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
Ensemble of MPI-ESM1-2-HR CMIP6 retrospective forecasts (hindcasts) without solar and ozone variability (i.e., set to the year 1850). The simulations are performed within the BMBF project "Solar contribution
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
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
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