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Exploring Potential Impact-Induced Magnetic Signatures at the Tunguska Event Epicenter Using UAV-Based Magnetometry

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11310%2F25%3A10499888" target="_blank" >RIV/00216208:11310/25:10499888 - isvavai.cz</a>

  • Alternative codes found

    RIV/68407700:21230/25:00385488

  • Result on the web

    <a href="https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=pTGP4TY~Ir" target="_blank" >https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=pTGP4TY~Ir</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1029/2024EA004194" target="_blank" >10.1029/2024EA004194</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Exploring Potential Impact-Induced Magnetic Signatures at the Tunguska Event Epicenter Using UAV-Based Magnetometry

  • Original language description

    The Tunguska event of 1908 remains the most significant atmospheric explosion in recorded history, yet its geophysical effects, particularly its impact on Earth&apos;s magnetic field, remain uncertain. This study presents the first detailed magnetometer survey of the Tunguska epicenter, aiming to map regional magnetic anomalies and assess potential impact-induced magnetization. The survey used unmanned aerial vehicle and covered approximately 30 square kilometers, revealing a complex pattern of magnetic anomalies that correlate with known geological structures. Notably, some anomalies exhibit spatial alignment with the presumed trajectory of the airburst (~300° azimuth), suggesting potential influence from the event. This spatial correlation raises the possibility that transient electromagnetic effects from the airburst, such as ionization-induced remagnetization or shock-induced changes in magnetic mineralogy, could have contributed to the observed anomaly distribution. However, due to the limitations of our data set, we cannot definitively attribute any observed anomalies to impact-related remagnetization. Our analysis identifies regions where future rock magnetic studies could provide further insights. We discuss possible mechanisms for transient remagnetization, including ionization effects and shock-induced mineral transformations, while emphasizing the necessity of future paleomagnetic sampling to test these hypotheses. These findings establish a foundational geophysical data set for future interdisciplinary investigations into the Tunguska event&apos;s environmental and geological consequences.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10505 - Geology

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2025

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Earth and Space Science

  • ISSN

    2333-5084

  • e-ISSN

    2333-5084

  • Volume of the periodical

    12

  • Issue of the periodical within the volume

    7

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    17

  • Pages from-to

    e2024EA004194

  • UT code for WoS article

    001530255800001

  • EID of the result in the Scopus database

    2-s2.0-105011284613