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SOOP nameproposed bycoordinatorestimated durationnotesStatus SOOP Kitchen (star) 
Work-In-Progress
Coronal-SynopticMetisF. Auchère
Covered by the synoptics outside RSWs. Metis plans on increasing cadence in support of PSP events in Feb.
Eruption-Watch L_FULL_HRES_HCAD_Eruption-WatchMetis

D. Spadaro


1 day, several instances

CME watch during Earth quadrature, or high-quality synoptic (Mar-29)


Not doing at PH1

2022-03-23 + 2022-03-29: SOOP split in two 1-day instances for RSW2 and 3, interleaved with Coronal-Dynamics and CH-Boundary-Expansion. See LTP06_planning_SOOPs.pptx

LTP06_planning_SOOPs_15July2021.pptx. This may be fine, since SPICE updated their plan after the SWT, but will ask Daniele to decide.

Coronal-Dynamics L_FULL_HRES_HCAD_Coronal-DynamicsMetis

D. Spadaro

A. Vourlidas


1 day, several instancesSOOP tentatively scheduled on 10 days in the middle of RSW2+3

2022-03-22 to 29: SOOP split in several 1 day instances, and interleaved with Eruption-Watch and CH-Boundary-Expansion, following instructions in LTP06_planning_SOOPs.pptx

Coronal-He-Abundance L_FULL_HRES_MCAD_Coronal-He-Abundance

Metis

V. Andretta

F. Auchère



Herschel sounding rocket launch during RSW1?

overlapping with the calibration SOOP

2022-03-07 16:00-20:00: SOOP has been scheduled as requested in RSWG_20210621_fauchere.pptx and using SOOP page as input + ML_Planning_2022_He.pdf

Note SPICE is not part of this SOOP instance, it is running cross-calibration with EIS/IRIS in parallel. The SPICE composition mosaic made on 2 March will be used for context.

Density-Fluctuations R_FULL_HRES_HCAD_Density-FluctuationsMetis

D. Spadaro



overlapping with L_FULL_HRES_HCAD_Coronal-Dynamics
CH-Boundary-Expansion L_BOTH_HRES_LCAD_CH-Boundary-ExpansionMetis

D. Spadaro


1 dayinterleaved with L_FULL_HRES_HCAD_Coronal-Dynamics

2022-03-26: SOOP created using input in LTP06_planning_SOOPs


<joint observations with near-Earth assets (e.g. LASCO)>MetisM. Romoli + (cross-calibration science RSWG)
COORD_CALIBRATION with Earth observatories has been scheduled around 6-8 March
proposal to run first part of this campaign at disk centre

full-disk helioseismology campaign

R_FULL_LRES_HCAD_Full-Disk-Helioseismology

PHIT. Appourchaux / J. Schou few days

angular separation Earth-Sun-SC between 17-18 degrees on 14 March 

Other opportunities on 19-24 January (before SDO eclipse season begins) and on 14-17 Feb.

Ideally before RSW1 starts (can be far from Sun, high resolution is not important); start around 1 Feb, running 4 days, (on-board processing will take several weeks, around 20 days)

2022-02-01 - 2022-02-05 (4d):

2022-01-20 – 2022-01-24 (4d):
R_FULL_LRES_HCAD_Full-Disk-Helioseismology

Based on seismology_campaignJH_TA.pptx

Note 

  • FDT refocus assumed part of preceding PHI_FDT_CALIB
  • Processing and flushing timeline has been reviewed and updated by J. Hirzberger. 
  • raw data placeholder had to be added to account for extra data production 
    • Question: is this the reason for the PHI_RAW_FDT_6 block from 2022-01-27T00:00 to 2022-02-20T00:00 ?
  • Note that flushes and data produced do not coincide, nor is it obvious which of these is correct.
    • It appears that the volume of the observations was insufficient. Will model the updated volume with the pre-existing flushes  
  • E-mail sent to PHI  
R_BOTH_HRES_MCAD_Bright-Points to be run at Earth-Sun crossing lineSPICE

Andrzej Fludra

D. Berghmans

S. Solanki



Could be run as part of the COORD_CALIBRATION with Earth observatories scheduled around 6-7 March
(40 minutes SPICE raster, coordinated with EUI & PHI burst in the middle of that period)

Sun-Earth line. A SOOP needs to be created (by A. Fludra).

