activity
20042024
most citedThe "Solar Model Problem" Solved by the Abundance of Neon in Stars of the Local Cosmos

204 citations · 3.1k across the 72 of their papers we have counts for

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Showing 2022Show all

8 papers · 1 filter

astro-ph.SR2022★ 19 cited

The First Flight of the Marshall Grazing Incidence X-ray Spectrometer (MaGIXS)

Sabrina L. Savage, Amy R. Winebarger, Ken Kobayashi +34

The Marshall Grazing Incidence X-ray Spectrometer (MaGIXS) sounding rocket experiment launched on July 30, 2021 from the White Sands Missile Range in New Mexico. MaGIXS is a unique…

astro-ph.SR2022★ 23 cited

The impact of multi-fluid effects in the solar chromosphere on the ponderomotive force under LTE and NEQ ionization conditions

Juan Martínez-Sykora, Bart De Pontieu, Viggo H. Hansteen +3

The ponderomotive force is suggested to be the main mechanism to produce the so-called first ionization potential (FIP) effect - the enrichment of low FIP elements observed in the…

astro-ph.SR2022★ 11 cited

Coronal Abundances in an Active Region: Evolution and Underlying Chromospheric and Transition Region Properties

Paola Testa, Juan Martinez-Sykora, Bart De Pontieu

The element abundances in the solar corona and solar wind are often different from those of the solar photosphere, typically with a relative enrichment of elements with low first i…

astro-ph.SR2022★ 12 cited

A Statistical Study of IRIS Observational Signatures of Nanoflares and Non-thermal Particles

Kyuhyoun Cho, Paola Testa, Bart De Pontieu +1

Nanoflares are regarded as one of the major mechanisms of magnetic energy release and coronal heating in the solar outer atmosphere. We conduct a statistical study on the response…

astro-ph.SR2022★ 1 cited

Diagnostics of non-Maxwellian electron distributions in solar active regions from Fe XII lines observed by Hinode/EIS and IRIS

G. Del Zanna, V. Polito, J. Dudík +3

We present joint Hinode/EIS and IRIS observations of Fe XII lines in active regions, both on-disk and off-limb. We use an improved calibration for the EIS data, and find that the 1…

astro-ph.SR2022

The Solar X-ray Corona

Paola Testa, Fabio Reale

The X-ray emission from the Sun reveals a very dynamic hot atmosphere, the corona, which is characterized by a complex morphology and broad range of timescales of variability and s…