IONOSPHERIC EFFECTS OF GEOSPACE STORM OF NOVEMBER 13–14, 2012

DOI: https://doi.org/10.15407/rpra19.02.170

I. F. Domnin, L. Ya. Emelyanov, S. V. Katsko, L. F. Chernogor

Abstract


The results of studying the F region and topside ionosphere response to the strong magnetic storm of November 13–14, 2012 (Kp max=6+) are presented. The observations are carried out by the Kharkiv incoherent scatter radar. The magnetic storm was accompanied by the ionospheric storm with sign-variable phases. This storm was featured by the presence of two positive and one negative phases of disturbance.

Key words: geospace storm, ionosphere storm phases, ionosphere, incoherent scattering

Manuscript submitted: 14.02.2014

Radio phys. radio astron.  2014, 19(2): 170-180

REFERENCES

 

1. CHERNOGOR, L. F. and DOMNIN, I. F., 2014. Physics of geocosmic storms. Kharkiv: V. N. Karazin Kharkiv National University Publ. (in Russian).

2. CHERNOGOR, L. F., GRIGORENKO, Ye. I., LYSENKO, V. N., and TARAN, V. I., 2007. Dynamic processes in the ionosphere during magnetic storms from the Kharkov in coherent scatter radar observations. Int. J. Geomagn. Aeron. vol. 7, no. 3, id. GI3001.

3. BUONSANTO, M. J., 1999. Ionospheric Storms: A Review. Space Sci. Rev. vol. 88, no. 3–4, pp. 563–601. doi:https://doi.org/10.1023/A:1005107532631

4. MIKHAILOV, A. V. and FOSTER, J. C., 1997. Daytime thermosphere above Millstone Hill during severe geomagnetic storms. J. Geophys. Res: Space Phys. vol. 102, is. A8, pp. 17275–17282.

5. DANILOV, A. D., 2001. F2 region response to geomagnetic disturbances. J. Atmos. Solar-Terr. Phys. vol. 63,Is. 5, pp. 441–449.

6. DOMNIN, I. F., EMELYANOV, L. Ya., KATSKO, S. V., LYASHENKO, M. V., and CHERNOGOR, L. F., 2013. Ionospheric effects of a magnetic storm November 13-15, 2012 In: Proc. 13-th Ukrainian Conf. On space research. Evpatoria, Ukraine. p. 52 (in Russian).

7. KATSKO, S. V., 2013. Geocosmic storm on November 14, 2012: the results of observations on the Kharkov non-coherent scattering radar. In: Sb. Tez. Doc. Conf. ION-2013 "Remote radio sounding of the ionosphere". Small Lighthouse, Crimea, Ukraine. p. 46 (in Russian).

8. CHERNOGOR, L. F., 2003. Physics of Earth, Atmosphere, and Geospace from the Standpoint of System Paradigm. Radio Phys. Radio Astron. vol. 8, no. 1, pp. 59–106 (in Russian).

9. CHERNOGOR, L. F., 2006. Earth–atmosphere–ionosphere–magnetosphere as an open dynamic nonlinear physical system (Part 1). Nelinejnyj mir. vol. 4, no. 12, pp. 655–697 (in Russian).

10. BARKHATOV, N. A. and BARKHATOVA, O. M., 2012. The identification of classes of ionospheric disturbances from long-term data on the critical frequency of the F2 layer. Geomagnetism and Aeronomy. vol. 52, no. 4, pp. 510–518 (in Russian).

11. MIKHAILOV, A. V., SKOBLIN, M. G., and FORSTER, M., 1995. Daytime F2-layer positive storm effect at middle and lower latitudes. Ann. Geophys. vol. 13, no. 5, pp. 532–540. DOI: https://doi.org/10.1007/s00585-995-0532-y

12. DANILOV, A. D. and MOROZOVA, L. D., 1985. Ionospheric storms in the F2 region. Morphology and physics (review). Geomagnetism and aeronomy. vol. 25, no. 5, pp. 705–721 (in Russian).

13. KRINBERG, I. A. and TASHCHILIN , A. V., 1984. Ionosphere and Plasmasphere. Moscow: Nauka Publ. (in Russian).

14. DANILOV, A. D., MOROZOVA, L. D., AND MIRMOVICH, E. G., 1985. On the possible nature of the positive phase of ionospheric storms. Geomagnetism and Aeronomy. vol. 25, no. 5, pp. 768–772 (in Russian).

15. CHERNOGOR, L. F., 2007. Earth–atmosphere–ionosphere–magnetosphere as an open dynamic nonlinear physicalsystem (Part 2). Nelinejnyj mir. vol. 5, no. 4, pp. 225-246 (in Russian).

16. CHERNOGOR, L. F., 2011. The Earth – atmosphere – geospace system: main properties and processes. Int. J. Remote Sens. vol. 32, no. 11, pp. 3199–3218. DOI: https://doi.org/10.1080/01431161.2010.541510

 


Keywords


geospace storm; ionosphere storm phases; ionosphere; incoherent scattering

Full Text:

PDF


Creative Commons License
Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)