Sun Climate Climate and Societal Impacts of Solar Variations - PowerPoint PPT Presentation

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Sun Climate Climate and Societal Impacts of Solar Variations

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Title: Sun Climate Climate and Societal Impacts of Solar Variations


1
Sun Climate Climate and Societal Impacts of
Solar Variations
  • Caspar Ammann, NCAR

2
Overview
  • Climatic challenges and their expected societal
    impacts
  • Could the continuous Sun-Climate link provide
    important insight?
  • Pathways of solar impact on Earths Climate and
    Society
  • What do we know about past solar impacts on
    climate / society?
  • Potentials and pitfalls, incl. The Little Ice
    Age
  • Medieval Climate Anomaly
  • What did climate look like, what was unusual?
  • Could it have been solar driven?
  • Model challenges
  • What is the signal of the 11-year cycle, how is
    it simulated?
  • What are the requirements for climate models and
    solar forcing data?
  • Summary Role of Sun for Climate Change impact
    research

3
Climate Change Challenges Sea Level
Satellite Altimetry / Surface observations More
rapid ice loss in Antarctica than
anticipatedPaleo records and Models Loss of
sections of W-Antarctica in previous Interglacials
4
Global Water Issues
5
Scientific Challenges AR5
( 1 ) CLIMATE SENSITIVITY Long, multi-century
projections to study Carbon Cycle
Feedbacks, Sea Level Change
  • ( 2 ) REGIONAL DYNAMICS Very high-res
    simulations of the next 20-30 years for
    regional prediction

6
Lessons from the Sun?
  • Eddy 1976 Sun Climate link

7
Pathways of solar impact on Climate
  • Direct radiative influence of total energy
    change
  • Indirect radiative effects through spectral
    variations
  • Indirect effects through Atmospheric Dynamics
    and possibly change in coupled variability

8
Direct radiative effects
9
Indirect radiative effects through spectral
changes Ozone
MgII
Temp
Strat O3
Tot. O3
Marsh et al. 2008 - WACCM
Hood 1997 Observations (de-seasonalized)
10
Solar Signal in NCEP/NCAR-Reanalysis Data
All years
QBO-E
Important imprint on anatural Mode of
Variability and Weather-noise NAO/AO
QBO-W
Geopot. Height Correlation Labitzke et al., 2006
11
What data do we have about past effects of the
Sun on Climate and Society?
  • Tree-Rings as climate indicators
  • Two examples of identified solar impact
  • Dangerous potential pitfalls

12
What are tree rings?
13
How do we know the date so precisely?
14
Effect of High Solar Activity on the Western
Drought?Apparently consistent Short- and
Long-term Response
Late Medieval High Solar?
22-yr Drought Cycle back to AD 800
Cook et al. 2004
15
Altai Mountains Ice Core Data
Ice Core Data (Schwikovski 2009)
16
Hidden Dangers Superposition Sun and Volcanoes
Solar
Volcanic
17
Medieval Climate Anomaly
  • What did climate look like?
  • Could it have been solar driven?

18
Medieval Time Sparse record
  • 1000 AD
  • 1500 AD
  • 1750 AD

19
Vikings in Greenland / N-America
Settlements in Greenland and NE North America
20
North America Mega Droughts
  • Solar related?
  • What other factorcould have suchlong timescales?

McDonald 2008
21
Effect of High Solar Activity on the Pacific
Calibration 11-yr Cycle Signal (only solar max)
SST anomalies (1856-2004)
Precip. anomalies
Van Loon et al. 2007
22
Solar Signal?(decadal/centennial?)
Solar effects in the Pacific Dynamics?
Volcanic effect(interannual)
Cobb et al., 2002
Adams et al., 2003
23
C-Z Model with full solar and volcanic forcing
Low-freq. Solar, high-freq. Volcanic
Ensemble mean Nino3 (100 realizations of CZ model)
Palymra coral isotopes (standardized to have same
mean and standard deviation as Nino3 composite
series)
40 year smooth
Mann et al., 2003
24
NCAR CCSM 3.0
IPCC AR4 Models Surface Temperatures Solar
11-year Cycle Max - Climatology
GFDL 2.1
GISS e_h
  • MICRO med-res

Source Van Loon, Meehl, Arblaster
25
Pacific SST as imposed driverWave pattern not
quite right far field
26
Challenges for Models
27
New Solar Module for Climate Studies for CCSM4
and WACCM
  • Goals of new implementation
  • Unified and consistent Solar input for CAM and
    WACCM
  • Flexible module to accommodate various solar
    specifications path for future replacement of
    current data input by physical model of the Sun
  • Independence from Radiative Transfer code base
  • Realistic solar variability representation
    through unrestricted spectral and temporal
    resolution of (CAM4 / WACCM)
  • Consistent information for radiative transfer
    and photolysis (WACCM)
  • Improved accuracy in new radiative transfer code
    of CAM4 (RRTMG)
  • Currently available data
  • Judith Lean TSI for 1610-2008
  • Judith Lean spectral data (1nm resolution) for
    1610-2008
  • New definitions developed by CCSM and WACCM
    (alphabetically) C. Ammann, W. Collins, A.
    Conley, B. Eaton, J.F Lamarque, D. Marsh, F. Vitt

28
Radiation Package (RRTMG or CAMRT)
Photolysis Package
Scale Factors on each band
Photon Fluxes
Solar Variability Coupler
Eventually Physical Solar Model
Flux on Radiation and Photolysis Boundaries
Spectrally Resolved Flux
File Data TSI Or Time Evolving Spectrum
Solar Specification
29
11 Year Solar Cycle in Atmosphere
Van Loon Shea., 1999
Coughlin Tung, 2004
30
Observations vs Model (even WACCM)
EMD NCEP EMD WACCM (incl ozone)
31
New Solar Time Series for 20th Century Is it good
enough for regional prediction?
Changes AR5 from AR4 (1) Smaller Trend!
(2) New TSI Level
32
Prediction Future Regional Moisture
Africa / Sahel Huge Uncertainty
US-Southwest Predictions Mega Drought
Drought and Heat Waves
20th century
21st century
Seager et al. 2007
33
Summary I
  • Solar irradiance variability has some, but small
    impact on the global mean temperature
  • Indirect effects through spectral radiation and
    its modulation of the upper and middle atmosphere
    might be very important for a correct dynamical
    response to solar forcing
  • Climate models need to be tested for minimal
    requirements to properly represent full
    atmospheric response that guides climate
  • How important is high-temporal freq. variation?
  • Progress is being made, but we are not there yet

34
Summary II
  • There is a need for a solid full atmospheric data
    assimilation product that allows for the
    identification of the 11-year solar cycle
  • Surface records need to be analyzed for
    systematic/continuous solar impact
  • Spectral solar irradiance data is needed that are
    linked to solar activity (11yr, Maunder-type)
  • Define benchmark-type experiments for GCMs on
    decadal to century scale solar impact to test
    their ability to reproduce regional response

35
THANK YOU !
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