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1.
David Kappel Gabriele Arnold Rainer Haus Giuseppe Piccioni Pierre Drossart 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
The successful long-duration radiation measurements performed by the VIRTIS instrument aboard ESA’s Venus Express spacecraft have provided an excellent collection of atmospheric and surface data that stand out due to their high temporal and spatial coverage of the planet and due to a high diversity of measurement and environmental conditions. 相似文献
2.
Lorenzo Borello Giuseppe Villero Matteo Dalla Vedova 《Aerospace Science and Technology》2009,13(8):475-487
The asymmetry limitation between left and right wing flap surfaces is one of the most severe requirements for the design of the actuation and control system. Each asymmetry exceeding a defined value must be detected and limited by appropriate monitoring devices equipped with a suitable software.In the design of a new flap control system the development of the asymmetry monitoring system plays a very important role and it is a very debated matter in industrial field. Nevertheless in scientific literature this topic is so neglected that, at the best of our knowledge, no paper dealing with the specific argument exists, except for the authors' works listed in the references.The currently used monitoring technique is based on the differential position control between left and right surfaces. Nevertheless in particularly severe conditions the above mentioned technique may be unable to prevent potentially critical asymmetries; in order to limit the above mentioned shortcomings, the authors proposed and developed some innovative monitoring techniques in previous papers. Their use generally reduces the asymmetry slightly, but in some cases it may have an unreliable behavior. In order to overcome the shortcomings of the previous models, in this work the authors develop and propose new different monitoring strategies and assess their positive effects on the maximum asymmetry following a torque tube failure. 相似文献
3.
Giuseppe Consolini Paola De Michelis Matthieu Kretzschmar 《Space Science Reviews》2006,122(1-4):293-299
Recent studies evidenced that the magnetotail dynamics looks like the one of an avalanching system. This fact has been related
with a near criticality dynamics and modelled by singular diffusion and transport equations. Here, we discuss some features
of the Earth’s magnetotail dynamics using a thermodynamic approach. In detail we discuss the role played by fluctuations in
singular diffusion and relaxation processes from a non-equilibrium thermodynamics point of view. Moreover, the emergence of
non-Gaussian statistics is discussed in the framework of the thermodynamics of composite systems. 相似文献
4.
Chang Tom Tam Sunny W.Y. Wu Cheng-Chin Consolini Giuseppe 《Space Science Reviews》2003,107(1-2):425-445
The first definitive observation that provided convincing evidence indicating certain turbulent space plasma processes are
in states of ‘complexity’ was the discovery of the apparent power-law probability distribution of solar flare intensities.
Recent statistical studies of complexity in space plasmas came from the AE index, UVI auroral imagery, and in-situ measurements
related to the dynamics of the plasma sheet in the Earth's magnetotail and the auroral zone.
In this review, we describe a theory of dynamical ‘complexity’ for space plasma systems far from equilibrium. We demonstrate
that the sporadic and localized interactions of magnetic coherent structures are the origin of ‘complexity’ in space plasmas.
Such interactions generate the anomalous diffusion, transport, acceleration, and evolution of the macroscopic states of the
overall dynamical systems.
Several illustrative examples are considered. These include: the dynamical multi- and cross-scale interactions of the macro-and
kinetic coherent structures in a sheared magnetic field geometry, the preferential acceleration of the bursty bulk flows in
the plasma sheet, and the onset of ‘fluctuation induced nonlinear instabilities’ that can lead to magnetic reconfigurations.
The technique of dynamical renormalization group is introduced and applied to the study of two-dimensional intermittent MHD
fluctuations and an analogous modified forest-fire model exhibiting forced and/or self-organized criticality [FSOC] and other
types of topological phase transitions.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
5.
