Physics
Scientific paper
Aug 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jgr....9813605i&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 98, no. A8, p. 13,605-13,625.
Physics
13
F Region, Ionospheric Electron Density, Particle Interactions, Plasma Waves, Radio Frequency Heating, Electron Energy, Incoherent Scatter Radar, Plasma Density
Scientific paper
Observations were made of the HF-modified ionosphere over Arecibo during the daytime and during the nighttime using chirped incoherent scatter radar. The daytime observations show a difference in the frequencies of the HF-induced plasma line (HFPL) and the photoelectron-enhanced (natural) plasma line (PEPL) at the same height of the order of 100 kHz. In addition, the daytime HFPL originates within about 200 m of the reflection height, often within 20 ms of HF turn-on, and may remain at that location for many seconds. A second HFPL source region was sometimes observed to form between approximately 1 and 4 km below the usual source region after 5 to 10 s of heating. During the nighttime, rapidly changing regions of HF-induced plasma lines spread over more than 3 km in height were observed; the existence of these regions appears to be strongly dependent on HF heating power. At times, frequency shifting and broadening of the PEPL during heating was noted; the shift in frequency is due to increasing electron temperature and the frequency broadening to the appearance of short-scale density striations. These effects continued even during periods when the heater remained on and the HF-induced line was not observed by the radar.
Hagfors Tor
Isham B.
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