[Ips-dsgr] IPS Daily Report - 17 March 09

rwc rwc at ips.gov.au
Wed Mar 18 10:38:29 EST 2009


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 17/2330Z MARCH 2009 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 17 MARCH AND FORECAST FOR 18 MARCH - 20 MARCH
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 17 Mar:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 17 Mar:  69/3


1B. SOLAR FORECAST
             18 Mar             19 Mar             20 Mar
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    70/5               70/5               70/5
COMMENT: The solar wind speed further declined to ~370km/s by 
the end of the UT day. The upcoming small coronal hole, near 
the solar equator and slightly west of the central meridian, 
is still visible in the SOHO spacecraft EIT 195 imagery. The 
resultant increase in solar wind speed and disturbance can already 
be seen at the STEREO-B spacecraft, which is ahead of the Earth 
in terms of solar rotation effects. The coronal hole high-speed 
solar-wind stream (HSSWS) should be geoeffective in 1-2 days, 
19-20th March UT. The IMF Bz was southwards at the ACE spacecraft 
for an extended period 14-22UT, causing prolonged merging with 
the geomagnetic field into the polar regions. The solar disc 
is presently spotless but AR1013 is due to return on the 18th 
if it survived rearside solar transit. 




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

Geomagnetic field for Australian Region 17 Mar: Quiet 

Estimated Indices 17 Mar :  A   K           
   Australian Region       4   12111211
      Darwin               4   12111212
      Townsville           7   22222222
      Learmonth            4   22012211
      Camden               2   11011111
      Canberra             1   11001100
      Hobart               2   11002101
      Casey(Ant)           8   23321222
    
Observed Regional daily pc3 Indices 17 Mar : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice_Springs        0   (Quiet)
      Camden               0   (Quiet)
      Gnangara             0   (Quiet)
      Canberra             0   (Quiet)
      Hobart               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 Space Environment Research Center, Japan.


Estimated AFr/Ap Indices 17 Mar : A 
           Fredericksburg         3
           Planetary              3                         

Observed AFr/Ap Indices 16 Mar :  A   K
           Fredericksburg         4
           Planetary              5   2111 1220     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
18 Mar     3    Quiet 
19 Mar     5    Quiet to unsettled 
20 Mar     5    Quiet to unsettled 
COMMENT: Expect quiet geomagnetic conditions for the next one 
to two days as the Vsw is still slowly decreasing and currently 
at near quiescent 370km/sec. The upcoming small coronal hole 
is near the solar equator and slightly west of the central meridian. 
The resultant increase in solar wind speed and disturbance can 
already be seen at the STEREO-B spacecraft, which is ahead of 
the Earth in terms of solar rotation effects. The coronal hole 
high-speed solar-wind stream (HSSWS) should be geoeffective in 
1-2 days, 19-20th March UT. The effect should only be moderate 
with Quiet-Unsettled with possibly sporadic Active geomagnetic 
conditions at mid-latitudes. The IMF Bz was southwards for an 
extended period 14-22UT today, causing prolonged merging with 
the geomagnetic field into the polar regions and an increase 
in activity to Storm levels in the auroral zone from ~20-24UT. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
18 Mar      Normal         Normal         Normal
19 Mar      Normal         Normal         Normal
20 Mar      Normal         Normal         Normal

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


Date   T index
17 Mar    -1

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Near predicted monthly values.
   Northern Australian Region:
      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 over the UT day.

Predicted Monthly T index for March:   3

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
18 Mar     0    0 to 5% below predicted monthly values 
19 Mar     0    Near predicted monthly values 
20 Mar     0    Near predicted monthly values 
COMMENT: Expect near or slightly below monthly predicted HF
frequencies 
for the next day. The effect of a small coronal hole should commence 
in ~2 days, 19th March UT, with slightly increased geomagnetic 
activity which will likely raise ionisation and HF frequencies 
to near monthly predicted levels for a day or two. Nightime blanketing
sporadic-E that obscured the F-layer was observed on the eastern 
seaboard. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 16 Mar
       Daily Proton Fluence >1 MeV:   9.3E+05
       Daily Proton Fluence >10 MeV:  1.9E+04
       Daily Electron Fluence >2 MeV: 9.90E+07   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability:10%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.0

ACE Satellite Solar Wind Day Averaged Data for 16 Mar
Speed: 422 km/sec  Density:    0.7 p/cc  Temp:    36600 K  Bz:   1 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. 
Occasionally IPS sends email promoting IPS products and 
services to its mailing list customers. If you do not wish to 
receive this promotional material please email 
no-spam at ips.gov.au with the subject header:UNSUBSCRIBE"





More information about the ips-dsgr mailing list