module_flatfield - derive line-of-sight observables

Synopsis

cosmic_ray_post input_series= camera= datum= hour=

cosmic_ray_post is post-processing the cosmic ray series (hmi.cosmic_rays) for false positives. The module processes 2 hours at a time, starting at the time given by the datum and hour argument

par Options

Mandatory arguments:

• input_series="string" where string is the series name of the intermediate flatfield (su_production.flatfield_fid)
• camera=cam, side camera: cam=1, front camera: cam=2
• datum="date" date="yyyy.mm.dd" TAI-day for which the intermediate flatfields have been calculated. End of TAI-day datum is T_START of updated flatfield
• hour=hour

Examples

Example 1:

cosmic_ray_post input_series="su_production.flatfield_fid" camera=2 datum="2010.10.09" hour=2

Synopsis

module_flatfield input_series= camera= datum= camera= cadence= cosmic_rays= flatfield= fsn_first= fsn_last= cosmic_ray_series

module_flatfield calculates the rotational flatfield by FID, and produces the cosmic ray records. Both are written to an intermediate series. The flatfield update is produced by module_flatfield_combine, and the cosmic ray series by cosmic_ray_post. If cosmic_ray_series is set to hmi.cosmic_rays, module_flatfield produces the final cosmic ray records directly.

Options

Mandatory arguments:

• input_series="string" where string is the series name of the input level 1 data (hmi.lev1 or hmi.lev1_nrt)
• camera=cam, side camera: cam=1, front camera: cam=2
• fid=fid: observable FID (10054-10159)
• datum="date" date="yyyy.mm.dd" TAI-day for which the flatfields and cosmic_rays are calculated. End of TAI-day datum is T_START of updated flatfield
• cadence=cadence: integer number in seconds for the cadence for the framelist that is run (Example: Framelist Mod C, front camera: cadence=45, side camera: cadence=135)
• cosmic_rays=flag: flag=1 if cosmic ray records should be produced, otherwise flag=0
• flatfield=flag: flag=1 if rotational flatfield should be produced, otherwise flag=0

Optional arguments:

• cosmic_ray_series="string" where string is the series name of the output cosmic ray series (default is "su_production.cosmic_rays")
• fsn_first: first FSN for which cosmic ray record is desired, which is included in the flatfield calculation, overrides argument datum: datum still needed for flatfield identification
• fsn_last: last FSN or which cosmic ray record is desired, which is included in the flatfield calculation, overrides argument datum

Examples

Example 1:

module_flatfield input_series="hmi.lev1" camera=2 datum="2010.10.09" fid=10059 camera=2 cosmic_rays=1 flatfield=1 cadence=45 
module_flatfield input_series="hmi.lev1" camera=2 datum="2010.10.09" fid=10059 camera=2 cosmic_rays=1 flatfield=1 cadence=45 fsn_first=12050442 fsn_last=12050459 cosmic_ray_series="hmi.cosmic_rays"