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last update
17:06 UTC
SFI: 87 | Ap index:  31  | Kp index:  2  ( 4 @17:45,  5 @20:45)| X-ray flux:  B5.4 
SW: Density= 1.5 p/cm3 | Speed= 675.0 km/s | Temp=335(x1000)K
IMF: Bx=-1.2nT | By=-3.1nT | Bz= -1.5 nT | Bt= 3.6 nT | Lat= -24.4 ° | Lon=248.4°
Sunspots: 33 | Area: 360 10-6/Hemi | New regions: 0
[i]X-ray flares: C=9 M=0 X=0 | Optical flares: M1=0 M2=0 M3=0 | Sub-flares=5
GONG images
The Global Oscillation Network Group (GONG) is a community-based program to conduct a detailed study of solar internal structure and dynamics using helioseismology. In order to exploit this new technique, GONG has developed a six-station network of extremely sensitive, and stable velocity imagers located around the Earth to obtain nearly continuous observations of the Sun's "five-minute" oscillations, or pulsations. You can check the stations' locations here.


Learmonth [VIDEO]
Udaipur[VIDEO]
El Teide[VIDEO]
Latest image from GONG: H-Alpha Learmonth Latest image from GONG: H-Alpha Udaipur Latest image from GONG: H-Alpha El Teide

Cerro Tololo[VIDEO]
Big Bear[VIDEO]
Mauna Loa [VIDEO]
Latest image from GONG: H-Alpha Cerro Tololo Latest image from GONG: H-Alpha Big Bear Latest image from GONG: H-Alpha Mauna Loa



GONG: Radiometer monitor
GONG: H-Alpha good observations monitor


Courtesy of NSO/GONG.
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