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ORACLE

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ORigin determination and improved detectAbility of Celestial to Local phEnomena...

ORigin determination and improved detectAbility of Celestial to Local phEnomena by the VLF technique The lower ionosphere (70–90 km), a ionized region in the Earth’s upper atmosphere, can be understood as a membrane acting as a sensor to different kinds of phenomena originating at Earth (e.g., lightning) or in space (e.g., space... ver más

04/08/2024

UBAH

213K€

Presupuesto del proyecto: 213K€

Líder del proyecto

UNIVERSITY OF BATH No se ha especificado una descripción o un objeto social para esta compañía.

TRL 4-5

Fecha límite participación Sin fecha límite de participación.

Financiación concedida El organismo H2020 notifico la concesión del proyecto el día 2024-08-04

MSCA-IF-2020: Individual Fellowships Objective:The goal of the Individual Fellowships is to enhance the creative and innovative potential...

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Este proyecto no cuenta con búsquedas de partenariado abiertas en este momento.

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1 Participantes

UBAH

212.93K€ | Lider

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Duración del proyecto: 40 meses Fecha Inicio: 2021-03-09
Fecha Fin: 2024-08-04

Líder del proyecto

UNIVERSITY OF BATH No se ha especificado una descripción o un objeto social para esta compañía.

TRL 4-5

Presupuesto del proyecto 213K€

Fecha límite de participación Sin fecha límite de participación.

Descripción del proyecto The lower ionosphere (70–90 km), a ionized region in the Earth’s upper atmosphere, can be understood as a membrane acting as a sensor to different kinds of phenomena originating at Earth (e.g., lightning) or in space (e.g., space weather). Unexpected strong changes in this region can influence dramatically the performance and reliability of navigation and communication. However, the impact of those phenomena in this region is difficult to quantify accurately. On one hand, this region is too high for balloons and on the other hand it is too low for satellites. In this project, Very Low Frequency (VLF) radio waves will be used because they propagate between the Earth surface and the ionosphere with low attenuation. The researcher will push forward novel scientific understanding of the properties of the lower ionosphere and magnetosphere. She will: (1) determine whether the day-to-day variability of the VLF signal during sunrise can be explained by the ozone variability at its upper boundary, (2) find the yet unknown generation mechanism of VLF banded emissions, and (3) improve the detectability of galactic gamma-ray bursts, known as the most energetic phenomena in the universe. The project is strongly multidisciplinary, involving perspectives and concepts from astrophysics, magnetospheric, ionospheric, atmospheric physics and big data handling. This will be developed by the researcher within the frame of interaction and cooperation with the host and secondments. The results of this proposal have the potential to convey new perspectives in ionospheric and magnetospheric studies and provide some answers to long standing issues within the field of space weather, which has become of central importance in many aspects of human life and industry. As a consequence, by completing this action, Europe will improve its know-how in the topic of this proposal and reinforce its position on a global scale. This project is in line with the EU commission sector on Space and Security.

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