output
19922026
Showing 2025 · astro-ph.SRShow all

8 papers · 2 filters

astro-ph.SR2025★ 1 cited

Oscillations of the solar photospheric magnetic field caused by the m = 1 high-latitude inertial mode

Stephan G. Heinemann, Zhi-Chao Liang, Laurent Gizon

Periodic oscillations at 338 nHz in the Earth frame are observed at high latitudes in direct Doppler velocity measurements. These oscillations correspond to the high-latitude…

astro-ph.SR2025★ 17 cited

Very Large Telescope Observations of Interstellar Comet 3I/ATLAS. II. From Quiescence to Glow: Dramatic Rise of Ni i Emission and Incipient CN Outgassing at Large Heliocentric Distances*

Rohan Rahatgaonkar, Juan Pablo Carvajal, Thomas H. Puzia +25

We report VLT spectroscopy of the interstellar comet 3I/ATLAS (C/2025~N1) from to ~au using X-shooter (300--550\,nm, ) and UVES (opt…

astro-ph.SR2025★ 3 cited

Validating the bright Gaia celestial reference frame with new VLBI astrometry of radio stars

Jingdong Zhang, Bo Zhang, Shuangjing Xu +1

There exist inconsistencies between the bright and faint Gaia Celestial Reference Frame 3 (Gaia-CRF3), which manifests as a systematic rotation and needs to be independently estima…

astro-ph.SR2025★ 4 cited

Intermittency in Interplanetary Coronal Mass Ejections Observed by Parker Solar Probe and Solar Orbiter

Julia Ruohotie, Simon Good, Christian Möstl +1

Intermittency has been studied extensively in the fast and slow solar winds but to a far lesser extent in interplanetary coronal mass ejections (ICMEs). While ICMEs are often chara…

astro-ph.SR2025★ 4 cited

Quantifying Uncertainties in Solar Wind Forecasting Due to Incomplete Solar Magnetic Field Information

Stephan G. Heinemann, Jens Pomoell, Ronald M. Caplan +5

Solar wind forecasting plays a crucial role in space weather prediction, yet significant uncertainties persist due to incomplete magnetic field observations of the Sun. Isolating t…

astro-ph.SR2025

Euclid Quick Data Release (Q1) Ultracool dwarfs in the Euclid Deep Field North

A. Mohandasan, R. L. Smart, C. Reylé +176

Ultracool dwarfs (UCDs) encompass the lowest mass stars and brown dwarfs, defining the stellar substellar boundary. They have significant potential for advancing the understanding…