scholarly journals Daytime high-latitude pulsations associated with solar wind dynamic pressure impulses and flux transfer events

1997 ◽  
Vol 102 (A1) ◽  
pp. 57-67 ◽  
Author(s):  
Oksana I. Yagodkina ◽  
Vyacheslav G. Vorobjev
Keyword(s):  
Solar Wind ◽  
High Latitude ◽  
Dynamic Pressure ◽  
Solar Wind Dynamic Pressure ◽  
Flux Transfer Events ◽  
Flux Transfer

High-latitude ground-based response to sudden changes in solar wind dynamic pressure

1996 ◽  
Vol 101 (A12) ◽  
pp. 27001-27013 ◽  
Author(s):  
R. J. Sitar ◽  
C. R. Clauer ◽  
E. Friis-Christensen
Keyword(s):  
Solar Wind ◽  
High Latitude ◽  
Dynamic Pressure ◽  
Solar Wind Dynamic Pressure

scholarly journals Geomagnetic response to solar wind dynamic pressure impulse events at high-latitude conjugate points

2013 ◽  
Vol 118 (10) ◽  
pp. 6055-6071 ◽  
Author(s):  
H. Kim ◽  
X. Cai ◽  
C. R. Clauer ◽  
B. S. R. Kunduri ◽  
J. Matzka ◽  
...  
Keyword(s):  
Solar Wind ◽  
High Latitude ◽  
Dynamic Pressure ◽  
Solar Wind Dynamic Pressure ◽  
Conjugate Points ◽  
Pressure Impulse

scholarly journals Effects of Abrupt Variations of Solar Wind Dynamic Pressure on the High-Latitude Ionosphere

2011 ◽  
Vol 2011 ◽  
pp. 1-8 ◽  
Author(s):  
Igino Coco ◽  
Ermanno Amata ◽  
Maria Federica Marcucci ◽  
Danila Ambrosino ◽  
Simon G. Shepherd
Keyword(s):  
Solar Wind ◽  
High Latitude ◽  
Statistical Study ◽  
Dynamic Pressure ◽  
Solar Wind Dynamic Pressure ◽  
Polar Cap ◽  
Radar Backscatter ◽  
Preliminary Results ◽  
Radar Network ◽  
High Latitude Ionosphere

We show the results of a statistical study on the effects in the high-latitude ionosphere of abrupt variations of solar wind dynamic pressure, using Super Dual Auroral Radar Network (SuperDARN) data in both hemispheres. We find that, during periods of quiet ionospheric conditions, the amount of radar backscatter increases when a variation in the dynamic pressure occurs, both positive (increase of the pressure) and negative (decrease of the pressure). We also investigate the behaviour of the Cross-Polar Cap Potential (CPCP) during pressure variations and show preliminary results.

scholarly journals High-Latitude Thermosphere Neutral Density Response to Solar Wind Dynamic Pressure Enhancement

2017 ◽  
Vol 122 (11) ◽  
pp. 11,559-11,578 ◽  
Author(s):  
Y. Shi ◽  
E. Zesta ◽  
H. K. Connor ◽  
Y.-J. Su ◽  
E. K. Sutton ◽  
...  
Keyword(s):  
Solar Wind ◽  
High Latitude ◽  
Dynamic Pressure ◽  
Solar Wind Dynamic Pressure ◽  
Neutral Density ◽  
Density Response

Solar wind dynamic pressure enhancements and polar auroras

1998 ◽  
Vol 22 (9) ◽  
pp. 1305-1308 ◽  
Author(s):  
Y Zhang ◽  
D.J McEwen ◽  
I Oznovich
Keyword(s):  
Solar Wind ◽  
Dynamic Pressure ◽  
Solar Wind Dynamic Pressure

The Effect of Solar Wind Mach Numbers on the Occurrence Rate of Flux Transfer Events at the Dayside Magnetopause

2019 ◽  
Vol 46 (8) ◽  
pp. 4106-4113 ◽  
Author(s):  
C. Chen ◽  
T. R. Sun ◽  
C. Wang ◽  
Z. H. Huang ◽  
B. B. Tang ◽  
...  
Keyword(s):  
Solar Wind ◽  
Occurrence Rate ◽  
Flux Transfer Events ◽  
Dayside Magnetopause ◽  
Mach Numbers ◽  
Flux Transfer
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