Wind-Ulysses in-situ thermal noise measurements of solar wind electron density and core temperature at solar maximum and minimum

2003 ◽  
Vol 32 (4) ◽  
pp. 491-496 ◽  
Author(s):  
C. Salem ◽  
S. Hoang ◽  
K. Issautier ◽  
M. Maksimovic ◽  
C. Perche
Keyword(s):  
Solar Wind ◽  
Electron Density ◽  
Core Temperature ◽  
Thermal Noise ◽  
Solar Maximum ◽  
Noise Measurements ◽  
Solar Wind Electron

Solar wind electron density and temperature over solar cycle 23: Thermal noise measurements on Wind

2005 ◽  
Vol 35 (12) ◽  
pp. 2141-2146 ◽  
Author(s):  
K. Issautier ◽  
C. Perche ◽  
S. Hoang ◽  
C. Lacombe ◽  
M. Maksimovic ◽  
...  
Keyword(s):  
Solar Wind ◽  
Solar Cycle ◽  
Electron Density ◽  
Thermal Noise ◽  
Solar Cycle 23 ◽  
Noise Measurements ◽  
Electron Density And Temperature ◽  
Solar Wind Electron

Solar wind radial and latitudinal structure: Electron density and core temperature from Ulysses thermal noise spectroscopy

1998 ◽  
Vol 103 (A2) ◽  
pp. 1969-1979 ◽  
Author(s):  
Karine Issautier ◽  
Nicole Meyer-Vernet ◽  
Michel Moncuquet ◽  
Sang Hoang
Keyword(s):  
Solar Wind ◽  
Electron Density ◽  
Core Temperature ◽  
Thermal Noise ◽  
Noise Spectroscopy

scholarly journals Asymmetric multifractal model for solar wind intermittent turbulence

2008 ◽  
Vol 15 (4) ◽  
pp. 615-620 ◽  
Author(s):  
A. Szczepaniak ◽  
W. M. Macek
Keyword(s):  
Solar Wind ◽  
Solar Maximum ◽  
Solar Wind Plasma ◽  
Intermittent Turbulence ◽  
Proposed Model ◽  
Scaling Parameters ◽  
Generalized Dimensions ◽  
Multifractal Nature ◽  
Turbulent Cascade

Abstract. We consider nonuniform energy transfer rate for solar wind turbulence depending on the solar cycle activity. To achieve this purpose we determine the generalized dimensions and singularity spectra for the experimental data of the solar wind measured in situ by Advanced Composition Explorer spacecraft during solar maximum (2001) and minimum (2006) at 1 AU. By determining the asymmetric singularity spectra we confirm the multifractal nature of different states of the solar wind. Moreover, for explanation of this asymmetry we propose a generalization of the usual so-called p-model, which involves eddies of different sizes for the turbulent cascade. Naturally, this generalization takes into account two different scaling parameters for sizes of eddies and one probability measure parameter, describing how the energy is transferred to smaller eddies. We show that the proposed model properly describes multifractality of the solar wind plasma.

Solar wind electron parameters from quasi-thermal noise spectroscopy and comparison with other measurements on Ulysses

1995 ◽  
Vol 100 (A10) ◽  
pp. 19881 ◽  
Author(s):  
M. Maksimovic ◽  
S. Hoang ◽  
N. Meyer-Vernet ◽  
M. Moncuquet ◽  
J.-L. Bougeret ◽  
...  
Keyword(s):  
Solar Wind ◽  
Thermal Noise ◽  
Noise Spectroscopy ◽  
Solar Wind Electron

In Situ Heating of the Nightside Martian Upper Atmosphere and Ionosphere: The Role of Solar Wind Electron Precipitation

2021 ◽  
Vol 909 (2) ◽  
pp. 108
Author(s):  
D.-D. Niu ◽  
J. Cui ◽  
H. Gu ◽  
X. -S. Wu ◽  
Y. -T. Cao ◽  
...  
Keyword(s):  
Solar Wind ◽  
Upper Atmosphere ◽  
Electron Precipitation ◽  
In Situ Heating ◽  
Solar Wind Electron

scholarly journals An Improved Solar Wind Electron Density Model for Pulsar Timing

2007 ◽  
Vol 671 (1) ◽  
pp. 907-911 ◽  
Author(s):  
X. P. You ◽  
G. B. Hobbs ◽  
W. A. Coles ◽  
R. N. Manchester ◽  
J. L. Han
Keyword(s):  
Solar Wind ◽  
Electron Density ◽  
Density Model ◽  
Pulsar Timing ◽  
Solar Wind Electron

Large-Scale Variation of Solar Wind Electron Properties from Quasi-Thermal Noise Spectroscopy: Ulysses Measurements

Solar Physics ◽  
2011 ◽  
Vol 271 (1-2) ◽  
pp. 141-148 ◽  
Author(s):  
G. Le Chat ◽  
K. Issautier ◽  
N. Meyer-Vernet ◽  
S. Hoang
Keyword(s):  
Solar Wind ◽  
Large Scale ◽  
Thermal Noise ◽  
Noise Spectroscopy ◽  
Solar Wind Electron ◽  
Scale Variation
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