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OK0NAG > SOLAR 01.09.11 13:33l 101 Lines 3484 Bytes #999 (0) @ EU
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_____________________________________________________________________
Solar-activity forecast for the period Sep 2 - 8, 2011
Activity level: mostly very low to low
Radio flux (10.7 cm): a fluctuation in the range 115-90 f.u.
Flares: weak (4-12/day), middle (0-1/period)
Relative sunspot number: in the range 80-110
Astronomical Institute, Solar Dept., Ondrejov, Czech Republic
e-mail: sunwatch(at)asu.cas.cz
(RWC Prague)
_____________________________________________________________________
Geomagnetic activity forecast for the period Sep 2 to Sep 8.
quiet: Sep 2 to Sep 8
quiet to unsettled: Sep 4
unsettled: Sep 3
active: 0
minor storm: 0
major storm: 0
severe storm: 0
Geomagnetic activity summary:
geomagnetic field was quiet from Aug 26 to Aug 31.
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 7, 9, 13 - 14, 16 - 17, 21, 27 - 28
mostly quiet: Sep 5 - 6, 8, 15, 18, 20, 22, 24, 26
quiet to unsettled: Sep 2, 4, 10 - 12, 19, 23, 25
quiet to active: Sep 19
quiet to minor storm: -
quiet to major storm: Sep 3
mostly unsettled: -
unsettled to active: -
unsettled to minor storm: -
active to minor storm: -
active to major storm: -
minor to major storm: -
Survey: quiet: Aug 30 - 31
mostly quiet: Aug 25, 27 - 28
quiet to unsettled: Aug 26, 29
quiet to active: Aug 23 - 24
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
Sep 3, (8 - 10,) 11 (- 12), 18 - 19, 24.
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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