Location of evaporation flows

Temperature of upflowing plasma

Location of hightest Vnt value

Measurement of reconnection inflow & outflow

Spatially resolving Doppler flows, line

broadenings to look for properties to compare

with predictions of models e.g. wave heating,

reconnection models.

High Doppler shifts, Vnt etc

Plumes, network brightenings, diffuse corona

with the aim of understanding solar wind

acceleration and coronal heating.