TY - JOUR
T1 - Scaling Laws for Light Absorption Enhancement Due to Nonrefractory Coating of Atmospheric Black Carbon Aerosol
AU - Chakrabarty, Rajan K.
AU - Heinson, William R.
N1 - Publisher Copyright:
© 2018 American Physical Society.
PY - 2018/11/19
Y1 - 2018/11/19
N2 - Black carbon (BC) aerosol, the strongest absorber of visible solar radiation in the atmosphere, contributes to a large uncertainty in direct radiative forcing estimates. A primary reason for this uncertainty is inaccurate parametrizations of the BC mass absorption cross section (MACBC) and its enhancement factor (EMACBC) - resulting from internal mixing with nonrefractory and nonlight absorbing materials - in climate models. Here, applying scaling theory to numerically exact electromagnetic calculations of simulated BC particles and observational data on BC light absorption, we show that MACBC and EMACBC evolve with increasing internal mixing ratios in simple power-law exponents of 1/3. Remarkably, MACBC remains inversely proportional to the wavelength of light at any mixing ratio. When mixing states are represented using mass-equivalent core-shell spheres, as is done in current climate models, it results in significant underprediction of MACBC. We elucidate the responsible mechanism based on shielding of photons by a sphere's skin depth and establish a correction factor that scales with a power-law exponent.
AB - Black carbon (BC) aerosol, the strongest absorber of visible solar radiation in the atmosphere, contributes to a large uncertainty in direct radiative forcing estimates. A primary reason for this uncertainty is inaccurate parametrizations of the BC mass absorption cross section (MACBC) and its enhancement factor (EMACBC) - resulting from internal mixing with nonrefractory and nonlight absorbing materials - in climate models. Here, applying scaling theory to numerically exact electromagnetic calculations of simulated BC particles and observational data on BC light absorption, we show that MACBC and EMACBC evolve with increasing internal mixing ratios in simple power-law exponents of 1/3. Remarkably, MACBC remains inversely proportional to the wavelength of light at any mixing ratio. When mixing states are represented using mass-equivalent core-shell spheres, as is done in current climate models, it results in significant underprediction of MACBC. We elucidate the responsible mechanism based on shielding of photons by a sphere's skin depth and establish a correction factor that scales with a power-law exponent.
UR - https://www.scopus.com/pages/publications/85057317382
U2 - 10.1103/PhysRevLett.121.218701
DO - 10.1103/PhysRevLett.121.218701
M3 - Article
C2 - 30517814
AN - SCOPUS:85057317382
SN - 0031-9007
VL - 121
JO - Physical Review Letters
JF - Physical Review Letters
IS - 21
M1 - 218701
ER -