OpenBCM V1.08-5-g2f4a (Linux)

Packet Radio Mailbox

IZ3LSV

[San Dona' di P. JN]

 Login: GUEST





  
OK1HH  > SOLAR    22.02.08 20:01l 60 Lines 1933 Bytes #999 (0) @ EU
BID : M2IOK0PPL05T
Read: GUEST
Subj: solar & geomagnetic activity forecast
Path: IZ3LSV<IW2OHX<I0TVL<DK0WUE<DB0RES<OK0PPL
Sent: 080222/1251z @:OK0PPL.#BOH.CZE.EU [Plzen JN69QR] obcm1.06
From: OK1HH @ OK0PPL.#BOH.CZE.EU (Franto)
To:   SOLAR @ EU
X-Info: No login password

_____________________________________________________________________

Solar-activity forecast for the period Feb 22 - 28, 2008

Activity level: very low
Radio flux (10.7 cm): a fluctuation in the range 67-73 f.u.
Flares: weak (0-3/day)
Relative sunspot number: in the range 0-22

Astronomical Institute, Solar Dept., Ondrejov, Czech Republic
e-mail: sunwatch(at)asu.cas.cz
(RWC Prague)
_____________________________________________________________________

Geomagnetic activity forecast for the period Feb 22 to Feb 28, 2008

quiet: Feb 22 to 26
quiet to unsettled: Feb 27
unsettled: Feb 28
active: 0
minor storm: 0
major storm: 0
severe storm: 0

Geomagnetic activity summary: geomagnetic field was quiet on
Feb 17 and 20, unsettled on Feb 14, 15, 16, 18 and 19.

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

unsettled to active: Feb (23,) Mar 2 (4,) 5, (6,) 9-11, 13(-14)
active to disturbed: Feb (24, 27,) 28, (29,) Mar 1, 8 (12, 16-17)
quiet: Feb (22,) 25-26, Mar (3, 7,) 15, 18

Survey: quiet -
        mostly quiet on: Feb 20
        quiet to unsettled on: Feb 17
        quiet to active on: Feb 14, 16, 18
        quiet to disturbed -
        mostly unsettled on: Feb 11-13, 15
        unsettled to active on: Feb 19
        unsettled to disturbed -
        mostly active -
        active to disturbed -
        disturbed -

   Notice: Days in brackets refer to a lower probability of possible
        solar activity enhancements depending on previous developments
        on the sun.

F. K. Janda, OK1HH, Czech Propagation Interested Group
e-mail: franta.janda(at)quick.cz
_____________________________________________________________________


Read previous mail | Read next mail


 18.10.2024 08:48:22lGo back Go up