1,815 research outputs found
Three months journeying of a Hawaiian monk seal
Hawaiian monk seals (Monachus schauinslandi) are endemic to the Hawaiian
Islands and are the most endangered species of marine mammal that lives
entirely within the jurisdiction of the United States. The species numbers
around 1300 and has been declining owing, among other things, to poor juvenile
survival which is evidently related to poor foraging success. Consequently,
data have been collected recently on the foraging habitats, movements, and
behaviors of monk seals throughout the Northwestern and main Hawaiian Islands.
Our work here is directed to exploring a data set located in a relatively
shallow offshore submerged bank (Penguin Bank) in our search of a model for a
seal's journey. The work ends by fitting a stochastic differential equation
(SDE) that mimics some aspects of the behavior of seals by working with
location data collected for one seal. The SDE is found by developing a time
varying potential function with two points of attraction. The times of location
are irregularly spaced and not close together geographically, leading to some
difficulties of interpretation. Synthetic plots generated using the model are
employed to assess its reasonableness spatially and temporally. One aspect is
that the animal stays mainly southwest of Molokai. The work led to the
estimation of the lengths and locations of the seal's foraging trips.Comment: Published in at http://dx.doi.org/10.1214/193940307000000473 the IMS
Collections (http://www.imstat.org/publications/imscollections.htm) by the
Institute of Mathematical Statistics (http://www.imstat.org
Large scale motions of Neptune's bow shock: Evidence for control of the shock position by the rotation phase of Neptune's magnetic field
The Voyager 2 spacecraft observed high levels of Langmuir waves before the inbound crossing of Neptune's bow shock, thereby signifying magnetic connection of the bow shock. The Langmuir waves occurred in multiple bursts throughout two distinct periods separated by an 85 minute absence of wave activity. The times of onsets, peaks, and disappearances of the waves were used together with the magnetic field directions and spacecraft position, to perform a 'remote-sensing' analysis of the shape and location of Neptune's bow shock prior to the inbound bow shock crossing. The bow shock is assumed to have a parabolidal shape with a nose location and flaring parameter determined independently for each wave event. The remote-sensing analysis give a shock position consistent with the time of the inbound shock crossing. The flaring parameter of the shock remains approximately constant throughout each period of wave activity but differs by a factor of 10 between the two periods. The absence of waves between two periods of wave activity coincides with a large rotation of the magnetic field and a large increase in the solar wind ram pressure' both these effects lead to magnetic disconnection of the spacecraft from shock. The planetwards motion of the shock's nose from 38.5 R(sub N) to 34.5 R(sub N) during the second time period occurred while the solar wind ram pressure remained constant to within 15 percent. This second period of planetwards motion of the shock is therefore strong evidence for Neptune's bow shock moving in response to the rotation of Neptune's oblique, tilted magnetic dipole. Normalizing the ram pressure, the remotely-sensed shock moves sunwards during the first wave period and planetwards in the second wave period. The maximum standoff distance occurs while the dipole axis is close to being perpendicular to the Sun-Neptune direction. The remote-sensing analysis provides strong evidence that the location of Neptune's bow shock is controlled by Neptune's rotation phase
High-performance 3D waveguide architecture for astronomical pupil-remapping interferometry
The detection and characterisation of extra-solar planets is a major theme
driving modern astronomy, with the vast majority of such measurements being
achieved by Doppler radial-velocity and transit observations. Another technique
-- direct imaging -- can access a parameter space that complements these
methods, and paves the way for future technologies capable of detailed
characterization of exoplanetary atmospheres and surfaces. However achieving
the required levels of performance with direct imaging, particularly from
ground-based telescopes which must contend with the Earth's turbulent
atmosphere, requires considerable sophistication in the instrument and
detection strategy. Here we demonstrate a new generation of photonic
pupil-remapping devices which build upon the interferometric framework
developed for the {\it Dragonfly} instrument: a high contrast waveguide-based
device which recovers robust complex visibility observables. New generation
Dragonfly devices overcome problems caused by interference from unguided light
and low throughput, promising unprecedented on-sky performance. Closure phase
measurement scatter of only has been achieved, with waveguide
throughputs of . This translates to a maximum contrast-ratio
sensitivity (between the host star and its orbiting planet) at
(1 detection) of (when a conventional
adaptive-optics (AO) system is used) or (for typical
`extreme-AO' performance), improving even further when random error is
minimised by averaging over multiple exposures. This is an order of magnitude
beyond conventional pupil-segmenting interferometry techniques (such as
aperture masking), allowing a previously inaccessible part of the star to
planet contrast-separation parameter space to be explored
Residual Votes and Abstentions in the 2016 Election
