A New Instrument for Balloon-Borne In Situ Aerosol Size Distribution Measurements, the Continuation of a 50 Year Record of Stratospheric Aerosols Measurements

被引:5
|
作者
Kalnajs, Lars E. [1 ]
Deshler, Terry [1 ]
机构
[1] Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO 80309 USA
基金
美国国家科学基金会;
关键词
aerosols; instrumentation; validation; COMPLEX REFRACTIVE-INDEX; SULFURIC-ACID; CORRELATIVE MEASUREMENTS; SAM-II; SATELLITE; DUSTSONDES;
D O I
10.1029/2022JD037485
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
Profiles of stratospheric aerosol size distributions have been measured using balloon-borne in situ optical particle counters, from Laramie, Wyoming (41 degrees N) since 1971. In 2019, this measurement record transitioned to the Laboratory for Atmospheric and Space Physics (LASP) in Boulder, Colorado (40 degrees N). The new LASP Optical Particle Counter (LOPC), the fourth generation of instruments used for this record, is smaller and lighter (2 kg) than prior instruments, measures aerosols with diameters >= 0.3-30 mu m in up to 450 size bins, with a flow rate of 20 L min(-1). The improved size resolution enables the complete measurement of size distributions, and calculation of aerosol extinction without fitting a priori distribution shapes. The higher flow provides the sensitivity required to measure super-micron particles in the stratosphere. The LOPC has been validated against prior Wyoming OPCs, through joint flights, laboratory comparisons, and statistical comparisons with the Wyoming record. The agreement between instruments is generally within the measurement uncertainty of +/- 10%-20% in sizing and +/- 10% in concentration, and within +/- 40% for calculated aerosol moments. The record is being continued with balloon soundings every 2 months from Colorado, coordinated with measurements of aerosol extinction from the SAGE III instrument on the International Space Station. Comparisons of aerosol extinction from the remote and in situ platforms have shown good agreement in the stratosphere, particularly for wavelengths < 755 nm and altitudes < 25 km. For extinction wavelengths > 1,021 nm and altitudes above 25 km SAGE III/International Space Station extinction has a low bias relative to the in situ measurements, yet still within the +/- 40% uncertainty.
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页数:14
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