Characterizing volcanic ash density and its implications on settling dynamics

Journal of Geophysical Research: Atmospheres American Geophysical Union 129:2 (2024) e2023JD039903

Authors:

Woon Sing Lau, Roy Grainger, Isabelle Taylor

Abstract:

Volcanic ash clouds are carefully monitored as they present a significant hazard to humans and aircraft. The primary tool for forecasting the transport of ash from a volcano is dispersion modelling. These models make a number of assumptions about the size, sphericity and density of the ash particles. Few studies have measured the density of ash particles or explored the impact that the assumption of ash density might have on the settling dynamics of ash particles. In this paper, the raw apparent density of 23 samples taken from 15 volcanoes are measured with gas pycnometry, and a negative linear relationship is found between the density and the silica content. For the basaltic ash samples, densities were measured for different particle sizes, showing that the density is approximately constant for particles smaller than 100 µm, beyond which it decreases with size. While this supports the current dispersion model used by the London Volcanic Ash Advisory Centre (VAAC), where the density is held at a constant (2.3 g cm-3), inputting the measured densities into a numerical simulation of settling velocity reveals a primary effect from the silica content changing this constant. The VAAC density overestimates ash removal times by up to 18 %. These density variations, including those varying with size beyond 100 µm, also impact short-range particle-size distribution (PSD) measurements and satellite retrievals of ash.

Modeling Noncondensing Compositional Convection for Applications to Super-Earth and Sub-Neptune Atmospheres

The Astrophysical Journal American Astronomical Society 961:1 (2024) 35

Authors:

Namrah Habib, Raymond T Pierrehumbert

Quasi-Biennial Oscillation

Chapter in Atmospheric Oscillations: Sources of Subseasonal-to-Seasonal Variability and Predictability, (2024) 253-275

Authors:

Y Wang, J Rao, Z Ju, SM Osprey

Abstract:

The Quasi-Biennial Oscillation (QBO) is one of the most cyclic phenomena in the atmosphere except for the annular and diurnal cycles, which provide the predictability source for subseasonal-to-seasonal forecasts on the globe. The QBO is generated by the interaction between the background circulation and the equatorial waves, which cover a wide spectrum consisting of those that are eastward-and westward-propagating. The QBO can affect the climate in both the Northern and Southern Hemispheres through at least three dynamic pathways, including the stratospheric polar vortex pathway, the subtropical downward-arching zonal wind pathway, and the tropical convection pathway. The impact of the QBO on the extratropics is projected to strengthen in future scenario experiments, although the maximum QBO wind magnitude gradually decreased in recent decades. As a newly emerging feature, the QBO disruption during the westerly phase is mainly caused by the extremely active Rossby waves from the extratropics. The QBO disruptions are likely to increase in a warmer climate background.

Energy‐meteorology education workshop at the International Conference on Energy and Meteorology

Weather Wiley 79:1 (2024) 34-35

Authors:

Matthew Wright, Juan A Añel, Hannah Mallinson

Global warming may be behind an increase in the frequency and intensity of cold spells

The Conversation, 2024

Authors:

B. Monge-Sanz

Abstract: