Ulysses Solar Wind Plasma Observations at High Southerly Latitudes

Details Ulysses Solar Wind Plasma Observations at High Southerly Latitudes Ulysses Solar Wind Plasma Observations at High Southerly Latitudes

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sci...268.1030p&link_type=abstract

Science, Volume 268, Issue 5213, pp. 1030-1033

Computer Science

141

Scientific paper

Solar wind plasma observations made by the Ulysses spacecraft through -80.2^circ solar latitude and continuing equatorward to -40.1^circ are summarized. Recurrent high-speed streams and corotating interaction regions dominated at middle latitudes. The speed of the solar wind was typically 700 to 800 kilometers per second poleward of -35^circ. Corotating reverse shocks persisted farther south than did forward shocks because of the tilt of the heliomagnetic streamer belt. Sporadic coronal mass ejections were seen as far south as -60.5^circ. Proton temperature was higher and the electron strahl was broader at higher latitudes. The high-latitude wind contained compressional, pressure-balanced, and Alfvenic structures.

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