echemi logo
Product
  • Product
  • Supplier
  • Inquiry
    Home > Biochemistry News > Biotechnology News > The Chinese Sky Eye reveals the dynamic evolution of the rapidly radio burst close to the environment

    The Chinese Sky Eye reveals the dynamic evolution of the rapidly radio burst close to the environment

    • Last Update: 2022-10-01
    • Source: Internet
    • Author: User
    Search more information of high quality chemicals, good prices and reliable suppliers, visit www.echemi.com

    Recently, relying on the National Astronomical Observatory of the Chinese Academy of Sciences and independently developed by China to independently develop the national major scientific and technological infrastructure "China Heavenly Eye" 500-meter aperture spherical radio telescope (FAST), a researcher led by the Department of Astronomy of the School of Physics of Peking University and the Institute of Astronomy and Astrophysics of Keweili, Li Kejia, a researcher of the National Astronomical Observatory of the Chinese Academy of Sciences, Zhu Weiwei, a researcher of the National Astronomical Observatory of the Chinese Academy of Sciences, and a researcher of the East Subo of the Institute of Astronomy and Astrophysics of Peking University.


    Fast radio bursts (FRBs) are occasional radio bursts in the universe
    .


    The FAST Priority and Major Scientific Research team used FAST to conduct long-term monitoring of FRB 20201124A, and detected 1863 burst pulse signals from this fast radio burst in 82-hour observations over 54 days, making it one of
    the most active repeat bursts.


    FAST's detection of nearly 2,000 outbreaks of the repetitive fast radio burst FRB 20201124A revealed a very complex, dynamically evolving, strong magnetic field environment of the burst, which is of great help
    in understanding how the fast radio burst and its surrounding environment produce a radio burst and affect its propagation.


    Xu Heng, a doctoral student jointly trained by Peking University and the National Astronomical Observatory of the Chinese Academy of Sciences, Chen Ping, a doctoral student of Peking University, and Jiarui Niu, a doctoral student of the National Astronomical Observatory of the Chinese Academy of Sciences, were deeply involved in this research
    .


    Figure 1: Short-scale evolution of Faraday's
    amount of rotation.


    Figure 2: Oscillation of line/circle polarity and polarization position angle detected in FRB 20201124A

    Figure 3: Spectral and high-resolution imaging observations of the host galaxy at FRB 20201124A via the Keck telescope

    This article is an English version of an article which is originally in the Chinese language on echemi.com and is provided for information purposes only. This website makes no representation or warranty of any kind, either expressed or implied, as to the accuracy, completeness ownership or reliability of the article or any translations thereof. If you have any concerns or complaints relating to the article, please send an email, providing a detailed description of the concern or complaint, to service@echemi.com. A staff member will contact you within 5 working days. Once verified, infringing content will be removed immediately.

    Contact Us

    The source of this page with content of products and services is from Internet, which doesn't represent ECHEMI's opinion. If you have any queries, please write to service@echemi.com. It will be replied within 5 days.

    Moreover, if you find any instances of plagiarism from the page, please send email to service@echemi.com with relevant evidence.