Прогноз Космічної Погоди - Обговорення
Випущено: 2024 May 17 0030 UTC
Надано Міністерством торгівлі США, NOAA, Центром прогнозування космічної погоди і опрацьовано SpaceWeatherLive.com
Сонячна активність
Підсумок за добу
Solar activity decreased to moderate levels. Newly numbered AR3685
(S13E64, Dso/beta-gamma) produced an M1.0 flare at 16/0804 UTC, which
was the largest of the period, as it began to rotate into view on the
eastern limb. Region 3679 (S10E18, Eso/beta-gamma) grew in overall size
while becoming somewhat less magnetically complex, losing the weak delta
signature in its leading penumbra. This active region was responsible
for a hand full of C-class flares, the largest of which was a C5.0 at
16/0634 UTC. Region 3672 (N18W37, Cao/beta) showed signs of evolution as
it gained new leading spots and produced a C4.0 flare at 16/0506 UTC.
Region 3674 (S12W03, Cso/beta) underwent evolution as well, gaining
pores and trailing spots, and was the culprit of a C3.2 flare at 16/1252
UTC.
An erupting filament structure was observed in GONG HA imagery beginning
at approximately 16/1500 UTC near N10W32. An apparent, subsequent CME
can be seen first in LASCO C2 coronagraph imagery just before 16/1800
UTC. Analysis and modeling of this event is currently underway to
determine any Earth-directed component.
Прогноз
Solar activity is expected to continue at moderate levels with a chance
for M-class flare activity (R1-2/Minor-Moderate radio blackouts) and a
slight chance for an isolated X-class flare event (R3 Strong radio
blackouts) through 19 May.
Заряджені Частинки
Підсумок за добу
The greater than 10 MeV proton flux was at S1 (Minor) solar radiation
storm levels with a peak flux of 22.3 pfu at 16/1115 UTC. The 2 MeV
electron flux was at normal to moderate levels.
Прогноз
The greater than 10 MeV proton flux is expected to gradually return to
near background levels over the course of 17 May and remain there
through the forecast period. The greater than 2 MeV electron flux is
expected to remain at normal to moderate levels through 19 May.
Сонячний Вітер
Підсумок за добу
Solar wind parameters were indicative of CME influences, likely from the
parting shot on the western limb from AR3664 back on 13 May. Total field
reached a peak of 17 nT at approximately 16/0611 UTC. During this time,
the Bz component underwent a sustained southward deflection of -6 to -13
nT. Solar wind speeds also increased slightly during this time to around
500 km/s before gradually decreasing to ~385 km/s. Phi became variable
beginning around 16/0705 UTC and became predominantly negative after
16/1355 UTC.
Прогноз
An additional enhancement is likely on 17 May due to the arrival of
glancing influences of a CME from 14 May. Solar wind parameters are
expected to slowly relax over the course of 18 May before yet another
enhancement is likely, due to glancing influences of a CME from 15 May.
Геопростір
Підсумок за добу
The geomagnetic field reached G2 (Moderate) storm levels.
Прогноз
Unsettled to active conditions are expected on 17 May due to glancing
CME effects from the 14 May CME. Quiet to unsettled levels are expected
on 18 May as any lingering effects weaken. Unsettled to active
conditions are expected once again on 19 May, this time due to glancing
CME effects from the 15 May CME. It should be noted that there is a
chance for isolated G1 (Minor) geomagnetic storming periods on 17 and 19
May due to any stronger than anticipated CME effects.