From the 1 of 7 papers with an AI index.
11 citations
- Institut für SonnenphysikDE3 papers
- Instituto de Astrofísica de CanariasES3 papers
- University of GrazAT3 papers
- Agenzia Spaziale ItalianaIT2 papers
- California State University, NorthridgeUS2 papers
- Instituto de Astrofísica de AndalucíaES2 papers
- Instituto Nacional de Técnica AeroespacialES2 papers
- Johns Hopkins University Applied Physics LaboratoryUS2 papers
- KU LeuvenBE2 papers
- Max Planck Institute for Solar System ResearchDE2 papers
- National Astronomical Observatory of JapanJP2 papers
- National Institute for Fusion ScienceJP2 papers
7 papers
High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona
Yuhang Gao, Hui Tian, Richard Morton +5
Using high‑cadence EUV images from Solar Orbiter, the authors detect a previously hidden population of high‑frequency kink MHD waves in solar polar coronal plumes, many with period…
Mixed phases in feedback Ising models
Yi-Ping Ma, Ivan Sudakow, P. L. Krapivsky
We study mean-field Ising models in which the coupling depends on the magnetization via a feedback function. We identify mixed phases (MPs) and show that they can be stable at zero…
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…
Giant Planet Atmospheres
Henrik Melin
The giant planets, Jupiter, Saturn, Uranus, and Neptune, all have vibrant and dynamic atmospheres. The iconic belt--zone structure of Jupiter, together with the Great Red Spot, is…
Synthesizing Sun-as-a-star flare spectra from high-resolution solar observations
M. De Wilde, A. G. M. Pietrow, M. K. Druett +22
Spatially resolved observations of the Sun and the astronomical sample size of stellar bodies are the respective key strengths of solar and stellar observations. However, the large…
Multi-line Wave Signatures in a Sunspot from Near-UV Sunrise III/SUSI Observations
Shahin Jafarzadeh, David B. Jess, Marco Stangalini +32
Magnetohydrodynamic waves redistribute energy in magnetic structures of the lower solar atmosphere, yet constraints on how wave power and dominant frequencies are organised above s…