HOP 0444

HINODE Operation Plan (HOP)

accepted on

15-sep-2022

HOP No.

HOP title

HOP 0444

Magnetic field structure of prominences solar tornadoes and spicules

plan term

2022/10/03-2022/10/13
2023/09/25-2023/09/29
2024/09/17-2024/09/26

proposer

name :

Labrosse, Schmieder, Peat

e-mail :

Nicolas.Labrosse[at]glasgow.ac.uk, brigitte.schmieder[at]obspm.fr

contact person in HINODE team

name :

Matthews, Culhane

e-mail :

sarah.matthews[at]ucl.ac.uk, j.culhane[at]ucl.ac.uk

abstract of observational proposal

Main Objective: Observations of magnetic prominences in multi wavelengths to see different structures and cavity

Scientific Justification: Themis was updated with adaptive optics in 2019 and since 2022 has a new polarimeter. We want to coordinate our observations with multi wavelength data.

request to SOT

HOP 373 (like 2019 Oct 01 with THEMIS):
Several fast map scans of the target filament throughout the observing period are requested. Programs such as SP 0x0175 (164"x164" fast map) are fine. If needed, the height and width of the scan can be adjusted to better fit the path of the filament channel on the disk.

request to XRT

HOP 373 (like 2019 Oct 01 with THEMIS):
Standard 2-filter active region program at a 1-2 minute cadence

request to EIS

HOP 373 (like 2019 Oct 01 with THEMIS) for detecting the dopplershifts in tornado:

EIS STUDY ID #573 raster_hefe3.

other participating instruments

IRIS requests:
1. OBSID for prominences far from the equator (at large latitudes).

3600111762 | Very large coarse 64-step raster 126x175 64s Mg II h/k Deep x 15 Spat | 1048.26 | 495.26 | 0.32 | 16.4+/-0.0 | 1048+/-0 | 0.0+/-0.0 | 0.0+/-0.0 | 16.4+/-0.0 | 0.0+/-0.0

2. For prominences near the equator and not too high (smaller number of steps).

3600609752 | Very large coarse 32-step raster 62x175 32s Mg II h/k Deep x 8 Spatia | 296.83 | 185.99 | 0.43 | 9.3+/-0.0 | 297+/-0 | 0.0+/-0.0 | 0.0+/-0.0 | 9.3+/-0.0 | 0.0+/-0.0

3. Very large sparse 64-step raster (smaller raster step).

3600111760 | Very large sparse 64-step raster 63x175 64s Mg II h/k Deep x 15 Spati | 1048.26 | 495.26 | 0.32 | 16.4+/-0.0 | 1048+/-0 | 0.0+/-0.0 | 0.0+/-0.0 | 16.4+/-0.0 | 0.0+/-0.0

4.1. Very large sparse 32-step raster (high telemetry).

3610609749 | Very large sparse 32-step raster 31x175 32s Mg II h/k Deep x 8 Spatia | 296.83 | 185.99 | 0.73 | 9.3+/-0.0 | 297+/-0 | 0.0+/-0.0 | 0.0+/-0.0 | 9.3+/-0.0 | 0.0+/-0.0

4.2. Small telemetry version of 4.1. OBSID.

3600609749 | Very large sparse 32-step raster 31x175 32s Mg II h/k Deep x 8 Spatia | 296.83 | 185.99 | 0.43 | 9.3+/-0.0 | 297+/-0 | 0.0+/-0.0 | 0.0+/-0.0 | 9.3+/-0.0 | 0.0+/-0.0

Additional instrument coordination:
coordination with NVST, Bialkov and Ondrejov