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<article xmlns:xlink="http://www.w3.org/1999/xlink">
  <front>
    <journal-meta>
      <journal-title-group>
        <journal-title>Industry, December</journal-title>
      </journal-title-group>
      <issn pub-type="ppub">1613-0073</issn>
    </journal-meta>
    <article-meta>
      <title-group>
        <article-title>of the Error in Determining the Location of Radio Emission Sources at Satellite Radio Monitoring</article-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author">
          <string-name>Aigul Kulakayeva</string-name>
          <email>aigul_k.pochta@mail.ru</email>
          <xref ref-type="aff" rid="aff1">1</xref>
          <xref ref-type="aff" rid="aff2">2</xref>
        </contrib>
        <contrib contrib-type="author">
          <string-name>Altay</string-name>
          <email>altayzf@mail.ru</email>
          <xref ref-type="aff" rid="aff1">1</xref>
        </contrib>
        <contrib contrib-type="author">
          <string-name>Aitmagambetov</string-name>
          <xref ref-type="aff" rid="aff1">1</xref>
          <xref ref-type="aff" rid="aff2">2</xref>
        </contrib>
        <contrib contrib-type="author">
          <string-name>Zhadyra</string-name>
          <xref ref-type="aff" rid="aff1">1</xref>
        </contrib>
        <contrib contrib-type="author">
          <string-name>Bagdat</string-name>
          <xref ref-type="aff" rid="aff1">1</xref>
        </contrib>
        <contrib contrib-type="author">
          <string-name>Kozhakhmetova</string-name>
          <xref ref-type="aff" rid="aff0">0</xref>
          <xref ref-type="aff" rid="aff1">1</xref>
          <xref ref-type="aff" rid="aff2">2</xref>
        </contrib>
        <contrib contrib-type="author">
          <string-name>Workshop</string-name>
          <xref ref-type="aff" rid="aff1">1</xref>
        </contrib>
        <aff id="aff0">
          <label>0</label>
          <institution>Almaty University of Power Engineering and Telecommunications named after G.Daukeev</institution>
          ,
          <addr-line>Baytursynuli St. 126/1</addr-line>
        </aff>
        <aff id="aff1">
          <label>1</label>
          <institution>Almaty</institution>
          ,
          <addr-line>050013</addr-line>
          ,
          <country country="KZ">Kazakhstan</country>
        </aff>
        <aff id="aff2">
          <label>2</label>
          <institution>International Information Technology University</institution>
          ,
          <addr-line>Manas St. 34/1, Almaty, 050040</addr-line>
          ,
          <country country="KZ">Kazakhstan</country>
        </aff>
      </contrib-group>
      <pub-date>
        <year>2023</year>
      </pub-date>
      <volume>0</volume>
      <fpage>6</fpage>
      <lpage>07</lpage>
      <abstract>
        <p>The work is devoted to the estimation of errors in determining the coordinates of the location groundbased radio emission sources at satellite radio monitoring. The proposed method of determining the coordinates of the source using angle-measuring methods based on one small spacecraft was chosen as the basis. The measured angular parameters were determined, which affect the accuracy of determining the latitude and longitude of the source. Calculations and analysis of the influence of determining the scanning angles of antennas in different planes on the errors in determining the coordinates of ground sources have been carried out. The obtained results of error calculations will allow us to determine the requirements for methods and equipment of radio monitoring to ensure a given accuracy in determining the location of ground-based radio emission sources. Radio frequency spectrum, radiomonitoring, radio-electronic means, satellite radio monitoring, source DTESI 2023: Proceedings of the 8th International Conference on Digital Technologies in Education, Science and 0000-0002-0143-085X (A. Kulakayeva); 0000-0002-7808-5273 (A. Aitmagambetov); 0000-0002-7808-5273 (Zh.</p>
      </abstract>
    </article-meta>
  </front>
  <body>
    <sec id="sec-1">
      <title>-</title>
      <p>of radio emissions, low Earth orbit satellite, geolocation</p>
    </sec>
    <sec id="sec-2">
      <title>1. Introduction</title>
      <p>
        The rapidly growing number of operating radio emission sources and radio networks is
significantly complicating the electromagnetic situation in conditions of a shortage of the radio
frequency spectrum (RFS) and requires improvement of the functions and mechanisms of the
radio monitoring system [
        <xref ref-type="bibr" rid="ref1 ref2 ref3">1-3</xref>
        ]. Currently, there are many approaches and methods to improve
the
efficiency
of
using
      </p>
      <p>RFCs
such
as:
software
defined
radio,
cognitive
radio,
dynamic/opportunistic spectrum access, spectrum sharing and licensed/unlicensed spectrum
aggregation and so on. All these approaches and methods are aimed at achieving optimal use of
the RFS and to improve the functions and mechanisms of the radio monitoring system. The
current radio</p>
      <p>
        monitoring systems are implemented on the basis of ground-based radio
monitoring facilities [
        <xref ref-type="bibr" rid="ref4 ref5 ref6">4-6</xref>
        ]. Using ground-based radio monitoring tools, providing complete,
reliable information about the real state of the RFS in a metropolitan area is a difficult task to
implement, and managing of RFS across the country is an even more difficult problem.
