activity
20092026
most citedSunrise III: Overview of Observatory and Instruments

32 citations · 60 across the 9 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

7 papers · 1 filter

astro-ph.SR2026

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…

astro-ph.SR2026★ 2 cited

Solar flare ribbons structured by uncombed chromospheric loops

L. P. Chitta, E. R. Priest, David Orozco Suárez +33

A part of the magnetic energy released during a flare is transported to the lower atmosphere. High-resolution observations show that flare ribbons, sites of energy deposition at th…

astro-ph.SR2025

Citizen CATE 2024: Extending Totality During the 8 April 2024 Total Solar Eclipse with a Distributed Network of Community Participants

Sarah A. Kovac, Amir Caspi, Daniel B. Seaton +240

The Citizen CATE 2024 next-generation experiment placed 43 identical telescope and camera setups along the path of totality during the total solar eclipse (TSE) on 8 April 2024 to…

astro-ph.SR2023

Quantifying Poynting flux in the Quiet Sun Photosphere

Dennis Tilipman, Maria Kazachenko, Benoit Tremblay +3

Poynting flux is the flux of magnetic energy, which is responsible for chromospheric and coronal heating in the solar atmosphere. It is defined as a cross product of electric and m…

astro-ph.SR2023

Improving the Understanding of Subsurface Structure and Dynamics of Solar Active Regions (A white paper submitted to the decadal survey for solar and space Physics (Heliophysics) -- SSPH 2024-2033)

S. C. Tripathy, K. Jain, D. Braun +14

The goal of helioseismology is to provide accurate information about the Sun's interior from the observations of the wave field at its surface. In the last three decades, both glob…

astro-ph.SR2020★ 15 cited

Solar disk center shows scattering polarization in the Sr I 4607 Å line

Franziska Zeuner, Rafael Manso Sainz, Alex Feller +5

Magnetic fields in turbulent, convective high- plasma naturally develop highly tangled and complex topologies---the solar photosphere being the paradigmatic example. These field…

astro-ph.SR2009★ 11 cited

Supersonic Evershed flow outside Sunspots

V. Martinez Pillet, Y. Katsukawa, K. G. Puschmann +1

We report on the discovery of mostly horizontal field channels just outside sunspot penumbrae (in the so-called `moat' region) that are seen to sustain supersonic flows (line-of-si…