590 citations
- Centre National de la Recherche ScientifiqueFR59 papers
- Goddard Space Flight CenterUS57 papers
- University College LondonGB36 papers
- Max Planck Institute for Solar System ResearchDE35 papers
- University of SheffieldGB34 papers
- KU LeuvenBE30 papers
- Université Paris-SaclayFR29 papers
- University of OsloNO29 papers
- George Mason UniversityUS26 papers
- University of GlasgowGB25 papers
- Queen Mary University of LondonGB24 papers
- Southwest Research InstituteUS22 papers
536 papers
An Approximate Bayesian Deep Learning Approach for Uncertainty-aware Differential Emission Measure Estimates in the Solar Corona from the SDO
N. Balodhi, R. J. Morton
Accurately estimating the temperature distribution of solar coronal plasma, known as the Differential Emission Measure (DEM), is vital for understanding the thermodynamics of the c…
Ion abundances in the plasma tail of 3I/ATLAS show that it is N2-rich
Lea Ferellec, Cyrielle Opitom, Colin Snodgrass
Interstellar objects allow us to compare the early planetary formation process in the Solar System and around other stars. The second and third interstellar objects, 2I/Borisov and…
High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona
Yuhang Gao, Hui Tian, Richard Morton +5
The acceleration and heating of the fast solar wind remain long-standing challenges in space physics. One type of leading theoretical models requires high-frequency magnetohydrodyn…
Multi-height Identification of Sausage and Fluting Eigenmodes in a Solar Pore
Shahin Jafarzadeh, David B. Jess, Marco Stangalini +34
Magnetic pores are compact, strongly magnetised waveguides in the lower solar atmosphere and therefore provide favourable conditions for identifying magnetohydrodynamic (MHD) wave…
Giant Planet Atmospheres
Henrik Melin
The giant planets, Jupiter, Saturn, Uranus, and Neptune, all have vibrant and dynamic atmospheres. The iconic belt--zone structure of Jupiter, together with the Great Red Spot, is…
Multi-line Wave Signatures in a Sunspot from Near-UV Sunrise III/SUSI Observations
Shahin Jafarzadeh, David B. Jess, Marco Stangalini +32
Magnetohydrodynamic waves redistribute energy in magnetic structures of the lower solar atmosphere, yet constraints on how wave power and dominant frequencies are organised above s…