2022-03-08 04:00-10:00 (6h):
SOOP created based on inputs in SOOP R_SMALL_Hres_Mcad_Bright_Points.xlsx and minimal requested TM.

PHI not part of SOOP as HMI will be available.

SPICE parameters as provided in input (modelled as SPICE_CMEWATCH)

SOOP page to be created based on SOOP_Bright_Points_Survey_R_SMALL_Hres_Mcad.docx

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SOOP nameproposed bycoordinatorestimated durationnotesStatus SOOP Kitchen (star) 
Work-In-Progress

high-cadence coronal dynamics (could be the Coronal-Dynamics SOOP or a variation with focus on high-res. on-disk obs.) 

EUI

In RSW2+3, for now we scheduled 5 days of offpointing to target + 10 days of disk-centre pointing + 5 days of offpointing to target
nanoflares R_BOTH_HRES_HCAD_NanoflaresEUI

D. Berghmans

S. Parenti 


In RSW2+3, for now we scheduled 5 days of offpointing to target + 10 days of disk-centre pointing + 5 days of offpointing to target

Depending on the objective, a different coordinator should be assigned.

RSW1 (for other windows see below for off-pointing)

2022-03-07 (3h): 3 different blocks of EUI observations (source: SOOPs_EUI LTP6-9).

2022-03-08 (3h): identical to AR observations above.


<long high-res campaign around perihelion (PHI, EUI, SPICE)>PHI
'long' means various hours at high cadence

could be run in RSW2+3, partially disk centre and partially offpointed

Can be combined with the EUI campaigns above.

Would be interesting at quadrature (RSW3), so that AIA at limb/centre can be combined with EUI/PHI at centre/limb. Both flavours can be run.




















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SOOP nameproposed bycoordinatorestimated durationnotesStatus SOOP Kitchen (star)
Work-In-Progress

slow wind connection science: RS-IS connection mosaic  L_SMALL_MRES_MCAD_Connection-MosaicAll

Alessandra Giunta, Natalia Prado, Don Hassler

& the Connection Mosaic SOOP WG


Connection mosaic scheduled on first day RSW1 (2 March) - still Metis compatible.

Could be repeated again at end RSW3 (without Metis).

PHI Full disk is enough. 

2022-03-02 to 03 (27h): First instance in RSW1 scheduled, based on input in Connection_Mosaic_slides_for_SWT_24jun21_UPDATED.pptx

2022-03-30 to 31 (27h): 2nd instance on 30 March updated to 27 hrs duration and modes updated based on input in slides above (without Metis).

slow wind connection science: source tracking L_SMALL_HRES_HCAD_Slow-Wind-ConnectionSWA, SPICE

D. Stansby



~ 5 days

L_SMALL_HRES_HCAD_Slow-Wind-Connection scheduled in RSW1, before and after cross-calibration with Earth 
→ these timings may not be ideal. IS payload is 2x as far from the Sun as during perihelion and Earth is seeing same scene.
The SOOP before cross-calibration has been removed to give more time for cross-calibrations with Earth.

A better opportunity closer to the Sun are the 5 days at start RSW2. We can still use Earth observations to help us with the connection modelling.

2022-03-03 to 06 (72h): First instance scheduled for RS instruments, except for Metis (incompatible with pointing away from disc centre from 2022-03-03T03:00:00).

2022-03-17 to 22 (6h short of 5 days): Second instance scheduled for RS instruments execept Metis, with slightly higher TM requirements.

Reference input: Slow wind SOOP plan.pdf

high-cadence coronal dynamics L_FULL_HRES_HCAD_Coronal-DynamicsEUI

D. Spadaro, A. Vourlidas



In RSW2+3, for now we scheduled 5 days of offpointing to target + 10 days of disk-centre pointing + 5 days of offpointing to target
nanoflares R_BOTH_HRES_HCAD_NanoflaresEUID. Berghmans, S. Parenti
In RSW2+3, for now we scheduled 5 days of offpointing to target + 10 days of disk-centre pointing + 5 days of offpointing to target

2022-03-17 (3h): Quiet Sun,

2022-03-17 (3h): Active region at intermediate angle,

Both with single cadence for EUI, other observations as per 2022-03-07/08 with the SOOP lasting for 30 minutes in each case.


