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Issautier Karine Hoang Sang Moncuquet Michel Meyer-Vernet Nicole 《Space Science Reviews》2001,97(1-4):105-108
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.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
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K. Issautier C. Perche S. Hoang C. Lacombe M. Maksimovic J.-L. Bougeret C. Salem 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,35(12):2141-2146
We present the solar wind plasma parameters obtained from the Wind spacecraft during more than nine years, encompassing almost the whole solar cycle 23. Since its launch in November 1994 Wind has frequently observed the in-ecliptic solar wind upstream of the Earth’s bow shock. The WIND/WAVES thermal noise receiver was specially designed to measure the in situ plasma thermal noise spectra, from which the electron density and temperature can be accurately determined. We present and discuss histograms of such measurements performed from 1994 to 2003. Using these large data sets, we study the density and core temperature variations with solar activity cycle and with different regimes of the solar wind. We confirm the anticorrelation of the electron density with the sunspot number, and obtain a positive correlation of the core temperature, with the sunspot number. 相似文献
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