Step 1: 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_IT_1.

WORK OR SCHOOL EMAILhow to contact you

Enter a valid work or school email address

FIRST NAME (GIVEN)*your given name

Enter your given name

LAST NAME (FAMILY)*your family name

Enter your family name

RUN NUMBER* max of 4 runs per day

choose run number for today 12345678910 Unless you want to overwrite it

KEYWORD/S* helps to sort and search the results of simulations

Enter a keyword

Step 2: SELECT MODEL VERSION

TIE-GCM version

2.0 2.5 Note: not all model parameters supported by all versions of the model

Step 3: SET THE SIMULATION TIME INTERVAL

At high latitudes Heelis electric potential model is used with time dependent input parameters.
Allowed interval (in which input data are available):
  Heelis: 1960/001 - 2023/120.
  Weimer: 1996/001 - 2023/120.

OUTPUT FREQUENCY fixed

START TIME fixed

YEAR* 1960 - 2023

choose year at the start of the run2023202220212020201920182017201620152014201320122011201020092008200720062005200420032002200120001999199819971996199519941993199219911990198919881987198619851984198319821981198019791978197719761975197419731972197119701969196819671966196519641963196219611960

DAY OF THE YEAR* 001 - 366leap year: 366 days
e.g. 2020, 2016, 2012

choose doy at the start of the run123456789101112131415161718192021222324252627282930313233343536373839404142434445464748495051525354555657585960616263646566676869707172737475767778798081828384858687888990919293949596979899100101102103104105106107108109110111112113114115116117118119120121122123124125126127128129130131132133134135136137138139140141142143144145146147148149150151152153154155156157158159160161162163164165166167168169170171172173174175176177178179180181182183184185186187188189190191192193194195196197198199200201202203204205206207208209210211212213214215216217218219220221222223224225226227228229230231232233234235236237238239240241242243244245246247248249250251252253254255256257258259260261262263264265266267268269270271272273274275276277278279280281282283284285286287288289290291292293294295296297298299300301302303304305306307308309310311312313314315316317318319320321322323324325326327328329330331332333334335336337338339340341342343344345346347348349350351352353354355356357358359360361362363364365366

RUN DURATION* up to 30 days

choose run duration 123456789101112131415161718192021222324252627282930

Step 4: CHOOSE THE RUN TYPE AND ELECTRIC POTENTIAL MODEL AT HIGH LATITUDES

EVENT with WEIMER2005

EVENT with HEELIS ET AL.1982

MODEL with WEIMER2005Please select values for: F107, Bx, By, Bz, Vx and SW.den

MODEL with HEELIS ET AL.1982Please select values for: F107 and Kp

f107

choose f107 (range 70 -200) 707172737475767778798081828384858687888990919293949596979899100101102103104105106107108109110111112113114115116117118119120121122123124125126127128129130131132133134135136137138139140141142143144145146147148149150151152153154155156157158159160161162163164165166167168169170171172173174175176177178179180181182183184185186187188189190191192193194195196197198199200 10.7cm solar radio flux

Kp

choose Kp (range 0 - 9) 0123456789 Kp index

Bx nT

interplanetary magnetic field

By nT-50 to 50

Bz nT-50 to 50

Vx300 to 1000

solar wind speed in km/s

SW.den1 to 30

solar wind density in #/cm³

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.

JUSTIFICATIONbrief description