2022-03-30 (6h): Active region, 30 minutes of observations without FSI, as per SWT_LTP06_Nano_Coords.pdf.

high-res imaging of a polar coronal hole

R_SMALL_HRES_MCAD_Polar-Observations 


A. Zhukovmin 2 hours

Idea is to point to the limb, with SPICE slit also covering off-limb corona above the coronal hole. Ideally close to perihelion to take advantage of the higher resolution.


2022-03-07 05:30 (3h) with shorter duration EUI/PHI high-res observations (30mins)

2022-03-30 06:00 (3h) with shorter duration EUI/PHI high-res observations (20mins)

2022-04-04 09:00 (39h) with shorter duration EUI/PHI high-res observations (13h20m)

SOOP instances have been added based on the input provided in SOOP_polar_AZhukov_20210621.pdf and EUI input https://docs.google.com/spreadsheets/d/1JE7MARnnZMg9--EgY_1bdJ7UultPOhd-zPMRELSgc2k

  • EUI observations adjusted to fit the input in slides above and EUI spreadsheet.
  • PHI and SPICE contribution not specified in much detail. Placeholders have been added
  • For PHI in first SOOP instance, raw data mode has been implemented upon request PHI team (email 17 Jun)

<follow solar region on disk for a long time, e.g. AR (>2 weeks)>

R_SMALL_MRES_MCAD_AR-Long-Term

PHI

Luis Bellot (PHI)

in coord with D. Berghmans (EUI) and M. Janvier (SPICE)


first 5 days of RSW2 reserved for target tracking (AR dynamics SOOP for now)

From input received from RSWG and SOOP coordinators, the SOOP will be run at the end of RSW2+3 (starting 31 March) and instead of AR dynamics, a TM-lighter soop will be used: R_SMALL_MRES_MCAD_AR-Long-Term

Science goals: monitor AR continuously for 4 days to: study AR decay, AR properties from 2 different vantage points, and sources slow solar wind.

Coordinate with Earth telescopes to extend AR coverage by a few days
Solar Orbiter takes over when AR is beyond limb as seen from Earth

pVSTP needed

2022-03-31T12:00 to 2022-04-04T09:00 (3d 21h): Original placeholder SOOP (AR-Dynamics) has been replaced by R_SMALL_MRES_MCAD_AR-Long-Term, as requested by SOOP coordinator in R_SMALL_MRES_MCAD_AR-Long-Term_plans_lbellot.pdf.

Note that SOOP starts later than requested in the slides because the connection mosaic preceding it has been extended to last 27h, as requested by F. Auchere.

Observation details have been added based on details in presentation above and spreadsheet EUI.

<look at AR near west limb around perihelion to connect with PSP>A. Vourlidas

A. Vourlidas



if we follow an AR in RSW2+3, choosing one on the West side of the Sun could be useful for connection science with PSP (note PSP will be rather far away)

Note: tradeoff with staying disk centred at quadrature => SWT agrees it would be more favourable to stay at disk centre during quadrature with Earth (= 29 March).

Coordinate with Earth assets.

N/A

multiple day AR following is scheduled for end RSW2+3, see row above 

support PSP perihelion in Feb
A. Zhukov

proposal to use SPICE OOF calibration = 3 hours at east limb or west limb. Note despite the name of the SOOP in SOOP Kitchen, this campaign is not just for SPICE but also for other instruments. The campaign described in Solar Orbiter SPICE Out-Of-Field Calibration is just being used to request the out of RSW manoeuvres to Flight Dynamics. The instrument contributions can be added on the timeline as needed.

