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| coronal/solar-wind MHD variables matching Br | coronal/solar-wind MHD simulation(s) using Br data in synoptic map format: (a) low-resolution daily one by K.H., using updated map, and (b) high-resolution model at PSI, using calbrated map (conducted every 27~28 days) |
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| . daily model : 1/day . external, high-res. model : 1 (or mode ?) / one CR, where to run (a few days after one CR ends)? |
. a) daily model : 1/day . b) high-res. model : 1 (or more ?) every 27.3-day Carrington Rotation period |
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| . 2D data (sampled on selected quatorial/meridional plane and sphere) will be archived. . ? 3D volume data ? because of large file size etc. |
. 2D cross-section data (sampled on selected quatorial/meridional plane and sphere) will be archived. . 3D volume data ? how to handle large files ? |
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| . one run will use 8 CPUs (or 16 on lws2?) or, outside Stanford | . a) daily MHD model will run on 8-CPU cluster machine, approximately 2~3 hours . b) |
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| . 1) Daily model : mostly ready . 2) External model : to decide the spatial resolution, where to run, etc. . 3) Input data preparetion : may need to make new (c-)codes replacing exisiting IDL code and others so that . input data format match each developer's preference. ===== Status of Code ===== . 70 % |
. a) Daily model : mostly ready as JSOC module: minor issue to handling data via JSOC/DRMS remaining . b) External model : the code is ready. the website for showing the results is well prepared by PSI. ===== Code ===== . a) 90 % . b) ~100% |
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| . to do ! | . a) Need to define the keyword to specify the daily-updated synoptic maps, in the JSOC context. . b) N/A, the high-resolution MARS code will run on external super-computers. The cadence is about a month. |
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| * none | * there are no major issues. |
HMI Pipeline Module - Module_Name_Here
coronal/solar-wind MHD simulation(s) using Br data in synoptic map format: (a) low-resolution daily one by K.H., using updated map, and (b) high-resolution model at PSI, using calbrated map (conducted every 27~28 days)
Module Inputs
- synoptic maps:
- a) preliminary daily-updated map for daily model calculation
- b) calibrated map for external model(s)
Module Outputs
- 1) Corona : field lines, synthetic LoS-integrated coronal density, temperature etc.
- 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
- Plots (images in format like gif or jpg) and
- 2D cross-section data (sampled on selected quatorial/meridional plane and sphere) will be archived.
- 3D volume data ? how to handle large files ?
Options
- a) daily MHD model will run on 8-CPU cluster machine, approximately 2~3 hours
- b)
Overall Status of Module
- a) Daily model : mostly ready as JSOC module: minor issue to handling data via JSOC/DRMS remaining
- b) External model : the code is ready. the website for showing the results is well prepared by PSI.
Code
- a) 90 %
- b) ~100%
Status of DRMS module
- a) Need to define the keyword to specify the daily-updated synoptic maps, in the JSOC context.
- b) N/A, the high-resolution MARS code will run on external super-computers. The cadence is about a month.
Issues needing resolution
- there are no major issues.
Responsible scientist
K. Hayashi
Remarks
- Back to ["HMIModuleTable"]
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