      </p>
      <p>
        Thus, one of the obvious ways to solve the problem of increasing the efficiency and expanding
the control area of radio monitoring systems is the creation of satellite radio monitoring systems
based on low-orbit small spacecraft (SS) [
        <xref ref-type="bibr" rid="ref7 ref8 ref9">7-9</xref>
        ]. Such systems are especially necessary for
countries with large territories in order to reduce the digital divide, promote economic growth,
social integration and meet consumer demand for new digital economy services and to solve
many scientific and technical problems. Thus, satellite technologies provide coverage of large
areas despite the difficult terrain and climatic conditions; they are reliable and generally not
      </p>
      <p>2020 Copyright for this paper by its authors.</p>
      <p>CEUR</p>
      <p>
        ceur-ws.org
subject to many of the risks that other terrestrial systems and communication networks are
exposed to, including factors such as accidental damage, theft, etc. Therefore, such systems should
be used in order to increase the efficiency of the radio monitoring system by using satellites as
radio monitoring stations [
        <xref ref-type="bibr" rid="ref10">10</xref>
        ]. Also in works [
        <xref ref-type="bibr" rid="ref11 ref12">11-12</xref>
        ], the development of mobile platform that
allows studying such a systems using augmented reality technology is considered.
      </p>
      <p>In radio monitoring, a special place is occupied by determining the location of radio emission
sources (RES), which is a complex task requiring the use of an automated complex of special
equipment with specified technical characteristics to determine the location of the studied radio
emission sources with maximum accuracy. Location estimation methods are necessary to
determine the location of radio emission sources. In radio monitoring systems, effective methods
and algorithms are needed to accurately determine the location of radio emission sources.
Currently for determine the location of RES, such methods are known based on the level of the
received signal strength (RSS - received signal strength), the phase of the carrier signal (POA
carrier phase of arrival), the time difference of arrival (TDOA), the angle of arrival (AoA) (or the
direction of arrival DOA), the frequency difference of arrival (FDOA), Doppler frequency
difference (DD) and combined methods consisting of two or more of the above methods The
classification of the most common methods for determining the location of radio sources is shown
in Figure 1.</p>
      <sec id="sec-2-1">
        <title>Methods for estimating the location of the RES</title>
      </sec>
      <sec id="sec-2-2">
        <title>Calculated</title>
      </sec>
      <sec id="sec-2-3">
        <title>Positional</title>
      </sec>
      <sec id="sec-2-4">
        <title>Amplitude</title>
      </sec>
      <sec id="sec-2-5">
        <title>Angular</title>
      </sec>
      <sec id="sec-2-6">
        <title>Rangefinder</title>
      </sec>
      <sec id="sec-2-7">
        <title>Combined</title>
      </sec>
      <sec id="sec-2-8">
        <title>Indirect (based on the information transmitted in the communication channel: IP address, service data of central stations, etc.)</title>
      </sec>
      <sec id="sec-2-9">
        <title>Difference</title>
      </sec>
      <sec id="sec-2-10">
        <title>Difference-angle (FDOA)</title>
      </sec>
      <sec id="sec-2-11">
        <title>Phase</title>
      </sec>
      <sec id="sec-2-12">
        <title>Frequency</title>
      </sec>
      <sec id="sec-2-13">
        <title>Pulse-phase</title>
      </sec>
      <sec id="sec-2-14">
        <title>Difference-rangefinder (TDOA)</title>
      </sec>
      <sec id="sec-2-15">
        <title>Amplitude</title>
      </sec>
      <sec id="sec-2-16">
        <title>Pulse</title>
      </sec>
      <sec id="sec-2-17">
        <title>Time Difference-anglerangefinder (FDOA&amp;TDOA)</title>
        <p>However, in practice, combined methods consisting of two or more of the above methods are
often used to increase reliability in determining the location of radio sources. This approach