2 offpointings requested and scheduled: to East limb on Feb 23, to West limb on Feb 27

2022-02-22 (3h): at East limb,

  • PHI/FDT
    • SYNOPTICS just before and after
  • SPICE:
    • SPICE_LIMB (SSPI_0000_CC8_111_EX8t_111) provisionally chosen as the SOOP Kitchen observation mode that most closely resembles what is being asked for in the large raster.
    • Comment in Google Spreadsheet provided : "4'' slit X 128 positions = 8.5' wide, start 2’ inside the limb, end 6.5’ above the limb, 8 spectral windows, double binning in Ly-β."  Solar Orbiter cannot point beyond the limb, so we assume that this off-pointing will be done with the mirror mechanism at the instrument level.

    • SPICE_SPECTRATLAS (SSPI_0000_CC8_111_sPBE_11B) has been used here to most closely match what is being asked for as the mini-raster, with reduced number of raster exposures (26 rather than 30). To be investigated by Andrzej Fludra for the future, but we model this for now.
  • EUI:
    • FSI: FSI_GENERIC_S_B (SEUI_0000_CC8_111_u7FA_111) used in the absence of an indicated observation type (ideal version)
    • HRI Ly-α: LYA_GENERIC (SEUI_0000_CC8_111_APjY_111) used in the absence of an indicated observation type (ideal version), with 2x2 binning (folded into the compression level → 30).
    • HRI EUV: EUV_GENERIC (SEUI_0000_CC8_111_AtaE_118) used in the absence of an indicated observation type (ideal version)

2022-02-26 (3h): at West limb,

  • PHI/FDT
    • SYNOPTICS just before and after(for only 30 minutes on each side)
  • SPICE:
    • SPICE_LIMB (SSPI_0000_CC8_111_EX8t_111) provisionally chosen as the SOOP Kitchen observation mode that most closely resembles what is being asked for in the large raster.
    • Comment in Google Spreadsheet provided : "4'' slit X 128 positions = 8.5' wide, start 2’ inside the limb, end 6.5’ above the limb, 8 spectral windows, double binning in Ly-β."  Solar Orbiter cannot point beyond the limb, so we assume that this off-pointing will be done with the mirror mechanism at the instrument level.

    • SPICE_SPECTRATLAS (SSPI_0000_CC8_114_sPBE_11C) used for mini-raster. Understood that Andrzej Fludra will refine this in future, but for now we model the plan with this configuration. 
  • EUI:
    • FSI: FSI_GENERIC_S_B (SEUI_0000_CC8_114_u7FA_11L) used in the absence of an indicated observation type (ideal version)
    • HRI Ly-α: LYA_GENERIC (SEUI_0000_CC8_114_APjY_113) used in the absence of an indicated observation type (ideal version), with 2x2 binning (folded into the compression level → 30).
    • HRI EUV: EUV_GENERIC (SEUI_0000_CC8_114_AtaE_11A) used in the absence of an indicated observation type (ideal version)

Reference: SOOP_PSP_support_202202_AZhukov_20210621.pdf, and Google spreadsheet entitled SOOP CC_OFFPOI_OOF of  

AR tracking close to perihelion


In RSW2+3, for now we scheduled 5 days of offpointing to target + 10 days of disk-centre pointing + 5 days of offpointing to target
Cross-calibration with Earth assets, pointing to particular targets (e.g. sunspots/ARs/limb/...)

Marco Romoli

RSWG + cross-calibration WG



COORD_CALIBRATION with Earth observatories has been scheduled 4-8 March
proposal: after a disk-centre pointed part for Metis, target pointing can be done (currently scheduled on 7-8 March)

Ideally targetted pointing. If not feasible, a predefined mosaic may work as well. Full disk mosaic would be great for outreach too (to be calculated how long that would take).

See above.

(star) Note that the SOOP scheduling is was first drafted in the child plan https://solarorbiter.esac.esa.int/soopkitchen/#/planning/child-plan/SOOP%20Coordination%20for%20NMP%20Segment%201 

Once confirmed by SWT, it will be got moved to the parent MLP plan https://solarorbiter.esac.esa.int/soopkitchen/#/planning/plan/Mission%20Level%20Plan%20for%20NMP%20Segment%201 and released at baseline 3, to be used as input for LTP6 planning.

Additional information

  • 20-23 Feb: good for connectivity science with Earth-based assets
  • 6 March: Jupiter transit

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