Anyway this power is much lower the power needed to observe 'normal whistler' man-generated. Reason is simple: requred energy 'expanded' in time. Seems factor should be ~10^4 or more? Regards, Alexan
Paul, can you give a reference (http is better, say arxive.org) to some review paper on cooperative effects in ionosphere? What does it mean? You mentioned 'cooperative D-layer' before. But i have ne
OK. I had misunderstand you. Certanly it will be good if amateurs cooperate with researchers. It seems to me vlf (or may be lf at least) is the only area where HAM's experiments can have some reseach
Some daily plots of the background noise amplitude at 8.97kHz, each point averaged across 12Hz for 120 seconds, and rescaled to 1Hz bandwidth: http://abelian.org/vlf/live/100305.9kHz.png http://abeli
By the way one can imagine some 'reverse whistler' if TX radiate apropriate FM signal which is 'de-chirped' by dispersion in ionosphere. Can you roughly estimate radiated power needed to observe such