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HINODE Operation Plan (HOP)

accepted on


 HOP No.

 HOP title

HOP 0395

DKIST/ViSP Science Verification Support

plan term


@ @


 name : de Wijn, Casini (POC) @  e-mail : dwijn[at]ucar.edu, casini[at]ucar.edu

contact person in HINODE team

 name : DeRosa, Shine @  e-mail : derosa[at]lmsal.com, shine[at]lmsal.com

 abstract of observational proposal
Main Objective: Provide supporting observations for the Science Verification of DKIST/ViSP

Scientific Justification: Hinode SOT/SP is the "gold standard" for photospheric polarimetry. Observations from SOT/SP in support of DKIST/ViSP during its Science Verification can be used to compare qualitative and quantitative measures to demonstrate that ViSP is producing high-quality science data.

 request to SOT
Normal maps, approx. 82"x82, repeating as telemetry allows.

 request to XRT

 request to EIS
For QS observation: Atlas_30 (EIS study #403)
For AR observation: EL_DHB_01 (EIS study #602)

 other participating instruments

IRIS: None

POC: Roberto Casini (casini@ucar.edu)

Dates: TBD, DKIST schedule is in a constant state of flux. Not earlier than late March 2020.

Time window: 18:00 to 24:00 UTC (08:00 - 14:00 Hawaii local time)

Target(s) of interest: Max Millennium target, or disk center in case of no activity

Previous HOPs:
Long-term Hinode SOT team member. I have several publications using SOT/FG and SOT/SP data, including a study of photospheric proxy-magnetometry, polarimetry with BFI, and most recently a study of polarization in the [O I] line with SOT/SP.

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