Source regions of the slow solar wind
- 1.1.2.1 Does slow wind originate from the over-expanded edges of coronal holes?
- 1.1.2.2 Does slow and intermediate solar wind originate from coronal loops outside of coronal holes?
- 1.1.2.3 Abundance of minor ions as a function of height in the corona as indicator of slow or fast wind
- 1.1.2.4 Study of density fluctuations in the extended corona as a function of the outflow velocity of the solar wind while evolving in the heliosphere
- 1.1.2.5 Structure and evolution of streamers
- 1.1.2.6 Disentangle the spatial and temporal variability of the slow wind
- 1.1.2.7 Trace streamer blobs and other structures through the outer corona and the heliosphere.
- 1.1.2.8 Determine the velocity, acceleration profile and the mass of the transient slow wind flows
Relevant SOOPs:
L_SMALL_MRES_MCAD_Composition-Mosaic