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HINODE Operation Plan (HOP)

accepted on

27-feb-2025


 HOP No.

 HOP title

HOP 0504

[SOOP: L_BOTH_LRES_MCAD_Pole-to-Pole] Pole to disk composition variation

plan term

2025/03/15-2025/03/15
2025/03/18-2025/03/19
2025/03/21-2025/03/21
2025/03/27-2025/03/27
2025/03/29-2025/04/03
2025/04/06-2025/04/27

@ @

proposer

 name : Janvier @  e-mail : miho.janvier[at]esa.int

contact person in HINODE team

 name : Kobelski, Duncan (NASA/MSFC) / Watanabe (NAOJ) / De Pontieu (LMSAL) @  e-mail : adam.kobelski[at]nasa.gov, jessie.m.duncan[at]nasa.gov, tet_watanabe[at]jcom.zaq.ne.jp, bdp[at]lmsal.com

 abstract of observational proposal
Main Objective: Coordinate Hinode/EIS and IRIS spectroscopic observations with Solar Orbiter's Pole-to-Pole SOOP to study plasma composition and dynamics across different solar latitudes and atmospheric heights.

Scientific Justification: The Pole-to-Pole SOOP takes the opportunity of the Solar Orbiter rapid latitudinal scan to acquire an extended dataset of different regions of the Sun. While for this first out-of-ecliptic orbit, the inclination is limited to 17 degrees, several opportunities are available to off point in order to observe different regions of the Sun. As such, this SOOP will provide an invaluable dataset to investigate how the plasma composition changes for different regions of the Sun located at different latitudes, as well as provide a time series of observations of the active regions belt in both hemispheres.

During the Pole-to-Pole SOOP, Solar Orbiter will be either disk center (when Metis observations take place) or we will have the flexibility to be targeting different regions of the Sun during several hours. For every instance of the Pole-to-Pole SOOP, a SPICE "composition study" will be running (duration of exactly 3h46min37s). During these observations, the study will raster one specific target (either at disk center, catching the active region belts), or a target opportunity such as active regions, and active regions and coronal holes boundaries. In the later cases, this will be important during the times when Solar Orbiter will be connected to the Sun, therefore providing for the first time context spectroscopy observations to in situ observations out of the ecliptic. The target opportunities will be decided during the pointing decision meetings, ~48h before the observations take place.

In order to augment the Solar Orbiter dataset during these times, and especially to understand how plasma composition and dynamics evolve at different latitudes and in different heights of the Sun's atmosphere, we would like to obtain a complementary dataset from both Hinode/EIS and IRIS.

The target of interest that will be picked during the pointing decision meeting.

 request to SOT
None

 request to XRT
None

 request to EIS
We request at least one run of the below study during each of the Solar Orbiter SPICE observation windows between March 15 - April 27, 2025. Each SOOP observation window is approximately 3h47m in duration, and the rough duration of the EIS study below is 1h.

STUDY ID 600
ACRONYM DHB_007_v2
RASTER ID 570
ACRONYM AbundRaster_v4
EXPOSURE TIMES (ms) 60000
FeXI 180.40
CaXV 182.10
FeX 184.33
FeVIII 185.21
FeXII 186.75
FeXI 188.40
CaXVII 192.47
CaXIV 194.10
FeXII 195.12
FeIX 197.86
CaXV 201.05
FeXIII 202.04
FeXIII 203.83
CaXVI 208.50
SXIII 256.48
SiX 258.37
SiX 261.04
FeXVI 262.98
SX 264.30
FeXIV 270.52
SiVII 275.40
MgV 276.30
MgVII 278.40
MgVII 280.39
FeXV 284.16

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

 remarks
Dates:
2025-03-15
2025-03-18
2025-03-19
2025-03-21
2025-03-27
2025-03-29
2025-03-30
2025-03-31 - 2025-04-01
2025-04-01
2025-04-02 - 2025-04-03
2025-04-06 - 2025-04-24
2025-04-25 - 2025-04-27

Time window: Below are the detailed times of the SOOP that will be run.
2025-03-15T01:00:00Z - 2025-03-15T04:46:37Z
2025-03-18T15:00:00Z - 2025-03-18T18:46:37Z
2025-03-18T23:00:00Z - 2025-03-18T23:00:00Z
2025-03-19T01:00:00Z - 2025-03-19T04:46:37Z
2025-03-21T04:01:10Z - 2025-03-21T07:47:47Z
2025-03-27T20:24:11Z - 2025-03-28T00:10:48Z
2025-03-29T13:00:00Z - 2025-03-29T16:46:37Z
2025-03-30T18:00:00Z - 2025-03-30T21:46:37Z
2025-03-31T05:00:00Z - 2025-03-31T08:46:37Z
2025-03-31T16:00:00Z - 2025-03-31T19:46:37Z
2025-04-01T05:00:00Z - 2025-04-01T08:46:37Z
2025-04-01T20:05:00Z - 2025-04-01T23:51:37Z
2025-04-02T19:30:00Z - 2025-04-02T23:16:37Z
2025-04-03T18:00:00Z - 2025-04-03T21:46:37Z
2025-04-07T03:30:00Z - 2025-04-07T07:16:37Z
2025-04-07T20:00:00Z - 2025-04-07T23:46:37Z
2025-04-08T20:00:00Z - 2025-04-08T23:46:37Z
2025-04-09T20:00:00Z - 2025-04-09T23:46:37Z
2025-04-10T20:00:00Z - 2025-04-10T23:46:37Z
2025-04-11T20:00:00Z - 2025-04-11T23:46:37Z
2025-04-12T20:00:00Z - 2025-04-12T23:46:37Z
2025-04-13T20:00:00Z - 2025-04-13T23:46:37Z
2025-04-14T20:00:00Z - 2025-04-14T23:46:37Z
2025-04-15T20:00:00Z - 2025-04-15T23:46:37Z
2025-04-16T20:00:00Z - 2025-04-16T23:46:37Z
2025-04-17T20:00:00Z - 2025-04-17T23:46:37Z
2025-04-18T20:00:00Z - 2025-04-18T23:46:37Z
2025-04-19T20:00:00Z - 2025-04-19T23:46:37Z
2025-04-20T20:00:00Z - 2025-04-20T23:46:37Z
2025-04-21T20:00:00Z - 2025-04-21T23:46:37Z
2025-04-23T02:00:00Z - 2025-04-23T05:46:37Z
2025-04-23T19:00:00Z - 2025-04-23T22:46:37Z
2025-04-24T13:00:00Z - 2025-04-24T16:46:37Z
2025-04-26T17:40:00Z - 2025-04-26T20:22:18Z
2025-04-27T18:40:00Z - 2025-04-27T21:22:18Z

Target(s) of interest: Target will be chosen during the pointing decision meeting. The target will vary between AR belt and the pole.

Previous HOPs:
None

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