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Spacecraft Heliospheric Observation of Collisions and Kinetic Wave Analysis in Various Environments

Project description

Innovative approaches to analysing weak shocks in unprecedented detail

Plasma shocks are ubiquitous in space, forming when fast-moving plasma flows, such as the solar wind, encounter obstacles like planetary magnetic fields or slower solar wind. The strength of these shocks depends on their Mach number, with strong shocks being well-studied, especially near Earth. However, weaker shocks remain poorly explored. With the support of the Marie Skłodowska-Curie Actions programme, the SHOCKWAVE project plans to use advanced spacecraft data to study these weaker shocks, focusing on their wave activity, jets and instabilities. Using a three-step approach, namely comparing shocks at different Mach ranges near Earth, analysing interplanetary shocks and studying transitions between weak and strong shocks, the proposed research will enhance understanding of shock physics across the solar system and its role in geomagnetic storms.

Objective

Plasma shocks are ubiquitous phenomena in space plasmas, emerging when a supersonic and super-Alfvénic plasma flow encounters an obstacle. The solar wind is such a flow with usually high Mach numbers. Solar wind shocks occur due to two obstacles: magnetic fields of planets or much slower solar wind in front of it. The Mach number dictates the shock strength: from strong (roughly > 5) to weak (1-4).

Spacecraft in Earth’s environment allowed us to study the terrestrial shock as an example of a strong shock in increasing detail in the past decades. The availability of shock measurements from other planets is increasing as well. However, most astrophysical shocks are weak, in particular shocks that have little to no in-situ measurements. The lower range of Mach number shocks is underexplored, especially with high resolution data (resolution of several seconds to milliseconds).

Our main goal is to utilize state-of-the-art spacecraft data to explore the lower Mach number range of shocks (including wave activity, jets, instabilities) and crosscheck the universality of our results with available events in the solar system. To tackle this project, we propose a 3-step analysis: 1) Comparing low and high Mach number range at the terrestrial shock, 2) Investigate interplanetary shocks using high-resolution data, and 3) Providing a comprehensive study on the transition of characteristics from low to high Mach number values.

The proposed research will be carried out in a 24-month project at the Queen Mary University of London. This institution hosts well-known international experts on shock physics and space plasma physics, providing outstanding expertise that perfectly matches the proposed efforts. The generated knowledge will deepen our understanding of shock physics with application throughout the solar system as well as general astrophysics. In particular we will apply the knowledge on interplanetary shocks, which are the precursor of strong geomagnetic storms at Earth.

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HORIZON-TMA-MSCA-PF-EF - HORIZON TMA MSCA Postdoctoral Fellowships - European Fellowships

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Call for proposal

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(opens in new window) HORIZON-MSCA-2024-PF-01

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Coordinator

QUEEN MARY UNIVERSITY OF LONDON
Net EU contribution

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€ 276 187,92
Address
327 MILE END ROAD
E1 4NS LONDON
United Kingdom

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Activity type
Higher or Secondary Education Establishments
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