Spectroscopic observations of coronal waves and coronal mass ejections

It is common to use imaging instruments such as EUV and X-ray imagers and coronagraphs to study large-scale phenomena such as coronal mass ejections and coronal waves. Although high resolution spectroscopy is generally limited to a small field of view, its importance in understanding global phenomena should not be under-estimated. I will review current spectroscopic observations of large-scale dynamic phenomena such as global coronal waves and coronal mass ejections. The aim is to determine plasma parameters such as flows, temperatures and densities to obtain a physical understanding of these phenomena.     

准确理解在新社会阶层中发展党员的问题

理解发展新社会阶层中的优秀分子入党这一问题,对大学生来讲有两方面的难点：一是如何理解拥有大量财产的人入党的问题;二是如何理解存在剥削行为的人入党的问题。笔从这两方面入手,进行必要的探讨和研究。     

“孔教会”与“新孔学”——对康有为、梁漱溟儒学重构的省察

近代以来,中国思想文化界掀起了一场声势浩大的文化自救运动,康有为"孔教会"与梁漱溟"新孔学"是其杰出代表。康有为、梁漱溟基于不同的学术立场和价值观念,对传统儒学的近现代重建提出独到的见解。仔细省察康有为、梁漱溟对儒学传统的反思,对于我们探寻儒学的未来前景有直接的借鉴价值。     

我国发展新一代中远程宽体民用飞机之我见

根据新一代中远程宽体民用飞机的发展现状和未来发展方向,凝练了我国发展新一代中远程宽体民用飞机将具有战略意义的个人认识,同时在概括我国将要发展的新一代中远程宽体民用飞机的技术特征之后,针对性地提出了相关技术发展方向,最后为怎样发展该民机战略性新型产业提出了粗浅想法.     

Coronal Mass Ejections

This workshop summary tries to distill the key difficulties and questions in the art of (I)CME physics and strategies to address them. (I)CMEs are multi-dimensional, multi-parameter, and multi-scale phenomena related to the solar dynamo, corona, and heliosphere. This workshop illustrates the immense progress made in describing and modeling these spectacular energetic solar events, but also shows clear shortcomings in our understanding of them.     

Data Grids and High Energy Physics: A Melbourne Perspective

The University of Melbourne, Experimental Particle Physics group recognises that the future of computing is an important issue for the scientific community. It is in the nature of research for the questions posed to become more complex, requiring larger computing resources for each generation of experiment. As institutes and universities around the world increasingly pool their resources and work together to solve these questions, the need arises for more sophisticated computing techniques. One such technique, grid computing, is under investigation by many institutes across many disciplines and is the focus of much development in the computing community. ‘The Grid’, as it is commonly named, is heralded as the future of computing for research, education, and industry alike. This paper will introduce the basic concepts of grid technologies including the Globus toolkit and data grids as of July 2002. It will highlight the challenges faced in developing appropriate resource brokers and schedulers, and will look at the future of grids within high energy physics. This revised version was published online in August 2006 with corrections to the Cover Date.     

The case for massive,evolving winds in black hole X-ray binaries

In the last decade, high-resolution X-ray spectroscopy has revolutionized our understanding of the role of accretion disk winds in black hole X-ray binaries. Here I present a brief review of the state of wind studies in black hole X-ray binaries, focusing on recent arguments that disk winds are not only extremely massive, but also highly variable. I show how new and archival observations at high timing and spectral resolution continue to highlight the intricate links between the inner accretion flow, relativistic jets, and accretion disk winds. Finally, I discuss methods to infer the driving mechanisms of observed disk winds and their implications for connections between mass accretion and ejection processes.     

Testing Modified Newtonian Dynamics with LISA Pathfinder

We suggest that LISA Pathfinder, a technology demonstrator for the future gravitational wave observatory LISA, could be used to carry out a direct experimental test of Modified Newtonian Dynamics (MOND). The LISA Pathfinder spacecraft is currently being built and the launch date is just a few years away. No modifications of the spacecraft are required, nor any interference with its nominal mission. The basic concept is to fly LISA Pathfinder through the region around the Sun-Earth saddle point, in an extended mission phase, once the original mission goals are achieved. We examine various strategies to reach the saddle point, and find that the preferred strategy, yielding relatively short transfer times of just over 1 year, probably involves a lunar fly-by. LISA Pathfinder will be able to probe the intermediate MOND regime, i.e. the transition between deep MOND and Newtonian gravity. We present robust estimates of the anomalous gravity gradients that LISA Pathfinder should be exposed to, based on MONDian effects as derived from the Tensor-Vector-Scalar (TeVeS) theory. The spacecraft speed and spatial scale of the MOND signal combine in a way that the spectral signature of the signal falls precisely into LISA Pathfinder’s measurement bandwidth. We find that if the gravity gradiometer on-board the spacecraft achieves its currently predicted sensitivity, these anomalous gradients could not just be detected, but measured in some detail.     

Dark Matter searches with GLAST

The Gamma-ray Large Area Space Telescope (GLAST), scheduled to be launched in fall 2007, is the next generation satellite for high-energy gamma-ray astronomy. The Large Area Telescope (LAT), GLAST main instrument, with a wide field of view (>2 sr), a large effective area (>8000 cm² at 1 GeV) and 20 MeV–300 GeV energy range, will provide excellent high energy gamma-ray observations for Dark Matter searches. In this paper we examine the potential of the LAT to detect gamma-rays coming from WIMPS annihilation in the context of supersymmetry. As an example, two search regions are investigated: the galactic center and the galactic satellites.