U.S.-India Cooperative Research: Joint Study of Solar Oscillations Gong Phase III, Award in Indian Rupees

小行星9710279 描述：该奖项支持美国-印度合作研究：太阳振荡研究第三阶段，将利用全球振荡网络组（GONG）的数据集研究太阳内部。 这个最近完成的由六个相同的环绕地球仪的振荡观测站组成的网络将对太阳进行24小时监视，并将产生独特的数据，这些数据不仅对太阳物理学，而且对天体物理学、日地物理学、天体物理学和核物理学都具有重要意义。 美国团队由图森国家太阳天文台（NSO）的John Leibacher领导，印度团队由Udaipur太阳天文台（USO）Udaipur的Arvind Bhatnagar和S.M. Chitre，塔塔基础研究所，孟买。 日震学的新领域是从太阳声波的发现发展而来的，太阳声波是从太阳内部随机激发的地震振动中发出的。 这种研究太阳内部结构和动力学的强大新工具可以探测太阳内部，其精度与地面地震学探测地球内部的精度相同。 在研究的第三阶段，美国和印度团队将在GONG数据刺激的众多领域进行合作研究。 这些包括倒置;太阳静力结构;太阳包层中的氦丰度;太阳振荡的激发机制;背景太阳光谱;太阳内部深处的全球磁场;近稳定流和磁场;以及确定性的去趋势。 范围：美国-这个大型国际项目的印度部分非常平衡。 对美国来说，乌代普具有大气清澈、与图森市截然相反的地球仪上独特的地理位置以及强大的基础设施资源等物理属性。 太阳物理学是印度科学家擅长的领域。 该项目将涉及USO工作人员和来自印度首屈一指的塔塔研究所的世界级研究人员。 对印度来说，该项目提供了进入日震学领域的机会，提供了最先进的仪器，并参与了重要的国际努力。 迄今为止，该项目已在美国出版了大量出版物，印度作家。 ***

9710279 Bhatnagar Description: This award supports the U.S.-India Cooperative Research: Study of Solar Oscillations Phase III, which will examine the Sun s interior utilizing the data set from the Global Oscillation Network Group (GONG). This recently completed network of six identical oscillation observing stations that circle the globe will keep the Sun under 24 hour surveillance and will yield unique data having importance not only for solar physics, but for astrophysics, solar-terrestrial physics, geophysics, and nuclear physics. The U.S. team is headed by John Leibacher of the National Solar Observatory (NSO), Tucson, and the Indian team by Arvind Bhatnagar, Udaipur Solar Observatory (USO) Udaipur, and S.M. Chitre, Tata Institute of Fundamental Research, Mumbai. The new field of helioseismology has evolved from the discovery of solar acoustic waves that emanate from randomly-excited seismic vibrations from within the Sun. This powerful new tool for studying the Sun s interior structure and dynamics can probe the interior of the Sun with the same precision that terrestrial seismology can probe the Earth s interior. During Phase III of the study, the U.S. and Indian teams will pursue collaborative research in numerous areas that have been stimulated by GONG data. These include inversions; hydrostatic Sun structure; helium abundance in the solar envelope; excitation mechanisms for solar oscillations; background solar spectrum; global magnetic fields in the sun s deep interior; nearly steady flows and magnetic fields; and deterministic detrending. Scope: The U.S.-India component of this large international project is exceptionally well balanced. For the United States, Udaipup has physical attributes such as atmospheric clarity and a unique geographic position on the globe diametrically opposite to Tucson, as well as strong infrastructural resources. Solar physics is a field in which Indian scientists excel. The project will involve USO staff and world cl ass researchers from India s premier Tata Institute. For India, the project offers entry to the field of helioseismology, state-of -the-art instrumentation, and involvement in an important international effort. This project has thus far yielded a large number of publications under U.S.-Indian authorship. ***