In Situ Aerosol Size Spectra Measurements in the Austral Polar Vortex Before and After the Hunga Tonga-Hunga Ha'apai Volcanic Eruption

IF 4.6 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY
Terry Deshler, Lars E. Kalnajs, Matthew Norgren, Yunqian Zhu, Jun Zhang
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Abstract

Aerosol from the Hunga Tonga-Hunga Ha'apai (HT-HH) volcanic eruption (20.6°S) in January 2022 were not incorporated into the austral polar vortex until the following year, March 2023. Within the polar vortex in situ profiles of aerosol size spectra were completed in the austral autumns of 2019 and 2023, from McMurdo Station, Antarctica (78˚S), 30 months prior to and 15 months after the HT-HH eruption. The measurements indicate that the HT-HH impact on aerosol size was primarily confined to particles with diameters >0.5 μm leading to differences in aerosol mass, surface area, and extinction from factors of 2–4 at the volcanic layer's peak below 20 km, increasing to ratios of 5–10 above 20 km. Effective radius, with radiative and microphysical implications, increased from ∼0.2 to ∼0.3 μm. An Earth system model with a modal aerosol package compares favorably with the in situ measurements of the HT-HH aerosol impact.

Abstract Image

洪加-汤加-洪加-哈帕伊火山爆发前后澳大拉西亚极地漩涡气溶胶粒度光谱原位测量结果
2022 年 1 月洪加汤加-洪加哈帕伊(HT-HH)火山爆发(南纬 20.6 度)产生的气溶胶直到第二年,即 2023 年 3 月才被纳入澳大利亚极地漩涡。在 HT-HH 火山喷发前 30 个月和喷发后 15 个月的 2019 年和 2023 年秋季,从南极洲麦克默多站(南纬 78˚)完成了极地漩涡内气溶胶粒度光谱的原位剖面测量。测量结果表明,HT-HH 对气溶胶大小的影响主要局限于直径为 0.5 微米的颗粒,导致气溶胶质量、表面积和消光的差异,在 20 千米以下的火山层峰值为 2-4 倍,在 20 千米以上为 5-10 倍。具有辐射和微物理影响的有效半径从 0.2 μm 增加到 0.3 μm。一个具有气溶胶模态包的地球系统模型与对 HT-HH 气溶胶影响的实地测量结果进行了比较。
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来源期刊
Geophysical Research Letters
Geophysical Research Letters 地学-地球科学综合
CiteScore
9.00
自引率
9.60%
发文量
1588
审稿时长
2.2 months
期刊介绍: Geophysical Research Letters (GRL) publishes high-impact, innovative, and timely research on major scientific advances in all the major geoscience disciplines. Papers are communications-length articles and should have broad and immediate implications in their discipline or across the geosciences. GRLmaintains the fastest turn-around of all high-impact publications in the geosciences and works closely with authors to ensure broad visibility of top papers.
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