scholarly journals Association of solar wind proton flux extremes with pseudostreamers

2013 ◽  
Vol 118 (6) ◽  
pp. 2834-2841 ◽  
Author(s):  
L. Zhao ◽  
S. E. Gibson ◽  
L. A. Fisk
2013 ◽  
Author(s):  
Liang Zhao ◽  
Sarah E. Gibson ◽  
Lennard A. Fisk

1980 ◽  
Vol 91 ◽  
pp. 155-158
Author(s):  
H. J. Fahr ◽  
H. W. Ripken ◽  
G. Lay

Solar wind protons impinging on interplanetary dust grains are trapped, deionized, and subsequently desorbed. The steady state distribution of desorbed neutral hydrogen inside of 0.4 AU can be deduced by observation of resonantly scattered solar 121.6 nm radiation. Calculated integral intensities and spectral profiles are given, showing the clear spectral separation of the different radiation components. Given a specific solar wind proton flux, the interplanetary dust distribution can be determined. Conversely, dust density profiles from zodiacal light measurements can be used to deduce solar wind proton fluxes at heliocentric distances of 0.4 to 0.15 AU. Observations of latitudinal and short-term temporal proton flux variations seem feasible.


Space Weather ◽  
2014 ◽  
Vol 12 (7) ◽  
pp. 499-507 ◽  
Author(s):  
Charles W. Smith ◽  
K. G. McCracken ◽  
Nathan A. Schwadron ◽  
Molly L. Goelzer

2018 ◽  
Vol 123 (7) ◽  
pp. 5289-5299 ◽  
Author(s):  
C. Lue ◽  
J. S. Halekas ◽  
A. R. Poppe ◽  
J. P. McFadden

1973 ◽  
Vol 78 (28) ◽  
pp. 6451-6468 ◽  
Author(s):  
W. C. Feldman ◽  
J. R. Asbridge ◽  
S. J. Bame ◽  
M. D. Montgomery

Solar Physics ◽  
2015 ◽  
Vol 290 (9) ◽  
pp. 2589-2615 ◽  
Author(s):  
Justyna M. Sokół ◽  
Paweł Swaczyna ◽  
Maciej Bzowski ◽  
Munetoshi Tokumaru
Keyword(s):  

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