<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">POS</journal-id><journal-title-group><journal-title>Positioning</journal-title></journal-title-group><issn pub-type="epub">2150-850X</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/pos.2012.31002</article-id><article-id pub-id-type="publisher-id">POS-17677</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Computer Science&amp;Communications</subject></subj-group></article-categories><title-group><article-title>
 
 
  Total Electron Content and Anomalous Appearance of GPS Satellites as Pointers to Epicentre Identification of Major Japan Earthquake of 2011
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>inakshi</surname><given-names>Devi</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ananda</surname><given-names>Kumar Barbara</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Physics, Gauhati University, Guwahati, India</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>md555@sify.com(ID)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>29</day><month>02</month><year>2012</year></pub-date><volume>03</volume><issue>01</issue><fpage>7</fpage><lpage>12</lpage><history><date date-type="received"><day>December</day>	<month>13rd,</month>	<year>2011</year></date><date date-type="rev-recd"><day>January</day>	<month>10th,</month>	<year>2012</year>	</date><date date-type="accepted"><day>January</day>	<month>16th,</month>	<year>2012</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  The paper presents an analysis of variations in Total Electron Content (TEC) observed through Global Positioning System (GPS) at Guwahati (26?10'N, 91?45'E), in relation to the Japan Earthquakes (EQs) of March 9 and 11, 2011. For this purpose, the azimuthal positions and trajectories of abnormally increased number of satellites at the epicentre location appearing into the Field Of View (FOV) of GPS antenna at Guwahati and consequent pseudo enhancement in TEC are taken as inputs. The paper discusses how the analysis results could provide warning alarms of two earthquakes possibly one on March 8 or 9 and the other on March 11 or 12, 2011 with epicenter positions around 135?E to 145?E and 35?N to 40?N, that coincides with location of Japan Earthquakes. A projected forecast on EQ magnitude of M &gt; 8.5 is also made. The explanations to the observed modifications in TEC features and abnormal increase in number of satellites are purported to be the result of coupling between lithosphere and troposphere forced in by pre-earthquake processes that had spread the zone of activities to as far as Guwahati.
 
</p></abstract><kwd-group><kwd>GPS-TEC; Earthquake; Satellite Track; Radio Refractive Index</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The prediction of earthquakes (EQs) by remote sensing methods is a challenging problem, as the observable precursive imprints from an EQ even from close knit stations may vary because of complexity in the preparatory process as well as that of the very targeted entities. Amongst many approaches adapted for this purpose, the use of Electromagnetic (EM) signals as tool of identification of EQ precursor has proved to be popular because of their realm of frequency range from VLF to VHF [1-4]. The fact that such signals carry characteristics of the atmosphere, the transporting media, the parameters like temperature, pressure of lower atmosphere (troposphere) and ionisation density as well as Total Electron Content (TEC) relevant to upper atmosphere (ionosphere), are used as instruments for identification of impending earthquake signatures [5-15].</p><p>In this paper TEC data of Gauhati (26˚10'N, 91˚45'E) along with associated factors will be utilized with aims to focusing on their capability of providing warning of Japan earthquakes of March 2011.</p></sec><sec id="s2"><title>2. Observations</title><p>In our earlier efforts to look for seismic effects on lowlatitude atmosphere, TEC variations obtained from dual frequency GPS observations at Gauhati University were taken as the prime parameters [5,10]. Here, we utilize TEC data along with the incidence of sudden increase in number of satellites appearing in Field Of View (FOV) of the GPS antenna at Guwahati [<xref ref-type="bibr" rid="scirp.17677-ref16">16</xref>] as inputs, for forecasting the major Japan Earthquakes of March 9 and 11, 2011 with magnitudes of 7.3 and 9 respectively, occurring at the same location of 38.322˚N, 142.369˚E.