Time-dependent tomographic reconstruction of the coronal electron density from 18 years of LASCO-C2

来源 :The Fourteenth International Solar Wind Conference (第十四届国际太阳 | 被引量 : 0次 | 上传用户：xutao6310794

【摘要】

：

【作者】

：

Lamy P. Vibert D. de Patoul J. Wojak J. Frazin R. Peillon C.

【机构】

：

Laboratoire d'Astrophysique de Marseille,CNRS/Aix-Marseille Université,France

【出处】

：

The Fourteenth International Solar Wind Conference (第十四届国际太阳

【发表日期】

：

2015年5期

下载到本地 , 更方便阅读

下载此文赞助VIP

声明 : 本文档内容版权归属内容提供方 , 如果您对本文有版权争议 , 可与客服联系进行内容授权或下架

论文部分内容阅读

Progress in understanding the physics of the corona and the solar wind depends upon the 3D-dimensionaldistributions of the plasma properties such as temperature,density and magnetic field in the solar corona.Solar rotational tomography(SRT) uses coronal images observed at multiple aspect angles provided by solar rotation to provide 3D reconstructions of the corona.

其他文献

The physics of the transition range:spacecraft observations and the 3D FLR-Landau-fluid simulations

The transition range of solar wind turbulence is the range of scales close to the ion gyroscale kρi～1,where turbulence properties undergo significant changes:turbulence becomes dispersive and kinetic

会议

The composition of solar wind turbulence near the spectral break:Processes and instabilities at kine

High speed streams are often characterized by a core proton temperature anisotropy such that Tp⊥＞Tp‖ and by a minority population of alpha particles such that(v)α‖＞(v)p‖,where(v)‖ is the component of

会议

Kinetic slow-mode waves in the solar wind and their possible role in turbulence dissipation and ion

The solar wind is permeated by all kinds of fluctuations ranging broadly inscales from those of the solar corona and inner heliosphere down to the local ionand electron plasma kinetic scales.

会议

Solar wind turbulent fluctuations at kinetic scales and their polarization:from coherent structures

The nature of the magnetic field fluctuations in the solar wind between the ion and electron scales is still under debate.

会议

Spectral Features of Magnetic Fluctuations around the Frequency Boundary Between Fluid and Kinetic R

We describe the spectral features of magnetic field fluctuations at scales located right after the break that marks the beginning of the kinetic regime.

会议

New insights into the properties and evolution of Solar Wind Electrons

We present a comprehensive statistical analysis of solar wind electrons using the electron analyzers of the 3D-Plasma instrument on the Wind spacecraft.

会议

First High-resolution Spectroscopic Observations of an Erupting Prominence Within a Coronal Mass Eje

Prominence eruptions associated with coronal mass ejections(CMEs) are among the origins of the transient solar wind disturbances.Spectroscopic observations of such eruptions,although relatively rare,c

会议

Dissipation and reconnection in boundary-driven reduced magnetohydrodynamics

Turbulence and magnetic reconnection are two fundamental processes that are critical for many laboratory,space,and astrophysical phenomena.

会议

High-resolution imaging of the solar wind source region:statistical study of the prevalent microjets

Recent IRIS observations revealed prevalence of intermittent small scale jets with apparent speeds of 80-250 km/s emanating from small-scale bright regions inside network boundaries of coronal holes(T

会议

Analysis of the energy spectral structure versus the different phases of a CME-driven shock

We will do simulations to show how the "break" energy spectra are formed in the CME-driven shock.Multiple spacecraft observations show a "break" at the energy range of 1-10MeV of proton energy spectra

会议

Time-dependent tomographic reconstruction of the coronal electron density from 18 years of LASCO-C2

与本文相关的学术论文