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Recent oppositely directed trends in solar climate forcings and the global mean surface air temperature. II. Different reconstructions of the total solar irradiance variation and dependence on response time scale

Recent oppositely directed trends in solar climate forcings and the global mean surface air temperature. II. Different reconstructions of the total solar irradiance variation and dependence on response time scale
Recent oppositely directed trends in solar climate forcings and the global mean surface air temperature. II. Different reconstructions of the total solar irradiance variation and dependence on response time scale
We have previously placed the solar contribution to recent global warming in context using observations and without recourse to climate models. It was shown that all solar forcings of climate have declined since 1987. The present paper extends that analysis to include the effects of the various time constants with which the Earth's climate system might react to solar forcing. The solar input waveform over the past 100 years is defined using observed and inferred galactic cosmic ray fluxes, valid for either a direct effect of cosmic rays on climate or an effect via their known correlation with total solar irradiance (TSI), or for a combination of the two. The implications, and the relative merits, of the various TSI composite data series are discussed and independent tests reveal that the PMOD composite used in our previous paper is the most realistic. Use of the ACRIM composite, which shows a rise in TSI over recent decades, is shown to be inconsistent with most published evidence for solar influences on pre-industrial climate. The conclusions of our previous paper, that solar forcing has declined over the past 20 years while surface air temperatures have continued to rise, are shown to apply for the full range of potential time constants for the climate response to the variations in the solar forcings.
solar variability, climate change, solar-terrestrial physics
1364-5021
1367-1385
Lockwood, Mike
d4b01615-f1c3-4fef-9e54-afaa976c3584
Fröhlich, Claus
3e724e66-303d-403d-bdf3-fddfe1e68889
Lockwood, Mike
d4b01615-f1c3-4fef-9e54-afaa976c3584
Fröhlich, Claus
3e724e66-303d-403d-bdf3-fddfe1e68889

Lockwood, Mike and Fröhlich, Claus (2008) Recent oppositely directed trends in solar climate forcings and the global mean surface air temperature. II. Different reconstructions of the total solar irradiance variation and dependence on response time scale. Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences, 464 (2094), 1367-1385. (doi:10.1098/rspa.2007.0347).

Record type: Article

Abstract

We have previously placed the solar contribution to recent global warming in context using observations and without recourse to climate models. It was shown that all solar forcings of climate have declined since 1987. The present paper extends that analysis to include the effects of the various time constants with which the Earth's climate system might react to solar forcing. The solar input waveform over the past 100 years is defined using observed and inferred galactic cosmic ray fluxes, valid for either a direct effect of cosmic rays on climate or an effect via their known correlation with total solar irradiance (TSI), or for a combination of the two. The implications, and the relative merits, of the various TSI composite data series are discussed and independent tests reveal that the PMOD composite used in our previous paper is the most realistic. Use of the ACRIM composite, which shows a rise in TSI over recent decades, is shown to be inconsistent with most published evidence for solar influences on pre-industrial climate. The conclusions of our previous paper, that solar forcing has declined over the past 20 years while surface air temperatures have continued to rise, are shown to apply for the full range of potential time constants for the climate response to the variations in the solar forcings.

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More information

Published date: 8 June 2008
Keywords: solar variability, climate change, solar-terrestrial physics

Identifiers

Local EPrints ID: 146875
URI: http://eprints.soton.ac.uk/id/eprint/146875
ISSN: 1364-5021
PURE UUID: 2c70218d-7ed6-4ee9-b527-836237513ab9

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Date deposited: 22 Apr 2010 14:39
Last modified: 14 Mar 2024 00:57

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Author: Mike Lockwood
Author: Claus Fröhlich

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