[Ips-dsgr] ASWFC Daily Report - 24 March 25 issued 2330 UT on 24 Mar 2025 [SEC=OFFICIAL]
Australian Space Weather Forecasting Centre
aswfc at bom.gov.au
Tue Mar 25 10:30:49 AEDT 2025
SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/24 MARCH 2025
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 24 MARCH AND FORECAST FOR 25 MARCH - 27 MARCH
STATUS INDICATORS SOL:** YELLOW ** MAG:** YELLOW ** ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 24 Mar: R0
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 24 Mar: 156/110
1B. SOLAR FORECAST
25 Mar 26 Mar 27 Mar
Activity R0, chance R1 R0, chance R1 R0, chance R1
Fadeouts None expected Possible Possible
10.7cm/SSN 162/116 165/119 160/114
COMMENT: Solar activity on UT day 24-Mar was R0, with no significant
solar flares. There are currently four numbered sunspot regions
on the solar disk. AR4036 (N07W64, beta-gamma) has grown over
the past day, however due to its location nearing the western
limb analysis is restricted. All other sunspot regions are either
stable or in decay. Solar activity is generally expected to be
R0, with isolated R1 flares possibly from AR4036. Apart from
AR4036 no regions currently have significant flare potential.
S0 solar radiation storm conditions were observed on UT day 24-Mar.
S0 solar radiation storm conditions are expected over 25-27 Mar.
No Earth-directed CMEs were observed on UT day 24-Mar. The solar
wind environment was mildly perturbed on UT day 24-Mar. The solar
wind speed ranged from near 450 to 350 km/s. The peak total interplanetary
field strength (IMF, Bt) was 15 nT and the north-south IMF component
range (Bz) was +10 to -9 nT. Bz was oriented southward for several
periods of the day. The source of the disturbance is not clear,
but is not considered CME related at this stage. The solar wind
environment is expected to be quiet for most of UT day 25-Mar,
but a large coronal hole dominating the southern solar hemisphere
may connect with the Earth over 26-27 Mar to enhance the solar
wind speed.
-----------------------------------------------------------
2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 24 Mar: G0
Estimated Indices 24 Mar : A K
Australian Region 11 33233321
Cocos Island 8 23232310
Darwin 11 33233321
Townsville 14 34333322
Learmonth 14 33333422
Alice Springs 12 33233322
Gingin 13 33233421
Canberra 11 33233321
Kennaook Cape Grim 14 33333421
Hobart 14 33333421
Estimated Antarctic Regional K Indices 24 Mar :
Macquarie Island 17 23344431
Casey 19 35532222
Mawson 35 66433443
Observed Regional daily pc3 Indices 24 Mar :
Darwin 0 (Quiet)
Townsville 0 (Quiet)
Learmonth 0 (Quiet)
Alice Springs 0 (Quiet)
Gingin 6 (Quiet)
Canberra 0 (Quiet)
Pc3 pulsations are high frequency (10-45 second period) variations
of the Earths magnetic field. Daily pc3-indices are the daily sum
of 20 minute pc3-indices for that station and have been shown to be
well correlated with rejection of high resolution aeromagnetic
survey flight-line data.
NOTE: Indices may have been generated from data obtained in
cooperation with the following organisations: Geoscience Australia,
University of Newcastle Space Physics Group, Australian Government
Antarctic Division and International Center for Space Weather
Science and Education, Japan.
Estimated AFr/Ap Indices 24 Mar : A
Fredericksburg 17
Planetary 23
Observed AFr/Ap Indices 23 Mar : A K
Fredericksburg 9
Planetary 12 3242 3322
2B. MAGNETIC FORECAST
Date Ap Conditions
25 Mar 13 G0, chance G1
26 Mar 18 G0-G1
27 Mar 22 G0-G1, chance of G2
COMMENT: ASWFC Geomagnetic Warning 21 was issued on 23 March
and is current for 25-27 Mar. G0 geomagnetic activity was observed
in the Australian region on UT day 24-Mar. G0-G2 geomagnetic
conditions were observed in the Antarctic region. G0 geomagnetic
conditions are expected on UT day 25-Mar, then bouts of G1 are
expected over 26-27 Mar due to the anticipated connection with
the large coronal hole currently dominating the southern solar
hemisphere.
-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
24 Mar Normal-fair Normal Fair
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
25 Mar Normal Normal Normal-fair
26 Mar Normal Normal-fair Fair
27 Mar Normal-fair Fair Fair-poor
COMMENT: HF radio propagation conditions were generally good
in the first half of the UT day 24-Mar, but became mildly depressed
in the latter half, especially in the southern hemisphere. HF
radio propagation conditions are expected to be normal on 25-Mar,
but some degradations and depressions may begin on 26-Mar in
high latitudes, and then further latitudes on 27-Mar due to expected
coronal hole activity.
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
24 Mar 148
Observed Australian Regional MUFs
Cocos Island Region:
Enhanced by 20% during local day.
Enhanced by 55% during local night.
Enhanced by 20% after local dawn.
Niue Island Region:
Mostly near predicted monthly values.
Enhanced by 20% after local dawn.
Northern Australian Region:
Enhanced by 15% during local day.
Enhanced by 15% during local night.
Southern Australian Region:
Enhanced by 15% during local day.
Enhanced by 15% during local night.
Antarctic Region (Casey/Davis/Mawson):
Depressed by 25% over the UT day.
Monthly T index:
Month T index
Feb 127
Mar 117
Apr 114
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
25 Mar 155 Near predicted monthly values to 15% enhanced
26 Mar 145 Near predicted monthly values to 15% enhanced
27 Mar 135 Near predicted monthly values to 20% depressed
COMMENT: Maximum usable frequencies (MUFs) in the Australian
region were mostly enhanced by 15% on UT day 24-Mar. Spread-F
was observed in Hobart during local night hours and sporadic-E
was observed in Norfolk Island. The enhancements to the MUFs
are expected to continue on 25-Mar, and possibly dampen on 26-Mar
but may still be intermittent. MUFs may become depressed up to
20% on UT day 27-Mar due to expected coronal hole activity.
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 23 Mar
Daily Proton Fluence >1 MeV: 4.0E+05
Daily Proton Fluence >10 MeV: 1.7E+04
Daily Electron Fluence >2 MeV: 9.20E+06 (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 2%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
X-ray background: C1.3
DSCOVR Satellite Solar Wind Day Averaged Data for 23 Mar
Speed: 428 km/sec Density: 7.6 p/cc Temp: 95000 K Bz: -1 nT
(Courtesy Space Weather Prediction Center, Boulder USA)
-----------------------------------------------------------
Australian Space Weather Forecasting Centre
Bureau of Meteorology
ASWFC at bom.gov.au
www.bom.gov.au | www.sws.bom.gov.au
More information about the ips-dsgr
mailing list