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Journal ArticleDOI

The global signal of the 11-year solar cycle in the stratosphere: observations and models

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TLDR
In this paper, two general circulation models (GCMs) with coupled stratospheric chemistry are used to simulate the impact of changes in solar output, showing that the difference between solar maximum and solar minimum for temperature and ozone are generally smaller than observed.
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This article is published in Journal of Atmospheric and Solar-Terrestrial Physics.The article was published on 2002-01-01. It has received 79 citations till now. The article focuses on the topics: Solar minimum & Solar maximum.

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Citations
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Journal ArticleDOI

Dynamical response to the solar cycle

TL;DR: In this paper, the authors investigated the effect of the 11-year solar cycle on the stratopause region where solar ultraviolet heating is greatest and found that the most important variation in solar forcing longer than the diurnal cycle is the annual cycle.
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The effects of solar variability on the Earth's climate

TL;DR: Observational data and radiative forcing considerations and the results of energy-balance models and general circulation models suggest that the warming during the latter part of the 20th century cannot be ascribed entirely to solar effects, but chemical and dynamical processes in the middle atmosphere may act to amplify the solar impact.
References
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Journal ArticleDOI

The NCEP/NCAR 40-Year Reanalysis Project

TL;DR: The NCEP/NCAR 40-yr reanalysis uses a frozen state-of-the-art global data assimilation system and a database as complete as possible, except that the horizontal resolution is T62 (about 210 km) as discussed by the authors.
Journal ArticleDOI

The Impact of Solar Variability on Climate

TL;DR: A general circulation model that simulated changes in solar irradiance and stratospheric ozone was used to investigate the response of the atmosphere to the 11-year solar activity cycle as discussed by the authors.
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Solar cycle variability, ozone, and climate

TL;DR: The model reproduces many observed 11-year oscillations, including the relatively long record of geopotential height variations, and implies that these oscillations are likely driven, at least in part, by solar variability.
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Detection and parameterization of variations in solar mid- and near-ultraviolet radiation (200-400 nm)

TL;DR: In this paper, the authors used a newly developed UV sunspot darkening index and the Mg index facular proxy to replicate the rotational modulation detected in both the broadband Nimbus 7 filter data (275-360 nm and 300-410 nm) and in SOLSTICE 1-nm spectra from 200 to 400 nm.
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Realistic quasi‐biennial oscillations in a simulation of the global climate

TL;DR: In this paper, the effects of these missing waves are parametrized in a comprehensive numerical model of the atmosphere, and the simulation of the climate is improved by the generation of a realistic quasi-biennial oscillation in the stratosphere.
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