Abstract
We study the impact of ionospheric disturbances on the Earth’s environment caused by the solar events that occurred from 20 April to 31 May 2010, using observations from the Mexican Array Radio Telescope (MEXART). During this period of time, several astronomical sources presented fluctuations in their radio signals. Wavelet analysis, together with complementary information such as the vertical total electron content (vTEC) and the Dst index, were used to identify and understand when the interplanetary scintillation (IPS) could be contaminated by ionospheric disturbances (IOND). We find that radio signal perturbations were sometimes associated with IOND and/or IPS fluctuations; however, in some cases, it was not possible to clearly identify their origin. Our Fourier and wavelet analyses showed that these fluctuations had frequencies in the range ≈ 0.01 Hz – ≈ 1.0 Hz (periodicities of 100 s to 1 s).
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Notes
Usually the vTEC is measured in TEC units (TECu), where 1 TECu=1016 m−2.
See the Large Angle and Spectroscopic (LASCO) CME catalog at http://cdaw.gsfc.nasa.gov/CME_list/ .
References
Araujo-Pradere, E.A.: 2005, GPS-derived total electron content response for the Bastille Day magnetic storm of 2000 at a low mid-latitude station. Geofís. Int. 44, 211.
Araujo-Pradere, E.A., Fuller-Rowell, T.J., Spencer, P.S.J.: 2006, Consistent features of TEC changes during ionospheric storms. J. Atmos. Solar-Terr. Phys. 68, 1834.
Carrillo-Vargas, A.: 2007, Construcción y calibración del radiotelescopio de centelleo interplanetario MEXART, Ph.D. Thesis, Univ. Nacional Autónoma de México.
Carrillo-Vargas, A., Pérez-Enríquez, H.R., Rodríguez-Martínez, M., López-Montes, R., Casillas-Pérez, G.A., Araujo-Pradere, E.A.: 2012, Ionospheric disturbances detected by MEXART. Adv. Space Res. 49, 11.
Cohen, A.S., Röttgering, H.J.A.: 2009, Probing fine-scale ionospheric structure with the Very Large Array Radio Telescope. Astron. J. 138, 439.
Erickson, W.C., Perley, R.A., Flatters, C., Kassim, N.E.: 2001, Ionospheric corrections for VLA observations using local GPS data. Astron. Astrophys. 366, 1071.
Gapper, G.R., Hewish, A., Purvis, A., Duffett-Smith, P.J.: 1982, Observing interplanetary disturbances from the ground. Nature 296, 633.
González-Esparza, J.A., Carrillo, A., Andrade, E., Pérez-Enríquez, R., Kurtz, S.: 2004, The MEXART interplanetary scintillation array in Mexico. Geofís. Int. 43, 61.
González-Esparza, J.A., Carrillo, A., Andrade, E., Sierra, P., Vazquez, S., Rodríguez, C., Pérez-Enríquez, R., Kurtz, S., Blanco-Cano, X.: 2006, Calibration and testing of the MEXART antenna using solar transits. Adv. Space Res. 38, 1824.
Hewish, A., Bravo, S.: 1986, The sources of large-scale heliospheric disturbances. Solar Phys. 106, 185.
Hewish, A., Duffet-Smith, P.J.: 1987, A new method of forecasting geomagnetic activity and proton showers. Planet. Space Sci. 35, 487.
Hewish, A., Scott, P.F., Wills, D.: 1964, Interplanetary scintillation of small diameter radio sources. Nature 203, 1214.
Jackson, B.V., Hick, P.L., Kojima, M., Yokobe, A.: 1998, Heliospheric tomography using interplanetary scintillation observations 1. Combined Nagoya and Cambridge data. J. Geophys. Res. 103, 12049.
Komjathy, A.: 1997, Global ionospheric total electron content mapping using the Global Positioning System, Technical Report No. 188, New Brunswick. Ph.D. Thesis, Univ. of New, Brunswick.
Langley, R.B.: 1996, Propagation of the GPS Signals, Lect. Notes Earth Sci. 103, 60.
López-Montes, R., Pérez-Enríquez, R., Araujo-Pradere, E.A.: 2012, The impact of large solar events on the total electron content of the ionosphere at mid latitudes. Adv. Space Res. 49(7), 1167.
