空间物理中的若干前沿科学问题

作者简介

《空间物理中的若干前沿科学问题》的集结出版是为了庆祝中国科学技术大学50周年华诞,所选论文的第一作者均为中国科学技术大学的毕业生校友。反映了这些校友在空间物理各个研究领域中的最新成就。

《空间物理中的若干前沿科学问题》共分为两部分,每一部分开头都有导言,然后是相关论文。第一部分涉及太阳及行星际物理,包括日冕和太阳风加热、日冕物质抛射及其行星际演化等。第二部分涉及磁层物理,包括地球?行星磁层中的一些物理过程。每一部分均包含理论和观测方面的文章。

《空间物理中的若干前沿科学问题》可供空间物理、太阳物理、等离子体物理及相关专业的本科生、研究生以及科研人员阅读。

书籍目录

Preface to the USTC Alumni's Series
Preface
Part One Solar and Heliospheric Physics
 Introduction
 A fast solar wind model with anisotropic proton
temperature
 On the cascade processes of Alfven waves in the
fast solar wind
 Transition region, coronal heating and the fast
solar wind
 A global 2.5-dimensional three fluid solar wind
model with alpha particles
 Ion pickup by finite amplitude parallel
propagating Alfvcn waves
 Formation of minor-ion charge states in the fast
solar wind: Roles of differential flow speeds of ions of the same
element
 Stagnated outflow of O+5 ions in the source
region of the slow solar wind at solar minimum
 On the outflow in an equatorial coronal
hole
 Time series study of EUV spicules observed by
SUMER/SOHO
 Heating of ions by Alfven waves via nonresonant
interactions
 RHESSI observation of chromospheric
evaporation
 RHESSI hard X-ray imaging spectroscopy of
extended sources and the physical properties of electron
acceleration regions in solar flares
 Equilibrium and catastrophe of coronal flux
ropes in axisymmetrical magnetic field
 A new non-pressure-balanced structure in
interplanetary space: Boundary layers of magnetic clouds
 Global distribution of coronal mass outputs and
its relation to solar magnetic field structures
 Identification of the magnetic cloud boundary
layers
 Magnetic structures inside boundary layers of
magnetic clouds
 Characteristics of the interplanetary coronal
mass ejections in the heliosphere between 0.3 and 5.4 AU
 Development of a strong shock in the outer
heliosphere
 Reconstruction of magnetic flux ropes in the
solar wind
 Multiple flux rope magnetic ejecta in the solar
wind :
 Multiple magnetic clouds. Several examples
during March - April 2001
Part Two Magnetospheric Physics
 Introduction
 On the ionospheric and reconnection potentials
of the earth. Results from global MHD simulations
 Electromagnetic waves downstream of
quasi-perpendicular shocks
 Magnetic spectral signatures in the terrestrial
plasma depletion layer. Hybrid simulations
 Whistler wave instabilities in collisionless
current sheet
 Joint observations by Cluster satellites of
bursty bulk flows in the magnetotail
 Variations of 0.7 - 6.0 MeV electrons at
geosynchronous orbit as a function of solar wind
 Correlation between the inner edge of outer
radiation belt electrons and the innermost plasmapause
location
 Whistler instability threshold condition of
energetic electrons by kappa distribution in space plasmas
 Relativistic diffusion coefficients for
superluminous (auroral kilometric radiation) wave modes in space
plasmas
 Polar cap arcs. a review
 Diurnal tides in mesosphere/low-thermosphere
(MLT) during 2002 at Wuhan (30.6°N, 114.4°E) using Canonical
Correlation Analysis
 Response of the magnetic field in the
geosynchronous orbit to solar wind dynamic pressure pulses
 Nongyrotropy of heavy newborn ions at comet
Grigg-Skjellerup and corresponding instability
 Three-dimensional, multispecies, high spatial
resolution MHD studies of the solar wind interaction with
Mars
 Comparisons between MHD model calculations and
observations of Cassini flybys of Titan

编辑推荐

《空间物理中的若干前沿科学问题》：当代科学技术基础理论与前沿问题研究丛书·中国科学技术大学校友文库。

内容概要

陆全明，中国科学技术大学长江学者特聘教授，博士生导师。1990年本科毕业于南京大学，1996年7月在中国科学技术大学获得博士学位，随后到中国科学院上海光学与精密机械研究所和日本筑波大学做博士后研究。2000年到中国科学技术大学地球和空间科学系任教，2004年被聘为教授。主要从事空间等离子体物理和粒子模拟高性能计算的研究工作，已在国内外期刊上发表论文80余篇。2005年入选教育部新世纪优秀人才支持计划，2006年获中国地球物理学会傅承义青年科技奖，2007年获国家自然科学基金委杰出青年基金资助，同年获中国青年科技奖，2009年入选“新世纪百千万人才工程”国家级人选，20t0年获聘为教育部长江学者特聘教授。王赤，中国科学院空间科学与应用研究中心副主任，研究员，博士生导师，空间天气学国家重点实验室主任。1990年本科毕业于中国科学技术大学地球和空间科学系，1998年美国麻省理工学院博士毕业后留校做博士后研究，2000年晋升为研究科学家。2001年作为中国科学院“百人计划”学者回国工作，2003年获国家自然科学基金委杰出青年基金资助，2004年获中国科学院“创新团队和国际合作伙伴计划”支持（团队负责人），2006d~国家基金委创新研究群体科学基金支持（群体负责人）。2005年担任“十一五”国家重大科技基础设施“东半球空间环境地基综合监测子午链”项目总工程师。2000年来以第一作者或合作者在国际重要学术刊物Nature、JGR、GRL上发表论文80余篇。荣获2003年全国留学归国人员先进个人、2006年中国青年科技奖、2006年“新世纪百千万人才工程”国家级人才。

章节摘录

版权页：插图：[46] The interest in ion cyclotron resonance as a mechanism to account for thetemperature anisotropy of protons and minor ions in the inner corona has been spurredby the recent ultraviolet spectral line observations in the corona by UVCS on SOHO Kohl et al, 1998, Li et al. 1998; Cranmer et al. , 1999]. However, a self-consistent approach considering the evolution of the spectrum of Alfv6n waves in theinner corona out to interplanetary space, together with the evolution of the solar wind,does not exist at present. This study is the first attempt at such a self-consistent approach.[47] In this paper we developed a numerical method which solves the electron-proton solar wind and Alfv6n wave spectrum equations simultaneously with high accuracyand efficiency. Using this technique, the radial evolution of the solar wind and the Alfv6nwave spectrum can be determined self-consistently for an arbitrarily prescribed tem-perature, density, and Alfvn wave spectrum at the coronal base. Given this approach,we investigate the nonlinear cascade effect on the heating and acceleration of the fastsolar wind and the radial evolution of the Alfv6n wave spectrum. For the first time, thecascade effect and the evolution of the Alfv+nic spectrum from the coronal base to 1 AUare investigated in a self-consistent manner. The processes described by the Kolmogorov and the Kraichnan cascade functions are tested.

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