136 research outputs found

    Early performance of constructed oyster reefs in Great Bay, New Hampshire

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    Several oyster reefs were constructed in Great Bay, New Hampshire using remotely-set oysters. A single large reef treatment and a cluster of several small reefs treatment were utilized to test hypotheses relevant to oyster restoration design, and to monitor early restoration reef performance. There was no significant difference in oyster size, density, and recruitment between two experimental reef structures, with both reef types having high survival and fast growth rates for the 2-year study. Both experimental reef structures had significantly higher recruitment rates than natural reefs in 2006, a year of relatively high recruitment (p \u3c 0.05), and elevated yet not significantly higher recruitment rates in 2005, a weak recruitment year (p = 0.078). In situ fluorometry data showed that a restored reef can significantly impact chlorophyll-a levels in overlying water within two years of reef construction. Individual oyster clearance rates ranged from 1.87 L/hr--2.41L/hr

    NEPA—Substantive Effectiveness Under a Procedural Mandate: Assessment of Oil and Gas EISs in the Mountain West

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    This paper empirically evaluates whether Environmental Impact Statements (EISs) for oil and natural gas field development projects lead to a significant reduction in environmental impacts. Based on our statistical analysis of projects within a four-state region, we conclude that EIS preparation does appear to produce final decisions that are substantially less impactive on the environment when compared to initially proposed projects. Impact reductions occur primarily between the Draft EIS and Final EIS, with minor reductions occurring between the Final EIS and Record of Decision. While reductions may be partially attributable to other legal requirements (such as Clean Air Act, Clean Water Act, or Endangered Species Act compliance or intervening economic and technological factors), external factors alone do not adequately explain impact reductions. We also found that the number of alternatives considered within an EIS affects the magnitude of impact reduction. EISs that consider a broader range of alternatives are more effective at reducing environmental impacts

    NEPA, FLPMA, and Impact Reduction: An Empirical Assessment of BLM Resource Management Planning in the Mountain West

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    This Article reviews Environmental Impact Statements (EIS) completed in conjunction with Resource Management Plan (RMP) revisions conducted by the Bureau of Land Management (BLM) in Colorado, Montana, Utah, and Wyoming between 2004 and 2014. Based on our review of sixteen EISs, we found that RMP revisions increased application of more protective surface use stipulations by statistically significant amounts without causing a statistically significant change in either the number of jobs created or the pace of oil and gas development. In fact, both the number of jobs created and wells drilled increased slightly despite strengthened environmental protections. We also found that Draft RMP EISs that are completed on an accelerated timeline come with a heightened risk that supplementation will be needed. The delays associated with preparing a Supplemental EIS far outweigh the timesaving associated with fast-tracking Draft EIS preparation and provide a strong caution against rushing the NEPA process

    NEPA and the Energy Policy Act of 2005 Statutory Categorical Exclusions: What Are the Environmental Costs of Expedited Oil and Gas Development?

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    A decade ago, concerned that National Environmental Policy Act (“NEPA”) compliance caused delays in permitting oil and gas (“O&G”) development on federal land, Congress enacted Section 390 of the Energy Policy Act (“EPAct”) of 2005. Section 390 is intended to expedite the environmental review of O&G development projects on federal lands. To effectuate that end Congress created several statutory categorical exclusions (“CEs”) to NEPA that apply to O&G development. Prior to the EPAct, the Bureau of Land Management (“BLM”) would permit new O&G development after conducting an Environmental Impact Statement (“EIS”) or Environmental Assessment (“EA”). EISs and EAs were the only NEPA compliance option available to the BLM because the agency had not promulgated regulations creating CEs for O&G projects. After the EPAct was passed, the BLM began permitting a substantial number of wells using the less rigorous CEs provided in Section 390. In fiscal years 2006 through 2008, the BLM used Section 390 CEs to permit approximately 28 percent of all wells nationally. States, members of Congress, and environmental groups have expressed concerns that the Section 390 CEs would lead to otherwise avoidable environmental impacts by circumventing conventional NEPA review. This article reviews 189 NEPA decisions and assesses whether the EPAct’s CEs result in more environmental harm then would occur had the projects undergone EA or EIS review

    NEPA and the Energy Policy Act of 2005 Statutory Categorical Exclusions: What Are the Environmental Costs of Expedited Oil and Gas Development?

