Journal cover Journal topic
Annales Geophysicae An interactive open-access journal of the European Geosciences Union
Journal topic

Journal metrics

IF value: 1.490
IF 5-year value: 1.445
IF 5-year
CiteScore value: 2.9
SNIP value: 0.789
IPP value: 1.48
SJR value: 0.74
Scimago H <br class='widget-line-break'>index value: 88
Scimago H
h5-index value: 21
Volume 32, issue 9
Ann. Geophys., 32, 1145–1152, 2014
© Author(s) 2014. This work is distributed under
the Creative Commons Attribution 3.0 License.
Ann. Geophys., 32, 1145–1152, 2014
© Author(s) 2014. This work is distributed under
the Creative Commons Attribution 3.0 License.

Regular paper 16 Sep 2014

Regular paper | 16 Sep 2014

Ionospheric shock waves triggered by rockets

C. H. Lin1,2, J. T. Lin1, C. H. Chen1, J. Y. Liu3,4, Y. Y. Sun3,5, Y. Kakinami6, M. Matsumura7, W. H. Chen1, H. Liu8, and R. J. Rau1 C. H. Lin et al.
  • 1Department of Earth Sciences, National Cheng Kung University, Tainan, Taiwan
  • 2Earth Dynamic System Research Center, National Cheng Kung University, Tainan, Taiwan
  • 3Institute of Space Science, National Central University, Chung-Li, Taoyuan, Taiwan
  • 4National Space Organization, Hsinchu, Taiwan
  • 5CIRES, University of Colorado at Boulder, Boulder, CO, USA
  • 6School of Systems Engineering, Kochi University of Technology, Kami, Kochi, Japan
  • 7National Institute of Polar Research, Research Organization of Information and Systems, Tokyo, Japan
  • 8Department of Earth and Planetary Science, Faculty of Science, Kyushu University, Fukuoka, Kyushu, Japan

Abstract. This paper presents a two-dimensional structure of the shock wave signatures in ionospheric electron density resulting from a rocket transit using the rate of change of the total electron content (TEC) derived from ground-based GPS receivers around Japan and Taiwan for the first time. From the TEC maps constructed for the 2009 North Korea (NK) Taepodong-2 and 2013 South Korea (SK) Korea Space Launch Vehicle-II (KSLV-II) rocket launches, features of the V-shaped shock wave fronts in TEC perturbations are prominently seen. These fronts, with periods of 100–600 s, produced by the propulsive blasts of the rockets appear immediately and then propagate perpendicularly outward from the rocket trajectory with supersonic velocities between 800–1200 m s−1 for both events. Additionally, clear rocket exhaust depletions of TECs are seen along the trajectory and are deflected by the background thermospheric neutral wind. Twenty minutes after the rocket transits, delayed electron density perturbation waves propagating along the bow wave direction appear with phase velocities of 800–1200 m s−1. According to their propagation character, these delayed waves may be generated by rocket exhaust plumes at earlier rocket locations at lower altitudes.

Publications Copernicus