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We present eclipse attacks on Ethereum nodes that exploit the peer-to-peer network used for neighbor discovery. Our attacks can be launched using only two hosts, each with a single IP address. Our ecl...
We present eclipse attacks on bitcoin’s peer-to-peer network. Our attack allows an adversary controlling a suffi- cient number of IP addresses to monopolize all connections to and from a victim bit...
Sel sh mining [9] is a well-known attack where a sel sh miner, under certain conditions, can gain a disproportionate share of reward by deviating from the honest behavior.
评估一种利用Eclipse治疗计划系统的基部剂量计划进行补偿(base dose plan compensation, BDPC)的调强放疗(IMRT)计划优化方法应用于上段食管癌的可行性。方法 选择19例上段食管癌患者,设计初始IMRT计划,并分别用BDPC法和热点冷点控制(hot and cold spot control, HCSC)法进一步优化。比较两种计划的靶区覆盖、适形指数(CI)、均...
We analyse simultaneous UBVR quiescent light curves of the cataclysmic variable V2051 Oph using the Physical Parameter Eclipse Mapping (PPEM) method in order to map the gas temperature and surface den...
Mapping the brightness distribution of exoplanets is the next frontier for exoplanet infrared photometry studies. For tidally-locked hot Jupiters that transit and are eclipsed by their host star with ...
The classical method for measure the Earth-Sun distance is due to Aristarchus and it is based upon the measure of the angle Moon-Earth-Sun when the Moon is exactly in quadrature. Such an angle is only...
The paper contains the preliminary result description of the photometric observations of the Moon surface during the total lunar eclipse of June, 15, 2011 conducted in southern Russia and Ukraine in t...
One of the greatest discoveries of modern times is that of the expanding Universe, almost invariably attributed to Hubble (1929). What is not widely known is that the original treatise by Lema顃re (192...
The Moon抯 changeable aspect during a lunar eclipse is largely attributableto variations in the refracted unscattered sunlight absorbed by the terres trial atmosphere that occur as the satellite crosse...
We measure secondary eclipses of the hot giant exoplanets CoRoT-1 at 3.6 and 4.5 μm, and CoRoT-2 at 3.6 μm, both using Warm Spitzer. We find that the Warm Spitzer mission is working very well for exop...
As part of the NASA EPOXI Mission of Opportunity, we observed seven known transiting extrasolar planet systems in order to construct time series photometry of extremely high phase coverage and precisi...
Transiting exoplanets provide access to data to study the mass-radius relation and internal structure of extrasolar plan-ets. Long-period transiting planets allow insight into planetary environments ...
Satellite Observation of the Umbra of the Moon during the Total Solar Eclipse on July 22, 2009。
It has been observed that some geophysical parameters could be changed during a solar eclipse. We have therefore measured gravity and magnetic fields during solar eclipses. We also measured the gravit...

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