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last update
16:25 UTC
SFI: 68 | Ap index:  27  | Kp index:  3  ( 0 @16:45,  0 @19:45)| X-ray flux:  A0.5 
SW: Density= 4.0 p/cm3 | Speed= 430.0 km/s | Temp=43(x1000)K
IMF: Bx=0.4nT | By=-7.9nT | Bz= 3.7 nT | Bt= 8.7 nT | Lat= 24.8 ° | Lon=272.8°
Sunspots: 0 | Area: 0 10-6/Hemi | New regions: 0
[i]X-ray flares: C=0 M=0 X=0 | Optical flares: M1=0 M2=0 M3=0 | Sub-flares=0
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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