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Full-Wave Modeling of Whistler Wave Propagation Through the Martian Ionosphere

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F25%3A10513143" target="_blank" >RIV/00216208:11320/25:10513143 - isvavai.cz</a>

  • Result on the web

    <a href="https://physics.mff.cuni.cz/wds/proc/pdf25/WDS25_10_f2_Rosicka.pdf" target="_blank" >https://physics.mff.cuni.cz/wds/proc/pdf25/WDS25_10_f2_Rosicka.pdf</a>

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Full-Wave Modeling of Whistler Wave Propagation Through the Martian Ionosphere

  • Original language description

    Lightning flashes have been observed on several planets in the Solar System.However, atmospheric discharges have not yet been detected on Mars, despite theoreticalmodels predicting their occurrence within dust devils. We present a full-wave simulation ofan electromagnetic signal generated by a hypothetical lightning discharge. We show that itcan exceptionally propagate through the Martian ionosphere in the form of a whistler, whichwould be detectable by spacecraft orbiting Mars. In our work, we consider ionosphericplasma with a Chapman profile consisting of electrons and O2+ions under the conditions ofa region with a strong crustal magnetic field. We model the transmission of a single planewave through the ionosphere with different initial wave vector directions, wave polarizationand frequencies. Under these conditions, we investigate the causes of attenuation, suchas different types of collisions or reflection of the wave at the lower boundary of theionosphere. In this work, we demonstrate that the transmition of whistler signals throughthe Martian ionosphere is possible, but the favorable conditions are rare

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10305 - Fluids and plasma physics (including surface physics)

Result continuities

  • Project

    <a href="/en/project/LUAUS23152" target="_blank" >LUAUS23152: Electrodynamics of magnetospheres and ionospheres of the Earth, Jupiter and Mars</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>S - Specificky vyzkum na vysokych skolach<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2025

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    WDS&apos;25 Proceedings of Contributed Papers - Physics

  • ISBN

    978-80-7378-532-1

  • ISSN

  • e-ISSN

  • Number of pages

    10

  • Pages from-to

    84-93

  • Publisher name

    Matfyzpress

  • Place of publication

    Prague

  • Event location

    Praha

  • Event date

    Jun 3, 2025

  • Type of event by nationality

    EUR - Evropská akce

  • UT code for WoS article