• BxByBzTransform

HMI Pipeline Module - Module_Name_Here

Transform vector magnetic field from image coordinates to heliocentric ecliptic coordinates. A projection method, Lambert's Azimuthal equivalent, will be used for this transformation. Vector transformation will base on the formulae specified by Hagyard (1987). This method preserves area. The module will be applied to ARPs only. Uncertainties will be estimated based on variance and covariance from the Inversion code.

Module Inputs

• Inputs: B_total, Filling Factor (under condition), inclination, azimuth and their uncertainties in image coordinates.

Module Outputs

• Output: Bxyz field components with uncertainties in heliocentric ecliptic coordinates (a.k.a. Stonyhurst).

Cadence

• 6 hours?

Archive

• No (?).

Options

• Indicate if there are any options when running the code

Overall Status of Module

• 60%

Status of Code

• Project.c from Rick.

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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