activity
20102023
most citedObservations of ubiquitous compressive waves in the Sun's chromosphere

203 citations · 1.9k across the 31 of their papers we have counts for

collaborators
Showing 2020Show all

7 papers · 1 filter

astro-ph.SR2020★ 112 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★ 18 cited

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★ 110 cited

Critical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)

Mark P. Rast, Nazaret Bello González, Luis Bellot Rubio +84

The Daniel K. Inouye Solar Telescope (DKIST) will revolutionize our ability to measure, understand and model the basic physical processes that control the structure and dynamics of…

astro-ph.SR2020★ 70 cited

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.SR2020★ 175 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.SR2020★ 27 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…

astro-ph.SR2020★ 52 cited

Is the High-Resolution Coronal Imager Resolving Coronal Strands? Results from AR 12712

Thomas Williams, Robert W. Walsh, Amy R. Winebarger +14

Following the success of the first mission, the High-Resolution Coronal Imager (Hi-C) was launched for a third time (Hi-C 2.1) on 29th May 2018 from the White Sands Missile Range,…