CTIO GONG
The Global Oscillation Network Group (GONG) is a community-based program consisting of 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.
For scientists: More details can be found on the science telescope page.
CTIO GONG
Name(s) |
CTIO GONG |
Status |
Operational |
Broad Science Goals |
Study of solar internal structure and dynamics using helioseismology. |
Site |
Cerro Tololo, Chile |
Location Coordinates |
30º 10’ 03.92’S 70º 48’ 19.84’W |
Altitude |
2174 meters (7133 feet) |
Enclosure |
Cargo container |
Type |
Optical system |
Optical Design |
Fourier Tachometer Instrument |
Field of View |
5 arcseconds |
Diameter: Primary M1 |
2.8 cm |
Material: Primary M1 |
N/A |
Diameter: Secondary M2 |
N/A |
Material: Secondary M2 |
N/A |
Mount |
Automated, portable installation |
First Light Date |
|
Adaptive Optics |
N/A |
Images taken with the CTIO GONG |
Link |
Images of the CTIO GONG |
Link |
Videos of the CTIO GONG |
Link |
Press Releases with the CTIO GONG |
Link |
|
Please help us to complete this page by emailing information and corrections to info@noirlab.edu.