印度天文学家利用Kodakanal Tower望远镜数据开发研究太阳磁场层的方法。 Indian astronomers develop method to study Sun's magnetic field layers using Kodaikanal Tower Telescope data.

印度天体物理学研究所的天文学家开发了一种方法,利用Kodaikanal Tower望远镜的数据,对太阳在太阳大气层不同层的磁场进行检查。 Astronomers at the Indian Institute of Astrophysics have developed a method to examine the Sun's magnetic field in different layers of the solar atmosphere using data from the Kodaikanal Tower Telescope. 这项研究同时利用多线分光谱测量,特别是氢-阿尔法线,目的是了解日冕热和太阳风机制等太阳现象。 The study, utilizing simultaneous multi-line spectropolarimetry, particularly the Hydrogen-alpha line, aims to understand solar phenomena like coronal heating and solar wind mechanisms. 研究人员的研究结果可能有助于揭示染色体中错综复杂的磁场分层,为DKIST、EST和NLST等未来望远镜提供洞察力。 The researchers' findings may help shed light on the intricate magnetic field stratification in the chromosphere, providing insights for future telescopes like the DKIST, EST, and NLST.