[Ips-dsgr] IPS Daily Report - 30 April 13 issued 2330 UT on 30 Apr 2013

Regional Warning Centre rwc at ips.gov.au
Wed May 1 09:30:24 EST 2013


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/30 APRIL 2013 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 30 APRIL AND FORECAST FOR 01 MAY - 03 MAY
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 30 Apr:  Low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 30 Apr: 154/109


1B. SOLAR FORECAST
             01 May             02 May             03 May
Activity     Low to moderate    Low to moderate    Low to moderate
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   155/109            160/114            165/119

COMMENT: Several low to mid C-class flares from regions 1730,1731 
and 1733 with the largest a C3.6 from 1730. Type III radio bursts 
were observed in association with some of the flares. A minor type 
II radio sweep at 1935UT yesterday, associated with a C flare 
and type IV radio noise burst, from AR1733 does not appear to 
have resulted in a geoeffective coronal mass ejection as it is 
small and angled south-west. AR1731 is still the largest 
of the 7 numbered active regions although it has declined to 
350 millionths of the disc. AR1730 is the most magnetically complex 
(beta-gamma-delta) and likely to flare. The cumulative probability 
across all the regions of isolated M/X flares is now moderate. 
Solar wind speed rose from low 340km/s up to moderate 440km/s 
at 14UT under the influence of coronal hole CH567, and then declined 
to ~380km/s. Interplanetary Magnetic Field north-south magnetic 
polarity was oscillating in the neutral +/- 5nT area indicating 
no large merging events with the geomagnetic field.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 30 Apr: Quiet

Estimated Indices 30 Apr : A   K           
   Australian Region       5   21122112
      Darwin               6   22122222
      Townsville           8   22232222
      Learmonth            8   22133212
      Alice Springs        4   21122111
      Culgoora             5   21122112
      Gingin               4   21022112
      Camden               4   11122102
      Canberra             4   11122102
      Hobart               5   11222112    

Estimated Antarctic Regional K Indices 30 Apr :
      Macquarie Island     1   10110000
      Casey                9   33223212
      Mawson              19   43232245
      Davis               13   33332---

Observed Regional daily pc3 Indices 30 Apr : 
      Darwin              11   (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 30 Apr : A 
           Fredericksburg         7
           Planetary              7                         

Observed AFr/Ap Indices 29 Apr :  A   K
           Fredericksburg         5
           Planetary              4   2100 1112     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
01 May     7    Quiet
02 May     5    Quiet
03 May     5    Quiet

COMMENT: Regional geomagnetic conditions were generally Quiet 
even though solar wind speed rose by 14UT to moderate 440km/s 
under the influence of coronal hole CH567, providing Unsettled conditions 
for 3-6 hours at some locations. Geomagnetic activity is expected 
to be predominantly Quiet for the next three days in the absence 
of prolonged southward IMF Bz or CMEs.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
01 May      Normal         Normal         Normal
02 May      Normal         Normal         Normal
03 May      Normal         Normal         Normal

COMMENT: Mostly normal HF conditions are expected for the next 
3 days.

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


Date   T index
30 Apr    84

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 35% during local day.
      Enhanced by 30% during local night.
   Niue Island Region:
      Enhanced by 15% during local day.
      Near predicted monthly values during local night.
   Northern Australian Region:
      Near predicted monthly values.
   Southern Australian and New Zealand Region:
      Mostly near predicted monthly values.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Enhanced by 15% over the UT day.

Predicted Monthly T index for April:  68

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
01 May    80    Near predicted monthly values
02 May    80    Near predicted monthly values
03 May    80    Near predicted monthly values

COMMENT: The HF propagation conditions were mostly normal during 
the UT day 30April at mid-latitudes. Strong enhancements at near-equatorial 
northern sites were observed, especially 08-09UT, from an enhanced 
equatorial anomaly, possibly caused by remnant activity after 
the geomagnetic disturbances of the previous days. Expect mostly 
normal HF frequency availability for next three days in the absence 
of significant geomagnetic or solar flare activity. There is 
a moderate chance of isolated M/X flares from at least 4 of the 
7 solar active regions, which if they occur during local daytime 
will cause short wave fadeouts of varying degrees.

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

GOES satellite data for 29 Apr
       Daily Proton Fluence >1 MeV:   3.3E+05
       Daily Proton Fluence >10 MeV:  1.2E+04
       Daily Electron Fluence >2 MeV: 7.60E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 9%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B7.3

ACE Satellite Solar Wind Day Averaged Data for 29 Apr
Speed: 397 km/sec  Density:    1.1 p/cc  Temp:    51500 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 

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