[Ips-dsgr] SWS Daily Report - 17 April 22 issued 2330 UT on 17 Apr 2022 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Mon Apr 18 09:30:50 EST 2022


SUBJ: SWS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/17 APRIL 2022 BY Space Weather Services
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 17 APRIL AND FORECAST FOR 18 APRIL - 20 APRIL
STATUS INDICATORS SOL:** RED **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://www.sws.bom.gov.au
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 17 Apr:  R3 (strong)

Flares    Max     Fadeout    Freq.  Sectors
  M1.8    0211UT  possible   lower  E. Asia/Aust.
  X1.2    0334UT  probable   all    E. Asia/Aust.
  M1.5    2002UT  possible   lower  East Pacific/
                                    North American
  M4.4    2234UT  possible   lower  East Pacific/
                                    North American

Observed 10.7 cm flux/Equivalent Sunspot Number for 17 Apr: 135/89


1B. SOLAR FORECAST
             18 Apr             19 Apr             20 Apr
Activity     R1-R3              R1-R3              R1-R3
Fadeouts     Probable           Probable           Probable
10.7cm/SSN   135/89             130/84             130/84

COMMENT: On UT day 17 Apr, solar activity was at R3 (strong) 
levels due to an X1.1 flare at 0334 UT from newly numbered region 
2994 (N14E65, Dko/beta-gamma). The flare was associated with 
a type II sweep, coronal mass ejection (CME) and radio noise 
bursts. There were also three M-class flares on 17 Apr from AR2993 
(N22E65, Dho/beta) and AR2992 (S34W70). Solar activity is expected 
to be at R1-R2 (minor to moderate) levels with a chance of R3 
(strong) flare levels 18-20 Apr. The small filament eruption 
from near S45W62 at 16/2028 UT produced a slow CME but this is 
not expected to be geoeffective. The CME associated with the 
X1.1 flare may just graze Earth with possible arrival from late 
on 19 Apr. There was a southward CME first observed in LASCO 
C2 at 17/1636 UT but the origin is unclear. There is another 
CME first observed at 17/2012 UT to the southwest. The solar 
wind speed range was 450-580 km/s on 17 Apr, trending lower until 
~~2010 UT and is now near 530 km/s. The peak total interplanetary 
magnetic field strength (IMF Bt) was 11 nT and the north-south 
IMF component (Bz) range was +10/-8 nT. The solar wind speed 
is expected to remain elevated on 18 Apr due to coronal hole 
wind stream effects, returning to nearer background levels over 
19 Apr. There is a chance of a mild CME impact from late on 19 
Apr, otherwise, settled conditions are expected on 20 Apr.

-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 17 Apr: G0

Estimated Indices 17 Apr : A   K           
   Australian Region       6   12222222
      Darwin               6   12222212
      Townsville           7   22222222
      Learmonth            7   22222222
      Alice Springs        6   12222222
      Gingin               7   22222222
      Canberra             6   12222222
      Hobart               6   12122222    

Estimated Antarctic Regional K Indices 17 Apr :
      Macquarie Island     6   12131221
      Casey               12   34332222
      Mawson              21   44444323

Observed Regional daily pc3 Indices 17 Apr : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               6   (Quiet)
      Canberra            36   (Quiet to unsettled)
      Hobart              37   (Quiet to unsettled)

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 17 Apr : A 
           Fredericksburg        10
           Planetary             12                         

Observed AFr/Ap Indices 16 Apr :  A   K
           Fredericksburg         7
           Planetary              6   1011 3222     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
18 Apr    11    G0
19 Apr     9    G0 with slight chance of G1 (minor) conditions 
                late in the period
20 Apr     9    G0 with slight chance of G1 (minor) conditions

COMMENT: G0 geomagnetic conditions were observed in the Australian 
and Antarctic regions on UT day 17 Apr. Weak coronal hole wind 
stream effects are expected to persist on 18 Apr then subside, 
with G0 conditions likely 18-20 Apr. There is a chance of a minor 
(G1) disturbance from late on 19 Apr due to the 17 Apr CME that 
may graze Earth.

-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
17 Apr      Normal         Normal         Normal         

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
18 Apr      Normal         Normal         Normal-fair
19 Apr      Normal         Normal         Normal-fair
20 Apr      Normal         Normal         Normal-fair

COMMENT: HF conditions were near normal on 17 Apr at all latitudes. 
Propagation conditions are expected to be normal 18-20 Apr with 
short-wave fadeouts likely.

-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
17 Apr    66

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 30% during local day.
      Enhanced by 15% during local night.
   Niue Island Region:
      Enhanced by 35% during local day.
      Near predicted monthly values during local night.
      Enhanced by 20% after local dawn.
   Northern Australian Region:
      Enhanced by 20% during local day.
      Near predicted monthly values during local night.
   Southern Australian Region:
      Mostly near predicted monthly values.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Enhanced by 15% over the UT day.

Monthly T index:
Month  T index
Mar      64
Apr      46
May      49

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
18 Apr    75    Near predicted monthly values to 25% enhanced
19 Apr    75    Near predicted monthly values to 25% enhanced
20 Apr    75    Near predicted monthly values to 25% enhanced

COMMENT: SWS SWF HF Communications Warning 35 was issued on 16 
April and is current for 16-18 Apr. Maximum usable frequencies 
(MUFs) on UT day 17 Apr were mostly enhanced at lower latitudes 
and nearer monthly predicted values at mid-latitudes. Night time 
spread F was observed at Hobart. MUFs are expected to be near 
predicted monthly values to 25% enhanced 18-20 Apr. Short-wave 
fadeouts are likely.

-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 16 Apr
       Daily Proton Fluence >1 MeV:   6.2E+04
       Daily Proton Fluence >10 MeV:  3.9E+04
       Daily Electron Fluence >2 MeV: 4.00E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 6%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C1.6

DSCOVR Satellite Solar Wind Day Averaged Data for 16 Apr
Speed: 543 km/sec  Density:    0.9 p/cc  Temp:   306000 K  Bz:   3 nT

(Courtesy Space Weather Prediction Center, Boulder USA)
-----------------------------------------------------------

Space Weather Services              email: asfc at bom.gov.au
Bureau of Meteorology
PO Box 1386                         WWW: http://www.sws.bom.gov.au
Haymarket NSW 1240  AUSTRALIA       FTP: ftp://ftp-out.sws.bom.gov.au
tel: +61 2 9213 8010                fax: +61 2 9213 8060 

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