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However up to now, we have only included it in R_SMALL_MRES_MCAD_AR-Long-Term, but this would only partially address it.

Relevant SOOPs:



    • Target: Coronal Holes, Quiet Sun, Active Region mainly on disk
    • Observing mode: Composition mapping (Doppler maps and composition) and Dynamics
    • Slit: 30” for Composition mapping and 4” for Dynamics
    • Exposure time/cadence and number of X positions: 180 s, X=32 for Composition mapping; 10 s, X=224 for Dynamics
    • Field of View: 16’×14’ for Composition mapping; 15’×11’ for Dynamics
    • Number of repetitions of the study: 1 for Composition mapping followed by 10 for Dynamic and 1 again for Composition mapping
    • Observation time: 1.6 hours for Composition mapping; 6.3 hours (0.63 hours per study) for Dynamics
    • Key SPICE lines to be included: Ne VIII 770 Å, Ne VIII 780 Å, Mg IX 706 Å, O II 718 Å, O IV 787 Å, O V 760.4 Å, O V 761 Å, O VI 1032 Å, O VI 1037 Å, Ne VI 999 Å, Ne VI 1010 Å, Mg VIII 772 Å, Mg VIII 782 Å, C III 977 Å, Fe III 1017 Å - 2 profiles and 13 intensities or 4 profiles and 11 intensities (maximum of 15) for Composition mapping;C III 977 Å, O VI 1032 Å, O VI 1037 Å, Ne VIII 770 Å – 10 lines (4 profiles and 6 intensities) for Dynamics 
    • Observing window preference: perihelion preferred
    • Other instruments: EUI, PHI, METIS, SoloHI, SWA, EPH, MAG
    • Comments: The choice of lines, and also the number of intensities and profiles, is flexible, although the sum of the intensities and profiles is constrained to a maximum (e.g 15 for composition mapping). While varying the number of intensities and profiles, within the maximum, has no effect on the duration of the study, it will have an effect on the telemetry.