Overview and update of the SPARC Data Initiative: comparison of stratospheric composition measurements from satellite limb sounders

The Stratosphere-troposphere Processes and their Role in Climate (SPARC) Data Initiative (SPARC, 2017) performed the first comprehensive assessment of currently available stratospheric composition measurements obtained from an international suite of space-based limb sounders. The initiative's main objectives were (1) to assess the state of data availability, (2) to compile time series of vertically resolved, zonal monthly mean trace gas and aerosol fields, and (3) to perform a detailed intercomparison of these time series, summarizing useful information and highlighting differences among datasets. The datasets extend over the region from the upper troposphere to the lower mesosphere (300–0.1 hPa) and are provided on a common latitude–pressure grid. They cover 26 different atmospheric constituents including the stratospheric trace gases of primary interest, ozone (O3) and water vapor (H2O), major long-lived trace gases (SF6, N2O, HF, CCl3F, CCl2F2, NOy), trace gases with intermediate lifetimes (HCl, CH4, CO, HNO3), and shorter-lived trace gases important to stratospheric chemistry including nitrogen-containing species (NO, NO2, NOx, N2O5, HNO4), halogens (BrO, ClO, ClONO2, HOCl), and other minor species (OH, HO2, CH2O, CH3CN), and aerosol. This overview of the SPARC Data Initiative introduces the updated versions of the SPARC Data Initiative time series for the extended time period 1979–2018 and provides information on the satellite instruments included in the assessment: LIMS, SAGE I/II/III, HALOE, UARS-MLS, POAM II/III, OSIRIS, SMR, MIPAS, GOMOS, SCIAMACHY, ACE-FTS, ACE-MAESTRO, Aura-MLS, HIRDLS, SMILES, and OMPS-LP. It describes the Data Initiative's top-down climatological validation approach to compare stratospheric composition measurements based on zonal monthly mean fields, which provides upper bounds to relative inter-instrument biases and an assessment of how well the instruments are able to capture geophysical features of the stratosphere. An update to previously published evaluations of O3 and H2O monthly mean time series is provided. In addition, example trace gas evaluations of methane (CH4), carbon monoxide (CO), a set of nitrogen species (NO, NO2, and HNO3), the reactive nitrogen family (NOy), and hydroperoxyl (HO2) are presented. The results highlight the quality, strengths and weaknesses, and representativeness of the different datasets. As a summary, the current state of our knowledge of stratospheric composition and variability is provided based on the overall consistency between the datasets. As such, the SPARC Data Initiative datasets and evaluations can serve as an atlas or reference of stratospheric composition and variability during the “golden age” of atmospheric limb sounding. The updated SPARC Data Initiative zonal monthly mean time series for each instrument are publicly available and accessible via the Zenodo data archive (Hegglin et al., 2020)

Planetary-wave-induced transport in the stratosphere

grantor: University of TorontoThe global mass circulation in the stratosphere is constrained by the downward control principle (Haynes et al. 1991). Stratospheric wave drag, produced by the breaking and dissipation of planetary waves, acts as a pump, drawing tracers from the equator to the pole and resulting in the observed Brewer-Dobson circulation. At present, the theoretical understanding of this process has limitations. It can be shown that for linear, small-amplitude waves, the Lagrangian mean velocities and the transformed Eulerian mean velocities are the same and are a direct result of the wave drag. However, it is not clear that this relationship holds in general; in particular, the stratosphere is clearly a nonlinear system with breaking planetary waves in the surf zone. Thus, while the existence of the wave-induced circulation is not under debate, its quantitative determination remains problematic. The purpose of this work is to include the effects of nonlinear, breaking waves by using a 3d primitive equations model to study the effect of the wave forcing on the traditional diagnostic quantities (the Eliassen-Palm flux divergence and the residual circulation) and to use off-line particle advection to quantify the resulting Lagrangian transport. Attention is deliberately focused on a weak forcing regime, so that sudden warmings do not occur, in order to test the theory in the cleanest possible context. It is shown that while the theory holds for small-amplitude and weakly nonlinear regimes, discrepancies arise in the strongly nonlinear regime. While the EP flux divergence is largely negative in the stratosphere, regions of reversed potential vorticity gradient lead to a positive EP flux divergence. Positive EP flux divergence can be associated with regions of dynamical instability, wherein there is in-situ generation of wave activity. Furthermore, the correspondence between the meridional residual and transport velocities becomes poor in regions where the flow is permitted to develop smaller scales through wave breaking. This is less true for the vertical transport and residual velocities, which seem to show better agreement, even in the surf zone and in regions of large amplitude waves. This is especially the case wherever particle paths are coherent, so that diabatic dispersion is minimized. The results from the primitive equations model are compared with those from the Canadian Middle Atmosphere Model to test the robustness of the results.Ph.D

Triacetin-based acetate supplementation as a chemotherapeutic adjuvant therapy in glioma.

Cancer is associated with epigenetic (i.e., histone hypoacetylation) and metabolic (i.e., aerobic glycolysis) alterations. Levels of N-acetyl-L-aspartate (NAA), the primary storage form of acetate in the brain, and aspartoacylase (ASPA), the enzyme responsible for NAA catalysis to generate acetate, are reduced in glioma; yet, few studies have investigated acetate as a potential therapeutic agent. This preclinical study sought to test the efficacy of the food additive Triacetin (glyceryl triacetate, GTA) as a novel therapy to increase acetate bioavailability in glioma cells. The growth-inhibitory effects of GTA, compared to the histone deacetylase inhibitor Vorinostat (SAHA), were assessed in established human glioma cell lines (HOG and Hs683 oligodendroglioma, U87 and U251 glioblastoma) and primary tumor-derived glioma stem-like cells (GSCs), relative to an oligodendrocyte progenitor line (Oli-Neu), normal astrocytes, and neural stem cells (NSCs) in vitro. GTA was also tested as a chemotherapeutic adjuvant with temozolomide (TMZ) in orthotopically grafted GSCs. GTA-induced cytostatic growth arrest in vitro comparable to Vorinostat, but, unlike Vorinostat, GTA did not alter astrocyte growth and promoted NSC expansion. GTA alone increased survival of mice engrafted with glioblastoma GSCs and potentiated TMZ to extend survival longer than TMZ alone. GTA was most effective on GSCs with a mesenchymal cell phenotype. Given that GTA has been chronically administered safely to infants with Canavan disease, a leukodystrophy due to ASPA mutation, GTA-mediated acetate supplementation may provide a novel, safe chemotherapeutic adjuvant to reduce the growth of glioma tumors, most notably the more rapidly proliferating, glycolytic and hypoacetylated mesenchymal glioma tumors