activity
20172021
most citedGlobal maps of the magnetic field in the solar corona

175 citations · 587 across the 9 of their papers we have counts for

collaborators

16 papers

astro-ph.SR202115 cited

A statistical study of propagating MHD kink waves in the quiescent corona

Ajay K. Tiwari, Richard J. Morton, James A. McLaughlin

The Coronal Multi-channel Polarimeter (CoMP) has opened up exciting opportunities to probe transverse MHD waves in the Sun's corona. The archive of CoMP data is utilised to generat…

astro-ph.SR2020112 cited

The Solar Orbiter Science Activity Plan: translating solar and heliospheric physics questions into action

I. Zouganelis, A. De Groof, A. P. Walsh +182

Solar Orbiter is the first space mission observing the solar plasma both in situ and remotely, from a close distance, in and out of the ecliptic. The ultimate goal is to understand…

astro-ph.SR2020

Effect of Coronal Loop Structure on Wave Heating by Phase Mixing

P. Pagano, I. De Moortel, R. J. Morton

The mechanism behind coronal heating still elude direct observation and modelling of viable theoretical processes and the subsequent effect on coronal structures is one of the key…

astro-ph.SR2020

Mapping the magnetic field in the solar corona through magnetoseismology

Zihao Yang, Hui Tian, Steven Tomczyk +4

Magnetoseismology, a technique of magnetic field diagnostics based on observations of magnetohydrodynamic (MHD) waves, has been widely used to estimate the field strengths of oscil…

astro-ph.SR2020175 cited

Global maps of the magnetic field in the solar corona

Zihao Yang, Christian Bethge, Hui Tian +10

Understanding many physical processes in the solar atmosphere requires determination of the magnetic field in each atmospheric layer. However, direct measurements of the magnetic f…

astro-ph.SR202027 cited

The drivers of active region outflows into the slow solar wind

David H. Brooks, Amy R. Winebarger, Sabrina Savage +13

Plasma outflows from the edges of active regions have been suggested as a possible source of the slow solar wind. Spectroscopic measurements show that these outflows have an enhanc…