scholarly journals Solar Flare Effects on 150‐km Echoes Observed Over Jicamarca: WACCM‐X Simulations

2019 ◽  
Vol 46 (20) ◽  
pp. 10951-10958 ◽  
Author(s):  
N. M. Pedatella ◽  
J. L. Chau ◽  
J. Vierinen ◽  
L. Qian ◽  
P. Reyes ◽  
...  
Keyword(s):  
Solar Flare ◽  
Solar Flare Effects

scholarly journals Solar Flare Effects Upon the Ionospheres of Earth and Mars

2008 ◽  
Author(s):  
Michael Mendillo ◽  
Paul Withers ◽  
Paul Song ◽  
John Foster ◽  
Michael Mendillo ◽  
...  
Keyword(s):  
Solar Flare ◽  
Solar Flare Effects

scholarly journals Possible Solar Flare Effects in the F Region of the Ionosphere

Nature ◽  
1961 ◽  
Vol 192 (4800) ◽  
pp. 347-347 ◽  
Author(s):  
G. H. MUNRO
Keyword(s):  
Solar Flare ◽  
F Region ◽  
Solar Flare Effects

Solar Flare Effects in Lunar Xenon

1971 ◽  
Vol 233 (41) ◽  
pp. 114-117 ◽  
Author(s):  
M. N. RAO ◽  
K. GOPALAN ◽  
V. S. VENKATAVARADAN ◽  
L. WILKENING
Keyword(s):  
Solar Flare ◽  
Solar Flare Effects

Solar flare effects in the ionosphere

1967 ◽  
Vol 72 (23) ◽  
pp. 6099-6103 ◽  
Author(s):  
Owen K. Garriott ◽  
Aldo V. da Rosa ◽  
Michael J. Davis ◽  
O. G. Villard
Keyword(s):  
Solar Flare ◽  
Solar Flare Effects

scholarly journals Modeling solar flare induced lower ionosphere changes using VLF/LF transmitter amplitude and phase observations at a midlatitude site

2013 ◽  
Vol 31 (4) ◽  
pp. 765-773 ◽  
Author(s):  
E. D. Schmitter
Keyword(s):  
Solar Flare ◽  
Continuous Monitoring ◽  
Lower Ionosphere ◽  
Signal Propagation ◽  
Electron Density Profile ◽  
Propagation Model ◽  
Inexpensive Method ◽  
Long Wave ◽  
Phase Data ◽  
Solar Flare Effects

Abstract. Remote sensing of the ionosphere bottom using long wave radio signal propagation is a still going strong and inexpensive method for continuous monitoring purposes. We present a propagation model describing the time development of solar flare effects. Based on monitored amplitude and phase data from VLF/LF transmitters gained at a mid-latitude site during the currently increasing solar cycle no. 24 a parameterized electron density profile is calculated as a function of time and fed into propagation calculations using the LWPC (Long Wave Propagation Capability). The model allows to include lower ionosphere recombination and attachment coefficients, as well as to identify the relevant forcing X-ray wavelength band, and is intended to be a small step forward to a better understanding of the solar–lower ionosphere interaction mechanisms within a consistent framework.

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