|
所在平台: Udemy |
课程主页: https://www.udemy.com/course/hydrogen-technologies/
课程评论：没有评论
课程名称：氢能技术硕士文凭 课程概述：氢能技术硕士文凭是一门富有趣味的课程，旨在为学生提供氢能技术的基础知识，包括不同的氢气生产、储存、运输方法以及氢气在各个领域的应用。此外，课程还将探讨该技术的发展机会、当前项目、未来项目及全球范围内氢能技术的多种活动。 课程内容包括： 1. 氢气统计的快速变化 2. 氢气生产方法 3. 氨中的氢气储存 4. 液体有机氢载体（LOHC） 5. 燃料电池 6. 燃料电池汽车（FCV）与电动汽车（EV）的平准化氢气成本（LCOE） 7. EV与FCV的能效比较 8. 盐穴氢气储存 9. 氢气的应用 10. 核反应堆与氢能技术 11. CANDU核反应堆在氢经济中的应用 12. 硫碘循环的高温气冷反应堆（VHTR） 13. 氢气的颜色分类 14. 最常见载体中氢气的含量 氢是元素符号为H、原子序数为1的化学元素，它是最轻的元素，通常以二聚体H2的气态存在。氢无色、无味、无毒，且极易燃烧。它是宇宙中最丰富的化学物质，约占普通物质的75%。氢在我们的地球上主要以水和有机化合物的分子形式存在。 该课程旨在帮助学生理解氢能技术的基础，关注当前的研究及其在未来的潜力。学生将获益于全球氢能技术发展的最新信息和趋势。
mastership Diploma in Hydrogen Technology is an interesting course where you can get knowledge about the fundamentals of hydrogen technologies like different methods of hydrogen production, storage, transportation and applications of hydrogen for various disciplines. Moreover, you will explore the development opportunities available in this technology, current projects, futuristic projects, and various worldwide activities in hydrogen technologies. The course discusses;1- Hydrogen Statistics Rapid Change2- Hydrogen Production3- Hydrogen Storage in Ammonia4- Hydrogen Statistics Rapid Change5- Liquid organic hydrogen carriers (LOHC)6- Fuel Cells7- Levelized Cost Of Hydrogen (LCOE) of Hydrogen for FCV8- Fuel Cell Vehicle (FCV) Versus EV Electric Vehicle (EV)9- EV and FCV Energy Efficiency10- Salt Cavern Hydrogen Storage11- Applications of Hydrogen12- Nuclear Reactors and Hydrogen Technology13- CANDU Nuclear Reactors for Hydrogen Economy14- Very High Temperature Reactor (VHTR) for Sulfur-Iodine Cycle 15- Hydrogen Colors16- Content of Hydrogen in most common carrierHydrogen is the chemical element with the symbol H and atomic number 1. Hydrogen is the lightest element. At standard conditions hydrogen is a gas of diatomic molecules having the formula H2. It is colorless, odorless, tasteless, non-toxic, and highly combustible. Hydrogen is the most abundant chemical substance in the universe, constituting roughly 75% of all normal matter.[9][note 1] Stars such as the Sun are mainly composed of hydrogen in the plasma state. Most of the hydrogen on Earth exists in molecular forms such as water and organic compounds. For the most common isotope of hydrogen (symbol 1H) each atom has one proton, one electron, and no neutrons. In the early universe, the formation of protons, the nuclei of hydrogen, occurred during the first second after the Big Bang. The emergence of neutral hydrogen atoms throughout the universe occurred about 370,000 years later during the recombination epoch, when the plasma had cooled enough for electrons to remain bound to protons. Hydrogen is nonmetallic, except at extremely high pressures, and readily forms a single covalent bond with most nonmetallic elements, forming compounds such as water and nearly all organic compounds. Hydrogen plays a particularly important role in acid-base reactions because these reactions usually involve the exchange of protons between soluble molecules. In ionic compounds, hydrogen can take the form of a negative charge (i.e., anion) where it is known as a hydride, or as a positively charged (i.e., cation) species denoted by the symbol H+. The H+ cation is simply a proton (symbol p) but its behavior in aqueous solutions and in ionic compounds involves screening of its electric charge by nearby polar molecules or anions. Because hydrogen is the only neutral atom for which the Schrödinger equation can be solved analytically, the study of its energetics and chemical bonding has played a key role in the development of quantum mechanics.
