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General description

The goal of this SOOP is to investigate the role of the small scales dynamics events in the frame of energy transport, deposition and dissipation in the corona. This includes to investigate the origin of small scales instabilities at the origin of eruptions. This SOOP can be used to investigate single events or do statistical studies. The target should vary in way to cover different coronal environments.


Observations requirement (baseline)


InstrumentModeComment

EUI

FSI synoptics
HRIs at < 10s cadence

HRIs cadence can vary within
a SOOP to allow longer time sequences

SPICE

High cadence dynamic study


STIX

Normal or high cadence mode


PHI

HRT at high cadence


Science objectives


SAP objectiveTargetDurationOpportunity
(e.g., orbital requirements, solar cycle phase, quadrature ...)

Operational constraints 

Additional comments

1.2.1.3 Contribution of flare-like events on all scales

AR

3h

Perihelion, alignment with Earth, quadrature

All high cadence instruments work together


1.2.1.5 Determine whether coronal heating is spatially localized or uniform, and time steady or transient or impulsive for a wide range of magnetic loops with different spatial scales.

AR, QS, CH

3h

Perihelion, alignment with Earth, quadrature

All high cadence instruments work together


1.2.1.6 Resolve the geometry of fine elemental loop strands

AR

1h

Perihelion, alignment with Earth, quadrature

All high cadence instruments work together


1.2.1.7 Detect and characterise waves in closed and open structures

AR, QS, CH

3h

Perihelion, alignment with Earth, quadrature

All high cadence instruments work together


1.2.1.8 Investigate the role of small scale magnetic flux emergence in energizing the above laying layers

QS, AR

3h

Perihelion, alignment with Earth, quadrature

All high cadence instruments work together

Observation of the same target for several days

2.1 How do CMEs evolve through the corona and inner heliosphere?

Prominence

10h

Limb observations at perihelion, with Earth, quadrature.

All high cadence instruments work together


4.1.4 Study the influence of cancellations at all heights in the atmosphere / 4.3.5  How do magnetic fields emerge on the solar surface (coalescence, magnetic loops, convective collapse?)

Quiet Sun

6h

Perihelion, disk center and polar regions

All high cadence instruments work together


Instances run / planned

LTP6:

2022-03-07, 2022-03-08, 2022-03-17, 2022-03-30 (SOOP coordinators: S. Parenti, D. Berghmans)

LTP11:

2023-03-29 (SOOP coordinators: Hardi Pater - Susanna Parenti)
2023-04-04, 2023-04-05 (SOOP coordinators: Susanna Parenti)
2023-04-10: (SOOP coordinators: Luis Bellot-Rubio)
2023-04-15: (SOOP coordinators: Susanna Parenti (EUI), Terry Kucera (SPICE))

Science outcomes

Mandal et al. 2022, A&A, 656, 16
Chitta et al. 2022, A&A, 667, A166
Nelson et al. submitted

Original SOOP proposers

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1 Comment

  1. SOOP ID in SOOP Kitchen = RB1