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  <head>
    <doi_batch_id>esdb-2026-PET2021def</doi_batch_id>
    <timestamp>20260101120000</timestamp>
    <depositor>
      <depositor_name>Geophysical Center RAS</depositor_name>
      <email_address>crossref@gcras.ru</email_address>
    </depositor>
    <registrant>Geophysical Center RAS</registrant>
  </head>
  <body>
    <database>
      <database_metadata language="en">
        <titles><title>ESDB repository</title></titles>
        <institution>
          <institution_name>Geophysical Center of the Russian Academy of Sciences (GC RAS)</institution_name>
          <institution_acronym>GCRAS</institution_acronym>
        </institution>
      </database_metadata>

      <dataset dataset_type="record">
        <titles><title>2021 definitive data from geomagnetic observatory Paratunka (IAGA
code: PET)</title></titles>

        <contributors>

          <person_name sequence="first"
                       contributor_role="author">
            <given_name>Ilkhambek Y.</given_name>
            <surname>Babakhanov</surname>


            <affiliations>

              <institution>Institute of Cosmophysical Research and Radio Wave Propagation, Far
Eastern Branch of the Russian Academy of Sciences (IKIR FEB RAS), Paratunka, Kamchatka, Russia</institution>

            </affiliations>

          </person_name>

          <person_name sequence="additional"
                       contributor_role="author">
            <given_name>Irina N.</given_name>
            <surname>Khomutova</surname>


            <affiliations>

              <institution>Institute of Cosmophysical Research and Radio Wave Propagation, Far
Eastern Branch of the Russian Academy of Sciences (IKIR FEB RAS), Paratunka, Kamchatka, Russia</institution>

            </affiliations>

          </person_name>

          <person_name sequence="additional"
                       contributor_role="author">
            <given_name>Olga S.</given_name>
            <surname>Bogunova</surname>


            <affiliations>

              <institution>Institute of Cosmophysical Research and Radio Wave Propagation, Far
Eastern Branch of the Russian Academy of Sciences (IKIR FEB RAS), Paratunka, Kamchatka, Russia</institution>

            </affiliations>

          </person_name>

          <person_name sequence="additional"
                       contributor_role="author">
            <given_name>Anastasiya F.</given_name>
            <surname>Raykevich</surname>


            <affiliations>

              <institution>Institute of Cosmophysical Research and Radio Wave Propagation, Far
Eastern Branch of the Russian Academy of Sciences (IKIR FEB RAS), Paratunka, Kamchatka, Russia</institution>

            </affiliations>

          </person_name>

          <person_name sequence="additional"
                       contributor_role="author">
            <given_name>Mikhail V.</given_name>
            <surname>Prikop</surname>

            <ORCID authenticated="true">https://orcid.org/0009-0002-5573-5728</ORCID>


            <affiliations>

              <institution>Institute of Solar-Terrestrial Physics of Siberian Branch of Russian
Academy of Sciences (ISTP SB RAS), Irkutsk, Russia</institution>

            </affiliations>

          </person_name>

        </contributors>

        <database_date>
          <publication_date>
            <year>2026</year>
          </publication_date>
        </database_date>
        <description>The dataset contains definitive minute values of the geomagnetic
field based on observations from the Paratunka INTERMAGNET magnetic
observatory (IAGA code: PET) for the period from 1 January to 31
December 2021. The components X (Northward), Y (Eastward), and Z
(Downward) are provided. Additionally, the quantity G=Fv-Fs is provided
— the difference between the magnitude of the field vector Fv calculated
from components X, Y, and Z and the magnitude of the total vector Fs
measured independently ...</description>
        <doi_data>
          <doi>10.2205/PET2021def</doi>
          <resource>https://esdb.wdcb.ru/doi/2026/pet2021def.html</resource>
        </doi_data>

        <citation_list>

          <citation key="ref1">
            <doi>10.1051/epjconf/202125402018</doi>

            <unstructured_citation>Khomutov, S.Y., Sapunov, V.A., Denisov, A.Y., Borodin, P.B., Kudin, D.V., Sidorov, R.V., Bebnev, A.S., Cherepanova, T.A., Kotikov, A.L., Kanonidi, K.K., Turbin, Y.G., &amp; Baryshev, P.E. (2021). Vector Overhauser magnetometer POS-4: experience and prospects of application. EPJ Web of Conferences, 254, 02018. https://doi.org/10.1051/epjconf/202125402018</unstructured_citation>

          </citation>

          <citation key="ref2">
            <doi>10.1007/978-3-031-50248-4_23</doi>

            <unstructured_citation>Gvozdarev, A.Y., Khomutov, S.Y., Arora, K., &amp; Chandrasekhar, P. (2023). About Some Small Effects in Magnetic Field at Observatories Paratunka (Kamchatka, Russia) and Choutuppal (India). Springer Proceedings in Earth and Environmental Sciences, 221-234. https://doi.org/10.1007/978-3-031-50248-4_23</unstructured_citation>

          </citation>

          <citation key="ref3">
            <doi>10.3390/app12042072</doi>

            <unstructured_citation>Mandrikova, O., Polozov, Y., &amp; Khomutov, S. (2022). Wavelet Model of Geomagnetic Field Variations and Its Application to Detect Short-Period Geomagnetic Anomalies. Applied Sciences, 12(4), 2072. https://doi.org/10.3390/app12042072</unstructured_citation>

          </citation>

        </citation_list>

      </dataset>

    </database>
  </body>
</doi_batch>