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Background for gravitational wave signal at LISA from refractive index of solar wind plasma

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21670%2F20%3A00346844" target="_blank" >RIV/68407700:21670/20:00346844 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1093/mnrasl/slaa155" target="_blank" >https://doi.org/10.1093/mnrasl/slaa155</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1093/mnrasl/slaa155" target="_blank" >10.1093/mnrasl/slaa155</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Background for gravitational wave signal at LISA from refractive index of solar wind plasma

  • Original language description

    A strong indication is presented that the space-based gravitational antennas, in particular the Laser Interferometer Space Antenna (LISA) concept introduced in 2017 in response to the ESA call for L3 mission concepts, are going to be sensitive to a strong background signal interfering with the prospected signal of gravitational waves. The false signal is due to variations in the electron number density of the solar wind, causing variations in the refractive index of plasma flowing through interplanetary space. As countermeasures, two solutions are proposed. The first solution is to deploy enough solar wind detectors to the LISA mission to allow for reliable knowledge of the solar wind background. The second solution is to equip the LISA interferometer with a second laser beam with a distinct wavelength to allow cancelling of the background solar wind signal from the interferometric data.

  • 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

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2020

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Monthly Notices of the Royal Astronomical Society

  • ISSN

    0035-8711

  • e-ISSN

    1365-2966

  • Volume of the periodical

    499

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    5

  • Pages from-to

    "L77"-"L81"

  • UT code for WoS article

    000587776700016

  • EID of the result in the Scopus database