[Ips-dsgr] IPS Daily Report - 26 October 13 issued 2343 UT on 26 Oct 2013

rwc rwc at ips.gov.au
Sun Oct 27 10:43:20 EST 2013


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/26 OCTOBER 2013 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 26 OCTOBER AND FORECAST FOR 27 OCTOBER - 29 OCTOBER
STATUS INDICATORS SOL:** YELLOW **   MAG:** RED **     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 26 Oct:  High

Flares    Max     Fadeout    Freq.  Sectors
  M2.3    0607UT  possible   lower  Mid East/Indian
  M1.2    0927UT  possible   lower  Mid East/Indian
  M1.5    0938UT  possible   lower  Mid East/Indian
  M1.8    1118UT  possible   lower  European
  M3.1    1927UT  possible   lower  East Pacific/
                                    North American
  M1.0    1955UT  possible   lower  East Pacific/
                                    North American

Observed 10.7 cm flux/Equivalent Sunspot Number for 26 Oct: 165/119


1B. SOLAR FORECAST
             27 Oct             28 Oct             29 Oct
Activity     Moderate           Moderate           Moderate
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   165/119            165/119            160/114

COMMENT: Region 1882(S08E59) produced five M-class flares today, 
along with a number of C-class events. Regions 1875(N07W36) and 
1877(S12W16) also produced a number of C-class events. An M1.5 
flare peaking at 0937UT from region 1882 was associated with 
a Type II radio burst observed in Learmonth spectrograph with 
estimated shock speed 1275 km/s. region 1882 increased in area 
add magnetic complexity, is classified a Dko spot region with 
a beta-gamma-delta magnetic configuration and is now 280mil in 
size. This region continues to have significant flaring potential. 
Region 1875 is the other region on the disk with significant 
flaring potential, classified an Ekc beta-gamma-delta region, 
the largest of the numbered active regions 660 mil in size and 
now in geoeffective position for CMEs. M-Class flares are expected 
and a chance of an isolated X-class flare for the next 3 days. 
A Disappearing Solar Filament (DSF) lifted off the SW Quadrant 
~~0800UT. SOHO observed several CMEs among which a CME first observed 
after 0230UT UT, probably associated to a C flare from region 
1875 and a second CME observed by after 0830UT and most likely 
associated with the DSF. The relevant period of imagery is not 
yet available to see whether they have an earth directed component. 
Further analysis will be given in tomorrow's report when imagery 
should be available. The Interplanetary Magnetic Field fluctuated 
in the quiescent +/-4nT range causing no significant merging/reconnection 
with the geomagnetic field. Solar wind was steady all day at 
the light 320 km/s level. EPAM ions (often a precursor to geomagnetic 
activity) increased over the UT. Proton flux (>10MeV) at geosynchronous 
orbit also increased but remained below the event threshold. 
Expect an increase in solar wind speed parameters on 28-29 October 
due to CME combined effects.

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

Geomagnetic field for Australian Region 26 Oct: Quiet

Estimated Indices 26 Oct : A   K           
   Australian Region       2   11100002
      Cocos Island         1   11100001
      Darwin               2   11100012
      Townsville           2   11100112
      Learmonth            4   21200103
      Alice Springs        2   11100002
      Culgoora             2   11100002
      Camden               2   11100002
      Canberra             0   00000002
      Launceston           2   11110102
      Hobart               2   11100002    

Estimated Antarctic Regional K Indices 26 Oct :
      Casey                8   34320002
      Mawson               7   31110024

Observed Regional daily pc3 Indices 26 Oct : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               0   (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 26 Oct : A 
           Fredericksburg         2
           Planetary              3                         

Observed AFr/Ap Indices 25 Oct :  A   K
           Fredericksburg         3
           Planetary              2   0000 1101     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
27 Oct    10    Quiet to Unsettled
28 Oct    25    Active
29 Oct    15    Unsettled to Active

COMMENT: Magnetic conditions have been mostly Quiet for the Australian 
region. Mostly Quiet to Unsettled conditions are expected on 
October 27, and Active with isolated minor storm conditions are 
expected on October 28 due to the expected merged arrival of 
CMEs among which the halo CME from the X2 flare on 25 October.

-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
26 Oct      Normal         Normal         Normal         

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
27 Oct      Normal         Normal         Normal
28 Oct      Normal         Normal         Normal-fair
29 Oct      Normal         Normal         Normal-fair

COMMENT: Mostly normal HF conditions are expected for the next 
few days with a chance of SWFs.

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


Date   T index
26 Oct   115

Observed Australian Regional MUFs
   Cocos Island Region:
      No data available.
   Niue Island Region:
      Enhanced by 30% during local day.
      Enhanced by 25% during local night.
   Northern Australian Region:
      Near predicted monthly values during local day.
      Enhanced by 30% during local night.
   Southern Australian and New Zealand Region:
      Enhanced by 15% during local day.
      Enhanced by 20% during local night.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Enhanced by 25% over the UT day.

Monthly T index:
Month  T index
Sep      68
Oct      72
Nov      70

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
27 Oct   100    Near to 15% above predicted monthly values
28 Oct    90    Near predicted monthly values
29 Oct    90    Near predicted monthly values

COMMENT: IPS SWF HF Communications Warning 30 was issued on 25 
October and is current for 26-28 Oct. HF conditions are still 
enhanced due to high levels of ionising EUV flux from multiple 
sunspot regions. Expected geomagnetic activity 28-29 Oct may 
reduce the maximum useable frequency from the currently enhanced 
levels. MUFs expected to be near predicted monthly values with 
a chance of depressed periods for Southern AUS/NZ regions 28-29 
Oct. Short wave fadeouts possible next two days with a reasonable 
chance of isolated M and X flares from solar active regions.

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

GOES satellite data for 25 Oct
       Daily Proton Fluence >1 MeV:   3.5E+05
       Daily Proton Fluence >10 MeV:  1.2E+04
       Daily Electron Fluence >2 MeV: 3.70E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 5%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C1.1

ACE Satellite Solar Wind Day Averaged Data for 25 Oct
Speed: 334 km/sec  Density:    1.7 p/cc  Temp:    40200 K  Bz:   0 nT

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

IPS Radio and Space Services        email: asfc at ips.gov.au
PO Box 1386                         WWW: http://www.ips.gov.au
Haymarket NSW 1240  AUSTRALIA       FTP: ftp://ftp.ips.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 IPS.  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://listserver.ips.gov.au/mailman/listinfo/"MAIL_LIST".
Information about training can be obtained from
http://listserver.ips.gov.au/mailman/listinfo/ips-training.
General information is available from
http://listserver.ips.gov.au/mailman/listinfo/ips-info.





More information about the ips-dsgr mailing list