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IMPTAM Submission Page

Request an IMPTAM Model Run

Please complete the form below. * Indicates a required field.


GENERATE YOUR REQUEST

Your run results will be published online under your Run Registration Number (FirstName_LastName_MMDDYY_ModelType_RunNumber) e.g. John_Smith_032511_IM_1.

Submissions that do not provide a real name of the submitter will be automatically rejected.

**You must agree to the CCMC Data Policy in order to submit a run**

Do you give your consent?
YES


Enter a valid work or school email address
Enter your given name
Enter your family name
Enter run number you have not used today already
Enter keywords
Enter NSF or NASA grant number
Step 2: Dates Range
Select or type a valid date and time in the suggested format, e.g. 2016/01/15 09:10:00
Select or type a valid date and time in the suggested format, e.g. 2016/01/15 09:10:00
Step 3: Select Output

Species

Satellites

The following satellite data is available when you select Electrons or Protons:

  • Geostationary (GOES15), orbit (time, xgsm [RE], ygsm [RE], zgsm [RE])

    • Electrons:
      • Energy [keV] vs. UT [hour] spectrograms of fluxes in [cm-2 s-1 sr-1 keV-1] in energy range of 1-300 keV
      • Pitch angle [deg] vs. UT [hour] spectrograms of fluxes in [cm-2 s-1 sr-1 keV-1] for energies of 10 keV, 50 keV, and 100 keV
    • Protons:
      • Energy [keV] vs. UT [hour] spectrograms of fluxes in [cm-2 s-1 sr-1 keV-1] in energy range of 1-300 keV
      • Pitch angle [deg] vs. UT [hour] spectrograms of fluxes in [cm-2 s-1 sr-1 keV-1] for energies of 10 keV, 50 keV, and 100 keV

  • MEO, orbit (time, xgsm [RE], ygsm [RE], zgsm [RE])

    • Electrons:
      • Energy [keV] vs. UT [hour] spectrograms of fluxes in [cm-2 s-1 sr-1 keV-1] in energy range of 1-300 keV
      • Pitch angle [deg] vs. UT [hour] spectrograms of fluxes in [cm-2 s-1 sr-1 keV-1] for energies of 10 keV, 50 keV, and 100 keV
    • Protons:
      • Energy [keV] vs. UT [hour] spectrograms of fluxes in [cm-2 s-1 sr-1 keV-1] in energy range of 1-300 keV
      • Pitch angle [deg] vs. UT [hour] spectrograms of fluxes in [cm-2 s-1 sr-1 keV-1] for energies of 10 keV, 50 keV, and 100 keV

  • Van Allen Probe A (VAP), orbit (time, xgsm [RE], ygsm [RE], zgsm [RE])

    • Electrons:
      • Energy [keV] vs. UT [hour] spectrograms of fluxes in [cm-2 s-1 sr-1 keV-1] in energy range of 1-300 keV
      • Pitch angle [deg] vs. UT [hour] spectrograms of fluxes in [cm-2 s-1 sr-1 keV-1] for energies of 10 keV, 50 keV, and 100 keV
    • Protons:
      • Energy [keV] vs. UT [hour] spectrograms of fluxes in [cm-2 s-1 sr-1 keV-1] in energy range of 1-300 keV
      • Pitch angle [deg] vs. UT [hour] spectrograms of fluxes in [cm-2 s-1 sr-1 keV-1] for energies of 10 keV, 50 keV, and 100 keV
OPTIONAL: SPECIAL REQUEST

ONLY if you require a customized simulation setup not provided by the standard submission options. Unlike the standard runs that are automatically processed, special requests are reviewed and manually modified by the CCMC staff. Please note that special requests are reviewed and manually modified by the CCMC staff and are executed only if resources are available.