Author/Authors :
B.T. Tsurutani، نويسنده , , J.K. Arballo ، نويسنده , , C. Galvan، نويسنده , , L.D. Zhang، نويسنده , , G.S. Lakhina ، نويسنده , , T. Hada، نويسنده , , J.S. Pickett، نويسنده , , D.A. Gurnett، نويسنده ,
Abstract :
Polar Cap Boundary Layer waves are ELF/VLF electric and magnetic waves detected on field lines adjacent to the polar cap, thus their name. Waves are present at this location 96% of the time. The wave latitude-local time distribution is shown to be the same as that of the auroral oval. The most intense waves are detected coincident with the strongest magnetic field gradients (field-aligned currents). Specific frequency bands of whistler mode-waves are identified: ∼200 Hz, 1–2 kHz and ∼5 kHz. Two types of intense electric waves are present: solitary bipolar pulses (electron holes) and ∼kHz electric turbulence. The PCBL waves are most likely a consequence of auroral zone field-aligned current instabilities. The currents have in turn been ascribed to be due to magnetospheric convection driven by the solar wind.