Runs on Request for Solar Models

Runs on Request Procedures

To initiate the request submission click on "Submit Request" button below.
Submission consists of the following steps:

Step 1: Registration

• You will be required to provide your first name, last name, telephone number, and e-mail.
• You will need your registration number when making inquiries about your requests and to view the results when the simulations have finished.

Step 2: Choose the model to run, the science question (a modeled run or simulation of real event) and the boundary condition type (time-independent/time-dependent).

At present time the only choice is MAS model with time-independent photospheric boundary conditions (uniform fixed photospheric density and temperature, and photospheric radial magnetic field distribution averaged over the selelcted Carrington rotation). More choices are comming soon.

Step 3: Set the simulation time interval

• Select Carrington rotation and specify the duration of the run.
• For MAS model you can also generate input file for modeled run. You will be given a choice to download Fortran code for generation of user-defined magnetograms. Later you can upload your magnetogram. You can view a sample run with user-generated input file.

Steps 4-6: Set the input parameters (simulation grid, photospheric boundary conditions, numerical simulation parameters, output frequency).

• Provide key word that will help to sort and search the results of simulations via our web-based interface (required). Provide brief comments about the run that may be helpful to other visitors.
• Here you have an opportunity to add comments and suggestions about this Web interface and describe additional desirable options of the output data analysis (not required).

The results of the run you requested will be made available to the general research community via our web-based interface. Any keywords and description you include will help our other visitors to better understand your simulation.

Submit Request

Simulations Results

These runs are provided for the space science community. If results from these runs are used in a scientific publication, we request that the authors acknowledge the CCMC and the originators of the computational model. View Simulation Results