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WGCM Meeting, Dubrovnik, 18-20 October 2015 Solar Forcing for CMIP6 Katja Matthes 1,2 and Bernd Funke 3 1 GEOMAR Helmholtz Centre for Ocean Research Kiel, Germany 2 Christian-Albrechts Universität zu Kiel, Kiel, Germany 3 Instituto de Astrofísica de Andalucía, CSIC, Granada, Spain
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Solar Forcing for CMIP6

Oct 04, 2021

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Page 1: Solar Forcing for CMIP6

WGCM Meeting, Dubrovnik, 18-20 October 2015  

Solar Forcing for CMIP6

Katja Matthes1,2 and Bernd Funke3

1GEOMAR Helmholtz Centre for Ocean Research Kiel, Germany 2Christian-Albrechts Universität zu Kiel, Kiel, Germany

3Instituto de Astrofísica de Andalucía, CSIC, Granada, Spain

Page 2: Solar Forcing for CMIP6

Overview

•  New reference SSI/TSI (and particle) forcing •  Future solar (SSI and particle) forcing

•  Final comments (solar forcing in PI control, solar ozone forcing)

2

Page 3: Solar Forcing for CMIP6

Relative Contribution to TSI

New SSI Reference!

-100

-50

0

50

100

150

200

6 S

SI

/ 6

TS

I [in

per

cent

]

200-400 400-700 700-1000 1000-2430

NR

LSS

IS

ATIR

EC

OS

IO

AR

SC

IAM

AC

HY

SO

RC

E

SU

SIM

WR

-2002

SO

RC

E reanalysis

NRLSSISATIRECOSIOARSCIAMACHYSORCE

WR-2002SUSIM

SORCE reanalysis

Ermolli, Matthes, Dudok de Witt et al., ACP (2013)

NRLSSI1 = standard so far (CMIP5, CCMVal, CCMI)

merged SATIRE+ NRLSSI2 = new reference data set

Page 4: Solar Forcing for CMIP6

0.1

1

10

100

Pre

ssu

re (

hP

a)

GEOSCCM NRLSSIGEOSCCM SORCEIC2D NRLSSIIC2D SORCEEMAC−FUB NRLSSIEMAC−FUB SORCEWACCM NRLSSIWACCM SORCEWACCM* NRLSSIECHAM6 NRLSSIHadGEM3 SORCEMMM NRLSSIMMM SORCE

−0.6 −0.4 −0.2 0 0.2 0.4 0.6

20

25

30

35

40

45

50

55

60

Heig

ht

(km

)

Shortwave Heating Rate

Stronger SSI forcing leads to stronger SW HR and temperature response!

SSI Impact on Atmospheric Response

Temperature

Ermolli, Matthes, Dudok de Witt et al., ACP (2013)

Page 5: Solar Forcing for CMIP6

New TSI Reference Value

5  

New TSI value 1360.8 ± 0.5 W m−2

Old TSI value 1365.4 ± 1.3 W m−2 (Kopp and Lean, 2011; Ermolli et al., 2013)

Courtesy T. Dudok de Wit (2015)

Page 6: Solar Forcing for CMIP6

New CMIP6 Reference Dataset

6  

1850 1900 1950 2000 2050 2100

CMIP6 solar forcing: one netcdf file SSI, TSI, F10.7cm, kp, ap, GCR, protons daily resolution, 1850-2300, 2 scenarios (ref, extreme min)

particle forcing: auroral electrons, solar protons, galactic cosmic rays

radiative forcing: TSI, SSI, F10.7cm

Page 7: Solar Forcing for CMIP6

7  

Two Future Scenarios

Reference future scenario  

Extreme Maunder Minimum future scenario  

Courtesy T. Dudok de Wit (2015)

Page 8: Solar Forcing for CMIP6

TSI: NRLSSI (ext=red, ref=black), SATIRE (ext=blue)

1 Jan1850

1 Jan1978

1 Jan2106

1 Jan2234

1359.5

1360.0

1360.5

1361.0

1361.5

1362.0

W/m

2

8  

Two Future Scenarios

Reference future scenario  

Extreme Maunder Minimum future scenario  

1850 1980 2100 2300

Page 9: Solar Forcing for CMIP6

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CMIP6 Solar Forcing

Current status CMIP6 solar forcing dataset: Option1: Reconstruction based on empirical scaling (sunspot number – solar modulation potential) (ready, grey curve above) Option2: Merged SSI/TSI dataset from NRLSSI2 and SATIRE-S models

(SATIRE-S ready, NRLSSI2 almost)

CMIP5  

CMIP6  

SATIRE-TS  

NRLSSI2  

Page 10: Solar Forcing for CMIP6

Summary

•  New reference SSI/TSI (+particle forcing) dataset ready by January 1st 2016 (1nm, daily resolution, 1850-2300, one netcdf file)

•  Will be validated in lbl and climate model simulations

(part of CMIP6 solar forcing special issue)

10  

Page 11: Solar Forcing for CMIP6

Final Remarks

•  Solar forcing for PI control experiment:

²  One constant value for TSI and SSI spectrum representative for 1850 solar cycle mean conditions

²  Optional: second PI control with solar cycle

variability but no long-term trend included

•  Solar ozone forcing timeseries is coordinated with CCMI ozone dataset (M. Hegglin)

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