output
20142026
most citedElectron scale structures and magnetic reconnection signatures in the turbulent magnetosheath

113 citations

21 papers

physics.space-ph2026★ 1 cited

Turbulent dynamo in the terrestrial magnetosheath

Zoltán Vörös, Owen Wyn Roberts, Yasuhito Narita +10

Dynamo action refers to energy exchange processes through which magnetic fields are generated at the expense of kinetic energy of the plasma flows. Dynamos can generate magnetic fi…

astro-ph.SR2024★ 4 cited

Variation of sunspot groups' polarity separation during their evolution

Judit Muraközy

During the emergence of sunspot groups the footpoints of their leading and following parts move apart. This diverging motion results in the stretching of the active regions, which…

astro-ph.GA2024★ 1 cited

Orbital dynamics in galactic potentials under mass transfer

Eduárd Illés, Dániel Jánosi, Tamás Kovács

Time-dependent potentials are common in galactic systems that undergo significant evolution, interactions, or encounters with other galaxies, or when there are dynamic processes li…

astro-ph.EP2024★ 7 cited

Mysterious non-detection of HeI (23S) transit absorption of GJ436b

M. S. Rumenskikh, M. L. Khodachenko, I. F. Shaikhislamov +4

Possible reasons for the non-detection of absorption in the metastable HeI(2^3S) line at transit observations of warm Neptune GJ436b, in spite of the well pronounced strong absorpt…

astro-ph.SR2023★ 19 cited

Asteroseismology and Spectropolarimetry of the Exoplanet Host Star Serpentis

Travis S. Metcalfe, Derek Buzasi, Daniel Huber +31

The bright star Ser hosts a hot Neptune with a minimum mass of 13.6 and a 15.5 day orbit. It also appears to be a solar analog, with a mean rotation period of 25.8 d…

physics.space-ph2023

Comparing 1-year GUMICS-4 simulations of the Terrestrial Magnetosphere with Cluster Measurements

Gabor Facsko, David Sibeck, Ilja Honkonen +18

We compare the predictions of the GUMICS4 global magnetohydrodynamic model for the interaction of the solar wind with the Earth's magnetosphere with Cluster~SC3 measurements for…