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Adaptively Refined MHD Solutions of Solar Eruptive Events
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GLM Observations from the Hunga Tonga Eruption on 15 January 2022 and thoughts on lightning data fusion
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From source to surface: Volcano geodesy and [some] advances in real-time eruption forecasting
No abstract provided
Volcanic Eruptions and Effects on our Climate
Volcanoes are an integral part of the Earth system and are formed by intrusions of magma that 'bubble up’ from Earth’s interior (e.g., lava lamp). They can form above thin areas of the Earth’s crust/ lithosphere known as ‘hot spots or mantle plumes’ such as the Hawaiian Islands or Yellowstone National Park. More commonly they form along ‘subduction zones’ where the thinner oceanic tectonic plates slide below the thicker continental plates. Many of the most active (and violent) volcanos lie along subduction zones known as the Pacific 'Ring of Fire’.
Another Look at Erupting Minifilaments at the Base of Solar X-Ray Polar Coronal “Standard” and “Blowout” Jets.
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Quantifying Energy Release in Solar Flares and Solar Eruptive Events: New Frontiers with a Next-Generation Solar Radio Facility
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Stratospheric Impacts of the Hunga Tonga-Hunga Ha’apai Eruption Water Vapor Injection
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Stratospheric Impacts of the Hunga Tonga-Hunga Ha’apai Eruption Water Vapor Injection
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The Impact of the January 2022 Eruptions of Hunga Tonga-Hunga Ha’apai on Stratospheric Ozone in the NASA GEOS Earth System Model
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Particle Size Distribution Parameters From Sage III/ISS Extinction Spectra, with Application to the 2022 Hunga Tonga Eruption
- SAGE data have been used to estimate particle size distribution (PSD) parameters - Mode radius - Distribution width (σ) - Measurement error is often neglected - Wrana et al. 2021 included error - Bimodal distributions have not been evaluated
Solar Coronal Jets, the Magnetic Flux Changes Leading to Jets, and Implications for Eruptions on Larger and Smaller Size Scales
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