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VA2OM > SOLAR 11.05.90 11:24l 69 Lines 3030 Bytes #999 (0) @ WW
BID : 7970_VE2PKT
Read: GUEST
Subj: Solar and Geomagnetic Activity
Path: IW8PGT<IZ3LSV<IK6IHL<IK7NXU<HB9ON<DK0WUE<PI8ZTM<PD1NL<PD0LPM<VE3CGR<
WG0A<N5MDT<VK3AT<VE2PKT
Sent: 260511/0916Z 7970@VE2PKT.#TRV.QC.CAN.NOAM LinBPQ6.0.25
:Product: Weekly Highlights and Forecasts
:Issued: 2026 May 11 0150 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC contact on the Web
# https://www.swpc.noaa.gov/content/subscription-services
#
# Weekly Highlights and Forecasts
#
Highlights of Solar and Geomagnetic Activity
04 - 10 May 2026
Solar activity reached high levels on 10 May due to an M5.7/2b flare
(R2-Moderate) at 10/1339UTC from Region 4436 (N19, L=330,
class/area=Dao/beta on 10 May), the strongest of the period.
Associated with the event was a Type II radio sweep (est. 650 km/s),
Tenflare (550sfu), and a CME signature first observed in coronagraph
imagery at 10/1348UTC towards the NE. Analysis and modeling of the
event is ongoing at the time of this writing.
Region 4424 (N17, L=192, class/area=Eai/160 on 30 Apr) also produced
an M-class event with an M1.8 flare (R1-Minor) observed at 04/0133
UTC. The other 10 numbered active regions on this visible disk were
either mostly quiet or only produced C-class activity during the
past week
No proton events were observed at geosynchronous orbit.
The greater than 2 MeV electron flux at geosynchronous orbit was at
normal to moderate levels throughout the summary period.
Geomagnetic field activity reached G2 (Moderate) geomagnetic storm
levels on 04 May and G1 (Minor) levels on 05 May due to influence
from a passing CME. Total magnetic field strength only reached a
peak of 11 nT during that time but Bz rotated as far southward as
-10 nT and was sustained southward from late on 04 May through
midday on 05 May. Despite the influence of a positive polarity
coronal hole beginning late on 07 May, the mostly northward Bz
component results in only quiet to unsettled conditions through the
end of the reporting period.
Forecast of Solar and Geomagnetic Activity
11 May - 06 June 2026
Solar activity is expected to be at low levels, with a chance for
M-class activity (R1/R2-Minor/Moderate), and a slight chance for
X-class (R3-Strong), throughout the outlook period due to the flare
potential of several active regions both currently on the visible
disk and those expected to return from the Sun's farside.
No proton events are expected at geosynchronous orbit.
The greater than 2 MeV electron flux at geosynchronous orbit is
expected to be at high levels on 17-20 May due to influence from a
recurrent, negative polarity coronal hole. The remainder of the
outlook period is likely to be at normal to moderate levels.
Geomagnetic field activity is likely to reach G1 (Minor) geomagnetic
storm levels over 15-17 May; active conditions are likely on 18 May,
23 May, 27 May, and 03 Jun; unsettled conditions are likely over 11
May, 13 May, 21-22 May, and 28 May - 31 May. All enhancements in
geomagnetic activity are due to the anticipated influence of
multiple, recurrent, coronal hole HSSs. The remainder of the outlook
period is likely to be at mostly quiet levels.
73 de VA2OM, SYSOP of VE2PKT
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