论文标题
在银河系的情况下，Heliosphere符合星际培养基
Heliosphere Meets Interstellar Medium, in a Galactic Context
论文作者
论文摘要
我们的气球内的物理状况是由太阳通过不断发展的星际环境的运动驱动的，这在很大程度上没有探索。下一代的外气球和星际探险家将通过深入深入到太阳的星际周围环境中，回答有关Heliosphere与非常本地星际介质（VLISM）关系的基本问题。这些未来任务的影响将通过同时进行的，跨学科的研究大大增强，这些研究检查地球球内的条件之间的直接连接，地球层的直接星际环境和较大的银河系ISM。在星系中，地球球和VLISM与它们的类似物的比较将限制塑造恒星天然喷气流的全球过程及其对ISM的持续影响。
The physical conditions within our heliosphere are driven by the Sun's motion through an evolving interstellar environment that remains largely unexplored. The next generation of outer heliosphere and interstellar explorers will answer fundamental questions about the heliosphere's relationship with the very local interstellar medium (VLISM) by diving deeper into the Sun's interstellar surroundings. The impact of these future missions will be vastly enhanced by concurrent, interdisciplinary studies that examine the direct connections between conditions within the heliosphere, the heliosphere's immediate interstellar environment, and the larger-scale Galactic ISM. Comparisons of the heliosphere and VLISM to their analogs across the Galaxy will constrain the global processes shaping both stellar astrospheres and their sustained impact on the ISM.
