10Be deposition in ice cores is widely used for solar reconstructions, but its interpretation is complicated by volcanic influences. Using the state-of-the-art aerosol-climate model ECHAM6.3-HAM2.3-SALSA2.0: 10Be, we assess the impacts of three major volcanic eruptions: Agung (1963), El Chichón (1982) and Pinatubo (1991). All eruptions enhance stratospheric 10Be sedimentation, increasing atmospheric 10Be below the injection altitude for several months, followed by stratospheric 10Be depletion that takes years to recover. Increases in tropospheric 10Be and deposition coincide with periods of strong stratosphere–troposphere exchange. Aerosol-induced sedimentation significantly enhances polar 10Be deposition subsequent to the Pinatubo and El Chichón eruptions but plays a limited role after the Agung eruption. Sensitivity experiments reveal that higher SO2 injections generally lead to nonlinear increases in global 10Be deposition. These results underscore the need to account for volcanic influences when interpreting and modeling polar 10Be records following major eruptions.
Mangroves host many marine species and support fisheries in developing (sub)tropical countries. The suitability of mangrove habitats depends strongly thier the water chemistry. Here, we show how global warming and rising atmospheric CO2 will reduce dissolved oxygen and increase CO2 in mangrove waters. Observations from 23 mangrove-lined estuaries worldwide revealed that most sites already experience mild (34%–43% of the time) or severe (6%–32%) hypercapnic hypoxia, that is, high CO2 and low oxygen conditions. Hypercapnic hypoxia mostly occurs during low tide, at low-salinity sites, and in warm tropical regions. Climate change will decrease oxygen concentrations by 5%–35% and increase CO2 concentrations by 8%–60% in mangrove waters by 2100. Overall, hypercapnic hypoxia events will occur more frequently, last longer, and become more severe. These shifts will reduce mangrove biodiversity and deteriorate habitat quality for commercially valuable fish. The strongest impact is expected in tropical developing countries.
Deep convective clouds regulate Earth's energy and moisture budgets, yet their impact on the atmospheric boundary layer (BL) composition remains underexplored. Using long-term observations from three mid-latitude sites, we show that deep convection (DC) consistently enhances nighttime surface ozone and is often accompanied by modest increases in ultrafine particle concentrations. Within the BL, the condensational growth of these transported ultrafine particles may contribute up to 60% of total cloud condensation nuclei (CCN). Mass flux calculations suggest that short-lived convective cores (∼30 min) account for ∼2% of total vertical air mass transport relative to steady entrainment, increasing to ∼13% when the trailing stratiform regions are included. These results show that DC provides an episodic but efficient pathway linking the free troposphere and BL, influencing oxidant budgets, CCN variability, and climate forcing. Accurately representing this process in climate models may help reduce uncertainties in climate projections, under both preindustrial and present-day conditions.
The sporadic E (Es) layer is a prominent ionospheric irregularity mainly driven by vertical wind shear at mid-latitudes. Hereby we statistically investigate for the first time Es responses to variations of the northern polar vortex (represented by NAM index) using long-term ionosonde observations over Japan (44 years) and Australia (34 years). The analysis reveals clear polar vortex modulation of Es, with increasing/decreasing foEs on low/high NAM days over Japan and decreasing foEs over Australia on low NAM days with a time lag of 5–7 days. This hemispheric asymmetry is largely attributed to nearly anti-phase wind shear responses in two hemispheres. Our results demonstrate the modulation of deep connection between stratosphere dynamics and ionospheric irregularities, emphasizing the importance atmosphere-ionosphere coupling. It suggests that the NAM index could be used to increase the accuracy of Es layer prediction and serve as indicator for assessing the risk of Es layer occurrence in advance. This has practical implications for fields such as radiocommunications and over-the-horizon radar.
Substorms are often described by a loading-unloading cycle, where onset follows gradual accumulation of solar wind magnetic flux in the magnetosphere. Yet observations indicate that intense substorms can also be directly driven, though the underlying mechanism remains unresolved. For the first time, global observations strongly indicate that substorm triggering is linked to enhanced dayside-driven convection and Region 1 FAC, supported by simulations. At 17:17UT during the May 2024 superstorm, a shock-compressed southward interplanetary magnetic field enhanced sunward convection and auroral currents. These rapidly extended to the nightside, initiating substorm expansion within 6 min. Simulations reproduce this response, revealing that dayside-driven convection of closed field lines depleted nightside flux and thinned the current sheet. This lowered onset threshold and triggered substorm expansion with negligible flux loading. Following onset, nightside flux loading became significant as a reconnection X-line formed near 10 Earth radii, extended azimuthally, and supported a global substorm current wedge.
Accurate forecasts of near-landfall TC characteristics (direction, translation speed, and intensity) are essential for timely disaster preparedness. Using best-track data (1951–2023), this study reveals a significant pre-landfall acceleration of TCs along the South China coast, with translation speed increasing by 35.5% and 16.4% during the 24 hr prior to landfall for eastbound and westbound cases, respectively. This acceleration is primarily contributed by the normal component of the translation vector. For westbound TCs, translation speed and its normal component increase with intensity, particularly at typhoon strength and above. Numerical simulations and diagnostic analyses attribute the acceleration to horizontal advection and diabatic heating, primarily driven by land-induced asymmetric flow and convection. These findings strengthen the current understanding of TC motion dynamics and support more effective disaster prevention and mitigation strategies as TCs approach coastal regions.
Pulse-like infrasound accompanying volcanic phenomena sometimes suggests interaction with water at the crater. We focus on pulse-like infrasound observed at Semisopochnoi Island in the Aleutian Arc, Alaska, during the phreatomagmatic activity on 13 July 2021. Overflight observations confirmed a small, ephemeral water lake on the crater floor in June 2021. We examined temporal variations in pulse-like infrasound activity, seismoacoustic amplitudes, and spectral characteristics. Pulse-like infrasound activity gradually became intermittent and waned at the end of the day. Seismic-infrasonic amplitude ratio decreased, while the infrasound frequency index increased with time. These results suggest less interaction with water due to drying out of the vent. Satellite observations also show increased ground surface temperatures inside the crater from 13 to 14 July. Numerical simulation suggests a significant topographic effect on the waveform and spectrum of the pulse-like infrasound, which should be considered before interpreting the source process.

