About shape of the interplanetary shock front

机译：关于行星际激波前锋的形状

获取原文

获取原文并翻译 | 示例

页面导航

摘要
著录项
相似文献
相关主题

摘要

The method of the interplanetary shock front shape determination has been developed. Weak large-scale asymmetry of the front has been revealed for two sets of the vector-normal to front components obtained from data of ACE experiment during from 1998 to 2003 years (199 measurements) and from 1998 to 2008 years (257 measurements). Axial symmetric shape of the front has been determined. It agrees in general with one calculated in the magneto-hydrodynamic approximation for conditions of the solar wind. Statistical method of the determination of a surface shape using set of the vector-normal to surface has been established.

机译：已经开发出行星际激波前形确定方法。从1998年至2003年（199个测量值）和1998年至2008年（257个测量值）的ACE实验数据获得的两组矢量法线到前部分量已显示出弱的大规模前部不对称性。前面的轴对称形状已确定。通常，它与用磁流体动力近似法计算的太阳风条件一致。已经建立了使用与表面正交的向量确定表面形状的统计方法。

著录项

来源
《Proceedings of the 32nd International Cosmic Ray Conference》|2011年|1-4|共4页
会议地点 Beijing(CN)
作者
PETUKHOV IVAN; PETUKHOV STANISLAV;
展开▼
作者单位

Institute of Cosmophysical Research and Aeronomy SB RAS;

Institute of Cosmophysical Research and Aeronomy SB RAS;

展开▼
会议组织
原文格式 PDF
正文语种 eng
中图分类宇宙射线强度变化;
关键词
Interplanetary shock front, vector-normal to front;

机译：行星际激波前，矢量法向前;

相似文献

外文文献
中文文献
专利

1. Mean shape of interplanetary shocks deduced from in situ observations and its relation with interplanetary CMEs [J] . M. Janvier, P. Démoulin, S. Dasso Astronomy and astrophysics . 2014,第19期

机译：由原位观测推导的行星际激波的平均形状及其与行星际CME的关系
2. Fine Structure of Interplanetary Shock Front-Results from BMSW Experiment with High Time Resolution [J] . N.L. Borodkova, V.G. Eselevich, G.N. Zastenker, Journal of Geophysical Research, A. Space Physics: JGR . 2019,第11期

机译：BMSW实验的白际休克前线的精细结构，具有高时间分辨率
3. Substorm Activity and Orientation of the Front of a Shock Wave of an Interplanetary Magnetic Cloud [J] . Barkhatov N. A., Vorobjev V. G., Revunov S. E., Geomagnetism and aeronomy . 2019,第4期

机译：跨境磁云冲击波前面的替代活动和方向
4. About shape of the interplanetary shock front [C] . PETUKHOV IVAN, PETUKHOV STANISLAV International Cosmic Ray Conference . 2011

机译：关于行星际震动前线的形状
5. A study of interplanetary shock geoeffectiveness controlled by impact angles using simulations and observations [D] . Oliveira, Denny M. 2015

机译：利用模拟和观测研究冲击角控制的行星际冲击地球效应
6. Front packs: is 15 safe? Evaluation of the effect of different front pack loads on 3D back shape and posture in asymptomatic young adults [O] . RS Moulstone, Josette Bettany-Saltikov 2010

机译：前包：15％安全吗？评估无症状年轻人中不同前背包负重对3D背部形状和姿势的影响
7. Structure on Interplanetary Shock Fronts: Type II Radio Burst Source Regions [O] . M. Pulupa, S. D. Bale 2008

机译：行星际激波前沿的结构：II型无线电突发源区
8. Increases in the low energy cosmic ray intensity at the front of propagating interplanetary shock waves [R] . Fisk, L. A. 1970

机译：传播的行星际冲击波前方的低能宇宙射线强度增加

About shape of the interplanetary shock front

摘要

著录项

相似文献

相关主题

期刊订阅