1.0KMI - Nagoya Universityhttps://www.kmi.nagoya-u.ac.jp/engMagnetic Turbulence and Reconnection in Galaxy Clusters: toward the Era of Square Kilometre Array Observatory - KMI - Nagoya Universityrich600338<blockquote class="wp-embedded-content" data-secret="FwRLvHdnHI"><a href="https://www.kmi.nagoya-u.ac.jp/eng/seminar/3336/">Magnetic Turbulence and Reconnection in Galaxy Clusters: toward the Era of Square Kilometre Array Observatory</a></blockquote><iframe sandbox="allow-scripts" security="restricted" src="https://www.kmi.nagoya-u.ac.jp/eng/seminar/3336/embed/#?secret=FwRLvHdnHI" width="600" height="338" title="“Magnetic Turbulence and Reconnection in Galaxy Clusters: toward the Era of Square Kilometre Array Observatory” — KMI - Nagoya University" data-secret="FwRLvHdnHI" frameborder="0" marginwidth="0" marginheight="0" scrolling="no" class="wp-embedded-content"></iframe><script type="text/javascript">
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“KMI colloquium” 14th May (Wed) 17：00 – 18 : 00 Speaker: Takuya Akahori (National Astronomical Observatory of Japan) Title: Magnetic Turbulence and Reconnection in Galaxy Clusters: toward the Era of Square Kilometre Array Place: ES635 & ZOOM Abstract: The intracluster medium (ICM) in galaxy clusters is expected to be magnetized and turbulent. But the origin and nature of the magnetic field poorly understood, remaining its true impact into the cosmology and the structure formation theory open. Recent astronomical telescopes such …https://www.kmi.nagoya-u.ac.jp/eng/wp-content/uploads/sites/2/2025/04/KMI-Colloquim_Akahori_20250514_poster2.png