2008
DOI: 10.1016/j.jastp.2008.03.017
|View full text |Cite
|
Sign up to set email alerts
|

Ionospheric effects of ground motion: The roles of magnetic field and nonlinearity

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

0
6
0

Year Published

2009
2009
2019
2019

Publication Types

Select...
7
1

Relationship

0
8

Authors

Journals

citations
Cited by 9 publications
(6 citation statements)
references
References 21 publications
0
6
0
Order By: Relevance
“…The acoustic wave propagated across the magnetic field lines and then excited an ion acoustic wave through the collision. The interaction between acoustic waves and magnetosonic waves in the ionosphere has been discussed [ Aburjania and Machabeli , ; Ostrovsky , ]. The results suggest that plasma perturbation might be excited by the acoustic wave generated by the rocket.…”
Section: Discussionmentioning
confidence: 99%
“…The acoustic wave propagated across the magnetic field lines and then excited an ion acoustic wave through the collision. The interaction between acoustic waves and magnetosonic waves in the ionosphere has been discussed [ Aburjania and Machabeli , ; Ostrovsky , ]. The results suggest that plasma perturbation might be excited by the acoustic wave generated by the rocket.…”
Section: Discussionmentioning
confidence: 99%
“…The observed spreading of the positive and negative phases of the slow ionospheric response can be attributed to the different speed of propagation for the positive and negative phases of the initial atmospheric disturbance (i.e., the compression‐rarefaction phases of the acoustic N wave). At some altitude where the magnetic pressure dominates the thermal pressure (at about 160–170 km) an acoustic wave propagating upward from the ground to ionospheric level transforms into the fast magnetic sound which is the same wave mode as the nonmagnetic sound [ Ostrovsky , 2008]. In cases in which magnetic forces dominate the displacement of plasma becomes mostly in direction across the magnetic field due to “frozen‐in” condition.…”
Section: Discussionmentioning
confidence: 99%
“…This causes steepening of the initial part of the wave, and the whole waveform approaches that of a shock wave (Naugolnykh and Ostrovsky, 1998, section 3.5). Magnetic field may weaken these processes above ∼120 km (Ostrovsky, 2008), and the slope of the wave front decreases and the wavelength extends up to tens of hundreds of kilometers at the height of the F-layer. Atmospheric viscosity also changes the waveform by isolating the wave with frequencies within a window of 3-10 mHz (Blanc, 1985).…”
Section: Discussionmentioning
confidence: 99%