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  • Continuous light  (1)
  • Animals
  • Plasma Physics
  • 2015-2019  (2)
  • 2019  (2)
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  • 2015-2019  (2)
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  • 1
    Publication Date: 2022-05-25
    Description: Author Posting. © The Author(s), 2018. This is the author's version of the work. It is posted here under a nonexclusive, irrevocable, paid-up, worldwide license granted to WHOI. It is made available for personal use, not for redistribution. The definitive version was published in Organic Geochemistry 125 (2018): 70-81, doi: 10.1016/j.orggeochem.2018.08.008.
    Description: Reconstructions of climate using leaf wax D/H ratios (δDwax) require accounting for the apparent isotopic fractionation (εapp) between plant source water and waxes. There have been conflicting publications on whether plants in the Arctic growing under 24-hour continuous light, fractionate less than temperate and tropical plants. In this study, we examine the effect of diurnal light (DL) versus 24-hour continuous light (CL) on the isotopic composition of leaf n-alkanes and n-acids in greenhouse experiments using two common Arctic plants (Eriophorum vaginatum, or tussock cottongrass and Betula nana, or dwarf birch). For E. vaginatum, the δDwax values of various wax homologues were 5–11‰ more positive for CL plants relative to their DL counterparts, whereas for B. nana, CL waxes were 3–24‰ more negative, suggesting that daylight length is not a unifying control on leaf wax D/H ratios of Arctic plants. The δ13Cwax of B. nana was more negative for plants grown in continuous light compared to diurnal light, reflecting lower water-use efficiency, associated with prolonged stomatal opening in the CL treatment. We modeled the impact of increasing stomatal conductance and effective flow path lengths (mimicking variable leaf morphologies) on the isotopic composition of leaf waters (δDlw) and find that variations in leaf-water enrichment may explain the variable δDwax responses seen between E. vaginatum and B. nana. We suggest that between-species differences in the δDlw response to light, and differences in the utilization of stored carbohydrates, were important for governing δDwax. Our greenhouse results suggest that Arctic plant leaf waxes do not consistently display reduced εapp values as a result of 24-hour day light, providing additional support for field observations.
    Description: We thank Fred Jackson and Chris Claussen of the Brown University Plant Environmental Center for assistance with growth chambers, Chelsea Parker for assistance in plant care, and Rafael Tarozo for laboratory assistance. We want to thank Trevor Porter and three anonymous reviewers for constructive comments to improve the manuscript. This work was funded by NSF Arctic Natural Sciences grant 1503846 to Yongsong Huang and James Russell and NSF-OPP grant 1603214 to Anne Giblin. We also acknowledge graduate support for Will Daniels from the Brown-MBL joint graduate program and the Institute at Brown for Environment and Society.
    Keywords: Leaf waxes ; Hydrogen isotopes ; Carbon isotopes ; Growth experiment ; Arctic ; Continuous light
    Repository Name: Woods Hole Open Access Server
    Type: Preprint
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  • 2
    Publication Date: 2019-11-28
    Description: Electrons are accelerated to nonthermal energies at shocks in space and astrophysical environments. While shock drift acceleration (SDA) has been considered a key process of electron acceleration at Earths bow shock, it has also been recognized that SDA needs to be combined with an additional stochastic process to explain the observed power-law energy spectra. Here, we show mildly energetic (0.5 keV) electrons are locally scattered (and accelerated while being conned) by magnetosonic-whistler waves within the shock transition layer, especially when the shock angle is large ((sub Bn) approximately equal or greater than 70). When measured by the Magnetospheric Multiscale mission at a high cadence, 0.5 keV electron ux increased exponentially in the shock transition layer. However, the ux prole was not entirely smooth and the uctuation showed temporal/spectral association with large-amplitude (B/B ~ 0.3), low-frequency (approximately equal or less than 0.1 (sub ce) where (sub ce) is the cyclotron frequency), obliquely propagating ((sub kB) ~ 3060, where (sub kB) is the angle between the wave vector and background magnetic eld) whistler waves, indicating that the particles were interacting with the waves. Particle simulations demonstrate that, although linear cyclotron resonances with 0.5 keV electrons are unlikely due to the obliquity and low frequencies of the waves, the electrons are still scattered beyond 90 pitch angle by (1) resonant mirroring (transit-time damping), (2) non-resonant mirroring, and (3) subharmonic cyclotron resonances. Such coupled nonlinear scattering processes are likely to provide the stochasticity needed to explain the power-law formation.
    Keywords: Plasma Physics
    Type: GSFC-E-DAA-TN75966 , The Astrophysical Journal (ISSN 0004-637X) (e-ISSN 1538-4357); 886; 1; 53
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