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  • 1
    Publication Date: 2024-04-22
    Description: Phenological responses to climate change frequently vary among trophic levels, which can result in increasing asynchrony between the peak energy requirements of consumers and the availability of resources. Migratory birds use multiple habitats with seasonal food resources along migration flyways. Spatially heterogeneous climate change could cause the phenology of food availability along the migration flyway to become desynchronized. Such heterogeneous shifts in food phenology could pose a challenge to migratory birds by reducing their opportunity for food availability along the migration path and consequently influencing their survival and reproduction. We develop a novel graph-based approach to quantify this problem and deploy it to evaluate the condition of the heterogeneous shifts in vegetation phenology for 16 migratory herbivorous waterfowl species in Asia. We show that climate change-induced heterogeneous shifts in vegetation phenology could cause a 12% loss of migration network integrity on average across all study species. Species that winter at relatively lower latitudes are subjected to a higher loss of integrity in their migration network. These findings highlight the susceptibility of migratory species to climate change. Our proposed methodological framework could be applied to migratory species in general to yield an accurate assessment of the exposure under climate change and help to identify actions for biodiversity conservation in the face of climate-related risks.
    Keywords: bird migration ; climate change ; graph-based approach ; heterogeneous shifts ; network integrity ; phenological asynchrony ; vegetation phenology
    Repository Name: National Museum of Natural History, Netherlands
    Type: info:eu-repo/semantics/article
    Format: application/pdf
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  • 2
    Publication Date: 2016-07-08
    Description: The MESSENGER spacecraft while in orbit about Mercury observed highly localized, ~3-s-long reductions in the dayside magnetospheric magnetic field, with amplitudes up to 90% of the ambient intensity. These magnetic field depressions are termed cusp filaments because they were observed from just poleward of the magnetospheric cusp to mid-latitudes, i.e., ~55° to 85° N. We analyzed 345 high- and low-altitude cusp filaments identified from MESSENGER magnetic field data to determine their physical properties. Minimum variance analysis indicates that most filaments resemble cylindrical flux tubes within which the magnetic field intensity decreases toward its central axis. If the filaments move over the spacecraft at an estimated magnetospheric convection speed of ~35 km/s, then they have a typical diameter of ~105 km or ~7 gyro-radii for 1 keV H + ions in a 300 nT magnetic field. During these events, MESSENGER's Fast Imaging Plasma Spectrometer observed H + ions with magnetosheath-like energies. MESSENGER observations during the spacecraft's final low-altitude campaign revealed that these cusp filaments likely extend down to Mercury's surface. We calculated an occurrence-rate-normalized integrated particle precipitation rate onto the surface from all filaments of (2.70 ± 0.09) × 10 25  s -1 . This precipitation rate is comparable to published estimates of the total precipitation rate in the larger-scale cusp. Overall, the MESSENGER observations analyzed here suggest that cusp filaments are the magnetospheric extensions of the flux transfer events that form at the magnetopause as a result of localized magnetic reconnection.
    Print ISSN: 0148-0227
    Topics: Geosciences , Physics
    Published by Wiley on behalf of American Geophysical Union (AGU).
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  • 3
    Publication Date: 2015-05-07
    Description: MESSENGER magnetic field and plasma measurements taken during crossings of Mercury's magnetotail from 2011 to 2014 have been examined for evidence of substorms. A total of 26 events were found during which an Earth-like growth phase was followed by clear near-tail expansion phase signatures. During the growth phase, just as at Earth, the thinning of the plasma sheet and the increase of the magnetic field intensity in the lobe is observed, but the fractional increase in field intensity could be ~ 3 to 5 times that at Earth. The average time scale of the growth phase is ~ 1 min . The dipolarization that marks the initiation of the substorm expansion phase is only a few seconds in duration. During the expansion phase, lasting ~ 1 min , the plasma sheet is observed to thicken and engulf the spacecraft. The duration of the substorm observed in this paper is consistent with previous observations of Mercury's Dungey cycle. The reconfiguration of the magnetotail during Mercury's substorm is very similar to that at Earth despite its very compressed time scale.
    Print ISSN: 0094-8276
    Electronic ISSN: 1944-8007
    Topics: Geosciences , Physics
    Published by Wiley on behalf of American Geophysical Union (AGU).
