Long-term variations of the solar wind proton parameters

1974 ◽  
Vol 79 (34) ◽  
pp. 5095-5108 ◽  
Author(s):  
L. Diodato ◽  
G. Moreno ◽  
C. Signorini ◽  
K. W. Ogilvie
Entropy ◽  
2018 ◽  
Vol 20 (10) ◽  
pp. 799 ◽  
Author(s):  
George Livadiotis

The paper derives the polytropic indices over the last two solar cycles (years 1995–2017) for the solar wind proton plasma near Earth (~1 AU). We use ~92-s datasets of proton plasma moments (speed, density, and temperature), measured from the Solar Wind Experiment instrument onboard Wind spacecraft, to estimate the moving averages of the polytropic index, as well as their weighted means and standard errors as a function of the solar wind speed and the year of measurements. The derived long-term behavior of the polytropic index agrees with the results of other previous methods. In particular, we find that the polytropic index remains quasi-constant with respect to the plasma flow speed, in agreement with earlier analyses of solar wind plasma. It is shown that most of the fluctuations of the polytropic index appear in the fast solar wind. The polytropic index remains quasi-constant, despite the frequent entropic variations. Therefore, on an annual basis, the polytropic index of the solar wind proton plasma near ~1 AU can be considered independent of the plasma flow speed. The estimated all-year weighted mean and its standard error is γ = 1.86 ± 0.09.


2016 ◽  
Vol 832 (1) ◽  
pp. 66 ◽  
Author(s):  
Heather A. Elliott ◽  
David J. McComas ◽  
Craig E. DeForest

2019 ◽  
Vol 124 (6) ◽  
pp. 4049-4063 ◽  
Author(s):  
A. A. Samsonov ◽  
Y. V. Bogdanova ◽  
G. Branduardi‐Raymont ◽  
J. Safrankova ◽  
Z. Nemecek ◽  
...  

2018 ◽  
Vol 13 (S340) ◽  
pp. 108-114
Author(s):  
Mathew J. Owens ◽  
Mike Lockwood ◽  
Pete Riley ◽  
Luke Barnard

AbstractReconstructions of long-term solar variability underpin our understanding of the solar dynamo, potential tropospheric climate implications and future space weather scenarios. Prior to direct spacecraft measurements of the heliospheric magnetic field (HMF) and solar wind, accurate annual reconstructions are possible using geomagnetic and sunspot records. On longer timescales, information about the HMF can be extracted from cosmogenic radionuclide records, particularly 14C in ancient trees and 10Be in ice sheets. These proxies, and what they reveal about the HMF and solar wind, are briefly reviewed here.


2001 ◽  
Vol 366 (1) ◽  
pp. 331-338 ◽  
Author(s):  
K. Scherer ◽  
E. Marsch ◽  
R. Schwenn ◽  
H. Rosenbauer

1978 ◽  
Vol 83 (A5) ◽  
pp. 2177 ◽  
Author(s):  
W. C. Feldman ◽  
J. R. Asbridge ◽  
S. J. Bame ◽  
J. T. Gosling

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