4.3 Article

Edge adapted wavelets, solar magnetic activity, and climate change

Journal

ASTROPHYSICS AND SPACE SCIENCE
Volume 326, Issue 2, Pages 181-189

Publisher

SPRINGER
DOI: 10.1007/s10509-009-0249-6

Keywords

Wavelet; Sunspot; Solar activity; Climate change

Funding

  1. SIDC-team
  2. World Data Center for the Sunspot Index, Royal Observatory of Belgium
  3. Monthly Report on the International Sunspot Numbe
  4. Solar Data Services
  5. National Geophysical Data Center
  6. National Oceanic and Atmospheric Administration, USa
  7. Global Glacier Length Temperature Reconstruction
  8. IGBP PAGES/World Data Center for Paleoclimatology
  9. Data Contribution Series [2005-059]
  10. NOAA/NCDC Paleoclimatology Program, Boulder CO, USA
  11. Central England Temperature
  12. Met Office Hadley Centre for Climate Change

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The continuous wavelet transform is adapted to account for signal truncation through renormalization and by modifying the shape of the analyzing window. Comparison is made of the instant, integrated, and mean wavelet power with previous algorithms. The edge adapted and renormalized admissible wavelet transforms are used to estimate the level of solar magnetic activity from the sunspot record. The solar activity is compared to Oerlemans' temperature reconstruction and to the Central England Temperature record. A correlation is seen for years between 1610 and 1990, followed by a strong deviation as the recently observed temperature increases.

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