</p><sec id="s2_1"><title>2.1. TEC<sub>noon</sub> Peak Variation and EQ Induced Features</title><p>We had shown that [5,10,11] TEC<sub>noon</sub> time peak (TEC<sub>noon</sub> peak) may provide EQ precursors when non seismic factors are removed from the data. For this purpose at least five quiet days (Q-days i.e., when geomagnetic influences are low) were selected near an EQ event and the maximum possible normal statistical flucutauions on the TEC<sub>noon</sub> peaks in these days were set through their Standard deviation (Sd) limits. The EQ induced features were then extracted by comparing the TEC<sub>noon</sub> peaks of relevant days with respect to the Q-day Sd limit [10,11]. This analysis shows some precursive features characterised by: 1) There is a rising trend on the magnitude of TEC<sub>noon</sub> peak a few days prior to an EQ exceeding the maximum excursion of Sd limit and 2) On attainment of this maximum, the TEC<sub>noon</sub> peak decreases and 3) On days near or at the trough of this decline, an earthquake is expected. The patterns 1) and 2) are considered as preludes to an earthquake when:</p><p>(1) The epicenter lies within &#177;5˚ about the observing station Guwahati, and magnitude of EQs, M ≥ 5.</p><p>(2) The epicenter lies beyond &#177;5˚ [unlike the (1) above] but the event occurs within the earthquake preparatory region.</p><p>Adapting this basic approach, we chart Q-day TEC <sub>noon </sub>peaks and the Sd limits on a routine basis. In <xref ref-type="fig" rid="fig1">Figure 1</xref>, the variations of this parameter around the Japan EQ events along with Q-day Sd margins are plotted. Here, both the vertical and oblique components of TEC<sub> noon</sub> peak have been taken into account [<xref ref-type="bibr" rid="scirp.17677-ref16">16</xref>]. The figure shows that in some days the TEC<sub>noon</sub> peaks exceed the maximum Sd limit followed by a tendency to decrease, conforming the pre-EQ preludes defined above. Thus taking theses prelude [1) and 2)], one can expect that two events of EQs might occur one on March 8-9 and the other on March 11 - 12, 2011. In the <xref ref-type="fig" rid="fig1">Figure 1</xref>, we marked these predicted EQ events by blue arrow heads and the red arrows mark the observed events. This technique suggests the probable day of an EQ only, but not the epicentre information. It is therefore necessary that along with these criteria a few more parameters should be taken for identification of the epicentre, as was done by Devi et al. [<xref ref-type="bibr" rid="scirp.17677-ref16">16</xref>], in case of the major China EQ of May 2008. The details are presented in the next section.</p></sec><sec id="s2_2"><title>2.2. Azimuth of Satellites Coming Within the Field of View of the GPS Receiver</title><p>In case of Sichean (China) EQ of 2008, Devi et al. [<xref ref-type="bibr" rid="scirp.17677-ref16">16</xref>] could identify the location of the epicentre through analysis of anomalous increase in appearance of GPS satellites at a particular zone. On the basis of this observation, we, as routine exercise, record the number of satellites coming in the FOV of our GPS antenna from different azimuth positions. The analysis showed that, in early part of March 2011 i.e. within the approaching days of Japan EQ., a large number of satellites made their appearance at azimuths not normally seen. In <xref ref-type="fig" rid="fig2">Figure 2</xref> the TEC values (&gt;40 U) recorded by the satellites from such azimuths are presented from March 6 to beyond the event of March 11, 2011. The anomalous appearance of satellites from azimuth positions (&gt;320), was detected on March 7 (2 days before the EQ of March 9) registering high TEC, similar to the observation in TEC<sub>noon</sub> peak of <xref ref-type="fig" rid="fig1">Figure 1</xref>. The satellite pass number decreased on March 8 and it reached almost normalcy on March 9 i.e., as of March 6. Interestingly, on March 10, large number of satellite passes again appeared from azimuth &gt;320 but it started declining from March 11. The TEC also registered correspondingly higher or lower values following the anomalous appearance pattern of satellite passes, as expected.