{"title":"广义各向异性κ食谱:Ulysses电子数据的二维拟合","authors":"K. Scherer, E. Husidic, M. Lazar, H. Fichtner","doi":"10.1093/mnras/staa3641","DOIUrl":null,"url":null,"abstract":"Observations in space plasmas reveal particle velocity distributions out of thermal equilibrium, with anisotropies (e.g., parallel drifts or/and different temperatures, $T_\\parallel$ - parallel and $T_\\perp$ - perpendicular, with respect to the background magnetic field), and multiple quasithermal and suprathermal populations with different properties. The recently introduced (isotropic) $\\kappa$-cookbook is generalized in the present paper to cover all these cases of anisotropic and multi-component distributions reported by the observations. We derive general analytical expressions for the velocity moments and show that the common (bi-)Maxwellian and (bi-)$\\kappa-$distributions are obtained as limiting cases of the generalized anisotropic $\\kappa$-cookbook (or recipes). Based on this generalization, a new 2D fitting procedure is introduced, with an improved level of confidence compared to the 1D fitting methods widely used to quantify the main properties of the observed distributions. The nonlinear least-squares fit is \\led{applied to electron data sets} measured by the Ulysses spacecraft confirming the existence of three different populations, a quasithermal core and two suprathermal (halo and strahl) components. In general, the best overall fit is given by the sum of a Maxwellian and two generalized $\\kappa$-distributions.","PeriodicalId":8493,"journal":{"name":"arXiv: Solar and Stellar Astrophysics","volume":"8 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2020-11-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"6","resultStr":"{\"title\":\"Generalized anisotropic κ-cookbook: 2D fitting of Ulysses electron data\",\"authors\":\"K. Scherer, E. Husidic, M. Lazar, H. Fichtner\",\"doi\":\"10.1093/mnras/staa3641\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Observations in space plasmas reveal particle velocity distributions out of thermal equilibrium, with anisotropies (e.g., parallel drifts or/and different temperatures, $T_\\\\parallel$ - parallel and $T_\\\\perp$ - perpendicular, with respect to the background magnetic field), and multiple quasithermal and suprathermal populations with different properties. The recently introduced (isotropic) $\\\\kappa$-cookbook is generalized in the present paper to cover all these cases of anisotropic and multi-component distributions reported by the observations. We derive general analytical expressions for the velocity moments and show that the common (bi-)Maxwellian and (bi-)$\\\\kappa-$distributions are obtained as limiting cases of the generalized anisotropic $\\\\kappa$-cookbook (or recipes). Based on this generalization, a new 2D fitting procedure is introduced, with an improved level of confidence compared to the 1D fitting methods widely used to quantify the main properties of the observed distributions. The nonlinear least-squares fit is \\\\led{applied to electron data sets} measured by the Ulysses spacecraft confirming the existence of three different populations, a quasithermal core and two suprathermal (halo and strahl) components. In general, the best overall fit is given by the sum of a Maxwellian and two generalized $\\\\kappa$-distributions.\",\"PeriodicalId\":8493,\"journal\":{\"name\":\"arXiv: Solar and Stellar Astrophysics\",\"volume\":\"8 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2020-11-17\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"6\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv: Solar and Stellar Astrophysics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1093/mnras/staa3641\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv: Solar and Stellar Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1093/mnras/staa3641","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 6
摘要
在空间等离子体中的观测揭示了热平衡之外的粒子速度分布,具有各向异性(例如,平行漂移或/和不同的温度,$T_\parallel$ -平行和$T_\perp$ -垂直,相对于背景磁场),以及具有不同性质的多个准热和超热群。本文对最近引进的(各向同性)$\kappa$ -cookbook进行了推广,以涵盖观测报告的各向异性和多分量分布的所有情况。我们推导了速度矩的一般解析表达式,并证明了一般的(bi-)麦克斯韦分布和(bi-) $\kappa-$分布作为广义各向异性$\kappa$ -食谱(或食谱)的极限情况。在此基础上,引入了一种新的二维拟合程序,与广泛用于量化观测分布的主要属性的一维拟合方法相比,该程序具有更高的置信度。尤利西斯航天器测量的非线性最小二乘拟合\led{applied to electron data sets}证实了三个不同种群的存在,一个准热核心和两个超热(晕和斯特拉尔)成分。一般来说,最佳的总体拟合是由麦克斯韦分布和两个广义$\kappa$ -分布的和给出的。
Generalized anisotropic κ-cookbook: 2D fitting of Ulysses electron data
Observations in space plasmas reveal particle velocity distributions out of thermal equilibrium, with anisotropies (e.g., parallel drifts or/and different temperatures, $T_\parallel$ - parallel and $T_\perp$ - perpendicular, with respect to the background magnetic field), and multiple quasithermal and suprathermal populations with different properties. The recently introduced (isotropic) $\kappa$-cookbook is generalized in the present paper to cover all these cases of anisotropic and multi-component distributions reported by the observations. We derive general analytical expressions for the velocity moments and show that the common (bi-)Maxwellian and (bi-)$\kappa-$distributions are obtained as limiting cases of the generalized anisotropic $\kappa$-cookbook (or recipes). Based on this generalization, a new 2D fitting procedure is introduced, with an improved level of confidence compared to the 1D fitting methods widely used to quantify the main properties of the observed distributions. The nonlinear least-squares fit is \led{applied to electron data sets} measured by the Ulysses spacecraft confirming the existence of three different populations, a quasithermal core and two suprathermal (halo and strahl) components. In general, the best overall fit is given by the sum of a Maxwellian and two generalized $\kappa$-distributions.