=================================== Weekly Space Weather Highlights =================================== Highlights of Solar and Geomagnetic Activity 03 - 09 May 2021 Solar activity was at very low to moderate levels. Region 2822 (N18, L=335, class/area Dsi/180 on 09 May) rotated onto the visible disk on 07 May and produced an M3/1n flare at 07/1904 UTC. Associated with this flare were type II (816 km/s) and Type IV radio sweeps as well as a non-Earth directed CME. C-class flares were observed on 08-09 May, including a long duration C2/Sf flare at 09/1449 UTC with an associated Type II (407 km/s) radio sweep and another CME beginning at 09/1436 UTC in SOHO/LASCO C2 imagery. A faint, partial-halo CME was also observed on 09 May associated with a 15 degree filament eruption centered near S22E10. The CME was first observed in C2 imagery beginning at 09/1124 UTC. The two CMEs from 09 May are being analyzed at the time of this report with the potential for at least one having an Earth-directed component. No proton events were observed at geosynchronous orbit. The greater than 2 MeV electron flux at geosynchronous orbit was at normal to moderate levels through the period. Solar wind parameters were weakly enhanced on 03-05 May under a positive polarity CH HSS. Solar wind speed increased to a maximum of 498 km/s at 03/2351 UTC while total field reached a maximum of 13 nT at 03/0500 UTC. The Bz component was mostly positive during this time resulting in quiet conditions. By midday on 05 May, solar wind speed had decreased to under 350 km/s and remained so through 09 May. Quiet conditions were observed for the rest of the period. Forecast of Solar and Geomagnetic Activity 10 May - 05 June 2021 Solar activity is expected to be very low to low with the chance for further M-class flares on 10-19 May as Region 2822 rotates across the visible disk. Very low to low levels are expected on 20-27 May with the return of old Region 2821 (S21, L=226). Very low levels are expected on 28 May-01 Jun. Very low to low levels are expected again on 02-05 Jun as Region 2822 rotates around the east limb. No proton events are expected at geosynchronous orbit. The greater than 2 MeV electron flux at geosynchronous orbit is expected to be reach high levels on 16-19 May and again on 21-24 May due to recurrent CH HSS influences. Geomagnetic field activity is expected to reach unsettled levels on 10, 12-13, 15-18, 20-21 May. Active levels are expected on 15-17 and 20 May and G1 (Minor) storm levels are likely on 16 May due to recurrent CH HSS effects.