scholarly journals Solar cycle dependence of solar wind energy coupling to the thermosphere

2011 ◽  
Vol 116 (A6) ◽  
pp. n/a-n/a ◽  
Author(s):  
William J. Burke
Keyword(s):  
Solar Wind ◽  
Solar Cycle ◽  
Wind Energy ◽  
Energy Coupling ◽  
Cycle Dependence ◽  
Solar Wind Energy

Magnetospheric modes and solar wind energy coupling efficiency

2010 ◽  
Vol 115 (A3) ◽  
pp. n/a-n/a ◽  
Author(s):  
T. I. Pulkkinen ◽  
M. Palmroth ◽  
H. E. J. Koskinen ◽  
T. V. Laitinen ◽  
C. C. Goodrich ◽  
...  
Keyword(s):  
Solar Wind ◽  
Wind Energy ◽  
Coupling Efficiency ◽  
Energy Coupling ◽  
Solar Wind Energy

Efficiency of solar wind energy coupling to the ionosphere

2012 ◽  
Vol 117 (A7) ◽  
pp. n/a-n/a ◽  
Author(s):  
Jianpeng Guo ◽  
Xueshang Feng ◽  
Barbara A. Emery ◽  
Yi Wang
Keyword(s):  
Solar Wind ◽  
Wind Energy ◽  
Energy Coupling ◽  
Solar Wind Energy

Solar cycle dependence of the solar wind dynamics: Pioneer Voyager, and Ulysses from 1 to 5 AU

1996 ◽  
Vol 101 (A11) ◽  
pp. 24359-24371 ◽  
Author(s):  
J. Américo González-Esparza ◽  
Edward J. Smith
Keyword(s):  
Solar Wind ◽  
Solar Cycle ◽  
Cycle Dependence

scholarly journals Proposing the solar‐wind energy flux hypothesis as a driver of inter‐annual variation in tropical tree reproductive effort

2019 ◽  
Vol 106 (11) ◽  
pp. 1519-1525
Author(s):  
J. Aaron Hogan ◽  
Christopher J. Nytch ◽  
John E. Bithorn ◽  
Jess K. Zimmerman
Keyword(s):  
Solar Wind ◽  
Wind Energy ◽  
Energy Flux ◽  
Annual Variation ◽  
Reproductive Effort ◽  
Tropical Tree ◽  
Solar Wind Energy

scholarly journals Solar cycle dependence of scaling in solar wind fluctuations

2008 ◽  
Vol 15 (3) ◽  
pp. 445-455 ◽  
Author(s):  
S. C. Chapman ◽  
B. Hnat ◽  
K. Kiyani
Keyword(s):  
Solar Wind ◽  
Solar Cycle ◽  
Momentum Flux ◽  
Magnetic Fluctuations ◽  
Mhd Turbulence ◽  
Scaling Properties ◽  
Two Component ◽  
Energy And Momentum ◽  
Cycle Dependence

Abstract. In this review we collate recent results for the statistical scaling properties of fluctuations in the solar wind with a view to synthesizing two descriptions: that of evolving MHD turbulence and that of a scaling signature of coronal origin that passively propagates with the solar wind. The scenario that emerges is that of coexistent signatures which map onto the well known "two component" picture of solar wind magnetic fluctuations. This highlights the need to consider quantities which track Alfvénic fluctuations, and energy and momentum flux densities to obtain a complete description of solar wind fluctuations.

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