Solar activity continued at very low levels. Region 296 (N13W18), a relatively large and moderately complex region, has been dormant for the duration of its transit on the visible disk. This region was in a slow decay phase over the past few days, but still shows some complexity. Region 301 (N22W05) though small, is in a slow growth phase, and exhibited considerable plage fluctuations and minor surging throughout the period. Newly numbered Region 306 (N05E76) rotated into view this period; a relatively large sunspot group is evident, but limb proximity hinders a more thorough analysis. This region was the likely source of a large CME observed off the NE limb early on 6 March. Three other new sunspot groups emerged today and were numbered as 303 (S18W47), 304 (S13W16), and 305 (S22E27).

Solar activity is expected to be low. Regions 296, 301, and 306 all have potential for C-class flares. There is a slight chance for an M-class flare from Regions 296 and 306.

The geomagnetic field was quiet to active. Isolated active periods were observed during local nighttime hours at all latitudes. The high speed coronal hole stream responsible for the disturbed periods over the past few days has gradually declined to near normal levels. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels again today.

The geomagnetic field is expected to be predominantly quiet to unsettled. Isolated active periods are possible at mostly higher latitudes.

  Спостережуваний       07 Mar 150
  Прогнозований   08 Mar-10 Mar  155/160/160
  Середнє значення за останні 90 днів        07 Mar 142

  Спостережуваний Afr/Ap 06 Mar  015/025
  За оцінками     Afr/Ap 07 Mar  012/012
  Прогнозований    Afr/Ap 08 Mar-10 Mar  010/012-010/012-008/010