MegaWave Radio Surveyor 是一项旨在探索低射频电磁波谱的空基干涉仪任务。该任务通过观测恒星空间天气、系外行星磁场及宇宙黑暗时期,旨在解决天体物理学与宇宙学中的关键科学问题。
arXiv:2608.26322v1 Announce Type: new Abstract: Several Decadal-level questions in astrophysics, exoplanets, astrobiology, and cosmology can be addressed only at low radio frequencies inaccessible from Earth. The MegaWave Radio Surveyor would open this largely-unexplored region of the electromagnetic spectrum with a space-based interferometer to (1)~Track the space weather of other stars; (2)~Detect magnetically-generated emission from exoplanets to probe their interiors and assess magnetic shielding of their atmospheres; (3)~Probe the Universe's evolution during the Dark Ages via the highly-redshifted HI hyperfine line; and (4)~Assess the role of cosmic rays and magnetic fields in the cosmic web. An Astrophysics Strategic Technology & Research Accelerator (ASTRA) Initiative concept, the MegaWave Radio Surveyor's science objectives respond to the Pathways to Discovery Decadal Survey and three other National Academies studies, and it would serve as a Formative Era mission in the Enduring Quests, Daring Visions roadmap. Developments in U.S. space industries enable this observatory to be realized. The MegaWave Radio Surveyor would offer a versatile, scalable, and resilient architecture capable of sensitive and simultaneous observations below 45~MHz and unprecedented angular resolution at these frequencies. The concept builds upon NASA's Sun Radio Interferometer Space Experiment (SunRISE), Star-Planet Activity Research CubeSat (SPARCS), and Lunar Surface Electromagnetics Experiment (LuSEE-Night).
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本站仅展示标题与摘要,正文版权归原作者及原发布机构所有。 原作者:T. Joseph W. Lazio (Michigan), Evgenya Shkolnik (ASU), James Aguirre (Pennsylvania), Stuart D. Bale (UC Berkeley), Judd Bowman (ASU), Ruby Byrne (Caltech), Joseph Callingham (ASTRON), Tracy E. Clarke (NRL), Ivey Davis (ASTRON), Tim Dolch (UNM), Peter Driscoll (Carnegie Science), Anastasia Fialkov (Cambridge), Steven Furlanetto (UCLA), Simona Giacintucci (NRL), Ravit Helled (Univ. Zurich), Jacqueline Hewitt (MIT), Phil Hopkins (Caltech), Andrea Isella (Rice), Daniel Jacobs (ASU), Eloy de Lera Acedo (Cambridge), Melodie M. Kao (Lowell Observatory), Mary Knapp (MIT/Haystack Observatory), L. V. E. Koopmans (Kapteyn Astronomical Institute), Nicholas Kern (Michigan), Jasmina Lazendic-Galloway (Eindhoven University of Technology), Susan T. Lepri (Michigan), R. O. Parke Loyd (Eureka Scientific), James P. Lux (JPL, Caltech), James P. Mason (APL/JHU), Raul Monsalve (Universidad Andr\'es Bello), Miguel Morales (Univ. Washington), Julian B. Mu\~noz (UT Austin), Rachel Osten (Johns Hopkins, STScI), J. Sebastian Pineda (CU Boulder), Jonathan Pober (Brown), Sam B. Ponnada (Chalmers), Leslie A. Rogers (Chicago), Saurabh Singh (Raman Research Institute), Jake D. Turner (Cornell), Jackie Villadsen (Bucknell), Philippe Zarka (Observatoire de Paris), John ZuHorne (Harvard-Smithsonian CfA), Ellen Zweibel (Univ. Wisconsin, Madison)。 原始页面