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Fig. 5

image

Joint density distribution between TEVs inferred from HO and HO spectra measured by the MIRO instrument. In this summary plot, all data (from August 2014 until July 2016) are shown excluding cases of low S/N based on the line area. Although there is a strong correlation it is apparent that the HO spectra yield higher velocity for a considerable fraction of the dataset (see text for details).

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