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| Deletions are marked like this. | Additions are marked like this. |
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| . List inputs here |
. Local magnetic field map at time and position of interest that will be probably determined by an active region recognition program. |
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| . List outputs here |
. 1) Three-dimensional volume data : all 3 components of magnetic field in the volume of interest. . 2) Plot, visualization . 2-a) Field-line projected onto the solar surface or viewed from the Earth and other directions. . 2-b) Map at the base (photosphere) about whether field be open or closed. (?) |
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| . Indicate nominal cadence on which module is run |
. Once / a few times per day |
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| . Indicate if/when products are archived |
. 3D data may be archive |
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| . Indicate if there are any options when running the code |
. Sizes in both horizontal and vertical directions be determined or given |
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| . Indicate estimate of percentage complete for the module |
. 1-a) Iterative solver for Laplace equation : almost done, including OpenMP parallelism. 100% as stand-alone code . 1-b) efficient methods such as Fourier methods : 30 % . 2) Drawer / plotter : 50 % |
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| . Name heritage or percent complete for Basic Code |
. 70 % |
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| . Indicate status of DRMS module version of module |
. Tested under stand-alone condition, . Not tested as DRMS or JSOC module |
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* List issues that still need to be resolved * Describe as many as you like |
* So far, "patch"-data prepared by hand is used for test. * Preparation of input data in a atutomatic/timely manner remaining |
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| . Give name of local coordinator for development of this module |
. K.Hayashi |
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* Back to ["HMIModuleTable"] * Back to FrontPage |
* Back to ["HMIModuleTable"] * Back to FrontPage |
HMI Pipeline Module - PotentialFeildLocal
Provide local potential field approximation in high resolution from HMI vector field data
Module Inputs
- Local magnetic field map at time and position of interest that will be probably determined by an active region recognition program.
Module Outputs
- 1) Three-dimensional volume data : all 3 components of magnetic field in the volume of interest.
- 2) Plot, visualization
- 2-a) Field-line projected onto the solar surface or viewed from the Earth and other directions.
- 2-b) Map at the base (photosphere) about whether field be open or closed. (?)
Cadence
- Once / a few times per day
Archive
- 3D data may be archive
Options
- Sizes in both horizontal and vertical directions be determined or given
Overall Status of Module
- 1-a) Iterative solver for Laplace equation : almost done, including OpenMP parallelism. 100% as stand-alone code
- 1-b) efficient methods such as Fourier methods : 30 %
- 2) Drawer / plotter : 50 %
Status of Code
- 70 %
Status of DRMS module
- Tested under stand-alone condition,
- Not tested as DRMS or JSOC module
Issues needing resolution
- So far, "patch"-data prepared by hand is used for test.
- Preparation of input data in a atutomatic/timely manner remaining
Responsible scientist
- K.Hayashi
Remarks
- Back to ["HMIModuleTable"]
Back to FrontPage