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Central anomaly magnetization high: constraints on the volcanic construction and architecture of seismic layer 2A at a fast-spreading mid-ocean ridge, the EPR at 9Âș30'â50'N
The central anomaly magnetization high (CAMH) is a zone of high crustal magnetization centered on the axis of the East Pacific Rise (EPR) and many other segments of the global mid-ocean ridge (MOR). The CAMH is thought to reflect the presence of recently emplaced and highly magnetic lavas. Forward models show that the complicated character of the near-bottom CAMH can be successfully reproduced by the convolution of a lava deposition distribution with a lava magnetization function that describes the variation in lava magnetization intensity with age. This lava magnetization function is the product of geomagnetic paleofield intensity, which has increased by a factor of 2 over the last 40 kyr, and low-temperature alteration, which decreases the remanence of lava with exposure to seawater. The success of the forward modeling justifies the inverse approach: deconvolution of the magnetic data for lava distribution and integration of that distribution for magnetic layer thickness. This approach is tested on two near-bottom magnetic profiles AL2767 and AL2771, collected using Alvin across the EPR axis at 9Âș31'N and 9Âș50'N. Our analysis of these data produces an estimate of the relative thickness of the magnetic lava layer, which is remarkably consistent with existing multichannel estimates of layer 2A thickness from lines CDP31 and CDP27. The similarity between magnetic layer and seismic layer 2A at the 9Âșâ10ÂșN segment of the EPR crest provides independent support to the notion that seismic layer 2A in young oceanic crust represents the highly magnetic lava layer, and that the velocity gradient at the base of layer 2A is related to the increasing number of higher velocity dikes with depth in the lavaâdike transition zone. The near-bottom magnetic anomaly character of the CAMH is a powerful indicator of the emplacement history of upper crust at MORs which allows prediction of the relative thickness and architecture of the extrusive lavas independent of other constraint
The Non-Exhaust Particulate Emissions Impact of EURO VI to Battery Electric Bus Fleet Transitions
There is already strong evidence that non-exhaust emissions (NEEs) are a significant source of
transport-related particulates, and an expectation that this will increase as we transition from
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conventional to heavier alternative technology vehicles. (1) Therefore, we need to ensure that our
existing commitment to zero (at tailpipe) emissions is complemented by an active effort to mitigate
any unintended consequences for NEEs. (2)
This work, led by FirstBus, and funded by the TRANSITION Clean Air Network funded by the Natural
Environment Research Council within the UKRI Clean Air Programme (3), uses the EURO VI-to-Battery
Electric Bus transition as a case study to explore options to: (a) improve inventorying information
available to fleet managers considering fleet upgrade options; and, (b) gather evidence on the
potential divergence between regulatory metrics, conventional emission factors, inventory model
predictions and the real-world outcomes as we migrate to what need to be significantly cleaner
technologies
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Continuous near-bottom gravity measurements made with a BGM-3 gravimeter in DSV Alvin on the East Pacific Rise crest near 9°31 'N and 9°50'N
A Bell BGM-3 gravimeter has been used to collect continuous, underway, near-bottom (3- to 10-m altitude) gravity measurements from the deep-diving submersible DSV Alvin during surveys on the East Pacific Rise (EPR) crest near 9° 31'N and 9° 50'N. Closely spaced (20- to 30-m) gravity measurements were made along transects up to 8 km-long in both regions. Repeatability of measurements made at the same location on different dives is ~ 0.3 mGal. Along-track spatial resolution of anomalies is ~130-160 m, with the limiting factors being precision and sampling rate of the pressure gauge depth data used to calculate vertical accelerations of the submersible. The average upper crustal density of the ridge crest determined from the relationship between depth and free-water gravity anomalies varies greatly between 9 °31 'N and 9° 50'N. Average upper crustal densities of2410 kg/m3 for the 9° 50'N area and 2690 kg/m3 for the 9° 31'N area were calculated. The different densities are not due to differing geometry of the Layer 2A-2B boundary or a regional cross-axis gravity gradient. Differences in porosity of the shallow crustal rocks, or a difference in the proportion of low-density extrusives to higher-density dikes and sills within Layer 2A in these two areas, are the likely causes of the different upper crustal densities. Bouguer gravity anomalies near the EPR axis are primarily