In June of 1992 a NASA sounding rocket was fired into the Arecibo heater be
am to provide in situ observations of artificially induced ionospheric irre
gularities. In this paper we provide a radar scattering calculation based o
n in situ data and compare the same with previous remote sensing experiment
s and with theory. The calculated backscatter cross section is in good agre
ement with prior observations over the Arecibo heater at 50 MHz. More impor
tant, when we scale the observed in situ power spectrum appropriately and c
ompare it with multiradar cross-sectional results from the Platteville, Col
orado experiments, we find a remarkably similar radar frequency dependence,
albeit one shifted to smaller scales over the higher-latitude site. Even t
hough the rms fluctuation level is almost the same over the Arecibo and Pla
tteville heaters, the shift in scales toward smaller structures over Platte
ville explains the much larger VHF radar cross section measured there. Comp
arison of our waveform and its power spectrum with similar predictions from
a recent theory shows excellent agreement for k values up to about 5 times
the breakpoint in the spectrum of the theoretical prediction. Taken togeth
er, these results give very strong evidence for the production of needle-li
ke solitary structures as the dominant final state when high-power radio wa
ves reflect from a magnetized plasma. The organization of these structures
by as yet unexplained processes may explain the scales between 10 m and 10
km which occur in the heated volume. Finally, the dominant needle-like fiel
d-aligned density depletions seem to support a second source of smaller-sca
le irregularities. This creates a second break in the power law slope from
its one-dimensional value of k(-4.3) predicted by theory to one more nearly
characterized by k(-3). The multiradar results from Platteville show a sim
ilar break, and we speculate that a density and/or temperature-gradient-dri
ven instability such as the drift wave is operating.