</p><sec id="s2_2_1"><title>Epicentre Position and Magnitude</title><p>With azimuth parameter as input, we calculated the position of satellites with respect to the observing station Guwahati. The result showed that on March 7 and 10, the FOV of the receiving antenna had increased significantly and satellites as far as from 35˚N to 40˚N and 135˚E to 145˚E were visible at Guwahati. This phenomenon being associated and identified with the epicentre of an impending EQ [<xref ref-type="bibr" rid="scirp.17677-ref16">16</xref>], we recorded warnings of two EQs of March 8 or 9 and on March 11 or 12 with probable epicenter at 35˚N to 40˚N and 135˚E to 145˚E. Next, to assess the magnitude (M) of these EQs, we estimated the limit of pre-seismic activity zone centered about the epicentre of an impending earthquake at a radius R = exp M (km), where M is the magnitude of earthquake [17,18]. Taking distance between the probable epicentre at 35˚N to 40˚N &amp; 135˚E to 145˚E and Guwahati as preseismic activity radius R, we predicted that the magnitude of the Japan EQ needs to be &gt;8.5.</p><p>It was seen that both the Japan EQs occurred within our estimated epicenter location and also predicted M corresponded to the observed magnitude of the March 11 EQ. But appearance of anomalous features prior to the EQ of March 9 with M = 7.3 is difficult to explain within the above theoretical ambit. In view of this fact, we suggested that this EQ was a precursor to the stronger one of March 11. Though perhaps speculative, this explanation has come from our routine analysis, that no other case of EQ with magnitude M ~ 7.0 and similar relative distance between Guwahati and epicentre location, had shown satellite pass variations as in <xref ref-type="fig" rid="fig2">Figure 2</xref>. Reappearance of this anomaly on March 10, both in terms of TEC<sub>noon </sub>peak and more significantly on satellite azimuth track records had suggested that a strong EQ of M ≥8.5 was on the anvil. The event of March 11 with M = 8.9 thus supported our projected prediction.</p></sec></sec></sec><sec id="s3"><title>3. Discussions and Conclusion</title><p>Increase in FOV of VHF signals, leading to anomalous increase in propagation path prior to and during an EQ is reported by many earlier workers by considering pre EQ modifications both at the lower and upper atmosphere. Such propagation of signal in the frequency range 50 MHz to 70 MHz were noted by Devi and Barbara as early as in 1984 [<xref ref-type="bibr" rid="scirp.17677-ref19">19</xref>] ,while they were conducting an experiment at Guwahati in search of beyond the horizon VHF TV signal propagation. Their primary interest at that time was to understand atmospheric situation favorable for anomalous VHF reception, which they associated latter with EQ preparatory modification in lower and upper atmosphere [<xref ref-type="bibr" rid="scirp.17677-ref20">20</xref>]. Kushida and Kushida [21,22], detected beyond Line Of Sight (LOS) signals from a transmitter in central Japan several days before the Kobe EQ of 17 January, 1995 (Magnitude M = 7.2) and they proposed this anomalous propagation of VHF (FM) signals to be due to ionospheric irregularities. Fukumoto et al. [23,24] also detected an abnormal enhancement in the over-horizon 77.1 MHz FM signal strength (with small incident angle &lt;20˚), from one week to the day of the EQ event and they associated this observation with modification in the troposphere, by EQ induced effects. Hayakawa et al. [<xref ref-type="bibr" rid="scirp.17677-ref25">25</xref>] have also shown presence of seismoatmospheric perturbations in association with VHF anomalous propagation.</p><p>The modifications seen in lower atmospheric variables like temperature, pressure, humidity, can be linked to parameters defined as the Radio Refractive Index (RRI). Further, such changes in atmospheric parameters are coupled to EQ time variations in Sea Surface Temperature (SST), Surface Latent Heat Flux (SLHF), prior to an EQ [26,27].