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411.
412.
First magnetospheric measurements of the three-dimensional velocity distributions for positive ions and electrons within the energy range 1 eV E/Q 45keV are reported. These velocity distributions are gained with quadrispherical Lepedeas on board the spacecraft ISEE-1 and -2. Three-dimensional bulk flows of protons in the vicinity of the magnetopause and within the dayside magnetosphere and dawn sector of the magnetotail are presented. Proton drift velocities within the magnetosphere and magnetotail can be directly determined and employed to calculate the corresponding quasi-static perpendicular electric fields and to provide quantitative analyses of kinematical models for plasma motions. Nonmonotonic features in the electron velocity distributions are found simultaneously with the presence of electron cyclotron harmonic electrostatic waves in the dayside magnetosphere. The relationship of the observed electron velocity distributions to expectations for resonant pitch-angle and energy diffusion is discussed, as well as the possibility of the existence of proton cyclotron harmonic instabilities. Examples of the signature of field-aligned acceleration of protons into the magnetosphere and the presence of low-energy ionospheric ions in the near-earth magnetotail are also presented. Perpendicular electrostatic fields can be calculated from the observed three-dimensional velocity distributions and are found to have typical magnitudes of 1 mV m-1. 相似文献
413.
414.
椭圆外切2n+1边形中切顶线三角形有向面积的定值定理及其应用 总被引:2,自引:0,他引:2
喻德生 《南昌航空工业学院学报》2003,17(1):10-12
本文给出椭圆外切2n 1边形中一类切顶线三角形有向面积的一个定值定理及其若干推论,其中包括射影几何中著名的Brisanchon定理在椭圆外切三角形中的情形。 相似文献
415.
A. Lange P. De Bernardis M. De Petris S. Masi F. Melchiorri E. Aquilini L. Martinis F. Scaramuzzi B. Melchiorri A. Boscaleri G. Romeo J. Bock Z. Chen M. Devlin M. Gervasi V. Hristov P. Mauskopf D. Osgood P. Richards P. Ade M. Griffin 《Space Science Reviews》1995,74(1-2):145-150
The BOOMERANG (Balloon Observations Of Millimetric Extragalactic RAdiation aNd Geophysics) experiment is an international effort to measure the Cosmic Microwave Background (CMB) anisotropy on angular scales of 20 to 4°, with unprecedented sensitivity, sky and spectral coverage. The telescope will be flown from Antarctica by NASA-NSBF with a long duration stratospheric balloon (7–14 days), and is presently scheduled for flight in 1995–1996. The experiment is designed to produce an image of the Cosmic Microwave Background with high sensitivity and large sky coverage. These data will tightly constrain the baryon density, the reionization history, and the formation of large-scale structure in the universe. BOOMERANG will test technologies and return science data that are essential to the design of a future space-borne mission to map CMB anisotropy. 相似文献
416.
Authors Index
Author Index 相似文献417.
G. A. Marzo A. Blanco F. De Carlo M. DElia S. Fonti A. C. Marra V. Orofino R. Politi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,33(12):2246-2251
Various indications seem to suggest that in the past the Martian climate allowed the presence of liquid water on the surface of the planet. It is therefore reasonable to think that bodies of standing water were once present in basins such as craters or depressions and that evaporite deposits of sulfates could have formed in these basins. The identification of such deposits, which might have survived in some regions of the planet, could confirm the present hypothesis about the ancient climate on Mars. Recent analyses of Mars spectra, obtained by ground-based observations, show bands consistent with sulfate features. If such data have to be interpreted with the aid of synthetic spectra, the knowledge of the complex refractive index of some sulfate is necessary. In this work we present the optical constants of submicron particles of gypsum (a typical hydrate–sulfate very common on Earth), derived by means of the dispersion theory from transmission spectra. We have performed the calculation of the optical constants in the wavelength range 2–70 μm, also in view of the wide spectral range covered by the Planetary Fourier Spectrometer (PFS) on board of the ESA space mission Mars Express. The data have been compared with optical constants obtained by other authors from reflectance measurements of particulate samples. 相似文献
418.
F Ballarini M Biaggi L De Biaggi A Ferrari A Ottolenghi A Panzarasa H G Paretzke M Pelliccioni P Sala D Scannicchio M Zankl 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(6):1338-1346
Distributions of absorbed dose and DNA clustered damage yields in various organs and tissues following the October 1989 solar particle event (SPE) were calculated by coupling the FLUKA Monte Carlo transport code with two anthropomorphic phantoms (a mathematical model and a voxel model), with the main aim of quantifying the role of the shielding features in modulating organ doses. The phantoms, which were assumed to be in deep space, were inserted into a shielding box of variable thickness and material and were irradiated with the proton spectra of the October 1989 event. Average numbers of DNA lesions per cell in different organs were calculated by adopting a technique already tested in previous works, consisting of integrating into "condensed-history" Monte Carlo transport codes--such as FLUKA--yields of radiobiological damage, either calculated with "event-by-event" track structure simulations, or taken from experimental works available in the literature. More specifically, the yields of "Complex Lesions" (or "CL", defined and calculated as a clustered DNA damage in a previous work) per unit dose and DNA mass (CL Gy-1 Da-1) due to the various beam components, including those derived from nuclear interactions with the shielding and the human body, were integrated in FLUKA. This provided spatial distributions of CL/cell yields in different organs, as well as distributions of absorbed doses. The contributions of primary protons and secondary hadrons were calculated separately, and the simulations were repeated for values of Al shielding thickness ranging between 1 and 20 g/cm2. Slight differences were found between the two phantom types. Skin and eye lenses were found to receive larger doses with respect to internal organs; however, shielding was more effective for skin and lenses. Secondary particles arising from nuclear interactions were found to have a minor role, although their relative contribution was found to be larger for the Complex Lesions than for the absorbed dose, due to their higher LET and thus higher biological effectiveness. 相似文献
419.
结构非线性对颤振特性的影响 总被引:1,自引:1,他引:1
基于描述函数法,对操纵系统的结构非线性问题,提出了用于描述函数法的耦合模态和非耦合的综合计算模型,使用跨音速非定常空气动力,对扑动间隙和旋转间隙进行研究,揭示了全动水平尾翼振动的根源主要是操纵间隙造成的,为其它同类问题提供了可行的工程分析方法。 相似文献
420.