基于先前CPI多维数据的天基雷达信号处理算法

为了消除单站天基雷达非稳态杂波图景的影响,讨论一种利用先前CPI（Coherent Processi     

Creating a space exploration industry

The article provides an overview of funding for space exploration to the Moon and Mars under NASA's direction, and presents an argument for the creation of a commercial space industry.     

Simulations of the microwave sky and of its “observations”

Here follows a preliminary report on the construction of fake millimeter and sub-millimeter skies, as observed by virtual instruments,e.g. the COBRA/SAMBA mission, using theoretical modeling and data extrapolations. Our goal is to create maps as realistic as possible of the relavant physical contributions which may contribute to the detected signals. This astrophysical modeling is followed by simulations of the measurement process itself by a given instrumental configuration. This will enable a precise determination of what can and cannot be achieved with a particular experimental configuration, and provide a feedback on how to improve the overall design. It is a key step on the way to define procedures for the separation of the different physical processes in the future observed maps. Note that this tool will also prove useful in preparing and analyzing current (e.g. balloon borne) Microwave Background experiments.     

Gamma-ray pulsars in the MeV region

Space Science Reviews - Most models for the magnetosphere of pulsars assume ultrarelativistic primary particles streaming along the field lines; the resulting curvature photons can initiate...     

CME dynamics using coronagraph and interplanetary ejecta data

In this work, we present a study of the coronal mass ejection (CME) dynamics using LASCO coronagraph observations combined with in-situ ACE plasma and magnetic field data, covering a continuous period of time from January 1997 to April 2001, complemented by few extreme events observed in 2001 and 2003. We show, for the first time, that the CME expansion speed correlates very well with the travel time to 1 AU of the interplanetary ejecta (or ICMEs) associated with the CMEs, as well as with their preceding shocks. The events analyzed in this work are a subset of the events studied in Schwenn et al. (2005), from which only the CMEs associated with interplanetary ejecta (ICMEs) were selected. Three models to predict CME travel time to Earth, two proposed by Gopalswamy et al. (2001) and one by Schwenn et al. (2005), were used to characterize the dynamical behavior of this set of events. Extreme events occurred in 2001 and 2003 were used to test the prediction capability of the models regarding CMEs with very high LASCO C3 speeds.     

航天器火工冲击环境数据外推技术研究

为了制定可靠的组件冲击试验条件,需要预示航天器火工冲击环境.在分析了航天器火工冲击环境预示的三类方法,包括试验法、数值分析法和数据外推法的基础上,详细总结和分析了数据外推法的国内外研究进展,并通过理论推导提出了新的数据外推公式;以大量火工冲击测量数据为参照,通过对比分析证明该数据外推公式比NASA和ESA的数据外推公式...