[Ips-dsgr] IPS Daily Report - 28 June 08

rwc rwc at ips.gov.au
Sun Jun 29 09:43:14 EST 2008


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 28/2330Z JUNE 2008 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 28 JUNE AND FORECAST FOR 29 JUNE - 01 JULY
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 28 Jun:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 28 Jun:  66/0

1B. SOLAR FORECAST
             29 Jun             30 Jun             01 Jul
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    65/0               65/0               65/0
COMMENT: Solar activity remained at very low levels for the 
last 24 hours. Due to the diminishing effect of a recurrent 
coronal hole the solar wind stream showed signs of gradual 
weakening today. The solar wind speed gradually decreased 
from 620 to 580 km/s during the UT day today. The north-south 
component of the interplanetary magentic field (Bz) showed 
minor (upto around +/- 4 nT) fluctuations on both sides of 
the normal value, staying mostly negative between 0300 and 
2000UT. Solar wind stream is expected to further weaken on 
29 June due to an expected continued weakening of the coronal 
hole effect. Solar activity is expected to remain at very low 
levels for the next 3 days. 
-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 28 Jun: Mostly quiet. 

Estimated Indices 28 Jun :  A   K           
   Australian Region       5   12122221
      Darwin               4   12121211
      Townsville           7   22222222
      Learmonth            8   22123322
      Camden               5   11122221
      Canberra             5   11122221
      Hobart               5   11122221
      Casey(Ant)           9   232223-2
    
Observed Regional daily pc3 Indices 28 Jun : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice_Springs        0   (Quiet)
      Culgoora             4   (Quiet)
      Camden               4   (Quiet)
      Gnangara             5   (Quiet)
      Canberra             4   (Quiet)
      Hobart               4   (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 Space Environment Research Center, Japan.


Estimated AFr/Ap Indices 28 Jun : A 
           Fredericksburg         8
           Planetary              8                         

Observed AFr/Ap Indices 27 Jun :  A   K
           Fredericksburg         7
           Planetary              8   3222 2222     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
29 Jun     6    Mostly quiet, isolated unsettled periods possible. 
30 Jun     5    Quiet 
01 Jul     5    Quiet 
COMMENT: Geomagnetic conditions declined to quiet levels on 
most locations today with some unsettled periods. The activity 
levels is expected to further decline as the coronal hole 
effect weakens further. Mostly quiet periods are expected 
for the next 3 days with some possibility of unsettled periods 
on 29 June, especially at high latitude locations. 

-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
28 Jun      Normal         Normal         Normal         
PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
29 Jun      Normal         Normal         Normal
30 Jun      Normal         Normal         Normal
01 Jul      Normal         Normal         Normal
COMMENT: Some depressions in MUFs on some low and mid 
latitude locations and minor to significant degradations 
in HF conditions on high latitude stations were observed 
on 28 June. HF conditions are expected to remain mostly 
normal on most locations for the next three days. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
28 Jun    -2

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Depressed by 20% during local day,
      Near predicted monthly values during local night.
   Northern Australian Region:
      Mostly near predicted monthly values,
   Southern Australian and New Zealand Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values with periods of some 
      enhancement and periods of minor to significant
      degradations. 

Predicted Monthly T index for June:   5

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
29 Jun     2    near predicted monthly values 
30 Jun     4    near predicted monthly values 
01 Jul     4    near predicted monthly values 
COMMENT: HF conditions around Aus/NZ regions are expected 
to remain mostly normal during the next three days. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 27 Jun
       Daily Proton Fluence >1 MeV:   1.2E+06
       Daily Proton Fluence >10 MeV:  1.8E+04
       Daily Electron Fluence >2 MeV: 3.60E+07   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 5%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.0

ACE Satellite Solar Wind Day Averaged Data for 27 Jun
Speed: 628 km/sec  Density:    0.7 p/cc  Temp:   189000 K  Bz:   1 nT

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


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