Open ilaria-quaglia opened 1 year ago
Sea salt burden increases of about 0.5 Tg in CARMA16_Ks0.4 compared with CARMA14, but is still 3.0 Tg lower than in MAM4 (average over 1990). This change also affected other species, particularly DUST.
However, the optical depth of sea salt decreases globally by 0.005, with positive changes only in some regions of the land.
@ilaria-quaglia, thanks so much! Very interesting. I checked the kappa for sea-salt, and it is actually above 1, so I guess this is not what we want anyways. We could run a test where we increase it to 1.5 or even 2. still in the range of observations. However, I think that as Brian Toon has noted without more bins, to that extent, we may not have much success. Let's continue working on the 22-bin model (larger bins for dust and sea-salt and see how that changes things). I will start some new MAM runs for 1980-2000 soon.
We discarded the idea of changing Kappa_SALT and we consider a new simulation without SOA photolysis. The first figure show the volume mixing ratio averaged over 1990 in CARMA and over 2016-2018 in MAM.
The second figure shows the differences between CARMA and MAM.
@ilaria-quaglia Thanks! Could you add the AOD comparisons for the different species? I am hoping that we are now higher than we were before....
Figure 1 shows the total AOD at 550 nm compared to MERRA, and the maps are averaged over the available volcanic quiescence period. The higher values in FWmaHIST_CARMA_nudged_16_no_soa_phot are due to the SOA (see Figure 2).
Figure 2 shows the global AOD at 550 nm for each species and average values over the available volcanic quiescence period are summarised in the following table.
We want to increase sea salt burden and extinction by modifying sea salt removal through hygroscopicity (Kappa_SALT from 1.0 to 0.4).
Cases in /glade/work/iquaglia/cases/