Lucek, E.A., Clark, T.D.G., Moore, V.: 1996, The use of various interplanetary scintillation indices within geomagnetic forecasts. Ann. Geophys. 14, 139.
Manoharan, P.K.: 2010, Evolution of near-Sun solar wind turbulence. In: Hasann, S.S., Rutten, R.J. (eds.) Magnetic Coupling Between the Interior and Atmosphere of the Sun, Astrophys. Space Sci. Proc. XII, Springer, Dordrecht, 324.
Manoharan, P.K., Ananthakrishnan, S.: 1990, Determination of solar-wind velocities using single-station measurements of interplanetary scintillation. Mon. Not. Roy. Astron. Soc. 244, 691.
Manoharan, P.K., Kojima, M., Misawa, H.: 1994, J. Geophys. Res. 99, 23411.
Mejia-Ambriz, J.C., Villanueva-Hernandez, P., Gonzalez-Esparza, J.A., Aguilar-Rodriguez, E., Jeyakumar, S.: 2010, Observations of Interplanetary Scintillation (IPS) using the Mexican Array Radio Telescope (MEXART). Solar Phys. 265, 309.
Milne, R.G.: 1976, Interplanetary scintillation power spectra. Aust. J. Phys. 29, 201.
Pérez-Enríquez, R., Carrillo, A., Kotsarenko, A., Cruz-Abeyro, J.A.L.: 2008, State of the inner heliosphere as given by the G index of interplanetary scintillation and the Dst index of geomagnetic activity. J. Geophys. Res. 113, 10107.
Pérez-Enríquez, R., Carrillo, A., Rodríguez, C.: 2006, Fractal character of G-index of IPS data for the period 1991–1994 obtained from multiscale wavelet analysis. Adv. Space Res. 38, 1819.
Purvis, A., Tappin, S.J., Rees, W.G., Hewish, A., Duffett-Smith, P.J.: 1987, The Cambridge IPS survey at 81.5 MHz. Mon. Not. Roy. Astron. Soc. 229, 589.
Shishov, V.I., Tyul’Bashev, S.A., Chashei, I.V., Subaev, I.A., Lapaev, K.A.: 2010, Interplanetary and ionosphere scintillation monitoring of radio sources ensemble at the solar activity minimum. Solar Phys. 265, 277.
Tappin, S.J., Hewish, A., Gapper, G.R.: 1984, Tracking a high-latitude corotating stream for more than half a solar rotation. Planet. Space Sci. 32, 1273.
Tsurutani, B.T., Verkhoglyadova, O.P., Mannucci, A.J., Lakhina, G.S., Li, G., Zank, G.P.: 2009, A brief review of “solar flare effects” on the ionosphere. Radio Sci. 44, RS0A17.
Woan, G.: 1995, Observations of long-lived solar wind streams during 1990 – 1993. Ann. Geophys. 13, 227.
Acknowledgements
The authors thank the MEXART team, in particular: A. González-Esparza (P. I. of MEXART), P. Villanueva, E. Andrade, and E. Aguilar, for technical support and provision of data. We also thank CORS, SOPAC, and UNAVCO for incorporating the data on their respective websites from which the GPS data can be freely downloaded. We are also grateful to NOAA-SWPC for access to the TEC calculation program. We also wish to thank the Servicio Sismológico Nacional and E. Cabral for providing some Mexican GPS data. This article was possible thanks to the PAPIIT-UNAM projects IN111509 and IA102514-2. M. Rodríguez-Martínez thanks REDCyTE and CONACyT for a postdoctoral fellowship supported by the project Estudio de la ionosfera y sus aplicaciones for the Mexican Space Agency (MSA). The authors finally thank the suggestions of M. Sánchez and S. Kurtz, which have improved this article.
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Rodríguez-Martínez, M., Pérez-Enríquez, H.R., Carrillo-Vargas, A. et al. Ionospheric Disturbances and Their Impact on IPS Using MEXART Observations. Sol Phys 289, 2677–2695 (2014). https://doi.org/10.1007/s11207-014-0496-8
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DOI: https://doi.org/10.1007/s11207-014-0496-8