Quota Studentships
Lead Research Organisation:
University College London
Department Name: Mullard Space Science Laboratory
Abstract
Doctoral Training Partnerships: a range of postgraduate training is funded by the Research Councils. For information on current funding routes, see the common terminology at https://www.ukri.org/apply-for-funding/how-we-fund-studentships/. Training grants may be to one organisation or to a consortia of research organisations. This portal will show the lead organisation only.
Organisations
People |
ORCID iD |
| A Smith (Training Grant Holder) |
Publications
Green L
(2010)
Photospheric flux cancellation and associated flux rope formation and eruption
in Astronomy & Astrophysics
Harra L
(2010)
Response of the Solar Atmosphere to the Emergence of 'Serpentine' Magnetic Field
in Solar Physics
Kanani S
(2010)
A new form of Saturn's magnetopause using a dynamic pressure balance model, based on in situ, multi-instrument Cassini measurements A NEW FORM OF SATURN'S MAGNETOPAUSE
in Journal of Geophysical Research: Space Physics
Kanani S
(2011)
Autumn MIST 2010
in Astronomy & Geophysics
Ma Y
(2011)
The importance of thermal electron heating in Titan's ionosphere: Comparison with Cassini T34 flyby THERMAL ELECTRON HEATING OF TITAN
in Journal of Geophysical Research: Space Physics
Martin-Carrillo A
(2012)
The relative and absolute timing accuracy of the EPIC-pn camera on XMM-Newton , from X-ray pulsations of the Crab and other pulsars
in Astronomy & Astrophysics
Masters A
(2010)
Cassini observations of a Kelvin-Helmholtz vortex in Saturn's outer magnetosphere A VORTEX IN SATURN'S OUTER MAGNETOSPHERE
in Journal of Geophysical Research: Space Physics
Michael M
(2011)
High-altitude charged aerosols in the atmosphere of Titan
in Planetary and Space Science
Németh Z
(2011)
Ion distributions of different Kronian plasma regions ION DISTRIBUTIONS OF KRONIAN PLASMA
in Journal of Geophysical Research: Space Physics
Valori G
(2011)
Nonlinear Force-Free Extrapolation of Emerging Flux with a Global Twist and Serpentine Fine Structures
in Solar Physics