Low‐Latitude Whistler‐Wave Spectra and Polarization From VEFI and CINDI Payloads on C/NOFS Satellite

Abstract

The Communication/Navigation Outage Forecast System (C/NOFS) satellite's VEFI payload performed frequent recordings of the vector electric field in the band 0-16 kHz during the epoch 2008-2014. The Vector Electric Field Instrument (VEFI) was supported by ion-composition data from the Coupled Ion Neutral Dynamics Investigation (CINDI) instrument. We focus here on statistics of these "burst-mode" recordings, of which 6,890 (mostly~12-s duration) records meet stringent quality-control criteria, allowing inference of the wave vector k and its orientation relative to the Earth's magnetic field B 0 . The 6,890 records occur between ±13°(geographic) latitude and between~400-and 850-km altitude, mostly in the topside ionosphere. The wave activity is dominated by terrestrial lightning. We analyze the whistler-wave intensity and polarization for each pixel in the time-frequency spectrogram for each record. We then gather weighted statistics on wave polarization, naturally weighted by wave intensity. In this manner we arrive at statistical results that represent the bulk of the energy flow due to whistler waves. Despite rather nonstationary statistics, we can reach three empirical results.a We see no evidence of a low-latitude suppression of whistler-wave activity, in contrast to the predictions of models of transmission through a laminar ionosphere. b The wave vector polar angle is always in the range 40°to 90°from parallel to B 0 . This indicates that the propagation at low latitudes is dominated by oblique, not ducted, whistlers. c At the lowest magnetic latitudes, the wave vector polar angle with respect to B 0 becomes nearly 90°.

Properties of Lightning Generated Whistlers Based on Van Allen Probes Observations and Their Global Effects on Radiation Belt Electron Loss

“…Wave normal angles show intermediate values (30°–50°) at L < 2 and at frequencies below 0.25 f LHR over 2 < L < 4, where f LHR represents the equatorial lower hybrid resonance frequency, which is approximately equal to f ce /43 in this region where the electron plasma frequency is larger than the electron cyclotron frequency. Overall, the majority of LGWs show oblique wave normal angles, indicating that they propagate preferentially in the unducted mode, consistent with the previous statistical results of oblique wave normal angles over 40°–90° (Jacobson et al, 2020). However, wave normal angles tend to be small at frequencies above 0.1 f ce , although not many LGWs are detected in this frequency range (Figure 3a).…”