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SOLCHECK will significantly advance the understanding and quantification of the solar contribution to past, present, and future climate evolution in the Northern Hemisphere on decadal to centennial timescales.
Ensemble of MPI-ESM1-2-HR CMIP6 historical simulations without solar and ozone variability (i.e., set to the year 1850). The simulations are performed within the BMBF project "Solar contribution to climate
Ensemble of MPI-ESM1-2-HR CMIP6 historical simulations with low-pass filtered solar and ozone variability (i.e., using a 33-years running-mean). The simulations are performed within the BMBF project "Solar
The ensemble consists of 8 ensemble members (r1-r8). The experimental setup is identical to the MPI-ESM1-2-HR historical CMIP6 simulations except for the solar and ozone variability (i.e., here low-pass
The ensemble consists of 8 ensemble members (r1-r8). The experimental setup is identical to the MPI-ESM1-2-HR historical CMIP6 simulations except for the solar and ozone variability (i.e., here low-pass
The ensemble consists of 8 ensemble members (r1-r8). The experimental setup is identical to the MPI-ESM1-2-HR historical CMIP6 simulations except for the solar and ozone variability (i.e., here low-pass
The ensemble consists of 8 ensemble members (r1-r8). The experimental setup is identical to the MPI-ESM1-2-HR historical CMIP6 simulations except for the solar and ozone variability (i.e., here low-pass
The ensemble consists of 8 ensemble members (r1-r8). The experimental setup is identical to the MPI-ESM1-2-HR historical CMIP6 simulations except for the solar and ozone variability (i.e., here low-pass
The ensemble consists of 8 ensemble members (r1-r8). The experimental setup is identical to the MPI-ESM1-2-HR historical CMIP6 simulations except for the solar and ozone variability (i.e., here low-pass
The ensemble consists of 8 ensemble members (r1-r8). The experimental setup is identical to the MPI-ESM1-2-HR historical CMIP6 simulations except for the solar and ozone variability (i.e., here low-pass
The ensemble consists of 8 ensemble members (r1-r8). The experimental setup is identical to the MPI-ESM1-2-HR historical CMIP6 simulations except for the solar and ozone variability (i.e., here low-pass
The ensemble consists of 8 ensemble members (r2, r4, r5, r6, r7, r8, r9, r10). The ensemble members r1 and r3 were incomplete and hence removed. The experimental setup is identical to the MPI-ESM1-2-HR
The ensemble consists of 8 ensemble members (r2, r4, r5, r6, r7, r8, r9, r10). The ensemble members r1 and r3 were incomplete and hence removed. The experimental setup is identical to the MPI-ESM1-2-HR
The ensemble consists of 8 ensemble members (r2, r4, r5, r6, r7, r8, r9, r10). The ensemble members r1 and r3 were incomplete and hence removed. The experimental setup is identical to the MPI-ESM1-2-HR
The ensemble consists of 8 ensemble members (r2, r4, r5, r6, r7, r8, r9, r10). The ensemble members r1 and r3 were incomplete and hence removed. The experimental setup is identical to the MPI-ESM1-2-HR