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Midlatitude atmospheric OH response to the most recent 11-y solar cycleCan Measurements of the Near-Infrared Solar Spectral Irradiance be Reconciled? A New Ground-Based Assessment Between 4,000 and 10,000 cm−1CMIP5 historical simulations (1850-2012) with GISS ModelE2Solar signals in CMIP-5 simulations: the ozone responseHigh solar cycle spectral variations inconsistent with stratospheric ozone observationsVariability of Sun-like stars: reproducing observed photometric trendsImpact of a potential 21st century “grand solar minimum” on surface temperatures and stratospheric ozoneCould a future “Grand Solar Minimum” like the Maunder Minimum stop global warming?Solar irradiance variabilityUV solar irradiance in observations and the NRLSSI and SATIRE-S modelsAssessing the relationship between spectral solar irradiance and stratospheric ozone using Bayesian inference
P2860
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P2860
description
im April 2012 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована у квітні 2012
@uk
name
How Does the Sun’s Spectrum Vary?
@en
How Does the Sun’s Spectrum Vary?
@nl
type
label
How Does the Sun’s Spectrum Vary?
@en
How Does the Sun’s Spectrum Vary?
@nl
prefLabel
How Does the Sun’s Spectrum Vary?
@en
How Does the Sun’s Spectrum Vary?
@nl
P1433
P1476
How Does the Sun’s Spectrum Vary?
@en
P2093
Judith L. Lean
Matthew T. DeLand
P304
P356
10.1175/JCLI-D-11-00571.1
P407
P577
2012-04-01T00:00:00Z