HMI Pipeline Module - Module_Name_Here

coronal/solar-wind MHD simulation(s) using Br data in synoptic map format:

• a) low-resolution daily, coronal MHD (here) by K.H., using updated map

• b) high-resolution model at PSI, using calibrated definitive map (every 27~28 days)

Module Inputs

• synoptic maps:
• a) preliminary daily-updated map for daily model calculation
• b) calibrated map

Module Outputs

• 1) graphics and 3D data of solar corona and interplanetary space
• 2) Interplanetary (at 30Rs): solar wind parameters (B, V, N, T) map

Cadence

• a) daily model : 1/day
• b) high-res. model : 1 (or more ?) every 27.3-day Carrington Rotation period

Archive

• 3D volume data will be archived

Options

• a) KH's low-resolution daily MHD model will be run on an 8-CPU cluster machine, on daily basis.
• b) High-resolution physics based coronal model by PSI (Predictive Science Inc.), on one-per-CR basis.

Overall Status of Module

• a) Daily model, mostly finished :(1) take synotpic map through JSOC/DRMS, (2) prepare intiial values (3) do MHD simulation (4) save 3D data in JSOC database.
• b) Interfaces with PSI model, mostly done : at Stanford JSOC site, (1) script to get PSI data via http protocol, (2) convert HDF4 to JSOC-favorite formats FITS (3) save the 3D data in JSOC database.

Code

• a) 100 % of MHD part in Fortran, 90 % of JSOC interface codes and scripts.
• b) 90 % of script (using wget) to fetch data via http, and 90% of JSOC interface codes and scripts.

Status of DRMS module

• a) Remaining issues : define keyword
• b) Remaining issues : define keyword

Issues needing resolution

• b) Need drill test runs.

Responsible scientist

K. Hayashi

Remarks

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