A winning proposal for the Innovative Research Program, 2009: Passive Radio Imaging for Applications in Water Resource Management, Glaciology, and Space Weather MonitoringInvestigators: Nick Zabotin and Oleg Godin, CIRES, University of Colorado Objective Background and Importance We anticipate a possibility of expanding the passive imaging technique to the area of HF radio wave propagation, where such applications as monitoring the water table level, measuring ice thickness or determining an altitude of ionospheric layers, are feasible. Implementing passive techniques in this field would have positive environmental and societal impact: the radio spectrum is densely occupied by various vital applications, and using new active sources of radio signals is often prohibited. Passive techniques allow using frequencies that may be unavailable for active methods. Low power consumption of passive sensors increases the time of their autonomous operation, while their low cost allow for a large number of networked sensors and an improved spatial resolution of tomographic inversions. Of course, frequencies and necessary data acquisition rates are many orders of magnitude higher for radio than for seismic waves. Passive imaging with HF radio waves would not be possible if not for the digital receivers that became available only recently. Radio noise in the HF band is present constantly. It is caused by multiple and globally-distributed sources of natural (lightning) and of technogenic (industrial noise and distant radio stations) origin. On the other hand, now we have numerous instruments incorporating modern fully digital HF receivers highly appropriate for measuring and studying the noise properties. Among them, first and foremost, there are four VIPIR systems just installed at Jicamarca Radio Observatory, Peru, at NASA’s Wallops Flight Facility, Virginia, at Tomsk State University, Russia, and in Boulder, Colorado. The photographs on the right show receiving antenna array and 8-channel fully digital HF radar installed at Wallops. The eight dipole antennas form two orthogonal lines, ~100 m in length, and allow accurate measurements of polarization, direction of arrival, and amplitude of the received signal. The primary purpose of the VIPIR systems is active radio sounding of the ionosphere. In this project, we will be using them in an innovative way. Research Plan 1) In many situations of practical interest, the incoming signal is a result of interference of a direct signal and a signal reflected from underlying surface(s) where a jump of the dielectric permittivity occurs (e.g., the water table level or the upper and lower boundaries of an ice layer; see a sketch below). In this situation, theory predicts a pronounced dependence of the noise auto- and crosscorrelation on wave polarization and thickness of the layer. This scheme may be used to retrieve the layer thickness from measurements of the correlation of polarization components of the signal.
2) Radio noise propagating in the vertical direction is usually relatively weak. However, its presence is still noticeable because of roughness of both the ground surface and the ionosphere boundary. Auto-correlation function of the amplitude of the electromagnetic noise field measured at a single location must show double peaks corresponding to the two-way propagation time between the ground and the ionosphere (see a sketch on the right). This property may be used to determine the altitude of the ionosphere, a quantity that strongly depends on the space weather conditions. Why is this innovative and important? Why is this interdisciplinary? Expected outcome |