Descripción del proyecto
Comprender la estructura de los choques sin colisiones
Las ondas de choque surgen en el aire y el agua de la Tierra y en una amplia gama de plasmas del Universo. En general, se trata de plasmas sin colisiones. El proyecto SHARP, financiado con fondos europeos, tiene por objeto contribuir a la comprensión de la estructura de los choques sin colisiones en diversos entornos y de los procesos de aceleración en todas las etapas del choque. El proyecto intensificará el aprovechamiento de los datos heliosféricos y realizará un análisis comparativo integrador del arco terrestre y de los choques planetarios e interplanetarios. SHARP combinará los resultados de las mediciones «in situ» de los choques heliosféricos y de los remanentes de supernovas con la observación a distancia de choques astrofísicos lejanos. Además, en el proyecto se desarrollará una base de datos de alto nivel que incluirá choques e instrumentos innovadores para el análisis de choques.
Objetivo
"SHARP aims to achieve a major leap in understanding of the structure of collisionless shocks in various environments and of the acceleration processes at all shock scales. This will be done by: (a) intensifying exploitation of the heliospheric data and performing a comprehensive comparative analysis of the Earth bow shock, planerary shocks, and interplanetary shocks, (b) establishing a collaboration of the world renown groups working together on all aspects of the shock physics, (c) utilizing and combining the knowledge obtained in in situ measurements on heliospheric shocks and in remote observations of distant astrophysical shocks, and (d) developing a high-level databases of shocks and advanced tools for the shock analysis and making them public. The research will encompass the three ""pillars"" of the shock physics: the shock structure, the shock energy deposition, and the radiation from the shock energized particles. The study will address the most fundamental unsolved issues of the shock physics: the structural changes of the shock with the increase of the Mach number, the intimate relation between the shock fields and the particle distributions, the injection problem, and the electron acceleration puzzle. The research will bridge over the in situ observed heliospheric shocks and supernovae remnant (SNR) shocks which are observed only indirectly, by emission from energized particles, by combining the knowledge of the heliospheric shock structure and constraints provided by the radiation measurements from SNR shocks. Starting with the observational data, the research will ultimately provide new diagnostic measures for the ongoing and future experiments, such that will allow to improve the efficiency of the measurements and data analysis, contribute to understanding of solar wind interaction with the Earth, and advance understanding of the most powerful accelerators in the Universe."
Ámbito científico
Programa(s)
Convocatoria de propuestas
Consulte otros proyectos de esta convocatoriaConvocatoria de subcontratación
H2020-SPACE-2020
Régimen de financiación
RIA - Research and Innovation actionCoordinador
00560 Helsinki
Finlandia