R
Richard Morton
Researcher at Northumbria University
Publications - 96
Citations - 3604
Richard Morton is an academic researcher from Northumbria University. The author has contributed to research in topics: Magnetohydrodynamics & Corona. The author has an hindex of 34, co-authored 92 publications receiving 2990 citations. Previous affiliations of Richard Morton include University of Sheffield & National Center for Atmospheric Research.
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Observations of ubiquitous compressive waves in the Sun/'s chromosphere
Richard Morton,Gary Verth,David B. Jess,David Kuridze,Michael S. Ruderman,Mihalis Mathioudakis,Robertus Erdélyi +6 more
TL;DR: The observed ubiquity and estimated energy flux associated with the detected magnetohydrodynamic waves suggest the chromosphere is a vast reservoir of wave energy with the potential to meet chromospheric and coronal heating requirements.
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Multiwavelength Studies of MHD Waves in the Solar Chromosphere
TL;DR: In this article, the authors review the recent progress made in characterising, categorising and interpreting oscillations manifesting in the solar chromosphere, with an impetus placed on their intrinsic energy properties.
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Investigating Alfvénic wave propagation in coronal open-field regions
TL;DR: It is demonstrated that counter-propagating Alfvénic waves exist in open coronal magnetic fields and key observational insights are revealed into the details of their generation, reflection in the upper atmosphere and outward propagation into the solar wind.
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Multiwavelength studies of MHD waves in the solar chromosphere: An overview of recent results
TL;DR: In this paper, the authors review the recent progress made in characterising, categorising and interpreting oscillations manifesting in the solar chromosphere, with an impetus placed on their intrinsic energetics.
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Observations of sausage modes in magnetic pores
TL;DR: In this paper, evidence for the observation of magnetohydrodynamic sausage modes in magnetic pores in the solar photosphere has been presented, where the empirical decomposition method of wave analysis is used to identify the oscillations detected through a 4170 A "blue continuum" filter observed with the Rapid Oscillations in the Solar Atmosphere (ROSA) instrument.