Ezequiel Echer

• Abstract

  This projects aims to perform data analyses of Jupiter auroral radio emissions from Nançay radiotelescope and from Cassini spacecraft. Recently a database of Nançay radiotelescopic decametric observations has been compiled from 1990 to 2018. Further, a catalog of radio emissions at kilometric, hectometric and decametric ranges from Cassini Jupiter flyby (2000-2001) has been compiled. Thes…

  Study of Jupiter magnetospheric auroral radio activity variability, AP.R
• Io: Interaction between Volcanic Activity and Jupiter's Magnetosphere, AO.R

• Abstract

  It is the aim of this project to continue the collaborative research about solar wind parameter variation effects on Jupiter auroral radio emissions. During the visit, will be done studies with radio emission data from Nançay radio-telescope and from Cassini spacecraft radio detector. This study will be performed during the Cassini Jupiter flyby, from the end of 2000 to the beginning of 2…

  Jupiter auroral radio response to solar wind variations, AV.EXT

(Only some records are available in English at this moment)

• Abstract

  The planet Venus, despite similarities in physical aspects with Earth, has some significant differences, among these differences is the absence of an intrinsic magnetic field on Venus. Even with the absence of the magnetic field, there is a formation of a magnetosphere by the interaction of the solar wind and the Venusian ionosphere, called the induced magnetosphere. Due to the flow of th…

  Study of ultra low frequency waves in the magnetosheath of Venus, BP.MS

• Abstract

  Jupiter is a powerful source of Decametric radio (DAM) emission, whose origin is associated to electron precipitation by Cyclotron-Maser Instability (CMI). It has been known for decades that the location of the satellite Io affects Jupiter's DAM emissions, which is explained by the Io-Jupiter electromagnetic interaction. The flow of Jupiter's magnetospheric plasma carrying magnetic field …

  Statistical study of possible Europa control of Jupiter decametric radio emissions, BP.MS

• Abstract

  When the solar wind interacts with the planetary obstacles, it defines a region called planetary magnetosphere. In planets which do not have an active magnetic field, as Mars, they are called induced magnetospheres, since they are formed due to the interaction of the solar wind plasma with the planet s ionosphere plasma. Altough Mars does not have currently a global magnetic field, its cr…

  Study of Mars crustal magnetic field displacement due to its interaction with the solar wind, BP.MS

(Only some records are available in English at this moment)

• Abstract

  This project aims to automate the identification of the plasma boundaries of the induced magnetosphere of Venus using machine learning methods. The induced magnetosphere is formed through solar wind interaction with the planetary upper atmosphere. The Venus Express (VEX) mission data (2006-2014), including electron density and magnetic field data from the ASPERA-4 and MAG instruments, res…

  Automatic Identification Of Venus Plasma Boundaries, BE.EP.MS

• Abstract

  When the solar wind interacts with the planetary obstacles, it defines a region called planetary magnetosphere. In planets which do not have an active magnetic field, as Mars, they are called induced magnetospheres, since they are formed due to the interaction of the solar wind with the planet's ionosphere. Although Mars does not have currently a global magnetic field, its crustal magneti…

  Study of Mars crustal magnetic field displacements due to its interaction with the solar wind, BE.EP.MS

• Abstract

  In planets that do not have an intrinsic magnetic field, the interaction with the solar wind with them occurs directly with the high atmosphere/ conductive ionosphere of the planet. The solar wind induces currents in the ionosphere that creates forces that tends to draw the solar wind around the planet; this type of magnetosphere is called as induced magnetosphere. The magnetosheath of th…

  A study on electron oscillations in the magnetosheath of mars with mars express observations, BE.EP.DR

(Only some records are available in English at this moment)