Prépublication
· 2026 arXiv
EN
A potentially super El Niño is forecasted in 2026, raising the need to anticipate land carbon-cycle risks before its impacts unfold. We develop a prospective early-warning framework that uses dynamic global vegetation models driven by an ensemble of ECMWF seas...
Xiaomeng Du, Runda Jiang et al.
#physics.ao-ph
Prépublication
· 2026 arXiv
EN
This work investigates the incidence of rapid ice-loss events in the Arctic, in which a substantial fraction of September sea-ice is lost in only a few years. Such events are seen to occur in climate model simulations forced with increasing greenhouse gas conc...
Matthew Patterson, Ioana Colfescu et al.
#physics.ao-ph
Prépublication
· 2026 arXiv
EN
Ensemble forecasts from the ECMWF's Integrated Forecasting System (IFS) and the Artificial Intelligence Forecasting System (AIFS-ENS) are compared using a multi-dimensional evaluation framework. Within this framework, the uncertainty is interpreted as the line...
Martin Bonte, Stéphane Vannitsem
#physics.ao-ph
Prépublication
· 2026 arXiv
EN
Aim. We try to understand the interaction of eccentricity tide and convection in icy satellites. Method. We use the numerical calculation of rotating convection with eccentricity tide in a spherical shell. Results. We have the following results. (1) Energy sca...
Jiachen Zheng, Xing Wei
#astro-ph.EP
Prépublication
· 2026 arXiv
EN
We present two and three dimensional direct numerical simulations of planar intrusions injected from a continuously supplied, narrow source into a linearly stratified ambient at the level of neutral buoyancy. The evolution passes through three phases. A lamina...
Hai Duc Vu, Murray Rudman et al.
#physics.flu-dyn
Prépublication
· 2026 arXiv
EN
A long-standing challenge in climate science since the Charney Report in 1979 is to determine how much the Earth's climate warms in response to a unit external energy input at the top of the atmosphere (TOA). In this study, we show from first principles that t...
Ming Cai, Jie Sun et al.
#physics.ao-ph
Prépublication
· 2026 arXiv
EN
Deep-learning models increasingly rival numerical simulation in Earth-system forecasting, yet forecast error alone cannot determine whether their learned input-output dependencies are physically consistent. Here we introduce sensitivity fidelity as an addition...
Qi Chen, Peng Zhan et al.
#cs.LG
Prépublication
· 2026 arXiv
EN
The notion of tipping points and related terminology have so far had inconsistent and sometimes confusing definitions in both scientific and popular literature. While it is difficult for the scientific community to align popular usage of the term tipping point...
Niklas Boers, Robert E. Kopp et al.
#physics.ao-ph
Prépublication
· 2026 arXiv
EN
Trends with stellar elemental abundances and condensation temperature have been proposed as a possible tracer of rocky planet formation. Here we present an alternative explanation, where we show that stellar activity (star spots) can also cause apparent abunda...
Andrew R. Casey, Megan Bedell et al.
#astro-ph.SR
Prépublication
· 2026 arXiv
EN
The cosmic reheating is an important epoch in the very early Universe, and has significant impacts on the primordial black hole (PBH) abundance and the scalar-induced gravitational wave (SIGW) spectrum. The relevant energy scale and the constituents of cosmic...
Qi-Lin Yang, Shi-Jie Wang et al.
#astro-ph.CO
Prépublication
· 2026 arXiv
EN
Recent exoplanet surveys reveal a systematic trend in the mass ratios of giant planet pairs ($> 30 M_\oplus$). Although the $M_{outer}/M_{inner}$ is broadly centered near unity, it exhibits a dependence on orbital separation. Compact pairs tend to have compara...
Bixuan Zhao, Hui Zhang et al.
#astro-ph.EP
Prépublication
· 2026 arXiv
EN
Ongoing stage IV galaxy surveys such as DESI or Euclid offer an unprecedented amount of information to study the large-scale structure of the Universe by mapping tens of millions of galaxies. Within the context of cosmic voids, already released and future cata...
Óscar Monllor-Berbegal, Susana Planelles et al.
#astro-ph.CO