Solar Wind Electron Observations Near Solar Maximum at High Latitudes From Thermal Noise Spectroscopy

Details Solar Wind Electron Observations Near Solar Maximum at High Latitudes From Thermal Noise Spectroscopy Solar Wind Electron Observations Near Solar Maximum at High Latitudes From Thermal Noise Spectroscopy

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ssrv...97..105i&link_type=abstract

Space Science Reviews, v. 97, Issue 1/4, p. 105-108 (2001).

Computer Science

3

Scientific paper

The Ulysses spacecraft is reaching high heliolatitudes during the approach to solar maximum. We show preliminary in situ electron observations from the URAP experiment, using thermal noise spectroscopy. This method is especially suited to measure accurately the electron density and thermal temperature. The data acquired in the period June September 2000 are compared to those obtained at similar heliolatitudes near solar activity minimum and in the ecliptic plane near both solar maximum and minimum.

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