makes it possible to eliminate the disadvantages of one method by supplementing the properties
of the other [13-16].</p>
        <p>
          Thus, to date, TDOA-FDOA and other combined methods have become the most widespread
in satellite systems. Such methods of determining the location of radio emission sources require
several low-orbit SS, which is inefficient from an economic point of view. Therefore, the method
of determining the coordinates of the source using the angle-measuring method, which is
proposed in [
          <xref ref-type="bibr" rid="ref7">7</xref>
          ], is more effective.
        </p>
        <p>The studies carried out in [17] showed that the application of the Kalman filter to the
implementation of the signal detection task turned out to be a successful solution. However, when
determining the location of radio emission sources with any degree of perfection and accuracy of
on-board radio measuring equipment, as well as regardless of the thoroughness of the
experiment, the measured value will always differ from the true one, since errors are inevitable
when measuring.</p>
        <p>When determining the location of a RES using one low-orbit SS with two active phased antenna
arrays (APAA) on board, the accuracy of estimating the coordinates of radio emission sources will
depend on a number of factors such as:
• signal level (signal-to-noise ratio) at the input of on-board measuring equipment;
• errors in determining the coordinates of the SS;
• errors in fixing phase angles between adjacent APAA elements Δφ;
• the width of the swinging sector of the APAA beams.</p>
      </sec>
    </sec>
    <sec id="sec-3">
      <title>2. Calculation of the error in determining the location of RES</title>
      <p>
        In this paper, the estimation of errors that will occur when determining the location of radio
emission sources using a single low-orbit SS is based on the angle-measuring method, with the
use of APAA-type scanning antennas on board the SS to determine the bearings on the RES. At the
same time, all coordinates of radio emission sources will be determined using the developed
algorithm, which is considered in [
        <xref ref-type="bibr" rid="ref7">7</xref>
        ], based on the angular method, where the coordinates of the
location of radio emission sources are determined based on the analysis of geometric ratios of
distances and angles between the SS, radio emission sources and the center of mass of the Earth,
bearings on the source of radio emission using iterations. Errors of scanning angles β1 and β2
were set in arbitrary form.
      </p>
      <p>In this paper, the area of radio monitoring is the territory of the Republic of Kazakhstan, which
is in the range of values from φ = 40° to φ = 56° north latitude (the average value of the radio
monitoring area is φ = 48°), as well as in the range of values from ν = 45° to ν = 87° east longitude.</p>
      <p>
        When determining the location of the RES by the algorithm and program presented in [
        <xref ref-type="bibr" rid="ref7">7</xref>
        ], the
latitude of the RES location is first determined. So, the length of latitude (parallel) 00 (equator) is
equal to 40.075,696 km. To find the length of one degree at latitude 00, it is necessary to divide
40.075,696 km by 3600, we get 40 075,696 km / 360° = 111,321377778 km/° (111321,377778
m/°). It turns out that at latitude 00 length 10 = 111,321377778 km /° or 111321,377778 m/°.
However, the length of the parallels are different - they increase as they approach the equator
and decrease towards the poles, 00 at the poles. The length of the parallel is different at different
latitudes and, accordingly, the length of 10 will also be different. To determine the length of 10, it
is necessary to multiply the length of one degree at the equator multiplied by the cosine of the
latitude angle. Taking into account the different parallel lengths at different latitudes, calculations
of the error in determining the latitude of radio emission sources were made. Table 1 shows the
results of calculating the error in determining the latitude of radio emission sources.
