC ISOTOPES IN THE ATMOSPHERE

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          NRLMSISE-00 empirical model of the atmosphere: Statistical comparisons and scientific issues

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            Timing and climate forcing of volcanic eruptions for the past 2,500 years.

            Volcanic eruptions contribute to climate variability, but quantifying these contributions has been limited by inconsistencies in the timing of atmospheric volcanic aerosol loading determined from ice cores and subsequent cooling from climate proxies such as tree rings. Here we resolve these inconsistencies and show that large eruptions in the tropics and high latitudes were primary drivers of interannual-to-decadal temperature variability in the Northern Hemisphere during the past 2,500 years. Our results are based on new records of atmospheric aerosol loading developed from high-resolution, multi-parameter measurements from an array of Greenland and Antarctic ice cores as well as distinctive age markers to constrain chronologies. Overall, cooling was proportional to the magnitude of volcanic forcing and persisted for up to ten years after some of the largest eruptive episodes. Our revised timescale more firmly implicates volcanic eruptions as catalysts in the major sixth-century pandemics, famines, and socioeconomic disruptions in Eurasia and Mesoamerica while allowing multi-millennium quantification of climate response to volcanic forcing.
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              Unusual activity of the Sun during recent decades compared to the previous 11,000 years.

              Direct observations of sunspot numbers are available for the past four centuries, but longer time series are required, for example, for the identification of a possible solar influence on climate and for testing models of the solar dynamo. Here we report a reconstruction of the sunspot number covering the past 11,400 years, based on dendrochronologically dated radiocarbon concentrations. We combine physics-based models for each of the processes connecting the radiocarbon concentration with sunspot number. According to our reconstruction, the level of solar activity during the past 70 years is exceptional, and the previous period of equally high activity occurred more than 8,000 years ago. We find that during the past 11,400 years the Sun spent only of the order of 10% of the time at a similarly high level of magnetic activity and almost all of the earlier high-activity periods were shorter than the present episode. Although the rarity of the current episode of high average sunspot numbers may indicate that the Sun has contributed to the unusual climate change during the twentieth century, we point out that solar variability is unlikely to have been the dominant cause of the strong warming during the past three decades.
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                Author and article information

                Journal
                Journal of Geophysical Research: Atmospheres
                J. Geophys. Res. Atmos.
                Wiley
                2169897X
                July 16 2016
                July 16 2016
                July 12 2016
                : 121
                : 13
                : 8125-8136
                Affiliations
                [1 ]Space Climate group; University of Oulu; Finland
                [2 ]Ioffe Physical-Technical Institute of Russian Academy of Sciences; St. Petersburg Russia
                [3 ]Sodankylä Geophysical Observatory (Oulu unit); University of Oulu; Finland
                Article
                10.1002/2016JD025034
                9984aeb7-ac68-4778-8280-95342022488b
                © 2016

                http://doi.wiley.com/10.1002/tdm_license_1.1

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