Vol. 68
Latest Volume
All Volumes
PIERM 130 [2024] PIERM 129 [2024] PIERM 128 [2024] PIERM 127 [2024] PIERM 126 [2024] PIERM 125 [2024] PIERM 124 [2024] PIERM 123 [2024] PIERM 122 [2023] PIERM 121 [2023] PIERM 120 [2023] PIERM 119 [2023] PIERM 118 [2023] PIERM 117 [2023] PIERM 116 [2023] PIERM 115 [2023] PIERM 114 [2022] PIERM 113 [2022] PIERM 112 [2022] PIERM 111 [2022] PIERM 110 [2022] PIERM 109 [2022] PIERM 108 [2022] PIERM 107 [2022] PIERM 106 [2021] PIERM 105 [2021] PIERM 104 [2021] PIERM 103 [2021] PIERM 102 [2021] PIERM 101 [2021] PIERM 100 [2021] PIERM 99 [2021] PIERM 98 [2020] PIERM 97 [2020] PIERM 96 [2020] PIERM 95 [2020] PIERM 94 [2020] PIERM 93 [2020] PIERM 92 [2020] PIERM 91 [2020] PIERM 90 [2020] PIERM 89 [2020] PIERM 88 [2020] PIERM 87 [2019] PIERM 86 [2019] PIERM 85 [2019] PIERM 84 [2019] PIERM 83 [2019] PIERM 82 [2019] PIERM 81 [2019] PIERM 80 [2019] PIERM 79 [2019] PIERM 78 [2019] PIERM 77 [2019] PIERM 76 [2018] PIERM 75 [2018] PIERM 74 [2018] PIERM 73 [2018] PIERM 72 [2018] PIERM 71 [2018] PIERM 70 [2018] PIERM 69 [2018] PIERM 68 [2018] PIERM 67 [2018] PIERM 66 [2018] PIERM 65 [2018] PIERM 64 [2018] PIERM 63 [2018] PIERM 62 [2017] PIERM 61 [2017] PIERM 60 [2017] PIERM 59 [2017] PIERM 58 [2017] PIERM 57 [2017] PIERM 56 [2017] PIERM 55 [2017] PIERM 54 [2017] PIERM 53 [2017] PIERM 52 [2016] PIERM 51 [2016] PIERM 50 [2016] PIERM 49 [2016] PIERM 48 [2016] PIERM 47 [2016] PIERM 46 [2016] PIERM 45 [2016] PIERM 44 [2015] PIERM 43 [2015] PIERM 42 [2015] PIERM 41 [2015] PIERM 40 [2014] PIERM 39 [2014] PIERM 38 [2014] PIERM 37 [2014] PIERM 36 [2014] PIERM 35 [2014] PIERM 34 [2014] PIERM 33 [2013] PIERM 32 [2013] PIERM 31 [2013] PIERM 30 [2013] PIERM 29 [2013] PIERM 28 [2013] PIERM 27 [2012] PIERM 26 [2012] PIERM 25 [2012] PIERM 24 [2012] PIERM 23 [2012] PIERM 22 [2012] PIERM 21 [2011] PIERM 20 [2011] PIERM 19 [2011] PIERM 18 [2011] PIERM 17 [2011] PIERM 16 [2011] PIERM 14 [2010] PIERM 13 [2010] PIERM 12 [2010] PIERM 11 [2010] PIERM 10 [2009] PIERM 9 [2009] PIERM 8 [2009] PIERM 7 [2009] PIERM 6 [2009] PIERM 5 [2008] PIERM 4 [2008] PIERM 3 [2008] PIERM 2 [2008] PIERM 1 [2008]
2018-04-28
VLF Monitoring System for Characterizing the Lower Region Ionospheric Layer
By
Progress In Electromagnetics Research M, Vol. 68, 31-39, 2018
Abstract
The main objective of the current work is to develop a Very Low Frequency (VLF) monitoring system for characterizing low layer ionosphere. Low layer ionosphere is important for communication, and some researchers stressed that lower layer ionosphere can be a precursor to earthquake event. The VLF monitoring system composed of a 1-m antenna, a preamplifier to amplify the signal, an ADC converter and a data acquisition system. The optimization of 1-m antenna received dual frequencies 19.2 kHz and 19.8 kHz from South Vijayanarayanam, India and North West Cape, Australia, respectively. Subsequently, a low pass filter was designed in the preamplifier to pass VLF signals from 0-30 kHz. The results revealed that the system was able to characterize diurnal variation: sunrise and sunset and detect changes in the lower layer ionosphere region due to Solar activity.
Citation
Nur Ain Zakaria, Afifah Taat, Siti Amalina Enche Abdul Rahim, Wan Zul Adli Wan Mokhtar, and Mohamad Huzaimy Bin Jusoh, "VLF Monitoring System for Characterizing the Lower Region Ionospheric Layer," Progress In Electromagnetics Research M, Vol. 68, 31-39, 2018.
doi:10.2528/PIERM17112802
References

1. Indira Devi, M., I. Khan, and D. N. Madhusudhana Rao, "A study of VLF wave propagation characteristics in the earth-ionosphere waveguide," Earth Planet and Space, Vol. 60, 737-741, Jul. 2008.
doi:10.1186/BF03352822

2. Contreira, D. B., F. S. Rodrigues, K. Makita, et al. "An experiment to study solar flare effects on radio-communication signals," Advances in Space Research, Vol. 36, 2455-2459, Mar. 2004.
doi:10.1016/j.asr.2004.03.019

3. Abd Rashid, M. M., M. Ismail, A. M. Hasbie, and R. Nordin, "Ionospheric disturbances triggered by solar flare events during solar maximum - May 2013," 2015 IEEE 12th Malaysia International Conference on Communications (MICC), Malaysia, 2015.

4. Kumar, A. and S. Kumar, "Space weather effects on the low latitude D-region ionosphere during solar minimum," Earth, Planets and Space, 66-76, 2014.

5. "The Earth's Ionosphere,", [Online], Available: http://solar-center.stanford.edu/SID/acti-vities/ionosphere.html, Accessed: Nov. 28, 2017.

6. Cohen, M. B., U. S. Inan, and E. W. Paschal, "Sensitive broadband ELF/VLF radio reception with the AWESOME instrument," IEEE Transaction on Geoscience and Remote Sensing, 1-15, 2009.

7. Harriman, S. K., W. Paschal, and U. S. Inan, "Magnetic sensor design for femtotesla low-frequency signals," IEEE Transaction on Geoscience and Remote Sensing, Vol. 48, 396-402, 2010.
doi:10.1109/TGRS.2009.2027694

8. Tan, L. M., "Development of TNU-SuperSID teaching module for observing the effects of solar activities on the lower ionosphere," Journal of Physical Science and Application, Vol. 5, 116-122, 2015.

9. Holt, C. A., "Basic amplifier configuration," Electronic Circuits Digital and Analog, 383-389, John Wiley & Sons, Canada, 1978.

10. Samanes, J. E., J. P. Raulin, and E. L. Macotela, "Estimating the VLF modal interference distance using The South America VLF network (SAVNET)," Radio Science, Vol. 50, 122-129, Feb. 2015.
doi:10.1002/2014RS005582

11. Muraoka, Y., "A new approach to mode conversion effects observed in a mid-latitude VLF transmission," Journal of Atmospheric and Terrestrial Physics, Vol. 44, 855-862, Oct. 1982.
doi:10.1016/0021-9169(82)90038-1