University of New Hampshire, Space Science Center, Durham, NH 03824, USA.
Science. 2014 Feb 28;343(6174):988-90. doi: 10.1126/science.1245026. Epub 2014 Feb 13.
Observations with the Interstellar Boundary Explorer (IBEX) have shown enhanced energetic neutral atom (ENA) emission from a narrow, circular ribbon likely centered on the direction of the local interstellar medium (LISM) magnetic field. Here, we show that recent determinations of the local interstellar velocity, based on interstellar atom measurements with IBEX, are consistent with the interstellar modulation of high-energy (tera-electron volts, TeV) cosmic rays and diffusive propagation from supernova sources revealed in global anisotropy maps of ground-based high-energy cosmic-ray observatories (Milagro, Asγ, and IceCube). Establishing a consistent local interstellar magnetic field direction using IBEX ENAs at hundreds to thousands of eV and galactic cosmic rays at tens of TeV has wide-ranging implications for the structure of our heliosphere and its interactions with the LISM, which is particularly important at the time when the Voyager spacecraft are leaving our heliosphere.
IBEX 的观测显示,来自一个狭窄的圆形带状物的高能中性原子(ENA)发射增强,该带状物可能集中在局部星际介质(LISM)磁场的方向上。在这里,我们表明,基于 IBEX 对星际原子的测量,最近对本地星际速度的确定与星际调制的高能(万亿电子伏特,TeV)宇宙射线以及来自超新星源的扩散传播一致,这些在地面高能宇宙射线观测站(Milagro、Asγ 和 IceCube)的全球各向异性图中得到揭示。使用 IBEX 在数百到数千电子伏特的 ENA 和数十 TeV 的银河宇宙射线来建立一致的本地星际磁场方向,对我们的日球层结构及其与 LISM 的相互作用具有广泛的影响,这在旅行者号飞船离开我们的日球层时尤为重要。