Voyager 1 (V1) observed q-Gaussian distributions of 1 hr increments of the components the magnetic field throughout the very local interstellar medium (VLISM) on scales on the order of 1 year, from 2013 through 2019, excluding the disturbed regions near two shocks. The intermittency of the components of B is described by q from the q-Gaussian distributions of 1 hr increments B as well as by the kurtosis K derived from the time series of the increments of . Farther than ∼5 au from the heliopause, Voyager 1 observed larger intermittency in the fluctuations of the predominantly transverse component B _N and in the nearly longitudinal component B _T of . The average values of q for the B _N component and transverse B _T component for these data in the VLISM are q=1.320.03 and q=1.220.03, respectively. The corresponding average values of the kurtosis are K=7.2 and K=4.9. Voyager 2 (V2) crossed the heliopause on 2018 November 5. Near the heliopause, in 2019, V2 observed large intermittency in 1 hr increments of the compressive component B _T and smaller intermittency in B _N. The Voyager 2 observations give q=1.510.06 and q=1.170.06 for the B _N and B _T components of B, respectively, as well as K=7.2 and K=12.3, respectively. The intermittency in B _T and B _N, observed by V2 near the heliopause was significantly larger than that observed by V1 when it was near the heliopause.

航海者 1 号 (V1)在 2013 年至 2019 年期间，在大约 1 年的尺度上观察了整个非常局域星际介质 (VLISM) 中磁场分量 1 小时增量的q -高斯分布，不包括两次冲击附近的扰动区域. 的成分的间歇乙通过描述q从q 1个小时增量-gaussian分布乙以及由峰度ķ从时间序列的增量的衍生。距离日球层顶约 5 天文单位以外，航海者 1 号观察到主要横向分量B _N的波动具有更大的间歇性并且在 的近纵向分量B _T中。的平均值q为乙 _Ñ分量和横向乙 _Ť组件，用于在VLISM这些数据是q = 1.320.03和q = 1.220.03，分别。对应的峰态平均值为K =7.2 和K =4.9。航海者 2 (V2) 于 2018 年 11 月 5 日穿越了日球层顶。 在 2019 年的日球层顶附近，V2 观察到压缩分量B _T以 1 小时增量为单位的大间歇性和B _{N 中}较小的间歇性。航海者 2 号观测给出q = 1.510.06和q = 1.170.06为乙 _Ñ和乙 _Ť的部件乙分别以及ķ = 7.2和ķ = 12.3，分别。V2在日球层顶附近观测到的B _T和B _N的间歇性显着大于V1在靠近日光层顶时观测到的间歇性。