The purpose of this course is to examine how Japan’s transformation into a modern nation was shaped and represented through visual culture. Great emphasis is placed on group work, as students are expected to actively collaborate with peers to analyze visual materials, share perspectives, and co-construct knowledge. Through these interactive and cooperative activities, students will also have the opportunity to enhance their English communication skills and connect with a community of internationally minded peers. この授業では、日本が近代国家へと変化していく過程を、当時の絵画や写真、広告などの「視覚資料」を通して学びます。授業では、オンライン教材やビデオ講義、歴史資料を用いながら、ディスカッションや課題に取り組みます。特にグループワークを重視しており、視覚資料の分析やプレゼンテーションなどを通して、学生同士が協力しながら学びを深めていきます。これらの活動を通して、視覚的リテラシー、歴史的思考力、異文化理解力を養うとともに、英語によるコミュニケーション能力の向上も目指します。国際的な視野を広げたい方や、英語を実践的に使って学びたい方に適した内容となっています。

目標： 実世界情報処理（IoT, CPS, AR, VR）に関する理解を深め、発展の方向性についての認識を持つ 目的： 1) IoT, CPS, AR, VRの特徴・意義を説明できる 2) それぞれの技術の要素技術の長所短所を説明できる 3) 日々のIoT, CPS, AR, VRに関するニュースを理解でき、自分の意見を構築できる Goal: To deepen understanding of real-world information processing (IoT, CPS, AR, VR) and awareness of development directions Objectives: 1) To be able to explain the characteristics and significance of IoT, CPS, AR, and VR 2) To be able to explain the advantages and disadvantages of the elemental technologies of each technology 3) To be able to understand the daily news about IoT, CPS, AR, VR and to be able to construct one's own opinion

太陽・天体プラズマ物理学を、磁気流体力学の観点で講義する。 理論的観点から、太陽・天体活動現象を題材にしながら、それらに磁気プラズマが関与し ているのを解説する。それが磁気流体力学によって理解できること、さらにその基礎方程 式を駆使して応用できるようになること、が目標である。 以下のような話題から扱う予定。 1. 磁気リコネクション 2. 星の内部熱対流と大規模流 3. 磁気浮力 4. ダイナモ 5. 星大気を伝わる磁気流体波動 6. 太陽風と磁気流体乱流 7.太陽大気中での 輻射磁気流体 The magnetohydrodynamics (MHD) of the solar (and astrophysical) plasmas are lectured basically from the theoretical point of view, aiming to show that the various solar and astrophysical phenomena can be understood by the framework of MHD. The topics will be: 1. Magnetic reconnection 2. Convection and large-scale flows of stellar interior 3. Magnetic buoyancy 4. Dynamo 5. MHD waves in stellar atmosphere 6. MHD turbulence in solar winds 7. radiative MHD in ths solar atmosphere 11月7日（火）のみ、講義室を変更し、340講義室にて講義を行います。 Only on Tuesday, November 7th, the lecture room will be changed and the lecture will be held in 340.

