Proposed SOOP Coordinators
R. Gomez Herrero, A. Vourlidas, S. Krucker, T. Horbury, C. Owen, A. Walsh
This SOOP is aimed at measuring variability in SEP events trough corona and heliosphere. IS instruments provide continuous observations while SoloHI gives spatial context.
Default SOOP duration: 10 days
Pointing requirements: disk centre
|SoloHI||SoloHI Shock or Turbulence and Synoptic modes||The distance to the sun will define the SoloHI mode: shock and turbulence mode, in combi with HI_SYN_PER to be scheduled only within 0.4AU, further out only synoptic modes (HI_SYN_NEAR or HI_SYN_FAR).|
|STIX||STIX Normal Mode||Needed only for 126.96.36.199|
|EPD||Triggered Burst Mode|
|MAG||MAG Normal Mode and MAG Burst Mode|
|RPW||RPW Normal Mode and RPW Burst Mode|
|SWA||SWA Triggered Mode or SWA Burst Mode (Scheduled)|
(e.g., orbital requirements, solar cycle phase, quadrature ...)
|188.8.131.52.3 Warped shock fronts|
Corona + Heliosphere
Gradual SEP events
Good radial spread.
Multiview point data preferred to address this objective
IS Triggered burst
Magnetic field, plasma wave and solar wind measurements to determine turbulence levels and identify shock passages
Good radial spread.
SoloHI is used with Solarprobe (turbulence mode).
Burst Modes: scheduled or triggered.
MAG: high-cadence magnetic field
RPW: high-cadence electric and magnetic field, power spectral densities
184.108.40.206 Measurements of SEP events time profiles and anisotropy in order to probe solar wind turbulence
|Statistics||Close to perihelion and different range of distances|
Needs to be done for a range of distances to monitor the SEP contributions from solar source and IP turbulence
SoloHI Turbulence mode
Also partly addressed by I_DEFAULT or L_IS_STIX.
|3.2.3 Properties of near-Sun shocks, their fluctuations and particle acceleration||Corona + Heliosphere|
MAG burst mode (good trigger needed)
SWA burst mode (triggered)
SoloHI Shock mode
Anik De Groof
SOOP ID in SOOP Kitchen = LI2