排序方式: 共有17条查询结果,搜索用时 234 毫秒
11.
Cord-Christian ROSSOW Norbert KROLL Dieter SCHWAMBORN 《中国航空学报》2006,19(2):134-150
德国在若干年前启动的国家CFD项目MEGAFLOW集中了DLR、大学以及航空工业界的许多CFD研究开发工作,目的是开发并验证能满足工业实践所要求的可靠并有效的数值工具,以对全机进行空气动力模拟.MEGAFLOW软件系统包括多区结构网格中求解N-S方程的软件FLOWer和在非结构网格中的软件TAU.两软件均已达到很高的成熟度并为DLR和德国航空工业广泛地应用于新飞机的设计过程.最近又启动了其后续项目MEGADESIGN和MegaOpt,旨在开发和增强外形设计及优化的有效数值方法.着重介绍了软件最近的改进及其计算粘性流动绕复杂飞机外形的能力. 相似文献
12.
I. Kutiev P. Marinov A. Belehaki B. Reinisch N. Jakowski 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
To improve the accuracy of the real time topside electron density profiles given by the Digisonde software a new model-assisted technique is used. This technique uses the Topside Sounder Model (TSM), which provides the plasma scale height (Hs), O+–H+ transition height (HT), and their ratio Rt = Hs/HT, derived from topside sounder data of Alouette and ISIS satellites. The Topside Sounder Model Profiler (TSMP) incorporates TSM and uses the model quantities as anchor points in construction of topside density (Ne) profiles. For any particular location, TSMP calculates topside Ne profiles by specifying the values of foF2 and hmF2. In the present version, TSMP takes the F2 peak characteristics – foF2, hmF2, and the scale height at hmF2 – from the Digisonde measurements. The paper shows results for the Digisonde stations Athens and Juliusruh. It is found that the topside scale height used in Digisonde reconstruction is less than that extracted from topside sounder profiles. Rough comparison of their bulk distributions showed that they differ by an average factor of 1.25 for locations of Athens and Juliusruh. When the Digisonde scale heights are adjusted by this factor, the reconstructed topside profiles are close to those provided by TSM. Compared with CHAMP reconstruction profiles in two cases, TSMP/Digisonde profiles show lower density between 400 and 2000 km. 相似文献
13.
Tilman Spohn Karsten Seiferlin Axel Hagermann Jörg Knollenberg Andrew J. Ball Marek Banaszkiewicz Johannes Benkhoff Stanislaw Gadomski Wojciech Gregorczyk Jerzy Grygorczuk Marek Hlond Günter Kargl Ekkehard Kührt Norbert Kömle Jacek Krasowski Wojciech Marczewski John C. Zarnecki 《Space Science Reviews》2007,128(1-4):339-362
MUPUS, the multi purpose sensor package onboard the Rosetta lander Philae, will measure the energy balance and the physical parameters in the near-surface layers – up to about 30 cm depth- of the
nucleus of Rosetta’s target comet Churyumov-Gerasimenko. Moreover it will monitor changes in these parameters over time as
the comet approaches the sun. Among the parameters studied are the density, the porosity, cohesion, the thermal diffusivity
and conductivity, and temperature. The data should increase our knowledge of how comets work, and how the coma gases form.
The data may also be used to constrain the microstructure of the nucleus material. Changes with time of physical properties
will reveal timescales and possibly the nature of processes that modify the material close to the surface. Thereby, the data
will indicate how pristine cometary matter sampled and analysed by other experiments on Philae really is. 相似文献
14.
M. Mainul Hoque N. Jakowski 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
With the increasing number of remote sensing satellites using the GPS radio occultation technique for atmospheric sounding, the estimation of higher order ionospheric effects and their mitigation have become relevant and important. Due to long ionospheric limb paths, GPS signals are strongly affected by ionospheric refraction during radio occultation. Standard dual-frequency GPS measurements may be used to estimate the first order term of the refractive index. However, non-linear terms such as the second and third order ionospheric terms and ray path bending effects are not considered in occultation measurements so far. Analysing selected CHAMP–GPS occultation events different higher order ionospheric terms are estimated and their effects on dual-frequency range estimation and total electron content (TEC) estimation are discussed. We have found that the separation between the GPS L1 and L2 ray paths exceeds the kilometer level during occultation for a vertical TEC level of more than 160 TEC units. Corresponding errors in the GPS dual-frequency range estimation and TEC estimation are found to exceed the meter and 10 TEC units level, respectively. 相似文献
15.
Claudia Borries Volker Wilken Knut Stanley Jacobsen Alberto García-Rigo Beata Dziak-Jankowska Guram Kervalishvili Norbert Jakowski Ioanna Tsagouri Manuel Hernández-Pajares Arthur A. Ferreira Mainul M. Hoque 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(2):919-920
16.
17.
Samaneh Sadighi P.T. Jayachandran N. Jakowski J.W. MacDougall 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009,44(11):1304-1308
In this paper we present the results of the comparison of the retrieved electron density profiles of the Ionospheric Radio Occultation (IRO) experiment on board CHAMP (CHAllenging Minisatellite Payload), with the ground ionosonde profiles for the Polar Regions. IRO retrieved electron density profiles from CHAMP are compared with Canadian Advanced Digital Ionosonde (CADI) measurements at two vertical sounding stations well within the Polar Cap, Eureka (geog. 80°13′ N; 86°11′ W) and Resolute Bay (geog. 74°41′ N; 94°54′ W). We compared the ionospheric parameters such as the peak electron density of the F-layer (NmF2) and the peak height of the F-layer (hmF2) for a 3-year period, 2004–2006. CHAMP derived NmF2 shows reasonable agreement with the ionosonde retrieved NmF2 for both the stations (0.76 and 0.71 correlation coefficient, for Eureka and Resolute Bay, respectively) whereas the hmF2 agreement is not that acceptable (0.25 and 0.37 correlation coefficient, respectively). The hmF2 from vertical sounding showed less spread than the CHAMP hmF2. 相似文献