宇宙から飛来する宇宙線、ガンマ線、ニュートリノなどを観測し、宇宙における高エネルギー天体現象や、暗黒物質などの素粒子物理を研究する分野を宇宙素粒子物理学（Astroparticle Physics）と呼ぶ。この分野の歴史的な成果として、CP対称性を破るK中間子などの新粒子の発見、最高エネルギー宇宙線の発見、ガンマ線バーストやブレーザーなどのブラックホール起源ガンマ線の検出、ニュートリノ振動の発見などが挙げられる。近年の観測技術の向上により、複数の観測手段を組み合わせて議論するマルチメッセンジャー天文学の時代となり、著しい発展を見せている分野である。この講義では、宇宙における高エネルギー粒子の起源や、それらの物理的性質、観測原理について基礎的なところから学ぶことを目標とする。講義内容については以下の英語版を参照。大きく3つに分かれている。 Astroparticle physics is a research field that studies high-energy astronomical phenomena and particle physics including dark matter via observations of cosmic rays, gamma-rays, neutrinos and so on. Some of representative discoveries done in this field are new particles such as kaon, which shows CP violation, ultra-high-energy cosmic rays, gamma-rays from black holes like gamma-ray bursts and blazars, and neutrino oscillation. Recent progress in the detector technology leads us to the era of multi-messenger astronomy, which is astronomy via collaborative observations of different species of particles. So this research field has been greatly developed in this decade. The purpose of this lecture is learning basics of origins of high-energy particles, physical properties of particles, and detection technique. The contents are divided into three parts as follows. １．Origin of High-energy Particles High-energy particles are accelerated somewhere in the universe, and produce secondary particles via interacting with other particles. Sources and the production mechanisms of such particles are not yet revealed, so numerous models have been proposed. In this lecture, we learn Fermi acceleration at shock waves as a promising particle acceleration mechanism, cosmic ray propagation in the interstellar medium, and emission mechanisms of gamma-rays and neutrinos. We also learn high-energy astrophysical phenomena as particle production sites. ２．Neutrino Physics Neutrinos have long been assumed to be massless, and the Standard Model of particle physics, based on this assumption, has been established as the paradigm that explains the results of many experiments to a high degree of accuracy. In 1998, however, it was discovered that neutrinos have finite mass and come in different flavors. The assumptions of the Standard Model turned out to be wrong, and this had a major impact on our understanding of particle physics and the nature. In this lecture, we will discuss the fundamental properties of neutrinos, their experimental verification mainly by neutrino oscillations, and the remaining unknowns and future experiments. ３．Dark Matter 　The mystery of dark matter is one of the most critical issues in cosmology and particle physics because it plays a leading role in shaping the universe and its potential to interrelate with various problems in particle physics. There are three main approaches to the experimental verification of dark matter: accelerator generation, indirect detection by observing signals from the decay and the annihilation of dark matter in space, and direct detection by capturing events in which dark matter around us collides with detectors. Research to elucidate the nature of dark matter is being actively pursued using all of these approaches. In this lecture, we will discuss various dark matter candidates and the principles and current status of direct and indirect search experiments for them.

宇宙空間プラズマの諸現象を理解するための基礎となるプラズマ物理学について解説する Plasma physics that provides the basis for understanding various space plasma phenomena will be discussed.

宇宙空間プラズマの諸現象を理解するための基礎となるプラズマ物理学について解説する

This is an introductory course on mathematical methods for public policy analysis, designed for GraSPP students without a strong background in mathematics. Students from non-economics, non-engineering, or non-science majors are especially welcomed. The course helps students develop a solid mathematical foundation, enabling them to apply essential mathematical techniques to public policy issues. It is structured into four parts: 1. differential calculus, 2. linear algebra, 3. multivariate calculus and constrained static optimization, 4. dynamic optimization and linear dynamic systems.

宇宙開発、宇宙科学の分野においても、電気電子工学の役割は重要である。本講義では、宇宙航空研究開発機構所属の教員などから、実際の宇宙分野での電気電子工学の応用例を紹介し、学部講義で習っている電気電子工学の基礎知識が実社会でどのように役立っているかを実感することを目的とする。／ Electrical and electronic engineering is important for space development and space science. The lecture provides actual application of electrical and electronic engineering in space by researchers of JAXA (Japan Aerospace Exploration Agency) and the University of Tokyo. The purpose of the lecture is that students learn how fundamental class in the University is useful for real society.

地球外物質に注目し，太陽系の起源と進化に関する物質科学の基礎と最先端を理解する． Lectures on the origin and early evolution of the Solar System through analysis of pristine extraterrestrial materials, laboratory experiments, and Solar System exploration and on basic physical chemistry and material science.

Learn about institutional design and spatial planning from global perspective.