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Influence of Solar Wind on Secondary Cosmic Rays and Atmospheric Electricity

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F21%3A00543869" target="_blank" >RIV/68378289:_____/21:00543869 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216208:11320/21:10439766

  • Result on the web

    <a href="https://www.frontiersin.org/articles/10.3389/feart.2021.671801/full" target="_blank" >https://www.frontiersin.org/articles/10.3389/feart.2021.671801/full</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.3389/feart.2021.671801" target="_blank" >10.3389/feart.2021.671801</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Influence of Solar Wind on Secondary Cosmic Rays and Atmospheric Electricity

  • Original language description

    A relationship between the heliospheric magnetic field, atmospheric electric field, lightning activity, and secondary cosmic rays measured on the high mount of Lomnický Štít (2,634 m a.s.l.), Slovakia, during the declining phase of the solar cycle 24 is investigated with a focus on variations related to solar rotation (about 27 days). The secondary cosmic rays are detected using a neutron monitor and the detector system SEVAN, which distinguishes between different particles and energies. Using spectral analysis, we found distinct ∼27-day periodicities in variations of Bx and By components of the heliospheric magnetic field and in pressure-corrected measurements of secondary cosmic rays. The 27-day variations of secondary cosmic rays, on average, advanced and lagged the variations of Bx and By components by about 40° and −140°, respectively. Distinct 27-day periodicities were found both in the neutron monitor and the SEVAN upper and middle detector measurements. A nondominant periodicity of ∼27 days was also found for lightning activity. A cross-spectral analysis between fluctuation of the lightning activity and fluctuation of the heliospheric magnetic field (HMF) showed that fluctuation of the lightning activity was in phase and in antiphase with Bx and By components of the HMF, respectively, which is in agreement with previous studies investigating the influence of solar activity on lightning. On the other hand, the ∼27-day periodicity was not significant in the atmospheric electric field measured in Slovakia and Czechia. Therefore, no substantial influence of Bx and By on the atmospheric electric field was observed at these middle-latitude stations.

  • 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

    10305 - Fluids and plasma physics (including surface physics)

Result continuities

  • Project

    <a href="/en/project/GA20-09671S" target="_blank" >GA20-09671S: Investigation of lightning discharges at different scales</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2021

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Frontiers in Earth Science

  • ISSN

    2296-6463

  • e-ISSN

    2296-6463

  • Volume of the periodical

    9

  • Issue of the periodical within the volume

    July

  • Country of publishing house

    CH - SWITZERLAND

  • Number of pages

    15

  • Pages from-to

    671801

  • UT code for WoS article

    000679385900001

  • EID of the result in the Scopus database

    2-s2.0-85111594090