small amplitude (0.5-2 mGal), are a few hundred meters across, and appear to be lineated parallel to the axis. Larger-amplitude Bouguer anomalies of up to 4 mGal were found at a few locations across the crestal plateau and are associated with pillow ridges composed of lavas which are clearly younger than the surrounding seafloor. These ridges have distinct chemical compositions compared to lavas from the axial summit collapse trough (ASCT) at the same latitude. Probable sources of the 0.5- to 2-mGal anomalies observed on the summit plateau include areas of collapsed and fissured terrain and dike swarms feeding melt through Layer 2A to the surface. A grid survey of the ridge axis near 9° 50'N shows Bouguer anomalies lineated along the axis, suggesting that dike swarms do contribute to the observed Bouguer anomalies. The along-axis continuity of the gravity anomalies is disrupted at a 75-m offset of the ASCT, suggesting that shallow feeders of lava to the surface may be segmented on a finer scale than the deeper crustal magmatic system. This initial study confirms the ability to conduct high-resolution, near-bottom, continuous gravity measurements from Alvin. It also provides important information on how the shallow crustal structure of a fast spreading mid-ocean ridge develops and how it varies with the surface morphology
High-resolution water column survey to identify active sublacustrine hydrothermal discharge zones within Lake Rotomahana, North Island, New Zealand
This paper is not subject to U.S. copyright. The definitive version was published in Journal of Volcanology and Geothermal Research 314 (2016): 142-155, doi:10.1016/j.jvolgeores.2015.07.037.Autonomous underwater vehicles were used to conduct a high-resolution water column survey of Lake Rotomahana using temperature, pH, turbidity, and oxidationâreduction potential (ORP) to identify active hydrothermal discharge zones within the lake. Five areas with active sublacustrine venting were identified: (1) the area of the historic Pink Terraces; (2) adjacent to the western shoreline subaerial âSteaming Cliffs,â boiling springs and geyser; (3) along the northern shoreline to the east of the Pink Terrace site; (4) the newly discovered Patiti hydrothermal system along the south margin of the 1886 Tarawera eruption rift zone; and (5) a location in the east basin (northeast of Patiti Island). The Pink Terrace hydrothermal system was active prior to the 1886 eruption of Mount Tarawera, but venting along the western shoreline, in the east basin, and the Patiti hydrothermal system appear to have been initiated in the aftermath of the eruption, similar to Waimangu Valley to the southwest. Different combinations of turbidity, pH anomalies (both positive and negative), and ORP responses suggest vent fluid compositions vary over short distances within the lake. The seasonal period of stratification limits vertical transport of heat to the surface layer and the hypolimnion temperature of Lake Rotomahana consequently increases with an average warming rate of ~ 0.010 °C/day due to both convective hydrothermal discharge and conductive geothermal heating. A sudden temperature increase occurred during our 2011 survey and was likely the response to an earthquake swarm just 11 days prior.Funding was provided by GNS Strategic Development Fund
Heat flow and near-seafloor magnetic anomalies highlight hydrothermal circulation at Brothers volcano caldera, southern Kermadec arc, New Zealand
Author Posting. © American Geophysical Union, 2019. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Geophysical Research Letters 46(14), (2019): 8252-8260, doi: 10.1029/2019GL083517.Brothers volcano is the most hydrothermally active volcano along the Kermadec arc, with distinct hydrothermal fields located on the caldera walls and on the postcollapse volcanic cones. These sites display very different styles of hydrothermal activity in terms of temperature, gas content, fluid chemistry, and associated mineralization. Here we show the results of a systematic heat flow survey integrated with nearâseafloor magnetic data acquired using remotely operated vehicles and autonomous underwater vehicles. Largeâscale circulation is structurally controlled, with a deep (~1â to 2âkm depth) central recharge through the caldera floor and lateral discharge along the caldera walls and at the summits of the postcollapse cones. Shallow (~ 0.1â0.2 km depth) circulation is characterized by smallâscale recharge zones located at a distance of ~ 0.1â0.2 km from the active vent sites.We thank the Captains and crews of the R/V Sonne, Thompson, and Tangaroa and the engineers from Wood Hole Oceanographic Institution and MARUM for the successful operation of ABE, Sentry, Quest 4000, and Jason. The heat flow data surveys were funded by NSF grant OCEâ1558356 (PI Susan Humphris) and a grant from the German Ministry for Education and Research BMBF, project no. 03G0253A (PI Andrea Koschinsky). Funding from the New Zealand Government (Ministry of Business, Innovation and Employment) helped enable this study. This paper was significantly improved by the comments from the Editor Rebecca Carey and from two unknown reviewers. The data used in this paper can be downloaded from the U.S. LamontâDoherty MGDS database.2020-01-1
