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OK0NAG > SOLAR 12.05.11 13:15l 96 Lines 3511 Bytes #999 (0) @ EU
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_____________________________________________________________________
Solar-activity forecast for the period May 13 - 19, 2011
Activity level: very low to low
Radio flux (10.7 cm): a fluctuation in the range 85-115 f.u.
Flares: weak (1-10/day)
Relative sunspot number: in the range 22-40
Astronomical Institute, Solar Dept., Ondrejov, Czech Republic
e-mail: sunwatch(at)asu.cas.cz
(RWC Prague)
_____________________________________________________________________
Geomagnetic activity forecast for the period May 13 to May 19, 2011
quiet: May 14
quiet to unsettled: May 13, 15 and 19
unsettled: May 16, 17 and 18
active: 0
minor storm: 0
major storm: 0
severe storm: 0
Geomagnetic activity summary:
geomagnetic field was quiet from May 5 to 9 and 11,
unsettled on May 10.
RWC Prague, Geophysical Institute Prague, Geomagnetic Dept,
Czech Republic
e-mail: geom(at)ig.cas.cz
_____________________________________________________________________
Geomagnetic activity forecast for the period of one solar rotation
Geomagnetic field during the following solar rotation should be:
quiet: May 13 - 14, 18 - 21, 23 - 25, 31, June 2, 4 - 6
mostly quiet: May 30, June 1
quiet to unsettled: May 22, 26 - 27, June 3
quiet to active: May 15 - 17
quiet to minor storm: -
quiet to major storm: -
mostly unsettled: -
unsettled to active: -
unsettled to minor storm: May 29, June 7
active to minor storm: -
active to major storm: May 28
minor to major storm: -
Survey: quiet: May 4, 6, 11
mostly quiet: May 8 - 9
quiet to unsettled: May 5, 7
quiet to active: May 10
quiet to minor storm: -
quiet to major storm:
mostly unsettled: -
unsettled to active: -
unsettled to minor storm: -
active to minor storm: -
active to major storm: -
minor to major storm: -
Notices:
High probability of changes in solar wind which may caused
changes in magnetosphere and ionosphere is expected about
May 15 - 17 and 20 - 21, (22, 25,) 27 - 28, June 6 - 7
Days in brackets refer to a lower probability of possible
activity enhancements depending on previous development
on the Sun.
F. K. Janda (OK1HH), Czech Propagation Interested Group
e-mail: ok1hh(at)rsys.cz
_____________________________________________________________________
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