[Ips-dsgr] SWS Daily Report - 24 April 17 issued 2330 UT on 24 Apr 2017 [SEC=UNCLASSIFIED]

Regional Warning Centre rwc at sws.bom.gov.au
Tue Apr 25 09:30:19 EST 2017


SUBJ: SWS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/24 APRIL 2017 BY Space Weather Services
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 24 APRIL AND FORECAST FOR 25 APRIL - 27 APRIL
STATUS INDICATORS SOL:GREEN   MAG:** YELLOW **     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 24 Apr:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 24 Apr:  80/20


1B. SOLAR FORECAST
             25 Apr             26 Apr             27 Apr
Activity     Very low to low    Very low to low    Very low to low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    80/20              80/20              82/23

COMMENT: Solar activity was very low for the UT day, 24 April, 
with no notable flares. Very low levels of solar activity is 
expected for the next 3 UT days (25-27 April) with chance of 
C-class flares. An eruptive filament was observed in the northeast 
quadrant (N36E32) at 24/0200 UT. It has triggered a CME which 
is first visible in LASCO C2 coronagraph imagery starting at 
approximately 24/0300 UT. Further information on the possible 
impact of this CME on earth will be given after the completion 
of the model runs. During the last 24 hours, the solar wind speed 
had declined gradually from 750 km/s at the beginning of the 
UT day to 600 km/s by the end of UT day. This is indicative of 
the beginning of the waning effects of the recurrent negative 
polarity coronal hole. The IMF Bt was mostly steady near 6 nT 
during the UT day. The Bz component varied between -5 nT and 
+5 nT. The two day outlook (25-26 April) is for the solar winds 
to gradually trend toward nominal levels as the coronal hole 
effects begin to wane.

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

Geomagnetic field for Australian Region 24 Apr: Quiet to Active

Estimated Indices 24 Apr : A   K           
   Australian Region      13   23343232
      Cocos Island         9   --232232
      Darwin              12   23343122
      Learmonth           19   33353333
      Alice Springs       13   23343232
      Norfolk Island      11   23342222
      Culgoora            16   23353232
      Gingin              18   23353333
      Camden              16   23353232
      Canberra            10   22342122
      Launceston          19   33353333
      Hobart              17   23453232    

Estimated Antarctic Regional K Indices 24 Apr :
      Macquarie Island    36   33564552
      Casey               19   44433333
      Mawson              70   56553775

Observed Regional daily pc3 Indices 24 Apr : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            4   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin              56   (Unsettled)
      Canberra            49   (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 24 Apr : A 
           Fredericksburg        20
           Planetary             28                         

Observed AFr/Ap Indices 23 Apr :  A   K
           Fredericksburg        24
           Planetary             35   4555 4444     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
25 Apr    20    Active
26 Apr    16    Active
27 Apr    16    Active

COMMENT: Magnetic conditions were from quiet to active levels 
across the Australian region during the UT day, 24 April. These 
disturbed magnetic conditions were caused by high speed streams 
from a recurrent, negative polarity coronal hole. Mostly unsettled 
to active conditions are expected for the UT days 25-26 April 
in response to the coronal hole effects. Isolated minor storm 
levels are possible on 25 April.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
25 Apr      Normal         Normal-fair    Fair
26 Apr      Normal         Normal-fair    Fair
27 Apr      Normal         Normal-fair    Fair

COMMENT: MUFs were mostly near monthly predicted values on the 
UT day 24 April. During 25 April MUFs are expected decrease, 
still remaining near predicted monthly values.

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


Date   T index
24 Apr     7

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

Monthly T index:
Month  T index
Mar      11
Apr      14
May      14

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
25 Apr    -5    Near predicted monthly values
26 Apr    -5    Near predicted monthly values
27 Apr     0    Near predicted monthly values

COMMENT: For the UT day, 24 April, MUFs over the Australian region 
were near the monthly predicted value. Mild depressions were 
also observed over the Southern Australian region. The outlook 
for the next two days (25 and 26 April) is for MUF levels to 
drop, but the MUFs are expected to remain near the predicted 
monthly levels. The degradations of MUFs are due to the storm 
induced ionospheric depression, which is expected to spread equatorwards 
from the polar regions. MUFs to expect recover from 27 April

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

GOES satellite data for 23 Apr
       Daily Proton Fluence >1 MeV:   4.7E+07
       Daily Proton Fluence >10 MeV:  1.6E+04
       Daily Electron Fluence >2 MeV: 4.00E+08   (moderate fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability:21%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A9.9

ACE Satellite Solar Wind Day Averaged Data for 23 Apr
Speed: 727 km/sec  Density:    8.0 p/cc  Temp:   683000 K  Bz:  -1 nT

(Courtesy Space Weather Prediction Center, Boulder USA)
ACE data can be incorrect during strong proton events.
-----------------------------------------------------------

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 

IMPORTANT: This e-mail, including any attachments, may contain,
confidential or copyright information.  The views expressed in 
this message are those of the individual sender, unless 
specifically stated to be the views of SWS.  If you are not 
the intended recipient, please contact the sender immediately 
and delete all copies of this e-mail and attachments. 
To unsubscribe from an IPS mail list either send an email to 
"MAIL_LIST"-leave at ips.gov.au or go to
http://www.sws.bom.gov.au/mailman/listinfo/"MAIL_LIST".
Information about training can be obtained from
http://www.sws.bom.gov.au/mailman/listinfo/ips-training.
General information is available from
http://www.sws.bom.gov.au/mailman/listinfo/ips-info.





More information about the ips-dsgr mailing list