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Archive
by Flamant, C., Chaboureau, J.-P., Chazette, P., Di Girolamo, P., Bourrianne, T., Totems, J. and Cacciani, M.
Abstract:
The study is focused on Intensive Observation Period (IOP) 14 of the Hydrological Cycle in the Mediterranean Experiment first Special Observing Period (HyMeX SOP 1) that took place from 17 to 19 October 2012 and was dedicated to the study of orographic rain in the Cévennes–Vivarais (CV) target area. During this IOP a dense dust plume originating from northern Africa (the Maghreb and Sahara) was observed to be transported over the Balearic Islands towards the south of France. The plume was characterized by an aerosol optical depth between 0.2 and 0.8 at 550 nm, highly variable in time and space over the western Mediterranean Basin. The impact of this dust plume, the biggest event observed during the 2-month-long HyMeX SOP 1, on the precipitation over the CV area has been analyzed using high-resolution simulations from the convection permitting mesoscale model Meso-NH (mesoscale non-hydrostatic model) validated against measurements obtained from numerous instruments deployed specifically during SOP 1 (ground-based/airborne water vapor and aerosol lidars, airborne microphysics probes) as well as space-borne aerosol products. The 4-day simulation reproduced realistically the temporal and spatial variability (including the vertical distribution) of the dust. The dust radiative impact led to an average 0.6 K heating at the altitude of the dust layer in the CV area (and up to +3 K locally) and an average 100 J kg−1 increase of most unstable convective available potential energy (and up to +900 J kg−1 locally) with respect to a simulation without prescribed dust aerosols. The rainfall amounts and location were only marginally affected by the dust radiative effect, even after 4 days of simulation. The transient nature of this radiative effect in dynamical environments such as those found in the vicinity of heavy precipitation events in the Mediterranean is not sufficient to impact 24 h of accumulated rainfall in the dust simulation.
Reference:
Flamant, C., Chaboureau, J.-P., Chazette, P., Di Girolamo, P., Bourrianne, T., Totems, J. and Cacciani, M., 2015: The radiative impact of desert dust on orographic rain in the Cévennes–Vivarais area: a case study from HyMeXAtmospheric Chemistry and Physics, 15, 12231-12249.
Bibtex Entry:
@Article{Flamant2015,
  Title                    = {The radiative impact of desert dust on orographic rain in the Cévennes–Vivarais area: a case study from HyMeX},
  Author                   = {Flamant, C. and Chaboureau, J.-P. and Chazette, P. and Di Girolamo, P. and Bourrianne, T. and Totems, J. and Cacciani, M.},
  Journal                  = {Atmospheric Chemistry and Physics},
  Year                     = {2015},

  Month                    = {November},
  Number                   = {21},
  Pages                    = {12231-12249},
  Volume                   = {15},

  __markedentry            = {[hymexw:]},
  Abstract                 = {The study is focused on Intensive Observation Period (IOP) 14 of the Hydrological Cycle in the Mediterranean Experiment first Special Observing Period (HyMeX SOP 1) that took place from 17 to 19 October 2012 and was dedicated to the study of orographic rain in the Cévennes–Vivarais (CV) target area. During this IOP a dense dust plume originating from northern Africa (the Maghreb and Sahara) was observed to be transported over the Balearic Islands towards the south of France. The plume was characterized by an aerosol optical depth between 0.2 and 0.8 at 550 nm, highly variable in time and space over the western Mediterranean Basin. The impact of this dust plume, the biggest event observed during the 2-month-long HyMeX SOP 1, on the precipitation over the CV area has been analyzed using high-resolution simulations from the convection permitting mesoscale model Meso-NH (mesoscale non-hydrostatic model) validated against measurements obtained from numerous instruments deployed specifically during SOP 1 (ground-based/airborne water vapor and aerosol lidars, airborne microphysics probes) as well as space-borne aerosol products. The 4-day simulation reproduced realistically the temporal and spatial variability (including the vertical distribution) of the dust. The dust radiative impact led to an average 0.6 K heating at the altitude of the dust layer in the CV area (and up to +3 K locally) and an average 100 J kg−1 increase of most unstable convective available potential energy (and up to +900 J kg−1 locally) with respect to a simulation without prescribed dust aerosols. The rainfall amounts and location were only marginally affected by the dust radiative effect, even after 4 days of simulation. The transient nature of this radiative effect in dynamical environments such as those found in the vicinity of heavy precipitation events in the Mediterranean is not sufficient to impact 24 h of accumulated rainfall in the dust simulation.},
  Copublication            = {7: 5 Fr, 2 It},
  Doi                      = {10.5194/acp-15-12231-2015},
  Owner                    = {hymexw},
  Timestamp                = {2016.01.07},
  Url                      = {http://www.atmos-chem-phys.net/15/12231/2015/}
}