Effective Radius of Ice Particles in Cirrus and Contrails

• Published in: Journal of the atmospheric sciences 2011-02, Vol.68 (2), p.300-321
• Main Authors: SCHUMANN, U, MAYER, B, GIERENS, K, UNTERSTRASSER, S, JESSBERGER, P, PETZOLD, A, VOIGT, C, GAYET, J.-F
• Format: Article
• Language: English
• Subjects: Age; Atoms & subatomic particles; Clouds; Contrails; Cross sections; Crystals; Earth, ocean, space; Exact sciences and technology; External geophysics; Habits; Humidity; Ice; Meteorology; Moisture content; Optical analysis; Optics; Particle size distribution; Physics of the high neutral atmosphere; Radiative forcing; Remote sensing; Water content; Water depth
• ISSN: 0022-4928; 1520-0469
• DOI: 10.1175/2010JAS3562.1

This paper discusses the ratio C between the volume mean radius and the effective radius of ice particles in cirrus and contrails. The volume mean radius is proportional to the third root of the ratio between ice water content and number of ice particles, and the effective radius measures the ratio between ice particle volume and projected cross-sectional area. For given ice water content and number concentration of ice particles, the optical depth scales linearly with C. Hence, C is an important input parameter for radiative forcing estimates. The ratio C in general depends strongly on the particle size distribution (PSD) and on the particle habits. For constant habits, C can be factored into a PSD and a habit factor. The PSD factor is generally less than one, while the habit factor is larger than one for convex or concave ice particles with random orientation. The value of C may get very small for power-law PSDs with exponent n between -4 and 0, which is often observed. For such PSDs, most of the particle volume is controlled by a few large particles, while most of the cross-sectional area is controlled by the many small particles. A new particle habit mix for contrail cirrus including small droxtal-shape particles is suggested. For measured cirrus and contrails, the dependence of C on volume mean particle radius, ambient humidity, and contrail age is determined. For cirrus, C varies typically between 0.4 and 1.1. In contrails, C = 0.7 plus or minus 0.3, with uncertainty ranges increasing with the volume radius and contrail age. For the small particles in young contrails, the extinction efficiency in the solar range deviates considerably from the geometric optics limit.