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Transform vector magnetic field from image coordinates to helio-central eclipse coordinates. A project method, Lambert's Azimuthal equivalent, will be used for this transformation. This method will preserves area. The module will be applied to ARPS only. Transform vector magnetic field from image coordinates to helio-central eclipse coordinates. A project method, Lambert's Azimuthal equivalent, will be used for this transformation. Vector transformation will base on the formulae specified by Hagyard (1987). This method will preserves area. The module will be applied to ARPS only.
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 . List inputs here  . Inputs:

HMI Pipeline Module - Module_Name_Here

Transform vector magnetic field from image coordinates to helio-central eclipse coordinates. A project method, Lambert's Azimuthal equivalent, will be used for this transformation. Vector transformation will base on the formulae specified by Hagyard (1987). This method will preserves area. The module will be applied to ARPS only.

Module Inputs
  • Inputs:

Module Outputs
  • List outputs here

Cadence
  • Indicate nominal cadence on which module is run

Archive
  • Indicate if/when products are archived

Options
  • Indicate if there are any options when running the code

Overall Status of Module
  • Indicate estimate of percentage complete for the module

Status of Code
  • Name heritage or percent complete for Basic Code

Status of DRMS module
  • Indicate status of DRMS module version of module

Issues needing resolution
  • List issues that still need to be resolved
  • Describe as many as you like

Responsible scientist
  • Give name of local coordinator for development of this module

Y. Liu

Remarks


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JsocWiki: BxByBzTransform (last edited 2013-05-01 04:35:26 by localhost)