Observing the Solar Wind with Interplanetary Scintillation
Observing the Solar Wind with Interplanetary Scintillation Observing the Solar Wind with Interplanetary Scintillation
1420MHz System ● 1420MHz system established for the remote sites in 2003. ● ● ● ● Protected astronomy band (cannot transmit here!). Requires replacement of several waveguide and other parts. Takes ~1.5 hours per antenna. Not possible to do this at Tromsø.
1420MHz System
- Page 1 and 2: Observing the Solar Wind with Inter
- Page 3 and 4: Radio Measurements Line of sight to
- Page 5 and 6: Cross-Correlation Cross-correlation
- Page 7 and 8: Longer Baselines If longer baseline
- Page 9 and 10: Tomography ● Many observations ta
- Page 11 and 12: Tomography Co-rotating analysis Com
- Page 13 and 14: Why EISCAT? ● ● ● ● Observi
- Page 15 and 16: Radio Source Tracking ● ● ●
- Page 17 and 18: Filter Settings Power Central Filte
- Page 19: Median Sampling ● ● Data usuall
- Page 23: Summary ● EISCAT used for observi
1420MHz System<br />
● 1420MHz system established for <strong>the</strong> remote sites in 2003.<br />
●<br />
●<br />
●<br />
●<br />
Protected astronomy band (cannot transmit here!).<br />
Requires replacement of several waveguide and o<strong>the</strong>r parts.<br />
Takes ~1.5 hours per antenna.<br />
Not possible to do this at Tromsø.
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