Welcome to the new CCMC website!

Please note that some pages may have moved during the migration. If you experience any issues with the new website, please reach out to gsfc-ccmc-support@lists.hq.nasa.gov.

Step 1: Generate a Registration Number for each Requested Run and select the Model.

Registration Number

The Registration Number is composed of your first name (GivenName), your last name (FamilyName), date (yyyymmdd),model type (GM - Global Magnetosphere, IT - Ionosphere/Thermosphere, SH -Solar/Heliosphere, PP - Postprocessing), and run identification number (RunNumber):
    GivenName_FamilyName_mmddyy_RunNumber,   e.g., Lutz_Rastaetter_20160101_PP_1.

At the present time you are allowed to make up to 5 different submissions on the the same date (mmddyy). For each new submission made on the same date you need to choose a new Run Number ("1", "2", "3", "4","5","6","7","8","9", or "10"). Multiple submissions made on the same date with the same Run Number will overwrite the previous submission. You can use this feature to resubmit the request on the same date. If you decide to cancel or modify your submission at later date, please contact the CCMC staff:

    e-mail: gsfc-dl-ccmc-ror@mail.nasa.gov

Please have registration numbers when making inquiries about your requests. You will need your registration number to view the results when the simulations have finished.

**You must agree to the CCMC DATA Collection Consent Agreement in order to submit a run**

Do you give your consent?
YES


First (Given) Name: (required)

Last (Family) Name: (required)

E-mail: (required)

Run Number:
Select a different Run Number if you have already requested any Post-Processing run today (unless you want to overwrite the request)


Title/Introduction

Key words

Post-Processing (PP) tools for Global Magnetosphere (GM) simulation:

AMPS

    AMPS (version as of 2016/02/02)
RECONX - Separator, Separatrix and Null Point Finder

    Glocer (version as of 2016/02/02)

CalcDeltaB - CCMC implementation of magnetic perturbation calculation

    version as of April 2018

Post-Processing (PP) tools for Local Physics (LP) simulation:

Distribution function for PIC model run

    Local Physics (LP) run name (search for runs; VPIC only, PIC-Hesse coming soon; P3D and PAMHD runs are not supported yet)