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  • 4
    Publication Date: 2015-12-09
    Description: Surface flow redistribution on flat ground from crusted bare soil to vegetated patches following intense rainfall events elevates plant available water above that provided by rainfall. The significance of this surface water redistribution to sustaining vegetation in arid and semi-arid regions is undisputed. What is disputed is the quantity and spatial distribution of the redistributed water. In eco-hydrological models, such non-uniform flows are described using the Saint-Venant equation (SVE) subject to a Manning roughness coefficient closure. To explore these assumptions in the most idealized setting, flume experiments were conducted using rigid cylinders representing rigid vegetation with varying density. Flow was induced along the streamwise x direction by adjusting the free water surface height H ( x ) between the upstream and downstream boundaries mimicking the non-uniformity encountered in nature. In natural settings, such H ( x ) variations arise due to contrasts in infiltration capacity and ponded depths during storms. The measured H ( x ) values in the flume were interpreted using the SVE augmented with progressively elaborate approximations to the roughness representation. The simplest approximation employs a friction factor derived from a drag coefficient ( C d ) for isolated cylinders in a locally (but not globally) uniform flow and upscaled using the rod density that was varied across experiments. Comparison between measured and modeled H ( x ) suggested that such a ‘naïve' approach over-predicts H ( x ). Blockage was then incorporated into the SVE model calculations but resulted in underestimation of H ( x ). Biases in modeled H ( x ) suggest that C d must be varying in x beyond what a local or bulk Reynolds number predicts. Inferred C d ( x ) from the flume experiments exhibited a near-parabolic shape most peaked in the densest canopy cases. The outcome of such C d ( x ) variations are then summarized in a bulk resistance formulation that may be beneficial to modeling runon-runoff processes on shallow slopes using SVE. This article is protected by copyright. All rights reserved.
    Print ISSN: 0043-1397
    Electronic ISSN: 1944-7973
    Topics: Architecture, Civil Engineering, Surveying , Geography
    Published by Wiley on behalf of American Geophysical Union (AGU).
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  • 5
    Publication Date: 2014-11-12
    Description: The current system associated with the boundary of plasma bubbles in the Earth's magnetotail has been studied by employing Cluster multi-point observations. We have investigated the currents in both the dipolarization front (DF, leading edge of the plasma bubble) and the trailing edge of the plasma bubble. The distribution of currents at the edge indicates that there is a current circuit in the boundary of a plasma bubble. The field-aligned currents (FACs) in the trailing edge of the plasma bubble are flowing toward the ionosphere (downward) on the dawnside and away from the ionosphere (upward) on the duskside, in the same sense as region-1 current. Together with previous studies of the current distributions in the DF and magnetic dip region, we have obtained a more complete picture of the current system surrounding the boundary of plasma bubble. This current system is very similar to the substorm current wedge predicted by MHD simulation models, but with much smaller scale.
    Print ISSN: 0094-8276
    Electronic ISSN: 1944-8007
    Topics: Geosciences , Physics
    Published by Wiley on behalf of American Geophysical Union (AGU).
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  • 6
    Publication Date: 2016-03-16
    Description: Small scale magnetic holes (SSMHs) in the magnetosphere plasma sheet are investigated in this paper. A developed electron magnetohydrodynamics (EMHD) soliton model is proposed as a new approach to SSMHs formation. The Biermann battery effect is taken into account in resolving the magnetic evolution equation with a slow mode solution in the weak nonlinear regime. Statistical investigation of SSMH observation data in the plasma sheet by Cluster is carried out in comparison with the theory. We apply multi-spacecraft data for distinguishing sheet-like or cylindrical SSMHs observed and clarified by the solitary wave in the EMHD model. Furthermore, the major parameters, such as amplitude, width, maximum magnetic field perturbation and perpendicular temperature variation of the SSMHs are found consistent with the theoretical analysis.
    Print ISSN: 0148-0227
    Topics: Geosciences , Physics
    Published by Wiley on behalf of American Geophysical Union (AGU).
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  • 7
    Publication Date: 2017-07-22
    Description: We analyzed MESSENGER magnetic field and plasma measurements taken during 319 crossings of Mercury's cross-tail current sheet. We found that the measured B Z in the current sheet is higher on the dawn-side than the dusk-side by a factor of ≈ 3 and the asymmetry decreases with downtail distance. This result is consistent with expectations based upon MHD stress balance. The magnetic fields threading the more stretched current sheet in the dusk-side have a higher plasma beta than those on the dawn-side, where they are less stretched. This asymmetric behavior is confirmed by mean current sheet thickness being greatest on the dawn-side. We propose that heavy planetary ion (e.g. Na + ) enhancements in the dusk-side current sheet provides the most likely explanation for the dawn-dusk current sheet asymmetries. We also report the direct measurement of Mercury's substorm current wedge (SCW) formation and estimate the total current due to pileup of magnetic flux to be ≈ 11 kA. The conductance at the foot of the field-lines required to close the SCW current is found to be ≈ 1.2 S, which is similar to earlier results derived from modelling of Mercury's Region 1 field-aligned currents. Hence, Mercury's regolith is sufficiently conductive for the current to flow radially, then across the surface of Mercury's highly conductive iron core. Mercury appears to be closely coupled to its night-side magnetosphere by mass loading of upward flowing heavy planetary ions, and electrodynamically by field-aligned currents that transfer momentum and energy to the night-side auroral oval crust and interior.
