Observing the Solar Wind with Interplanetary Scintillation
Observing the Solar Wind with Interplanetary Scintillation Observing the Solar Wind with Interplanetary Scintillation
Tomography
Tomography Co-rotating analysis Combination of methods Images courtesy M. Bisi (Aberystwyth) and B. Jackson (UCSD) EISCAT IPS line of sight through tomographic image of CME. CME gave Earth glancing blow; registered in ACE spacecraft data.
- 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: Tomography ● Many observations ta
- 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 and 20: Median Sampling ● ● Data usuall
- Page 21 and 22: 1420MHz System
- Page 23: Summary ● EISCAT used for observi
Tomography<br />
Co-rotating analysis<br />
Combination of methods<br />
Images courtesy M. Bisi (Aberystwyth) and B. Jackson (UCSD)<br />
EISCAT IPS line of sight through tomographic<br />
image of CME. CME gave Earth glancing blow;<br />
registered in ACE spacecraft data.
Change language