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HINODE Operation Plan (HOP)

accepted on

23-feb-2023


 HOP No.

 HOP title

HOP 0457

[SOOP: Nanoflares] New run of the IHOP 429 in conjunction with the Solar Orbiter

plan term

2023/04/04-2023/04/05
2023/04/11-2023/04/11
2024/04/04-2024/04/04

@ @

proposer

 name : Parenti @  e-mail : susanna.parenti[at]universite-paris-saclay.fr

contact person in HINODE team

 name : Savage, Watanabe, De Pontieu @  e-mail : sabrina.savage[at]nasa.gov, watanabe.tetsuya[at]nao.ac.jp, bdp[at]lmsal.com

 abstract of observational proposal
Main Objective: The general purpose is to study small scale dynamics events, as explained in HOP 429.

Scientific Justification:
This Solar Orbiter orbit will be equivalent to the 2022 one. We will have QS, AR and limb pointing, but with a more active Sun. We will run longer high cadence/resolution periods with EUI/HRI and the support of Hinode will be a highly valuable gain. In some of the Solar Orbiter run we use new instrument modes, to extract the best from the data.

 request to SOT
April 4, 04:08 UT to 07:10 UT (QS observations): 82hx123h normal maps, repeat as many as possible. We estimate that each map will take 40 minutes to complete and will generate 0.5Gb of data.
April 5, 22:05 UT to April 6, 00:25 UT (AR observations): large 320hx164h fast single maps, minimum 2 starting at the beginning of the time interval, or (if telemetry allows) 3 to cover the full period. We estimate that each map will take about 60 minutes to complete and will generate 0.5Gb of data.
April 11 (AR observations): Starting at 23:15 UT on April 11, we request a large 320hx164h fast map during the PHI high cadence. We estimate that the map will take about 60 minutes to complete and will generate 0.5Gb of data.
Solar rotation tracking should be used for all observations. For the target pointings, please refer to the table on the coordination page linked under Additional Instrument Coordination.

 request to XRT
April 4 04:08 - 07:10: QS pointing:
- XOB #1CCD: HOP429 CH 384x384 at 1064 1048, Al/poly + Ti/poly (5.6s) and thin-Be (16s) with G-band (1ms/1ms leak), 30s cad
April 5 22:05 - March 6 00:25: AR pointing (Track pointing)
- XOB #1CCE: HOP429 AR 384x384 at 1064 1048, Al/poly and thin-Be (AEC3) with G-band (1ms/1msleak), 30s cad
April 11 21: 05 - April 12 00:05: AR pointing (Track pointing)
- XOB #1CCE: HOP429 AR 384x384 at 1064 1048, Al/poly and thin-Be (AEC3) with G-band (1ms/1ms leak), 30s cad

 request to EIS
---(2024)
Studies:  #404 - Atlas_60 as context raster at beginning and end of observing period and #540 CLASP-1_60x512_OBS_  (RASTER ID 515 , line list ID 161) as much as possible (with the priority as stated below in the Remarks section).

---(2023)
April 4 04:08 - 07:10: QS pointing:
- Atlas_60 #404 as context raster
- EL_DHB_02_v2 #631 for dynamic study
April 5 22:05 - March 6 00:25: AR pointing (Track pointing)
- Atlas_60 #404 as context raster
- EL_DHB_01 #602 for dynamic study
April 11 21: 05 - April 12 00:05: AR pointing (Track pointing)
- Atlas_60 #404 as context raster
- EL_DHB_01 #602 for dynamic study

 other participating instruments
Additional instrument coordination: Solar Orbiter [SOOP: R_BOTH_HRES_HCAD_nanoflares]
https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Solar+Orbiter+Planning+-+for+coordination+with+external+parties

 remarks
---(2024)
Target:  Quiet Sun

Times:   04 April 2024 02:20 to 16:04 UT with priority times 15:30 to 16:00 during EUI/HRI high cadence and 08:16 to 15:30 UT during SPICE high cadence

---(2023)
Dates: Apr 4, Apr 5, Appri 11

Time window: Times at Orbiter, to be converted
April  4 04:08 - April  4 07:10: QS pointing.
April  5 22:05 - April  6 00:25: AR pointing
April 11 21:05 - April 12 00:05: AR pointing
Refer to coordination page in Additional Instrument Coordination.

Target(s) of interest: QS & AR
---

Previous HOPs: IHOP 429
Additional remarks:
Some of the studies have to be finalized.
Details of the timing for each study will be posted in a second version of this document

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