Formation of Minor‐Ion Charge States in the Fast Solar Wind: Roles of Differential Flow Speeds of Ions of the Same Element

2003 ◽  
Vol 582 (1) ◽  
pp. 467-474 ◽  
Author(s):  
Y. Chen ◽  
R. Esser ◽  
Y. Hu
2007 ◽  
Vol 660 (2) ◽  
pp. 1642-1652 ◽  
Author(s):  
J. Martin Laming ◽  
Susan T. Lepri

2017 ◽  
Vol 13 (S335) ◽  
pp. 87-89
Author(s):  
Andrzej Fludra ◽  
Enrico Landi

AbstractWe present a new technique to study joint observations of EUV spectral line intensities and in situ charge states of the fast solar wind. We solve the time-dependent equation for ionization and recombination for a chosen element and calculate the charge state evolution along the open magnetic fields for elements such as C, O, Ne, Mg, Si and Fe. Comparing predicted spectral lines intensities above the limb and in situ charge states to observations from SOHO/SUMER and Ulysses/SWICS, we test how well the modelled thermodynamic parameters of the solar wind reproduce observations. We outline the application of this method to Solar Orbiter data.


Author(s):  
L. Adhikari ◽  
G.P. Zank ◽  
L.-L. Zhao ◽  
M. Nakanotani ◽  
S. Tasnim

2010 ◽  
Vol 709 (2) ◽  
pp. 993-1002 ◽  
Author(s):  
Stefano Pucci ◽  
Øystein Lie-Svendsen ◽  
Ruth Esser

Solar Physics ◽  
2017 ◽  
Vol 292 (9) ◽  
Author(s):  
Peter Bochsler ◽  
Andrzej Fludra ◽  
Alessandra Giunta
Keyword(s):  

Author(s):  
G. Gogoberidze ◽  
E. Gorgaslidze

We study spectral features of Alfvénic turbulence in fast solar wind. We propose a general, instrument independent method to estimate the uncertainty in velocity fluctuations obtained by in-situ satellite observations in the solar wind. We show that when the measurement uncertainties of the velocity fluctuations are taken into account the less energetic Elsasser spectrum obeys a unique power law scaling throughout the inertial range as prevailing theories of magnetohydrodynamic turbulence predict.


2020 ◽  
Vol 889 (1) ◽  
pp. L14
Author(s):  
G. Q. Zhao ◽  
H. Q. Feng ◽  
D. J. Wu ◽  
J. Huang ◽  
Y. Zhao ◽  
...  

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