    Get PDF
    A decade ago, concerned that National Environmental Policy Act (“NEPA”) compliance caused delays in permitting oil and gas (“O&G”) development on federal land, Congress enacted Section 390 of the Energy Policy Act (“EPAct”) of 2005. Section 390 is intended to expedite the environmental review of O&G development projects on federal lands. To effectuate that end Congress created several statutory categorical exclusions (“CEs”) to NEPA that apply to O&G development. Prior to the EPAct, the Bureau of Land Management (“BLM”) would permit new O&G development after conducting an Environmental Impact Statement (“EIS”) or Environmental Assessment (“EA”). EISs and EAs were the only NEPA compliance option available to the BLM because the agency had not promulgated regulations creating CEs for O&G projects. After the EPAct was passed, the BLM began permitting a substantial number of wells using the less rigorous CEs provided in Section 390. In fiscal years 2006 through 2008, the BLM used Section 390 CEs to permit approximately 28 percent of all wells nationally. States, members of Congress, and environmental groups have expressed concerns that the Section 390 CEs would lead to otherwise avoidable environmental impacts by circumventing conventional NEPA review. This article reviews 189 NEPA decisions and assesses whether the EPAct’s CEs result in more environmental harm then would occur had the projects undergone EA or EIS review

    Reef Structure Alternatives for Restoration of Oyster (Crassostrea virginica) Populations in New Hampshire

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    Eastern oyster (Crassostrea virginica) populations in New Hampshire have experienced severe declines since the 1990s, and restoration of oyster populations has been a major goal for New Hampshire management agencies. The most widely used technique in recent years in New Hampshire has been spat seeding which involves setting larvae from disease-resistant and/or fast-growth broodstock onto cultch material in large shore-based tanks, then distributing the spat attached to cultch onto the bottom to initiate reef restoration. This approach has the dual potential of providing direct population enhancement as well as introduction to the local gene pool of disease-resistance and/or fast-growth potential. Although spat seeding has been shown to be an effective technique much remains to be learned about the overall restoration process, particularly specific design criteria, the most effective combinations of methods, and long-term viability of restored bottom areas. The present project was designed in part based on results of earlier experimental work (mainly the use of spat seeding) to address the general management question: How should reefs be structurally enhanced (if at all) to enhance oyster populations and improve spat set

    Abundances of Iron-Binding Photosynthetic and Nitrogen-Fixing Proteins of Trichodesmium Both in Culture and In Situ from the North Atlantic

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    Marine cyanobacteria of the genus Trichodesmium occur throughout the oligotrophic tropical and subtropical oceans, where they can dominate the diazotrophic community in regions with high inputs of the trace metal iron (Fe). Iron is necessary for the functionality of enzymes involved in the processes of both photosynthesis and nitrogen fixation. We combined laboratory and field-based quantifications of the absolute concentrations of key enzymes involved in both photosynthesis and nitrogen fixation to determine how Trichodesmium allocates resources to these processes. We determined that protein level responses of Trichodesmium to iron-starvation involve down-regulation of the nitrogen fixation apparatus. In contrast, the photosynthetic apparatus is largely maintained, although re-arrangements do occur, including accumulation of the iron-stress-induced chlorophyll-binding protein IsiA. Data from natural populations of Trichodesmium spp. collected in the North Atlantic demonstrated a protein profile similar to iron-starved Trichodesmium in culture, suggestive of acclimation towards a minimal iron requirement even within an oceanic region receiving a high iron-flux. Estimates of cellular metabolic iron requirements are consistent with the availability of this trace metal playing a major role in restricting the biomass and activity of Trichodesmium throughout much of the subtropical ocean

    The hydrogen-poor superluminous supernova iPTF 13ajg and its host galaxy in absorption and emission

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    We present imaging and spectroscopy of a hydrogen-poor superluminous supernova (SLSN) discovered by the intermediate Palomar Transient Factory, iPTF 13ajg. At a redshift of z = 0.7403, derived from narrow absorption lines, iPTF 13ajg peaked at an absolute magnitude of M u, AB = -22.5, one of the most luminous supernovae to date. The observed bolometric peak luminosity of iPTF 13ajg is 3.2 × 1044 erg s-1, while the estimated total radiated energy is 1.3 × 1051 erg. We detect narrow absorption lines of Mg I, Mg II, and Fe II, associated with the cold interstellar medium in the host galaxy, at two different epochs with X-shooter at the Very Large Telescope. From Voigt profile fitting, we derive the column densities log N(Mg I) =11.94 ± 0.06, log N(Mg II) =14.7 ± 0.3, and log N(Fe II) =14.25 ± 0.10. These column densities, as well as the Mg I and Mg II equivalent widths of a sample of hydrogen-poor SLSNe taken from the literature, are at the low end of those derived for gamma-ray bursts (GRBs) whose progenitors are also thought to be massive stars. This suggests that the environments of hydrogen-poor SLSNe and GRBs are different. From the nondetection of Fe II fine-structure absorption lines, we derive a lower limit on the distance between the supernova and the narrow-line absorbing gas of 50 pc. The neutral gas responsible for the absorption in iPTF 13ajg exhibits a single narrow component with a low velocity width, ΔV = 76 km s-1, indicating a low-mass host galaxy. No host galaxy emission lines are detected, leading to an upper limit on the unobscured star formation rate (SFR) of SFR. Late-time imaging shows the iPTF 13ajg host galaxy to be faint, with g AB 27.0 and R AB ≥ 26.0 mag, corresponding to M B, Vega ≳ -17.7 mag. © 2014. The American Astronomical Society. All rights reserved.
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