The article analyses the possibility of the forward scatter radar method for detecting large-sized cosmic objects when using emission of the Sun as probing signals. The method of the forward scatter radar is based on the phenomenon of a significant increase the bistatic target radar cross section when the probe signal is scattered forward, i.e. along direction of the principal beam of locator pattern.
|Conference||Signal Processing Symposium, SPSympo 2019|
|Abbreviated title||SPSympo 2019|
|Period||17/09/19 → 19/09/19|
- forward scatter effect