Over at the Cosmoquest Forum, I saw this listing:
Earth-based radio astronomy below frequencies of 30MHz is severely restricted due to man-made interference, ionospheric distortion and almost complete non-transparency of the ionosphere below 10MHz. Therefore, this narrow spectral band remains possibly the last unexplored frequency range in radio astronomy.
http://arxiv.org/abs/1505.04711
Then I remembered this:
http://science.nasa.gov/science-news/science-at-nasa/2007/25jun_l2/
Wish-list missions for the Ares V range from a 150-meter-wide (492 ft) radio telescope dish to detect whispers from deep space to a 5-meter cube of super-pure water encased in light detectors to assay cosmic rays by their light flashes as they crash through the water. An optical telescope with a primary mirror up to 8 m (26 ft.) in diameter could search star populations in the Milky Way and nearby galaxies for the "fossil record" of their evolution. It could also hunt for "Earthshine spectra," faint signs of life in the light reflected by exoplanets.
But I wonder if the Earth-Sun Lagrange points are far out enough.
So here is a question. Could the Oort and the heliopause act as 'ground clutter' in blocking faint signals from any extant civilizations?
Earth-based radio astronomy below frequencies of 30MHz is severely restricted due to man-made interference, ionospheric distortion and almost complete non-transparency of the ionosphere below 10MHz. Therefore, this narrow spectral band remains possibly the last unexplored frequency range in radio astronomy.
http://arxiv.org/abs/1505.04711
Then I remembered this:
http://science.nasa.gov/science-news/science-at-nasa/2007/25jun_l2/
Wish-list missions for the Ares V range from a 150-meter-wide (492 ft) radio telescope dish to detect whispers from deep space to a 5-meter cube of super-pure water encased in light detectors to assay cosmic rays by their light flashes as they crash through the water. An optical telescope with a primary mirror up to 8 m (26 ft.) in diameter could search star populations in the Milky Way and nearby galaxies for the "fossil record" of their evolution. It could also hunt for "Earthshine spectra," faint signs of life in the light reflected by exoplanets.
But I wonder if the Earth-Sun Lagrange points are far out enough.
So here is a question. Could the Oort and the heliopause act as 'ground clutter' in blocking faint signals from any extant civilizations?