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1.2.1.2 Energy and mass flux in the corona. Loss in form of conduction, radiation, gravitational enthalpy, and kinetic energy fluxes into the accelerating solar wind plasma.

 

 

Operational requirements table: 

This table will be filled before the SAP meeting (16-17 November), please come back later!

 

Requirement
YES / NO / Not required / MAYBE / GOOD TO HAVE / NUMBERS
Remarks
Duration of the observations  
Perihelion  
RS window  
High latitude  
Solar cycle dependence  
Radial dependence  
Linkage science  
Multiple orbits  
Far side observations  
Earth observations  
EMC Quiet  
SPP  
Instruments 

 

 


Required observations:

  • SWASWA Normal Mode, A few hours of connected observations, other instruments: ALL.
  • MAGMAG Normal Mode.
  • EUIEUI synoptic mode (S). Modes Q (EUI Quiet Sun mode (Q)), C (EUI Coronal hole mode (C)) and A (EUI Active Region mode (A)) with min observation time 1h ( ? ). HRI Ly-alpha, 174 (FSI 304 with same cadence?). Other instruments: SPICE.
  • PHI

    FDT medium  resolution data

    Requirement

    FOV [pixels]

    1024 x 1024

    Parameters

    Ic, vLOS, B

    duration

    10 days

    cadence

    1/(10 min)

    N orbits

    2

    solar distance

    entire orbit

    PHI operating mode

    2

    co-ordination

    ?

  • METIS
    • Measurement of the solar wind outflow velocity gradient in the outer corona, to localise regions of energy deposition, via Doppler dimming of the HI Lyα intensity in the field of view 1.5-2.9 degrees. Measurement of the magnetic field topology through the global corona configuration. Measurements of the brightness fluctuation spectra.
    • Products:
      • Global maps of outflow velocity in corona.
      • Global maps of the electron density in corona/coronal configuration.
      • Brightness fluctuation spectra.
    • Modes:
      • WIND (min. obs time 2 hr, data volume ≤ 300 Mb)
      • MAGTOP (min. obs time 2 hr, data volume ≤ 480 Mb)
            Repeated each day in available observation windows.
      • FLUCTS (min. obs time 1 hr, data volume  ~ 2 Gb) at perihelion. 
    • Other instruments: PHI, EUI, SPICE, STIX.
  • All instruments.

Duration:

  • A few hours of connected observations.

Other constraints:

  • Connected observations.

 

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