Alberto Buzzoni Giuseppe Altavilla Siwei Fan Carolin Frueh Italo Foppiani Marco Micheli Jaime Nomen Noelia Sánchez-Ortiz 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(1):371-393
We report on extensive photometry and low-resolution () spectroscopy of the deep-space debris WT1190F, which impacted Earth offshore from Sri Lanka, on 2015 November 13. In spite of its likely artificial origin (as a relic of some past lunar mission), the case offered important points of discussion for its suggestive connection with the envisaged scenario for a (potentially far more dangerous) natural impactor, like an asteroid or a comet.Our observations indicate for WT1190F an absolute magnitude , with a flat dependence of reflectance on the phase angle, such as ?mag?deg?1. The detected short-timescale variability suggests that the body was likely spinning with a period twice the nominal figure of , as from the observed lightcurve. In the color domain, WT1190F closely resembled the Planck deep-space probe. This match, together with a depressed reflectance around 4000 and 8500 Å may be suggestive of a “grey” (aluminized) surface texture.The spinning pattern remained in place also along the object fiery entry in the atmosphere, a feature that may have partly shielded the body along its fireball phase perhaps leading a large fraction of its mass to survive intact, now lying underwater along a tight (?km) strip of sea, at a depth of 1500?m or less.Under the assumption of Lambertian scatter, an inferred size of ?cm is obtained for WT1190F. By accounting for non-gravitational dynamical perturbations, the Area-to-Mass ratio of the body was in the range ?m2?kg?1.Both these figures resulted compatible with the two prevailing candidates to WT1190F’s identity, namely the Athena II Trans-Lunar Injection Stage of the Lunar Prospector mission, and the ascent stage of the Apollo 10 lunar module, callsign “Snoopy”. Both candidates have been analyzed in some detail here through accurate 3D CAD design mockup modelling and BRDF reflectance rendering to derive the inherent photometric properties to be compared with the observations. 相似文献
6.
Noriyuki Matsunaga Giuseppe Bono Xiaodian Chen Richard de Grijs Laura Inno Shogo Nishiyama 《Space Science Reviews》2018,214(4):74
Here we discuss impacts of distance determinations on the Galactic disk traced by relatively young objects. The Galactic disk, \(\sim40~\mbox{kpc}\) in diameter, is a cross-road of studies on the methods of measuring distances, interstellar extinction, evolution of galaxies, and other subjects of interest in astronomy. A proper treatment of interstellar extinction is, for example, crucial for estimating distances to stars in the disk outside the small range of the solar neighborhood. We’ll review the current status of relevant studies and discuss some new approaches to the extinction law. When the extinction law is reasonably constrained, distance indicators found in today and future surveys are telling us stellar distribution and more throughout the Galactic disk. Among several useful distance indicators, the focus of this review is Cepheids and open clusters (especially contact binaries in clusters). These tracers are particularly useful for addressing the metallicity gradient of the Galactic disk, an important feature for which comparison between observations and theoretical models can reveal the evolution of the disk. 相似文献
7.
This work deals with the aerodynamic database development of the Intermediate Experiment Vehicle. 相似文献
8.
We review some aspects of low latitudes (L≤2) geomagnetic field variations associated with magnetospheric pulsations as well
as with continuous and impulsive variations of the solar wind (SW) pressure.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
9.
Giuseppe Nisticò Spiros Patsourakos Volker Bothmer Gaetano Zimbardo 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Coronal hole jets are fast ejections of plasma occurring within coronal holes, observed at Extreme-UltraViolet (EUV) and X-ray wavelengths. Recent observations of jets by the STEREO and Hinode missions show that they are transient phenomena which occur at much higher rates than large-scale impulsive phenomena like flares and Coronal Mass Ejections (CMEs). In this paper we describe some typical characteristics of coronal jets observed by the SECCHI instruments of STEREO spacecraft. We show an example of 3D reconstruction of the helical structure for a south pole jet, and present how the angular distribution of the jet position angles changes from the Extreme-UltraViolet-Imager (EUVI) field of view to the CORonagraph1 (COR1) (height ∼2.0 R⊙ heliocentric distance) field of view. Then we discuss a preliminary temperature determination for the jet plasma by using the filter ratio method at 171 and 195 Å and applying a technique for subtracting the EUV background radiation. The results show that jets are characterized by electron temperatures ranging between 0.8 and 1.3 MK. We present the thermal structure of the jet as temperature maps and we describe its thermal evolution. 相似文献
10.
Giuseppe Nisticò Gaetano Zimbardo 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
Recently a new model for explaining the observations of preferential heating of heavy ions in the polar solar corona was proposed ( and ). In that model the ion energization mechanism is the ion reflection off supercritical quasi-perpendicular collisionless shocks in the corona and the subsequent acceleration by the motional electric field E = −V × B/c. The mechanism of heavy ion reflection is based on ion gyration in the magnetic overshoot of the shock. The acceleration due to the motional electric field is perpendicular to the magnetic field, giving rise to large temperature anisotropy with T⊥ ? T∥, in agreement with SoHO observations. Such a model is tested here by means of a one dimensional test particle simulation where ions are launched toward electric and magnetic profiles representing the shock transition. We study the dynamics of O5+, as representative of coronal heavy ions for Alfvénic Mach numbers of 2–4, as appropriate to solar corona. It is found that O5+ ions are easily reflected and gain more than mass proportional energy with respect to protons. 相似文献