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1988
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Deletions are marked like this. | Additions are marked like this. |
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. 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 ? |
. 3D volume data will be archived |
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. b) | . b) HDF file provided by PSI once a CR period will be first converted to FITS format then send to DRMS |
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. 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. |
. a) Daily model, mostly finished :(1) take synotpic map through JSOC/DRMS, (2) prepare intiial values (3) do MHD simulation (4) send 3D data to JSOC. . b) External PSI model : mostly done : (1) script to get PSI data at their website, (2) convert HDF4 to JSOC-favorite format (3) send the 3D data to JSOC. |
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. a) 90 % . b) ~100% |
. a) 100 % of MHD part in Fortran, 99 % of C-wrapper . b) 99 % of script (using wget) to fetch data via http, and 99% of C-code to push the 3D data to JSOC |
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. 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. |
. a) Remaining issues : define keyword. . b) Remaining issues : do define keyword other than physics unit and CR number. |
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* there are no major issues. | * On j8.q and j.q, some code returns NaN even though the data is OK. o.q and o8.q do not have such problem.....unnnn |
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
- 3D volume data will be archived
Options
- a) daily MHD model will run on 8-CPU cluster machine, approximately 2~3 hours
- b) HDF file provided by PSI once a CR period will be first converted to FITS format then send to DRMS
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) send 3D data to JSOC.
- b) External PSI model : mostly done : (1) script to get PSI data at their website, (2) convert HDF4 to JSOC-favorite format (3) send the 3D data to JSOC.
Code
- a) 100 % of MHD part in Fortran, 99 % of C-wrapper
- b) 99 % of script (using wget) to fetch data via http, and 99% of C-code to push the 3D data to JSOC
Status of DRMS module
- a) Remaining issues : define keyword.
- b) Remaining issues : do define keyword other than physics unit and CR number.
Issues needing resolution
- On j8.q and j.q, some code returns NaN even though the data is OK. o.q and o8.q do not have such problem.....unnnn
Responsible scientist
K. Hayashi
Remarks
- Back to ["HMIModuleTable"]
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