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ON THE IMPORTANCE OF POLARIZATION IN HELIOSPHERIC IMAGERS S. J. Tappin RAL Space Introduction ● ● ● Heliospheric imagers, have been shown to be a powerful tool for tracking CMEs (and other solar wind structures) through the heliosphere. Hitherto they have only detected total intensity. Coronagraphs

, AM mo wind S, li rain many, mo vis, PM mo wind SW, good, NIGHT li wind SE, clear - KMD LV Tue Jul 29:1.AM ,li wind E,good,.PM,mo wind NW, mo rain many, poor,NIGHT, li wind var,2, AM li wind SE, li rain few, mo vis.PM mo wind W, good,NIGHT li wind E,p/cloud - KMD Example of hazard warning message LV

indicates the similarities between the scenarios. Table 2 SRES scenarios that are most similar to the new RCPs, in terms of median global temperature increase by 2100 References Caesar, J., Palin, E., Liddicoat, S et al. Response of the HadGEM2 Earth System Model to Future Greenhouse Gas Emissions Pathways

as the average temperature increases cold extremes currently can and do still occur, for example the ’Beast from the East’ in 2018 resulted in the coldest March day on record with a maximum of -4.7 °C recorded at Tredegar in South Wales. However, during the 2010’s these occurrences have been outnumbered