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3.1.2.4 Explore the fact that only some of the hard X-ray peaks are related to escaping electrons, while others are not (Benz et al., 2005).

 

Required observations:

  • SWASWA Normal Mode, several hours, perihelion, other instruments: RPW, MAG, EPD, STIX.
  • MAGMAG Normal Mode
  • STIX
  • EUIFSI Synoptic mode (S). EUI FD 174, 304, cadence 10 min. EUI HR 174 and Ly-alpha, cadence 1 min for 30 min before and during X-ray peak.
  • EPD: All sensors: spectra, composition, fluxes, directional information, together with IS instruments. Solar source identification by RS instruments (full disk imaging). Also coordinated multi-s/c SEP observation campaigns with SPP & other missions.

Duration:

  • Several hours.

Other constraints:

  • Perihelion.