[Ips-dsgr] SWS Daily Report - 15 May 22 issued 2331 UT on 15 May 2022 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Mon May 16 09:31:04 EST 2022


SUBJ: SWS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/15 MAY 2022 BY Space Weather Services
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 15 MAY AND FORECAST FOR 16 MAY - 18 MAY
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 15 May: R1

Flares    Max     Fadeout    Freq.  Sectors
  M2.2    0008UT  possible   lower  West Pacific

Observed 10.7 cm flux/Equivalent Sunspot Number for 15 May: 154/109


1B. SOLAR FORECAST
             16 May             17 May             18 May
Activity     R0-R1		R0-R1		   R0-R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   154/109            152/107            152/107

COMMENT: Solar activity on UT day 15-May was at R1 level, with 
a M2.2 flare originating from beyond the northeast limb (N10) 
at 15/0008UT. There are currently eight numbered regions on the 
solar disk, although no significant flaring activity has been 
observed in addition to the single M-class flare. Regions 3007 
(S23W22, beta), 3010 (S14E35, beta) and 3011 (N12E48, beta) are 
the most complex regions. Solar activity is expected to be at 
R0-R1 levels on 16-18 May, with a slight chance of R2 level. 
No Earth-directed CMEs have been observed. ACE EPAM data indicated 
an energetic ion enhancement event beginning at around 15/1100UT, 
although this returned to near background levels from 15/1800UT. 
The solar wind speed on 15-May was enhanced, ranging from 428-580 
km/s, most likely due to the combined impact of the earlier CME 
and coronal hole effects. The solar wind speed is currently near 
533 km/s. The peak total interplanetary magnetic field strength 
(IMF Bt) was 15 nT and the north-south IMF component (Bz) range 
was +8 to -9 nT. Bz was intermittently southward between 0017-0321UT. 
The solar wind speed is expected to continue to be enhanced over 
16-18 May due to coronal hole effects.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 15 May: G0

Estimated Indices 15 May : A   K           
   Australian Region       9   33213311
      Darwin               9   33213311
      Learmonth           11   33323311
      Alice Springs        9   33213311
      Gingin               7   23212310
      Canberra             6   23212210
      Hobart               7   23213300    

Estimated Antarctic Regional K Indices 15 May :
      Macquarie Island     7   22322300
      Casey               13   44332221
      Mawson              13   34432212

Observed Regional daily pc3 Indices 15 May : 
      Darwin               0   (Quiet)
      Townsville          NA
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin              49   (Unsettled)
      Canberra            28   (Quiet to unsettled)
      Hobart              56   (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 15 May : A 
           Fredericksburg        11
           Planetary             14                         

Observed AFr/Ap Indices 14 May :  A   K
           Fredericksburg         9
           Planetary              7   2222 1322     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
16 May    15    G0-G1
17 May    10    G0
18 May     7    G0

COMMENT: G0 geomagnetic conditions were observed in both the 
Australian and Antarctic regions on UT day 15-May. G0 conditions 
are likely for the Australian region during 16-18 May, with a 
chance of G1 conditions due to coronal hole effects.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
15 May      Normal         Normal         Normal         

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
16 May      Normal         Normal         Normal-fair
17 May      Normal         Normal         Normal-fair
18 May      Normal         Normal         Normal

COMMENT: Mostly normal HF propagation conditions are expected 
for 16-18 May. Short-wave fadeouts are possible during this period.

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


Date   T index
15 May    94

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 40% during local day.
      Enhanced by 25% during local night.
   Niue Island Region:
      Enhanced by 20% during local day.
      Enhanced by 45% during local night.
      Enhanced by 25% after local dawn.
   Northern Australian Region:
      Enhanced by 30% during local day.
      Enhanced by 50% during local night.
   Southern Australian Region:
      Enhanced by 20% during local day.
      Enhanced by 25% during local night.
      Enhanced by 25% after local dawn.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Enhanced by 15% over the UT day.

Monthly T index:
Month  T index
Apr      77
May      51
Jun      54

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
16 May    80    Near to 15% above predicted monthly values
17 May    80    Near to 15% above predicted monthly values
18 May    80    Near to 15% above predicted monthly values

COMMENT: SWS SWF HF Communications Warning 43 was issued on 14 
May and is current for 15-16 May. Maximum usable frequencies 
(MUFs) on UT day 15-May were near monthly predicted values to 
mildly enhanced. Spread-F was observed at Hobart during night 
hours. MUFs are expected to be mostly near monthly predicted 
values to slightly enhanced during 16-18 May, although there 
is a chance that slight depressions may be observed at mid-high 
latitudes due to geomagnetic disturbances. Short-wave fadeouts 
are possible during this period.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 14 May
       Daily Proton Fluence >1 MeV:   3.0E+05
       Daily Proton Fluence >10 MeV:  4.0E+04
       Daily Electron Fluence >2 MeV: 1.20E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C1.1

DSCOVR Satellite Solar Wind Day Averaged Data for 14 May
Speed: 347 km/sec  Density:   12.5 p/cc  Temp:    49700 K  Bz:   2 nT

(Courtesy Space Weather Prediction Center, Boulder USA)
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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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