Interpretation of gravity and magnetic anomalies at Lake Rotomahana: geological and hydrothermal implications
Author Posting. © The Author(s), 2015. This is the author's version of the work. It is posted here for personal use, not for redistribution. The definitive version was published in Journal of Volcanology and Geothermal Research 314 (2016): 84-94, doi:10.1016/j.jvolgeores.2015.07.002.We investigate the geological and hydrothermal setting at Lake Rotomahana, using recently collected
potential-field data, integrated with pre-existing regional gravity and aeromagnetic compilations. The
lake is located on the southwest margin of the Okataina Volcanic Center (Haroharo caldera) and had
well-known, pre-1886 Tarawera eruption hydrothermal manifestations (the famous Pink and White
Terraces). Its present physiography was set by the caldera collapse during the 1886 eruption, together
with the appearance of surface activities at the Waimangu Valley. Gravity models suggest subsidence
associated with the Haroharo caldera is wider than the previously mapped extent of the caldera
margins. Magnetic anomalies closely correlate with heat-flux data and surface hydrothermal
manifestations and indicate that the west and northwestern shore of Lake Rotomahana are
characterized by a large, well-developed hydrothermal field. The field extends beyond the lake area
with deep connections to the Waimangu area to the south. On the south, the contact between
hydrothermally demagnetized and magnetized rocks strikes along a structural lineament with high
heat-flux and bubble plumes which suggest hydrothermal activity occurring west of Patiti Island. The
absence of a well-defined demagnetization anomaly at this location suggests a very young age for the
underlying geothermal system which was likely generated by the 1886 Tarawera eruption. Locally
confined intense magnetic anomalies on the north shore of Lake Rotomahana are interpreted as
basalts dikes with high magnetization. Some appear to have been emplaced before the 1886 Tarawera
eruption. A dike located in proximity of the southwest lake shore may be related to the structural
lineament controlling the development of the Patiti geothermal system, and could have been
originated from the 1886 Tarawera eruption.Science funding provided by GNS Science Strategic Development
Fund
3-D focused inversion of near-seafloor magnetic data with application to the Brothers volcano hydrothermal system, Southern Pacific Ocean, New Zealand
Author Posting. © American Geophysical Union, 2012. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Journal of Geophysical Research 117 (2012): B10102, doi:10.1029/2012JB009349.We describe and apply a new inversion method for 3-D modeling of magnetic anomalies designed for general application but which is particularly useful for the interpretation of near-seafloor magnetic anomalies. The crust subsurface is modeled by a set of prismatic cells, each with uniform magnetization, that together reproduce the observed magnetic field. This problem is linear with respect to the magnetization, and the number of cells is normally greater than the amount of available data. Thus, the solution is obtained by solving an under-determined linear problem. A focused solution, exhibiting sharp boundaries between different magnetization domains, is obtained by allowing the amplitudes of magnetization to vary between a pre-determined range and by minimizing the region of the 3-D space where the source shows large variations, i.e., large gradients. A regularization functional based on a depth-weighting function is also introduced in order to counter-act the natural decay of the magnetic field intensity with depth. The inversion method has been used to explore the characteristics of the submarine hydrothermal system of Brothers volcano in the Kermadec arc, by inverting near-bottom magnetic data acquired by Autonomous Underwater Vehicles (AUVs). Different surface expressions of the hydrothermal vent fields show specific vertical structures in their underlying demagnetization regions that we interpret to represent hydrothermal upflow zones. For example, at focused vent sites the demagnetized conduits are vertical, pipe-like structures extending to depths of ~1000 m below the seafloor, whereas at diffuse vent sites the demagnetization regions are characterized by thin and inclined conduits.This contribution was made possible through funding by the New Zealand
Foundation for Research, Science and Technology (FRST contract
C05X0406) and by the Royal Society of New Zealand by the Marsden Fund
(grant GNS1003).2013-04-1
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