Routine Space Environment Product (Daily)
Issued by NWS

Home |  Current Version |  Previous Version |  Graphics & Text |  Print | Product List |  Glossary On
Versions: 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16
831
FXXX12 KWNP 171231
DAYDIS

:Product: Forecast Discussion
:Issued: 2024 Jul 17 1230 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC contact on the Web
# http://www.swpc.noaa.gov/wwire.html
#
#             Forecast Discussion
#
Solar Activity

.24 hr Summary...
Solar activity reached high levels as Region 3738, no longer visible,
produced and X1.9/1B flare (R3-Strong) at 16/1326 UTC. Accompanying the
flare were Type II (398 km/s) and Type IV radio sweeps, a Castelli U
radio signature, as well as a CME off the W limb beginning at 16/1336
UTC in SOHO/LASCO C2 imagery. Analysis of the CME showed no
Earth-directed component.

Next, Region 3753 (N11W50, Dai/beta) produced a M1.6/1N flare at 16/2124
UTC, and Region 3744 (N16W30, Cao/beta) responded with a M1.9 flare at
16/2206 UTC. Type II and IV radio sweeps were reported by USAF
observatories in association with the M1.9 flare event. However, both of
these flares appear have to produced faint shock as observed by SOHO
LASCO C2 imagery first seen just before 16/2312 UTC. Modeling of these
events suggests mostly shock arrival first by midday on 20 Jul followed
by a second shock arrival early on the 21st.

Finally, Region 3743 (S09W44, Eai/beta) was the culprit of a M5.0/2B
flare at 17/0639 UTC, which was quickly followed by an additional M3.4
flare at 0708 UTC. Both flares were accompanied by type II radio sweeps
with the former having a tenflare of 560 SFU and a type IV sweep as
well. Although, GOES SUVI 304 imagery suggests the presence of ejecta
from the M5 flare event, we currently await updated SOHO LASCO
coronagraph imagery to preform a proper analysis to determine the
presence of any Earth-directed CME.

.Forecast...
Solar activity is likely to be moderate (R1-R2, Minor-Moderate) with a
chance for further X-class flares (R3, Strong) on 17 Jul. X-class flare
probabilities are expected to decrease to a slight chance on 18-19 Jul
as Region 3738 rotates further around the W limb.

Energetic Particle

.24 hr Summary...
The greater than 2 MeV electron flux was at normal to moderate levels
and the greater than 10 MeV proton flux was steady at background levels.

.Forecast...
The greater than 2 MeV electron flux is expected to be at normal to
moderate levels on 17-19 Jul. There is a chance for S1 (Minor) storm
levels on 17 Jul due to the location and flare potential of Region
3738. As region 3738 rotates further around the west limb on 18-19 Jul,
probabilities decrease to a slight chance.

Solar Wind

.24 hr Summary...
Solar wind parameters reflected waning CME influence. Total field
decreased from 14 nT to 6-7 nT, and the Bz component was mostly benign.
Solar wind speeds gradually increased to near 400 km/s before gradually
decreasing to ~360 km/s. Phi angle was predominantly positive.

.Forecast...
Solar wind parameters are expected to continue to diminish through the
remainder of 17 Jul. By mid to late on 18 Jul, conditions are likely to
become enhanced due to the onset of a negative polarity CH HSS.

Geospace

.24 hr Summary...
The geomagnetic field was quiet to unsettled.

.Forecast...
Quiet to unsettled levels are expected through 19 Jul with active
periods likely on 18 Jul due to the onset of a negative polarity CH HSS.