空間物理中的若干前沿科學(xué)問題

出版時(shí)間:2011-1  出版社:中國(guó)科學(xué)技術(shù)大學(xué)出版社  作者:陸全明,王赤 主編  頁數(shù):663  
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內(nèi)容概要

《空間物理中的若干前沿科學(xué)問題》的集結(jié)出版是為了慶祝中國(guó)科學(xué)技術(shù)大學(xué)50周年華誕,所選論文的第一作者均為中國(guó)科學(xué)技術(shù)大學(xué)的畢業(yè)生校友。反映了這些校友在空間物理各個(gè)研究領(lǐng)域中的最新成就。
《空間物理中的若干前沿科學(xué)問題》共分為兩部分,每一部分開頭都有導(dǎo)言,然后是相關(guān)論文。第一部分涉及太陽及行星際物理,包括日冕和太陽風(fēng)加熱、日冕物質(zhì)拋射及其行星際演化等。第二部分涉及磁層物理,包括地球?行星磁層中的一些物理過程。每一部分均包含理論和觀測(cè)方面的文章。
本書可供空間物理、太陽物理、等離子體物理及相關(guān)專業(yè)的本科生、研究生以及科研人員閱讀。

作者簡(jiǎn)介

陸全明,中國(guó)科學(xué)技術(shù)大學(xué)長(zhǎng)江學(xué)者特聘教授,博士生導(dǎo)師。1990年本科畢業(yè)于南京大學(xué),1996年7月在中國(guó)科學(xué)技術(shù)大學(xué)獲得博士學(xué)位,隨后到中國(guó)科學(xué)院上海光學(xué)與精密機(jī)械研究所和日本筑波大學(xué)做博士后研究。2000年到中國(guó)科學(xué)技術(shù)大學(xué)地球和空間科學(xué)系任教,2004年被聘為教授。主要從事空間等離子體物理和粒子模擬高性能計(jì)算的研究工作,已在國(guó)內(nèi)外期刊上發(fā)表論文80余篇。2005年入選教育部新世紀(jì)優(yōu)秀人才支持計(jì)劃,2006年獲中國(guó)地球物理學(xué)會(huì)傅承義青年科技獎(jiǎng),2007年獲國(guó)家自然科學(xué)基金委杰出青年基金資助,同年獲中國(guó)青年科技獎(jiǎng),2009年入選“新世紀(jì)百千萬人才工程”國(guó)家級(jí)人選,20t0年獲聘為教育部長(zhǎng)江學(xué)者特聘教授。王赤,中國(guó)科學(xué)院空間科學(xué)與應(yīng)用研究中心副主任,研究員,博士生導(dǎo)師,空間天氣學(xué)國(guó)家重點(diǎn)實(shí)驗(yàn)室主任。1990年本科畢業(yè)于中國(guó)科學(xué)技術(shù)大學(xué)地球和空間科學(xué)系,1998年美國(guó)麻省理工學(xué)院博士畢業(yè)后留校做博士后研究,2000年晉升為研究科學(xué)家。2001年作為中國(guó)科學(xué)院“百人計(jì)劃”學(xué)者回國(guó)工作,2003年獲國(guó)家自然科學(xué)基金委杰出青年基金資助,2004年獲中國(guó)科學(xué)院“創(chuàng)新團(tuán)隊(duì)和國(guó)際合作伙伴計(jì)劃”支持(團(tuán)隊(duì)負(fù)責(zé)人),2006d~國(guó)家基金委創(chuàng)新研究群體科學(xué)基金支持(群體負(fù)責(zé)人)。2005年擔(dān)任“十一五”國(guó)家重大科技基礎(chǔ)設(shè)施“東半球空間環(huán)境地基綜合監(jiān)測(cè)子午鏈”項(xiàng)目總工程師。2000年來以第一作者或合作者在國(guó)際重要學(xué)術(shù)刊物Nature、JGR、GRL上發(fā)表論文80余篇。榮獲2003年全國(guó)留學(xué)歸國(guó)人員先進(jìn)個(gè)人、2006年中國(guó)青年科技獎(jiǎng)、2006年“新世紀(jì)百千萬人才工程”國(guó)家級(jí)人才。

書籍目錄

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

章節(jié)摘錄

版權(quán)頁:插圖:[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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《空間物理中的若干前沿科學(xué)問題》:當(dāng)代科學(xué)技術(shù)基礎(chǔ)理論與前沿問題研究叢書·中國(guó)科學(xué)技術(shù)大學(xué)校友文庫。

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