The Coupled Magnetosphere-Ionosphere-Thermosphere (CMIT) model is comprised of three models:
The three models that comprise CMIT exchange the following variables at the appropriate boundary conditions:
Variable |
Computed by |
Sent to |
|
---|---|---|---|
current |
LFM |
MIX |
|
density |
LFM |
MIX |
|
soundSpeed |
LFM |
MIX |
|
|
|
|
|
Potential |
MIX |
LFM & TIEGCM |
|
Energy |
MIX |
TIEGCM |
|
Flux |
MIX |
TIEGCM |
|
|
|
|
|
Pedersen Conductance |
TIEGCM |
MIX |
|
Hall Conductance |
TIEGCM |
MIX |
|
field-aligned curent |
TIEGCM |
MIX |
These three models share data with one another to simulate the Magnetosphere, Ionosphere & Thermosphere. See the flow-chart below for a basic idea of how these models communicate with one another.
Word |
Definition |
---|---|
Timestep |
The timestep (in seconds) for a parictular model. The models that comprise CMIT operate at different time cadences. The diagram below shows the time exchange rates between the models. |
Exchange |
Data transfer between models. Can operate in two modes: file exchange or InterComm |
File Exchange |
(aka adhoc) data is exchanged using file system I/O drop files |
InterComm |
Data is exchanged over the network. Significantly better performance than file exchange mode |
Run |
A CMIT simulation over hours, days, weeks. Can be split up into sequences (aka segments) |
Sequence |
(aka segment) CMIT exchanges over a small period of time (1 to 4 hours). Multiple sequences comprise a CMIT run. |
The following diagram shows