Abstract
Measurements of solar irradiance have revealed variations at all the sampled time scales (ranging from minutes to the length of the solar cycle). One important task of models is to identify the causes of the observed (total and spectral) irradiance variations. Another major aim is to reconstruct irradiance over time scales longer than sampled by direct measurements in order to consider if and to what extent solar irradiance variations may be responsible for global climate change. Here, we describe recent efforts to model solar irradiance over the current and the previous two solar cycles. These irradiance models are remarkably successful in reproducing the observed total and spectral irradiance, although further improvements are still possible.
| Original language | English |
|---|---|
| Pages (from-to) | 376-383 |
| Number of pages | 8 |
| Journal | Advances in Space Research |
| Volume | 35 |
| Issue number | 3 |
| DOIs | |
| Publication status | Published - 2005 |
UN SDGs
This output contributes to the following UN Sustainable Development Goals (SDGs)
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SDG 13 Climate Action
Keywords
- Solar activity
- Solar irradiance
- Solar magnetic field
- Solar-terrestrial relations
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