空間物理中的若干前沿科學問題

內容概要

《空間物理中的若干前沿科學問題》的集結出版是為了慶祝中國科學技術大學50周年華誕，所選論文的第一作者均為中國科學技術大學的畢業(yè)生校友。反映了這些校友在空間物理各個研究領域中的最新成就。
《空間物理中的若干前沿科學問題》共分為兩部分，每一部分開頭都有導言，然后是相關論文。第一部分涉及太陽及行星際物理，包括日冕和太陽風加熱、日冕物質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專業(yè)的本科生、研究生以及科研人員閱讀。

作者簡介

陸全明，中國科學技術大學長江學者特聘教授，博士生導師。1990年本科畢業(yè)于南京大學，1996年7月在中國科學技術大學獲得博士學位，隨后到中國科學院上海光學與精密機械研究所和日本筑波大學做博士后研究。2000年到中國科學技術大學地球和空間科學系任教，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算的研究工作，已在國內外期刊上發(fā)表論文80余篇。2005年入選教育部新世紀優(yōu)秀人才支持計劃，2006年獲中國地球物理學會傅承義青年科技獎，2007年獲國家自然科學基金委杰出青年基金資助，同年獲中國青年科技獎，2009年入選“新世紀百千萬人才工程”國家級人選，20t0年獲聘為教育部長江學者特聘教授。王赤，中國科學院空間科學與應用研究中心副主任，研究員，博士生導師，空間天氣學國家重點實驗室主任。1990年本科畢業(yè)于中國科學技術大學地球和空間科學系，1998年美國麻省理工學院博士畢業(yè)后留校做博士后研究，2000年晉升為研究科學家。2001年作為中國科學院“百人計劃”學者回國工作，2003年獲國家自然科學基金委杰出青年基金資助，2004年獲中國科學院“創(chuàng)新團隊和國際合作伙伴計劃”支持（團隊負責人），2006d~國家基金委創(chuàng)新研究群體科學基金支持（群體負責人）。2005年擔任“十一五”國家重大科技基礎設施“東半球空間環(huán)境地基綜合監(jiān)測子午鏈”項目總工程師。2000年來以第一作者或合作者在國際重要學術刊物Nature、JGR、GRL上發(fā)表論文80余篇。榮獲2003年全國留學歸國人員先進個人、2006年中國青年科技獎、2006年“新世紀百千萬人才工程”國家級人才。

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問題》：當代科學技術基礎理論與前沿問題研究叢書·中國科學技術大學校友文庫。

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