Interpretation of vector electric field measurements of bursty Langmuir waves in the cusp

Abstract

An analysis of auroral Langmuir waves in the cusp observed by two high‐frequency electric field instruments on the TRICE high‐flyer sounding rocket shows many examples of Langmuir wave bursts modulated at approximately 10 kHz. Previous studies have explained these and similar observations as the result of beating between waves with very close frequencies near the Langmuir cutoff, resulting from either wave‐wave interactions or independent linear excitations. The unique three‐dimensional (3‐D) data set provided by the NASA Goddard Space Flight Center TAEFWD instrument shows that up to 25% of waveforms selected from the most intense bursts exhibit anisotropic modulations, i.e., the beat nulls and peaks are not aligned in time across the three perpendicular electric field components. Modulations of this type arise when superposed wave normal modes possess differing polarizations, and simulations using wave modes calculated with the J‐WHAMP numerical dispersion code show (1) that waves with differing polarizations can exist in conditions like those observed by TRICE‐High and (2) that superpositions of such waves can produce anisotropic modulation. Fourier analysis of the 3‐D waveform data suggests that both linear and elliptically polarized waves are present near the Langmuir cutoff at these times. These observations illustrate how 3‐D measurements can give valuable insight into the nature of wave interactions in the auroral plasma environment.