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OK0NAG > SOLAR 08.09.11 13:48l 102 Lines 3558 Bytes #999 (0) @ EU
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_____________________________________________________________________
Solar-activity forecast for the period Sep 9 - 15, 2011
Activity level: mostly low to moderate
Radio flux (10.7 cm): a fluctuation in the range 95-120 f.u.
Flares: weak (3-10/day), middle (1-3/period), large (0-2/period)
Relative sunspot number: in the range 80-100
Astronomical Institute, Solar Dept., Ondrejov, Czech Republic
e-mail: sunwatch(at)asu.cas.cz
(RWC Prague)
_____________________________________________________________________
Geomagnetic activity forecast for the period Sep 9 to Sep 15, 2011
quiet: Sep 14 and 15
quiet to unsettled: Sep 13
unsettled: Sep 12
active: Sep 11
minor storm: Sep 9 and 10
major storm: 0
severe storm: 0
Geomagnetic activity summary:
geomagnetic field was quiet on Sep 1, 2, 5, 6 and 7,
unsettled on Sep 3 and 4.
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: Sep 15 - 18, 27 - 28
mostly quiet: Sep 13 - 14, 26, 29
quiet to unsettled: Sep 19, 24 - 25
quiet to active: Sep 11 - 12, Oct 4 - 5
quiet to minor storm: Sep 9, 20
quiet to major storm: -
mostly unsettled: -
unsettled to active: Sep 21 - 23, 30, Oct 1 - 3
unsettled to minor storm: Sep 10
active to minor storm: -
active to major storm: -
minor to major storm: -
Survey: quiet: Aug 31, Sep 1
mostly quiet: Sep 6
quiet to unsettled: Sep 2, 4 - 5, 7
quiet to active: -
quiet to minor storm: -
quiet to major storm: -
mostly unsettled: Sep 3
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
Sep 9 - 12, 18 - 19, 24, 29, Oct 1.
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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