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HINODE Operation Plan (HOP)

accepted on

20-jan-2022


 HOP No.

 HOP title

HOP 0432

Solar Orbiter Polarimetric and Helioseismic Imager (SO/PHI) co-observations around perihelion passage

plan term

2022/03/22-2022/03/22

@ @

proposer

 name : Valori, Orozco-Suarez, Hirzberger, Lagg, &  SO/PHI team @  e-mail : valori[at]mps.mpg.de, orozco[at]iaa.es, hirzberger[at]mps.mpg.de, lagg[at]mps.mpg.de

contact person in HINODE team

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

 abstract of observational proposal
Main Objective: Coordinated observations with the Solar Orbiter (SO) Polarimetric and Helioseismic Imager (PHI) High-Resolution Telescope (HRT), close to SO perihelion in the second remote sensing window (RSW2) of the first orbit of SO Nominal Mission Phase (NMP) that will take place in early March 2022.  

Scientific Justification: SO was successfully launched on Feb.10, 2020. All its onboard instruments are performing nominally and were commissioned during the early phase of the mission. Among them, SO/PHI provides maps of the vector magnetic field and line-of-sight velocities with two telescopes (Full Disk Telescope, FDT, and HRT).  
One of the main scientific opportunities offered by SO is stereoscopic observation in conjunction with Earth- or near-Earth observatories. The difference in viewing angle bears important consequences on the possibility of comparing and merging such observations, as the  optical path from the two viewpoints can be very different. In order to assess the general feasibility of stereoscopic observations, a thorough comparison of the spectropolarimetric properties of Hinode/SOT-SP and SO/PHI-HRT is necessary.    
The SO/PHI-HRT calibration observation for this HOP will take place when SO is at 0.335AU, i.e. close to SO perihelion, where the HRT pixelsize will be 121km, while being at an angle of about 50.19deg longitude and 0.69deg latitude (on 2022-03-22T09:40:00) with Earth. The specific goal of these coordinated observations is to perform cross-calibrations between Hinode/SOT-SP and SO/PHI-HRT when the angular separation is relevant for stereoscopic observations, at the highest resolution of the current orbit.  
In conjunction with the companion HOP gSolar Orbiter Polarimetric and Helioseismic Imager (SO/PHI) co-observationsh by D. Orozco, the observations provided by this HOP will attain cross calibration both at Earth-Sun line and at a finite separation angle with highest HRT resolution that will provide the quantitative foundations of all future investigations combining Hinode/SOT-SP and SO/PHI-HRT. The cross-calibration of SO/PHI-HRT has not been performed yet (a previous attempt was hampered by a procedural mistake in one of the SO instruments -not PHI). Since SO is already in the Nominal Mission Phase, the cross-calibration planned by the two companion HOPs is of utmost importance, and a top priority of the PHI instrument team.  
The SO/PHI-HRT observations relevant to this proposal are planned as dedicated, PHI calibration observations, and are carried out by the PHI instrument team itself.  

 request to SOT
Science support for high-resolution campaign. We require SOT/SP for Mar 22, 09:40 - 10:40 UT
We request a series of repeating 20hx164h normal maps at the highest available signal-to-noise. If telemetry allows, we request 2-sided maps.
Pointing: Disk center from the perspective of Solar Orbiter. The exact pointing coordinates from the perspective Earth will be provided several days in advance.
We estimate that 6 such normal maps can be taken within the 1-hour duration of the SO/PHI HRT observation.

 request to XRT
a low telemetry CME watch program

 request to EIS
If the target is an AR:
     Atlas_60 (study 404) -> 165 kBits @ JPEG 90
 OR  HPW021VEL260x512v2 (study 569) -> 133 kBits @ JPEG 85
If telemetry allows, please also intersperse with:
     DHB_007_v3 (study 601) -> 37 kbits @ JPEG 90

If the target is QS:
     Atlas_120  (study 405) -> 165 kBits @ JPEG 90

 other participating instruments
IRIS requests (program recommended by the instrument team):  
3620258057 | Very large dense 64-step raster 20.8x175 64s Deep x 8 FUV spectrall | 602.00 | 1255.59 | 1.42 | 9.4+/-0.1 | 602+/-0 | 37.6+/-0.0 | 37.6+/-0.0 | 37.6+/-0.0 | 37.6+/-0.0

 remarks
Dates:  We request support for calibration activities during the high-resolution observations on  22 March 2022 : HRT will perform one-hour of high-resolution observations at one-minute cadence.  

Time window:  On March 22nd, from 09:40 to 10:40 UT.  
It is important to take into account that the specific times (UT) above may be subject to slight changes, and are still to be confirmed. Exact times will be fixed around two weeks (worst case) prior observation
starts.

Target(s) of interest:  HRT calibrations use observations at disk center, as seen from SO Point-of-View(POV). SO/PHI HRT field of view at perihelion is about 300h x 300h.

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