[Ips-dsgr] IPS Daily Report - 01 March 16 issued 2330 UT on 01 Mar 2016 [SEC=UNCLASSIFIED]

Regional Warning Centre rwc at ips.gov.au
Wed Mar 2 10:30:32 EST 2016


SUBJ: SWS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/01 MARCH 2016 BY Space Weather Services
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 01 MARCH AND FORECAST FOR 02 MARCH - 04 MARCH
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 01 Mar:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 01 Mar:  97/44


1B. SOLAR FORECAST
             02 Mar             03 Mar             04 Mar
Activity     Very low to low    Very low to low    Very low to low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN   100/48             105/54             105/54

COMMENT: The solar activity was at very low levels for the UT 
day, 1 March, with no C-class flares. There are currently three 
numbered Earth facing sunspot regions on the solar disk. The 
2-day outlook (2-3 March) is for very low solar activity with 
weak chance of smaller C-class flares. A large eruptive filament,approximately 
18 degrees long, was observed on the northeast limb (N20E80) 
at about 01/0800 UT. Inspection of the LASCO coronagraph imagery 
reveals that this event generated a Coronal Mass Ejections (CME) 
with a shock speed of 576 km/s. Preliminary model runs indicate 
that the CME is not expected to have an impact at Earth. The 
solar wind has elevated from nearly 300 km/s to almost 400 km/s 
during the past 24 hrs. These moderate enhancements in the solar 
wind speed is associated with high speed streams emanating from 
a northern hemisphere coronal hole. The Bz component of the IMF 
fluctuated between -8 nT and 8 nT. Bt was between 5-15 nT. The 
outlook for 2 March is for the solar winds to remain slightly 
elevated in response to the coronal hole. On 3 March, it is expected 
that the solar winds will gradually trend towards ambient levels 
as the effects of the coronal hole wane.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 01 Mar: Quiet to Unsettled

Estimated Indices 01 Mar : A   K           
   Australian Region       6   13221212
      Cocos Island         4   12211201
      Darwin               6   23211202
      Townsville           7   23221212
      Learmonth            7   23221212
      Norfolk Island       5   13221102
      Culgoora             6   -3211212
      Gingin               4   22211201
      Camden               6   13221212
      Canberra             5   13211202
      Melbourne            6   13221212
      Launceston           7   23221212
      Hobart               6   13221112    

Estimated Antarctic Regional K Indices 01 Mar :
      Macquarie Island     5   12231101
      Casey               16   35432113
      Mawson               9   33322212

Observed Regional daily pc3 Indices 01 Mar : 
      Darwin              NA
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             0   (Quiet)
      Melbourne            6   (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 01 Mar : A 
           Fredericksburg         8
           Planetary             10                         

Observed AFr/Ap Indices 29 Feb :  A   K
           Fredericksburg         4
           Planetary              3   2001 1012     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
02 Mar    12    Unsettled
03 Mar     6    Quiet
04 Mar     6    Quiet

COMMENT: The geomagnetic conditions were mostly quiet to unsettled 
during the last 24 hours (1 Feb). The outlook for UT day 2 March 
is for mostly quiet to unsettled conditions. These conditions 
are forecasted due to the expected moderately high solar wind 
speeds associated with high speed streams emanating from a Northern 
Hemisphere coronal hole. Geomagnetic conditions are expected 
to return to mostly quiet levels on UT day 3 March as the effects 
of the coronal hole wanes.

-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
01 Mar      Normal         Normal         Normal         

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
02 Mar      Normal         Normal         Normal-fair
03 Mar      Normal         Normal         Normal
04 Mar      Normal         Normal         Normal

COMMENT: Observed MUF's for the UT day 1 March were slightly 
above the predicted monthly values. Similar conditions are expected 
for UT day 2 March in the mid and low latitudes regions. The 
high latitude regions could experience MUF depressions associated 
with forecasted active geomagnetic conditions.

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


Date   T index
01 Mar    70

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values during local day.
      Enhanced by 15% during local night.
   Niue Island Region:
      Near predicted monthly values during local day.
      Depressed by 15% during local night.
   Northern Australian Region:
      Near predicted monthly values.
   Southern Australian Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Enhanced by 20% over the UT day.

Monthly T index:
Month  T index
Feb      64
Mar      50
Apr      51

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
02 Mar    60    Near predicted monthly values
03 Mar    60    Near predicted monthly values
04 Mar    60    Near predicted monthly values

COMMENT: Mostly near predicted monthly MUF values were observed 
in the Australian region on 29-Feb. Near monthly predicted values 
are expected for the next three days.

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

GOES satellite data for 29 Feb
       Daily Proton Fluence >1 MeV:   3.2E+05
       Daily Proton Fluence >10 MeV:  1.3E+04
       Daily Electron Fluence >2 MeV: 2.30E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 4%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B1.5

ACE Satellite Solar Wind Day Averaged Data for 29 Feb
Speed: 340 km/sec  Density:    2.1 p/cc  Temp:    33000 K  Bz:   2 nT

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

Space Weather Services              email: asfc at ips.gov.au
Bureau of Meteorology
PO Box 1386                         WWW: http://www.sws.bom.gov.au
Haymarket NSW 1240  AUSTRALIA       FTP: ftp://ftp-out.sws.bom.gov.au
tel: +61 2 9213 8010                fax: +61 2 9213 8060 

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