[Ips-dsgr] IPS Daily Report - 07 September 05

rwc rwc at ips.gov.au
Thu Sep 8 09:53:12 EST 2005


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 07/2330Z SEPTEMBER 2005 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 07 SEPTEMBER AND FORECAST FOR 08 SEPTEMBER - 10 SEPTEMBER
STATUS INDICATORS SOL:** RED **   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 07 Sep:  Moderate

Flares    Max     Fadeout    Freq.  Sectors
  M1.2 06/2305UT  possible   lower  West Pacific
  Y1.7    1740UT  possible   lower  South American/
                                    Atlantic

Observed 10.7 cm flux/Equivalent Sunspot Number for 07 Sep: 100/48

1B. SOLAR FORECAST
             08 Sep             09 Sep             10 Sep
Activity     Moderate to high   Moderate to high   Moderate to high
Fadeouts     Probable           Probable           Probable
10.7cm/SSN   110/60             120/72             120/72
COMMENT: Solar activity was high on 07 September as an X17 flare 
was observed around 1740UT from a very active region 808(S12E82), 
which is currently rotating onto the visible disk. This flare, 
the 4th largest flare in the last 15 years, was associated to 
a Type II and IV radio bursts and a fast and bright CME. This 
CME is not earthward directed. The solar wind speed decreased 
from 430 to 380 km/s during the UT day today. The north-south 
component of the interplanetary magnetic field (Bz) remained 
slightly to moderately southward during the first half of the 
UT day and slightly to moderately northward during the second 
half. Solar activity is expected to remain at moderate to high 
levels during the next few days as the region 808 fully rotates 
onto the visible disk. The proton flux is currently increasing 
and the >10MeV protons may cross the 10 pfu threshold on 
08 September. 

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

Geomagnetic field for Australian Region 07 Sep: Quiet to Unsettled 

Estimated Indices 07 Sep :  A   K           
   Australian Region       5   2213 1011
      Learmonth            4   2213 0000
      Culgoora             5   2113 2111
      Canberra             5   2213 2001
      Hobart               6   2213 2011
      Casey(Ant)           8   2333 1111
    
Observed Regional daily pc3 Indices 07 Sep : 
      Townsville          NA
      Learmonth           NA
      Culgoora            NA
      Canberra            NA
      Hobart              11   (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. 


Estimated AFr/Ap Indices 07 Sep : A 
           Fredericksburg        10
           Planetary             10                         

Observed AFr/Ap Indices 06 Sep :  A   K
           Fredericksburg         6
           Planetary              9   3202 2312     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
08 Sep     8    Quiet to Unsettled 
09 Sep    14    Quiet to unsettled, isolated active periods possible. 
10 Sep    10    Quiet to Unsettled 
COMMENT: Mostly quiet to unsettled conditions are expected during 
the next three days with some possibility of isolated active 
periods on 09 September. A weak (16nT) impulse was observed in 
the IPS magnetometer data at 1123UT on 07 Sep. 
-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
07 Sep      Normal         Normal-fair    Normal-poor    
PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
08 Sep      Normal-fair    Normal-fair    Normal-poor   
09 Sep      Normal-fair    Normal-fair    Normal-poor   
10 Sep      Normal-fair    Normal-fair    Normal-poor   
COMMENT: Sever shortwave fadeouts were observed in the daylit 
regions around 1717UT on 07 September due to a large flare (X17) 
around this time. Due to the presence of a very active region 
on the visible disk, more flares are expected. This may cause 
shortwave fadeouts in the daylit regions during the next few 
days. However, if the flare activities don't happen, mostly 
normal conditions may be expected in most regions. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
07 Sep    11

Observed Australian Regional MUFs
   Equatorial PNG Region:
      Near predicted monthly values during local day,
      Depressed by 35% during local night.
   Northern Australian Region:
      Near predicted monthly values during local day,
      Depressed by 15% during local night.
   Southern Australian and New Zealand Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Scott Base):
      Near predicted monthly values over the UT day
      with significant degradations

Predicted Monthly T index for September:  24

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
08 Sep    20    near predicted monthly values 
09 Sep    18    near predicted monthly values 
10 Sep    20    near predicted monthly values 
COMMENT: Due to a good possibility of strong flare activities 
from a  very active regions short wave fadeouts may be 
observed during the day time in the next few days. However, 
if the flare activities don't happen, mostly normal conditions 
may be expected in most Aus/NZ regions during the next few days. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 06 Sep
       Daily Proton Fluence >1 MeV:   1.2E+06
       Daily Proton Fluence >10 MeV:  2.1E+04
       Daily Electron Fluence >2 MeV: 1.30E+09 (very high fluence)  
Electron Fluence Daily Deep Dielectric Discharge Probability:33%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B3.4

ACE Satellite Solar Wind Day Averaged Data for 06 Sep
Speed: 446 km/sec  Density:    2.5 p/cc  Temp:    75600 K  Bz:   0 nT

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