Titlebook: Information Management and Big Data; 8th Annual Internati Juan Antonio Lossio-Ventura,Jorge Valverde-Rebaza, Conference proceedings 2022 Th

Individual

誰(shuí)在削木頭

Edwin Alvarez-Mamani,Harley Vera-Olivera,José L. Soncco-álvarezs the edge of the inner disk, the Galactic Bar and the Galactic Center. The difference becomes even more compelling if we take into account that metal abundances are based on young stellar tracers (classical Cepheids, Red Supergiants, Luminous Blue Variables). Finally, we briefly outline the possibl

murmur

take into account the Bernoulli effect; see Chapter 6 for details). The integral multiplicity depends also on the value .) of gravitational acceleration which is a function of the latitude and varies with time because of the gravitational influence of the Moon and the Sun, and on the vertical distr

HAIL

faction

語(yǔ)言學(xué)

phlegm

Arturo Flores,Alessandro Morales,Gianfranco Campos,Jorge Gelso underground into a unique giant multidirectional detector in space, which moves and rotates with Earth for continuous determination of CR space-rigidity distribution function in the interval from about one GV up to about thousand GV. To prolong this spectrum into smaller and higher energy range are

使糾纏

Airton Huamán,Marco Huancahuari,Lenis Wongt the same radius of 42 AU in 1987 and for anomalous cosmic rays this ratio is only 0.1–0.2. This suggests a dramatically different entry of particles into the heliosphere in the two cycles for both types of particles as well as significantly different particle flow characteristics in the outer heli

不可侵犯

Geraldine Puntillo,Alonso Salazar,Lenis Wongs been a steady improvement in theoretical understanding of cosmic ray behavior through the use of ever more sophisticated numerical models. This milestone in cosmic ray studies was celebrated with a Workshop on Cos- mic Rays in the Heliosphere which was convened by L. A. Fisk, J. R. Jokipii.

返老還童

Pablo Del Aguila,Dante Roque,Lenis Wongrons from the beam collide with optical photons from the expanding envelope. In this paper we present self-consistent solutions to the rate equations for the energy loss due to collective processes and calculate the momentum transferred to the envelope by the beam. We then comment on the expected X-