</p><p>These associations suggest the existence of interaction between lithosphere and the near earth environment. In this connection, we may refer to the reports of variations seen in ocean energy balance after the strong Gujrat EQ of January 26, 2001 [<xref ref-type="bibr" rid="scirp.17677-ref28">28</xref>] and changes in ocean, land, meteorological parameters after Sumatra earthquake of 26 December 2004 [<xref ref-type="bibr" rid="scirp.17677-ref29">29</xref>]. The detection of SLHF anomaly two weeks before the EQs of 14 August 2003 and 1 March 2004 in Greece [<xref ref-type="bibr" rid="scirp.17677-ref30">30</xref>] may also be referred to. Further, presence of interactive processes between the surface variabilities and near atmosphere environment with special reference to an impending EQ was also detected by Devi et al. [<xref ref-type="bibr" rid="scirp.17677-ref20">20</xref>] from SODAR (Sonic Detection and Ranging).</p><p>Thus, a change in RRI prior to an EQ is expected, as it is a function of temperature, pressure and humidity and is often expressed in terms of its gradient i.e. dN/dh given by relation (1):</p><disp-formula id="scirp.17677-formula65896"><label>(1)</label><graphic position="anchor" xlink:href="2-8501031\b32a7ee1-b7d8-4041-98eb-15cc3ab4b9d9.jpg"  xlink:type="simple"/></disp-formula><p>In the Equation (1), T is the temperature, P the pressure and e the relative humidity. Any change in this gradient, will modify the ray path geometry [31,32]. Thus, there will be situations in the atmosphere favourable for generation of ‘atmospheric duct’, when a ray may be trapped and may progress in a waveguide mode, far extending the normal propagation limit, when the refractive index decreases with height much more rapidly than the normal lapse rate. As the ray trajectory changes with refractive index gradient, its relation with effective Earth’s radius does also change and therefore, the ray path gets modified accordingly [14,16,20].</p><p>The appearance of satellites beyond the normally visible horizon prior to the Japan EQ, suggests that the increase in FOV has occurred due to modification in RRI, which in its turn has changed the earth’s curvature with respect to the ray path radius. The increased number of visible satellites will cause significant pseudo enhancements in TEC as noted on March 7 and 10, prior to the EQs. This enhancement in TEC on March 7 is also interesting as the magnitude of EQ on March 9, did not attain the required magnitude of 8.5 to show its effect on the TEC, at Guwahati. Such modification especially in satellite track position however suggested that a stronger EQ was yet to occur in this location. We could further substantiate this point through anomalous features seen on March 10 and subsequent occurrence of the major EQ of March 11.</p><p>It is also important here to mention that a magnetic storm that occurred on March 10-11 might modulate the TEC on these days. Thus, to examine storm effect on the pseudo enhancement in noon time TEC, this parameter is</p><p>displayed in <xref ref-type="fig" rid="fig3">Figure 3</xref> along with Dst values i.e., the “disturbance amplitude, storm time” of the month. The figure suggests that changes in TEC are associated with factors other than magnetic storm and significantly, it shows the presence of pre EQ effect on TEC on March 7 and 10. The slow decrease of TEC after the strong EQ of March 11 is perhaps associated with seven strong seismic events on the same day with one aftershock that trailed to March 12, as shown in <xref ref-type="fig" rid="fig4">Figure 4</xref>. Further, the modification in satellite azimuth status suggests that the effect is more associated with lithospheric-atmospheric coupling processes, rather than magnetic storm induced changes in the ionisation density at the ionosphere [16,33]. However, further work is necessary to isolate storm induced effect on TEC from the EQ.</p></sec><sec id="s4"><title>REFERENCES</title></sec><sec id="s5"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.17677-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">M. B. Gokhberg, V. A. Morgounov, T. Yoshino and I. Tomi- zawa, “Determination of the Characteristics of Ionospheric Disturbance in the near Zone of the Earthquake Epicenter,” Journal of Geophysical Research, Vol. 87, No. B9, 1982, pp. 7824-7828. doi:10.1029/JB087iB09p07824</mixed-citation></ref><ref id="scirp.17677-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">M. Parrot and M. M. 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