    Print ISSN: 0148-0227
    Topics: Geosciences , Physics
    Published by Wiley on behalf of American Geophysical Union (AGU).
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  • 8
    Publication Date: 2016-12-25
    Description: The structure, X-line location and magnetohydrodynamics (MHD) stress balance of Mercury's magnetotail were examined between -2.6 〈  X MSM  〈 -1.4 R M using MESSENGER measurements observed from 319 central plasma sheet (CPS) crossings. The mean plasma β in the CPS calculated from MESSENGER data is ~ 6. The CPS magnetic field was southward (i.e., tailward of X-line) ~ 2 – 18% of the time. Extrapolation of downtail variations in B Z indicates an average X-line location at -3 R M . Modelling of magnetic field measurements produced a cross-tail current sheet (CS) thickness, current density and inner CS edge location of 0.39 R M , 92 nA/m 2 and -1.22 R M , respectively. Application of MHD stress balance suggests that heavy planetary ions may be important in maintaining stress balance within Mercury's CPS. Qualitative similarities between Mercury's and Earth's magnetotail are remarkable given the differences in upstream conditions, internal plasma composition, finite gyro-radius scaling, and Mercury's lack of ionosphere.
    Print ISSN: 0094-8276
    Electronic ISSN: 1944-8007
    Topics: Geosciences , Physics
    Published by Wiley on behalf of American Geophysical Union (AGU).
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  • 9
    Publication Date: 2016-11-03
    Description: Isotope measurements were performed on dissolved NO 3 − , NH 4 + and suspended particulate total N along a salinity gradient in the Pearl River Estuary (PRE) to investigate seasonal changes in main N sources and its biogeochemical processing under the influence of monsoon climate. Our data revealed that municipal sewage and re-mineralized soil organic N were the major sources of DIN (NO 3 − and/or NH 4 + ) in freshwater during winter and summer, respectively, whereas phytoplankton biomass was a major component of PN in both seasons. In low salinity waters (〈2–3), nitrification was proved to be a significant NO 3 − source via NH 4 + consumption, with N isotope effects of −15.3‰ in summer and −23.7‰ in winter for NH 4 + oxidation. The contribution of nitrification to the total NO 3 − pool was smaller in summer than in winter, most likely due to freshwater dilution. At mid-salinities (3–20), δ 15 N values of PN were similar to those of NO 3 − and NH 4 + in summer, reflecting a strong coupling between assimilation and remineralization. In winter, however, higher δ 15 N NH4 but lower δ 15 N NO3 than δ 15 N PN were observed, even though δ 15 N PN was similar between summer and winter. Intense sediment-water interaction and resuspension of sediments during winter appeared largely responsible for the decoupling. At high salinities, the greater enrichment in δ 18 O NO3 than in δ 15 N NO3 (up to 15.6‰) in winter suggests that atmospheric deposition may contribute to NO 3 − delivery during the dry season. Overall, these results show the importance of seasonal variability in physical forcing on biological N sources and its turnover processes in the highly dynamic river-dominated estuary. This article is protected by copyright. All rights reserved.
    Print ISSN: 0148-0227
    Topics: Geosciences , Physics
    Published by Wiley on behalf of American Geophysical Union (AGU).
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  • 10
    Publication Date: 2014-06-12
    Description: Electric fields associated with dipolarization fronts (DFs) have been investigated in the magnetotail plasma sheet using Cluster observations. We have studied each term in the generalized Ohm's law using data obtained from the multi-spacecraft Cluster. Our results show that in the plasma flow frame electric fields are directed normal to the DF in the magnetic dip region ahead of the DF as well as in the DF layer, but in opposite directions. Case and statistical studies show that the Hall electric field is important while the electron pressure gradient term is much smaller. The ions decouple from the magnetic field in the DF layer and dip region ( E  +  V i  ×  B  ≠ 0), whereas electrons remain frozen-in ( E  +  V e  ×  B  = ∇ p e / n e e ).
    Print ISSN: 0148-0227
    Topics: Geosciences , Physics
    Published by Wiley on behalf of American Geophysical Union (AGU).
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