An upper bound on the solar radar cross section at 50 MHz

Details An upper bound on the solar radar cross section at 50 MHz An upper bound on the solar radar cross section at 50 MHz

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jgra..11104102c&link_type=abstract

Journal of Geophysical Research, Volume 111, Issue A4, CiteID A04102

Astronomy and Astrophysics

Astrophysics

Solar Physics, Astrophysics, And Astronomy: Corona, Solar Physics, Astrophysics, And Astronomy: Instruments And Techniques, Space Weather: Solar Effects, Interplanetary Physics: Mhd Waves And Turbulence (2752, 6050, 7836), Radio Science: Radar Astronomy

Scientific paper

We have made 16 unsuccessful attempts, in February and October 2003, and February 2004, to observe solar echoes using the 50 MHz radar at Jicamarca in Peru. The upper bound that we have determined on the solar cross section is significantly lower than the average of earlier reported observations. In this paper we will describe the observations, discuss the noise and interference from solar bursts, and suggest possible reasons why the echo might be weaker than expected.

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