esdb-2026-PET2023def 20260101120000 Geophysical Center RAS crossref@gcras.ru Geophysical Center RAS Geophysical Center of the Russian Academy of Sciences (GC RAS) GCRAS Irina N. Khomutova Institute of Cosmophysical Research and Radio Wave Propagation, Far Eastern Branch of the Russian Academy of Sciences (IKIR FEB RAS), Paratunka, Kamchatka, Russia Olga S. Bogunova Institute of Cosmophysical Research and Radio Wave Propagation, Far Eastern Branch of the Russian Academy of Sciences (IKIR FEB RAS), Paratunka, Kamchatka, Russia Anastasiya F. Raykevich Institute of Cosmophysical Research and Radio Wave Propagation, Far Eastern Branch of the Russian Academy of Sciences (IKIR FEB RAS), Paratunka, Kamchatka, Russia Irina V. Shiryaeva Institute of Cosmophysical Research and Radio Wave Propagation, Far Eastern Branch of the Russian Academy of Sciences (IKIR FEB RAS), Paratunka, Kamchatka, Russia Alexey Y. Gvozdarev Institute of Cosmophysical Research and Radio Wave Propagation, Far Eastern Branch of the Russian Academy of Sciences (IKIR FEB RAS), Paratunka, Kamchatka, Russia Mikhail V. Prikop https://orcid.org/0009-0002-5573-5728 Institute of Solar-Terrestrial Physics of Siberian Branch of Russian Academy of Sciences (ISTP SB RAS), Irkutsk, Russia 2026 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 2023. 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 ... 10.2205/PET2023def https://esdb.wdcb.ru/doi/2026/pet2023def.html