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

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

The MAVEN Solar Wind Electron Analyzer

2016 ◽  
Vol 200 (1-4) ◽  
pp. 495-528 ◽  
Author(s):  
D. L. Mitchell ◽  
C. Mazelle ◽  
J.-A. Sauvaud ◽  
J.-J. Thocaven ◽  
J. Rouzaud ◽  
...  
Keyword(s):  
Solar Wind ◽  
Solar Wind Electron

Electron density and conductance in the auroral ionosphere during substorms. Influence of solar wind and plasma sheet state.

2021 ◽  
Author(s):  
Nikita Stepanov ◽  
Victor Sergeev ◽  
Maria Shukhtina ◽  
Yasunobu Ogawa ◽  
Xiangning Chu
Keyword(s):  
Solar Wind ◽  
Electron Density ◽  
Plasma Sheet ◽  
Auroral Ionosphere

scholarly journals Galactic structure and turbulence, pulsar distances, and the intergalactic medium

2012 ◽  
Vol 8 (S291) ◽  
pp. 211-216 ◽  
Author(s):  
J. M. Cordes
Keyword(s):  
Electron Density ◽  
Intergalactic Medium ◽  
Galactic Structure ◽  
Density Model ◽  
Radio Bursts ◽  
Radio Waves ◽  
Next Generation ◽  
Scattering Measurements ◽  
Galactic Model ◽  
Multi Wavelength

AbstractThis paper summarizes how multi-wavelength measurements will be aggregated to determine Galactic structure in the interstellar medium (ISM) and produce the next-generation electron density model. Fluctuations in density and magnetic field from parsec scales down to about 1000 km cause a number of propagation effects in both radio waves and cosmic rays. Density microstructure appears to include Kolmogorov-like turbulence. The next generation electron-density model, NE2012, will include about double the number of lines of sight with dispersion and scattering measurements and it will be anchored with a much larger number of pulsar parallax distances. The foreground Galactic model is crucial for inferring similar ionized structures in the intergalactic medium (IGM) from scattering measurements on high-z objects. Intergalactic scattering is discussed with reference to distant sources of radio bursts. In particular, the cosmological radio scattering horizon is defined along with its analog for the ISM.

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