Rolling Grant

Lead Research Organisation: University College London
Department Name: Mullard Space Science Laboratory

Abstract

A Rolling Grant is designed to support a programme of research within a particular domain. The domain in this case is Space Science, in particular the fields of: 1. Compact Objects (Black Holes and Neutron Stars, seeking to understand the physics associated with the enormously compact objects. this includes studying Gamma-ray bursts (giant supernovae in distant galaxies), isolated neutron stars including those with gigantic magnetic fields, and black holes); 2. Galaxy Formation and Evolution (Understanding these processes using extremely sophisticated computer modelling techniques. Looking at the role of Active Galactic Nuclei, the history of star formation and the role of feedback) 3. Magnetic Coupling and the Heliosphere (The emergence of magnetic field structures on the Sun, how solar eruptions are triggered, the creation of the Solar Wind and how it affects the Earth); 4. Plasma Physics of the Terrestrial and Planetary Environments (The Earth and some other planets are surrounded and protected by magnetic fields which provide a local laboratory for fundamental research into how charged particles interact with complex magnetic field structures. Through the use of in-situ space probes we will study these processes to gain a fuller understanding of this important physics. Many solar system bodies do not have a protective magnetic field and so we will also study the these interactions, especially planets and moons with an atmospheres (e.g. Mars and Titan)); 5. Planetary Surfaces (The surfaces of planets, particularly Mars, provide interesting and alternative geological and meteorological settings to the Earth. We plan to use the plethora of observational data available from currently orbiting spacecraft to study in great detail these terrains). 6. Enabling technologies (Miniature, very low temperature coolers, auroral imagers and plasma analysers will be developed. New methods of constructing 3-dimensional models of planetary surfaces will be produced. A study will be made (with impact trials) of the survivability of an instrumented penetrator into ice at around 700 miles per hour).

Publications

10 25 50

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Teh W (2012) Electron dynamics in the reconnection ion diffusion region in Journal of Geophysical Research: Space Physics

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Thompson W (2011) 3D Reconstruction of a Rotating Erupting Prominence in Solar Physics

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Tiengo A (2011) X-ray and optical observations of the closest isolated radio pulsar? X-ray and optical search for PSR J2144-3933 in Monthly Notices of the Royal Astronomical Society: Letters

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Tinetti G (2012) EChO Exoplanet characterisation observatory in Experimental Astronomy

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Tokar R (2012) Detection of exospheric O 2 + at Saturn's moon Dione in Geophysical Research Letters

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Turolla R (2011) IS SGR 0418+5729 INDEED A WANING MAGNETAR? in The Astrophysical Journal

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Török T (2014) The evolution of writhe in kink-unstable flux ropes and erupting filaments in Plasma Physics and Controlled Fusion

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Vande Putte D (2010) A kinematic study of open clusters: implications for their origin Open cluster orbits: implications for origin in Monthly Notices of the Royal Astronomical Society

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Vande Putte, D. V. And Garnier, T. P. And Ferreras, I. And Mignani, R. P. And Cropper, M. (2011) Kinematic study of open clusters (Vande Putte+, 2010) in VizieR Online Data Catalog

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Vargas Domínguez S (2011) On Signatures of Twisted Magnetic Flux Tube Emergence in Solar Physics

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Viganò D (2012) The influence of magnetic field geometry on magnetars X-ray spectra in Journal of Physics: Conference Series

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Wallace A (2010) Pre-Flare Flows in the Corona in Solar Physics

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Walsh A (2013) Sources of electron pitch angle anisotropy in the magnetotail plasma sheet in Journal of Geophysical Research: Space Physics

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Walsh A (2010) 10 years of the Cluster mission in Astronomy & Geophysics

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Walsh A (2010) Comprehensive ground-based and in situ observations of substorm expansion phase onset in Journal of Geophysical Research: Space Physics

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Walsh A (2013) An indication of the existence of a solar wind strahl at 10 AU in Geophysical Research Letters

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Warner N (2011) Constraints on the origin and evolution of Iani Chaos, Mars in Journal of Geophysical Research

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Wei Y (2012) A teardrop-shaped ionosphere at Venus in tenuous solar wind in Planetary and Space Science

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Weidner C (2013) The (galaxy-wide) IMF in giant elliptical galaxies: from top to bottom in Monthly Notices of the Royal Astronomical Society

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Wild J (2011) Midnight sector observations of auroral omega bands MIDNIGHT SECTOR AURORAL OMEGA BANDS in Journal of Geophysical Research: Space Physics

 
Description Significant improved understanding in the fields of astrophysics, space plasma physics, solar physics, planetary sciences and instrumentation
Exploitation Route Through peer reviewed publications
Sectors Other

 
Description Consolidated Grants
Amount £2,537,157 (GBP)
Funding ID ST/N000722/1 
Organisation Science and Technologies Facilities Council (STFC) 
Sector Public
Country United Kingdom
Start 04/2016 
End 03/2019
 
Description Consolidated Grants
Amount £1,138,583 (GBP)
Funding ID ST/N000811/1 
Organisation Science and Technologies Facilities Council (STFC) 
Sector Public
Country United Kingdom
Start 04/2016 
End 03/2019
 
Description STFC Consolidated Grant
Amount £2,145,073 (GBP)
Funding ID ST/K000977/1 
Organisation Science and Technologies Facilities Council (STFC) 
Sector Public
Country United Kingdom
Start 04/2013 
End 03/2017
 
Title Cryogenic system elements 
Description Elements of millK Adiabatic Demagnetisation Refrigerators including heatswitches and magnets. Magnets, cryogenics, vacuum 
Type Of Technology Systems, Materials & Instrumental Engineering 
Year Produced 2011 
Impact Development will lead to minaturization of coolers which will make them more suitable for space and ground-based applications