SOLAR CYCLE ACTIVITY REPORT MARCH 23_2023
ALL QUIET. Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C1 event observed at 12:01 UTC on March 22 from Region 3257 (S28E40).
There are currently 6 numbered sunspot regions on the solar disk: AR3256 AR3257, AR3259, AR3260, AR3261 and new region AR3262
AR3251, AR3258 are gone
The total number of sunspots has increased to 81 (21 of these are grouped into 6 y active regions) NOAA forecasts for the next 24h: 95% chance for C flares, 10% chance for M flares and 1% chance for X flares. All regions have now stable magnetic fields.
● Auroral Activity
The geomagnetic field has been at quiet to active levels for the past 24 hours. Solar wind speed reached a peak of 567 km/s at 11:12 UTC on March 22. Maximum planetary index Kp4
Aurora Oval
		
		
	
	
		 
	
● Current Conditions at 04:30 UTC on March 23
▪︎ Geospace quiet
▪︎Geomagnetic conditions now : Kp 1
▪︎Solar wind speed record: 447.1 km/sec (Elevated speed)
▪︎ density: 7.14 p/cm3 (low density)
▪︎Neutron Counts today: -3.1% Below Average
▪︎X-ray Solar Flare: C1 at 23:20 UTC
▪︎Sunspot number: 81 (SN 70 March 22)
SpaceWeather.com
SpaceWeatherlive..com
				
			ALL QUIET. Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C1 event observed at 12:01 UTC on March 22 from Region 3257 (S28E40).
There are currently 6 numbered sunspot regions on the solar disk: AR3256 AR3257, AR3259, AR3260, AR3261 and new region AR3262
AR3251, AR3258 are gone
The total number of sunspots has increased to 81 (21 of these are grouped into 6 y active regions) NOAA forecasts for the next 24h: 95% chance for C flares, 10% chance for M flares and 1% chance for X flares. All regions have now stable magnetic fields.
● Auroral Activity
The geomagnetic field has been at quiet to active levels for the past 24 hours. Solar wind speed reached a peak of 567 km/s at 11:12 UTC on March 22. Maximum planetary index Kp4
GEOMAGNETIC STORM WATCH: NOAA forecasters say that G2-class (Moderate) geomagnetic storms are possible on March 24th when solar wind flowing from a large hole in the sun's atmosphere is expected to reach Earth. During such storms, auroras have been seen in the USA as far south as, e.g., New York and Idaho. SpaceWeather.com
Aurora Oval
● Current Conditions at 04:30 UTC on March 23
▪︎ Geospace quiet
▪︎Geomagnetic conditions now : Kp 1
▪︎Solar wind speed record: 447.1 km/sec (Elevated speed)
▪︎ density: 7.14 p/cm3 (low density)
▪︎Neutron Counts today: -3.1% Below Average
▪︎X-ray Solar Flare: C1 at 23:20 UTC
▪︎Sunspot number: 81 (SN 70 March 22)
SpaceWeather.com
SpaceWeatherlive..com
 
	 
 
		 
					
				 
 
		 
  STEVE (Strong Thermal Emission Velocity Enhancement) is similar to aurora, but is not, it appears as a ribbon of purple and green light in the sky and is caused by ribbons of hot plasma (+3000 °C) flowing ..... through the Earth's magnetosphere at speeds in excess of 6 km/s (13,000 mph). These ribbons appear during strong storms. This phenomenon had not been scientifically investigated or described until late 2016.
 STEVE (Strong Thermal Emission Velocity Enhancement) is similar to aurora, but is not, it appears as a ribbon of purple and green light in the sky and is caused by ribbons of hot plasma (+3000 °C) flowing ..... through the Earth's magnetosphere at speeds in excess of 6 km/s (13,000 mph). These ribbons appear during strong storms. This phenomenon had not been scientifically investigated or described until late 2016.  
 
		 Residents of Moscow will get a chance to see the Northern Lights
Residents of Moscow will get a chance to see the Northern Lights 


 
 
		 
 
		 Still have to work on pure non-anticipational ‘drive’ to create our reality
 Still have to work on pure non-anticipational ‘drive’ to create our reality 
 
		 
 
		 
 
		