The dependences of the latitude error on the errors in determining the scanning angles β1 and
β2 (βmid) that arise when determining the latitude of the RES location are shown in Figure 2.
b)
Figure 2: Errors arising in determining the latitude of the RES in degrees (a), in linear dimensions
(b)
      </p>
      <p>
        After determining the latitude of the RES (φ) according to the algorithm and program
presented in [
        <xref ref-type="bibr" rid="ref7">7</xref>
        ], the longitude of the terrestrial RES ν is further determined. To do this, you need
to find the direction to the RES using the angle μ. It is also necessary to determine the sign of the
correction for longitude η, which is determined relative to the direction: the longitude of the SS
(θ) is the western direction (–), the eastern direction (+). After determining the sign of the
correction for longitude η, it is necessary to find the longitude of the terrestrial RES (ν).
      </p>
      <p>Also, when calculating, it is necessary to take into account the longitude lines, which are called
meridians. The length of the meridian is equal to 40,008.55 km. To find the length of one degree
in any meridian, it is necessary to divide 40,008.55 km by 360°, we get 40,008.55 km / 360° =
111,134861111 km/° (111134,861111 m/°). It turns out that the length of 10 = 111,134861111
km / ° or 111134,861111 m / ° and this length is the same in all meridians. Therefore, when
calculating the error in determining the longitude of radio emission sources, the length of 10 will
be the same everywhere. The calculated values of the longitude determination error are
presented in Tables 2 and 3.
The dependences of the error on the errors in determining the scanning angles that arise when
determining the longitude of the location of the RES depending on the scanning angle µ
(correction sign "+") are shown in Figures 3 and 4.
b)
Figure 4: Errors arising in determining the longitude of radio emission sources a) in degrees and
b) in linear dimensions (correction sign "+")
The dependences of the longitude error on the errors in determining the scanning angles µ
that occur when determining the longitude of the location of the RES (correction sign "-") are
shown in Figures 5 and 6.</p>
      <p>Thus, when determining the coordinates of radio emission sources, the errors will grow
linearly depending on the errors of the scanning angles β1 and β2 and on the angle µ, on which
the choice of longitude correction angle η2 or η1 depends, which are shown in Figures 7 and 8.</p>
      <p>The use of spacecraft in radio monitoring systems will make it possible to determine the
parameters of signals and the location of radio-electronic means over a large area with a diverse
terrain, which will increase the efficiency of radio monitoring systems. Therefore, taking into
account and estimating errors that occur when determining angular parameters using a single
low-orbit SS is a very important task, since the accuracy of determining the location of the RES
depends on the values of these errors. As the calculations have shown, the errors made in this
work will grow linearly depending on the errors in determining the scanning angles. Therefore,
in order to minimize these errors, it is necessary to carry out multiple measurements of the
coordinates of the ground source of radio emission, in which the bearings are determined at
several points of the orbit in the visibility zone of the low-orbit SS.</p>
    </sec>
    <sec id="sec-4">
      <title>3. Conclusion</title>
      <p>When estimating the errors that will occur when determining the location of radio emission
sources using a single low-orbit SS, it was found that the errors will grow linearly depending on
the errors of the scanning angles β1 and β2 and on the angle µ, on which the choice of longitude
correction angle η2 or η1 depends.</p>
      <p>The obtained results of error calculations will allow us to determine the requirements for
methods and equipment of radio monitoring to ensure a given accuracy in determining the
location of ground-based radio emission sources.</p>
      <p>To improve the accuracy of determining the coordinates of radio emission sources, it is
necessary to find new methods of angular measurements, or to carry out multiple measurements
of the coordinates of a ground-based radio emission source, in which the bearings are determined
at several points of the orbit in the visibility zone of a low-orbit spacecraft.</p>
      <p>In addition, in order to implement radio monitoring systems based on small spacecraft, it is
necessary to conduct a number of studies related to the evaluation and analysis of signals
received by an on-board measuring receiver, evaluation of the accuracy of various location
determination methods, selection of spacecraft designs and orbits.</p>
    </sec>
    <sec id="sec-5">
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