Published July 2013 | Version v1
Journal article

Investigation of acoustic gravity waves created by anomalous heat sources: experiments and theoretical analysis

  • 1. Space Propulsion Laboratory, Massachusetts Institute of Technology (MIT), Cambridge, MA 02139 (United States)

Description

We have been investigating high-power radio wave-induced acoustic gravity waves (AGWs) at Gakona, Alaska, using the High-frequency Active Aurora Research Program (HAARP) heating facility (i.e. HF heater) and extensive diagnostic instruments. This work was aimed at performing a controlled study of the space plasma turbulence triggered by the AGWs originating from anomalous heat sources, as observed in our earlier experiments at Arecibo, Puerto Rico (Pradipta 2007 MS Thesis MIT Press, Cambridge, MA). The HF heater operated in continuous wave (CW) O-mode can heat ionospheric plasmas effectively to yield a depleted magnetic flux tube as rising plasma bubbles (Lee et al 1998 Geophys. Res. Lett. 25 579). Two processes are responsible for the depletion of the magnetic flux tube: (i) thermal expansion and (ii) chemical reactions caused by heated ions. The depleted plasmas create large density gradients that can augment spread F processes via generalized Rayleigh–Taylor instabilities (Lee et al 1999 Geophys. Res. Lett. 26 37). It is thus expected that the temperature of neutral particles in the heated ionospheric region can be increased. Such a heat source in the neutral atmosphere may potentially generate AGWs in the form of traveling ionospheric plasma disturbances (TIPDs). We should point out that these TIPDs have features distinctively different from electric and magnetic field (ExB) drifts of HF wave-induced large-scale non-propagating plasma structures. Moreover, it was noted in our recent study of naturally occurring AGW-induced TIDs that only large-scale AGWs can propagate upward to reach higher altitudes. Thus, in our Gakona experiments we select optimum heating schemes for HF wave-induced AGWs that can be distinguished from the naturally occurring ones. The generation and propagation of AGWs are monitored by MUIR (Modular Ultra high-frequency Ionospheric Radar), Digisonde and GPS/low-earth-orbit satellites. Our theoretical and experimental studies have shown that anomalous heat sources produced by, for example, global warming can become potential causes inducing extensive large-scale turbulence in the neutral atmosphere and space plasmas. (paper)

Availability note (English)

Available from http://dx.doi.org/10.1088/0031-8949/2013/T155/014028

Additional details

Publishing Information

Journal Title
Physica Scripta (Online)
Journal Volume
2013
Journal Issue
T155
Journal Page Range
[4 p.]
ISSN
1402-4896

Conference

Title
3. international conference on turbulent mixing and beyond
Dates
21-28 Aug 2011
Place
Trieste (Italy)