A conjugate study of Pc3-4 pulsations at cusp latitudes: Is there a clock angle effect?

Pc3-4 (15-50 mHz) pulsations are often observed during daytime hours in the Earth's magnetosphere and on the ground. The ion foreshock region of the s olar wind upstream of Earth is now understood to be a major source of these waves, and the general dependence of their occurrence in the magnetosphere on the cone angle of the interplanetary magnetic field (IMF) is well attes ted. However, there have also been suggestions that the IMF clock angle sho uld introduce latitudinal or local time asymmetries in wave occurrence, and in particular, that Pc3-4 pulsations might preferentially reach northern v ersus southern high-latitude regions. In order to test this latter suggesti on, we have compared a full year's (1997) data from two cusp-latitude stati ons, Sondrestromfjord, Greenland, and South Pole, Antarctica, both near 74 degrees corrected geomagnetic latitude. Our data show the usual strong IMF cone angle control of Pc3-4 wave occurrence/amplitude but also indicate tha t occurrence and relative amplitude are essentially identical near both cus ps; any clock angle control is at most a second-order effect, not detectabl e in our analysis. We further find little seasonal dependence in the ratio of power in the two cusp regions other than that attributable to difference s in solar illumination. These observations, in conjunction with the well-k nown sharp cutoff in wa,ve activity for cone angles above 45 degrees, indic ate that only those perturbations occurring at the subsolar bow shock can r each the magnetopause and propagate to any location in the dayside magnetos phere. In addition, the absence of a clock: angle effect supports earlier s uggestions that Pc3-4 signals in the magnetosheath do not cross streamlines and thus do not propagate as waves, but are rather convected as spatial st ructures in the highly turbulent, high-beta downstream magnetosheath plasma .