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        <formatdesc>Electric field hence the velocity function for the Bremsstrahlung Radiation Pattern</formatdesc>
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        <name>
          <family>Yucemoz</family>
          <given>Mert</given>
        </name>
        <id>M.Yucemoz@bath.ac.uk</id>
        <orcid>0000-0002-0829-0749</orcid>
        <affiliation>University of Bath</affiliation>
        <contact>TRUE</contact>
      </item>
    </creators>
    <contributors>
      <item>
        <type>Supervisor</type>
        <name>
          <family>Fullekrug</family>
          <given>Martin</given>
        </name>
        <id>M.Fullekrug@bath.ac.uk</id>
        <orcid>0000-0003-4588-3591</orcid>
        <affiliation>University of Bath</affiliation>
      </item>
      <item>
        <type>Other</type>
        <name>
          <family>Hill</family>
          <given>Adrian</given>
        </name>
        <id>A.T.Hill@bath.ac.uk</id>
        <affiliation>University of Bath</affiliation>
      </item>
    </contributors>
    <title>Dataset for &quot;Asymmetric Backward Peaking Radiation Pattern from a Relativistic Particle Accelerated by Lightning Leader Tip Electric Field&quot;</title>
    <subjects>
      <item>BP0010</item>
      <item>BP0060</item>
      <item>BP0090</item>
      <item>BS0010</item>
      <item>GJ0060</item>
      <item>KC0010</item>
      <item>KF0020</item>
    </subjects>
    <divisions>
      <item>dept_elec_eng</item>
    </divisions>
    <keywords>Mathematical code, Particle Acceleration, Bremsstrahlung, Atmospheric Electrodynamics, Radiation Patterns of a Charged Relativistic particle, Theoretical Physics, Theoretical Modelling, Mathematical Physics</keywords>
    <note>The mathematical Maple code is just the mathematical code version of the actual, original theory created from scratch on paper. Maple code is just used to simulate the constructed theory. In order to run the code, start from the very beginning of the code where it says `restart;`. In addition, `restart;` is just there to clear the memory of the Maple software every time when simulating new results with new parameters or with different equations. This enables Maple to get rid of any unrequired numbers, definitions or assumptions that could cause confusions in the results of the new simulation.</note>
    <abstract>The purpose of the data is to mathematically model radiation intensity and patterns around a single charged relativistic/non-relativistic particle (electron) specifically for the bremsstrahlung process where the particle is assumed to be rotating in anti-clockwise direction. The dataset consists of four separate Maple worksheets. The first one models the bremsstrahlung particle trajectory. The second one models particle velocity from the leader tip electric field that accelerates particles to relativistic speeds. The third and fourth are worksheets that model the radiation patterns of the bremsstrahlung process around a charged relativistic/non-relativistic particle and it incorporates all the information used in first and second Maple worksheets about particle trajectory and the leader tip electric field, and hence the particle velocity arising from the electric field.</abstract>
    <date>2021-05-19</date>
    <publisher>University of Bath</publisher>
    <full_text_status>public</full_text_status>
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        <funder_name>Engineering and Physical Sciences Research Council</funder_name>
        <funder_id>https://doi.org/10.13039/501100000266</funder_id>
        <grant_id>2095240</grant_id>
        <project_name>Studentship - Electromagnetic Emissions from Energetic Charged Particles Generated by Lightning Discharges</project_name>
      </item>
      <item>
        <funder_name>Met Office</funder_name>
        <funder_id>https://doi.org/10.13039/501100000847</funder_id>
        <grant_id>EG-EE1077</grant_id>
        <project_name>PhD Studentship: &quot;Electromagnetic Emissions from Energetic Charged Particles Generated by Lightning Discharges&quot;</project_name>
      </item>
      <item>
        <funder_name>Natural Environment Research Council</funder_name>
        <funder_id>https://doi.org/10.13039/501100000270</funder_id>
        <grant_id>NE/L012669/1</grant_id>
        <project_name>Radio Tomography for Atmospheric Science</project_name>
      </item>
      <item>
        <funder_name>Natural Environment Research Council</funder_name>
        <funder_id>https://doi.org/10.13039/501100000270</funder_id>
        <grant_id>NE/H024921/1</grant_id>
        <project_name>Relativistic Electron Beams Above Thunderclouds</project_name>
      </item>
      <item>
        <funder_name>Engineering and Physical Sciences Research Council</funder_name>
        <funder_id>https://doi.org/10.13039/501100000266</funder_id>
        <grant_id>EP/N509589/1</grant_id>
        <project_name>DTP 2016-2017 University of Bath</project_name>
      </item>
    </funding>
    <research_centres>
      <item>cent_spa_atmo_oce</item>
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    <techinfo>The .mw files are Maple worksheets, written using Maple software version 2018.2. At the time of simulation, this operated on both Windows 64-bit and macOS X Catalina.</techinfo>
    <language>en</language>
    <version>1</version>
    <doi>10.15125/BATH-00810</doi>
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