This paper provides a preliminary analysis of the increase in the residual vote rate from 2012 to 2016, when it increased from 0.99% to 1.87% nationwide. It is reasonable to assume that this spike in the residual vote rate is due to a rise in abstentions. However, there are currently other trends in election administration, such as an increasing reliance on vote-by-mail, that could also be driving up the residual vote rate. And, even if the recent up-tick in the residual vote rate is primarily due to an increase in abstentions in 2016, it is not a priori obvious that the source of new abstentions was equally distributed among disaffected Democrats and Republicans. The analysis in this paper relies on a combination of public opinion data and election returns to address these issues. We find, first, that the increase in abstentions in 2016 was most likely due to disaffected Republicans, rather than an across-the-board phenomenon. We also confirm that the increase in the 2016 residual vote rate was not due to changes in voting technologies between 2012 and 2016. We address three issues in the conclusion that this analysis raises: (1) the potential for the growth of protest voting in the U.S., (2) the likelihood that there is a significant under-reporting of voter abstentions in public opinion surveys, leaving a role for aggregate analysis to study this phenomenon, and (3) cautions about the use of the residual vote rate as a metric to gauge the accuracy of voting technologies
Separation of river networkâscale nitrogen removal among the main channel and two transient storage compartments
Transient storage (TS) zones are important areas of dissolved inorganic nitrogen (DIN) processing in rivers. We assessed sensitivities regarding the relative impact that the main channel (MC), surface TS (STS), and hyporheic TS (HTS) have on network denitrification using a model applied to the Ipswich River in Massachusetts, United States. STS and HTS connectivity and size were parameterized using the results of in situ solute tracer studies in firstâ through fifthâorder reaches. DIN removal was simulated in all compartments for every river grid cell using reactivity derived from Lotic Intersite Nitrogen Experiment (LINX2) studies, hydraulic characteristics, and simulated discharge. Model results suggest that although MCâtoâSTS connectivity is greater than MCâtoâHTS connectivity at the reach scale, at basin scales, there is a high probability of water entering the HTS at some point along its flow path through the river network. Assuming our best empirical estimates of hydraulic parameters and reactivity, the MC, HTS, and STS removed approximately 38%, 21%, and 14% of total DIN inputs during a typical base flow period, respectively. There is considerable uncertainty in many of the parameters, particularly the estimates of reaction rates in the different compartments. Using sensitivity analyses, we found that the size of TS is more important for DIN removal processes than its connectivity with the MC when reactivity is low to moderate, whereas TS connectivity is more important when reaction rates are rapid. Our work suggests a network perspective is needed to understand how connectivity, residence times, and reactivity interact to influence DIN processing in hierarchical river systems
Foliar Micronutrient Application for High-Yield Maize
Nebraska soils are generally micronutrient sufficient. However, critical levels for current yields have not been validated. From 2013 to 2015, 26 on-farm paired comparison strip-trials were conducted across Nebraska to test the effect of foliar-applied micronutrients on maize (Zea mays L.) yield and foliar nutrient concentrations. Treatments were applied from V6 to V14 at sites with 10.9 to 16.4 Mg haâ1 yield. Soils ranged from silty clays to fine sands. Soil micronutrient availability and tissue concentrations were all above critical levels for deficiency. Significant grain yield increases were few. Micronutrient concentrations for leaf growth that occurred after foliar applications were increased 4 to 9 mg Zn kgâ1 at 5 of 17 sites with application of 87 to 119 g Zn haâ1, 12 to 16 mg kgâ1 Mn at 2 of 17 sites with application of 87 to 89 g Mn haâ1, and an average of 8.1 mg kgâ1 Fe across 10 sites showing signs of Fe deficiency with application of 123 g foliar Fe ha-1. Foliar B concentration was not affected by B application. Increases in nutrient concentrations were not related to grain yield responses except for Mn (r = 0.54). The mean, significant grain yield response to 123 g foliar Fe haâ1 was 0.4 Mg haâ1 for the 10 sites with Fe deficiency symptoms. On average, maize yield response to foliar Fe application can be profitable if Fe deficiency symptoms are observed. Response to other foliar micronutrient applications is not likely to be profitable without solid evidence of a nutrient deficiency
Direct Measurement of the Quantum Wavefunction
Central to quantum theory, the wavefunction is the complex distribution used
to completely describe a quantum system. Despite its fundamental role, it is
typically introduced as an abstract element of the theory with no explicit
definition. Rather, physicists come to a working understanding of the
wavefunction through its use to calculate measurement outcome probabilities via
the Born Rule. Presently, scientists determine the wavefunction through
tomographic methods, which estimate the wavefunction that is most consistent
with a diverse collection of measurements. The indirectness of these methods
compounds the problem of defining the wavefunction. Here we show that the
wavefunction can be measured directly by the sequential measurement of two
complementary variables of the system. The crux of our method is that the first
measurement is performed in a gentle way (i.e. weak measurement) so as not to
invalidate the second. The result is that the real and imaginary components of
the wavefunction appear directly on our measurement apparatus. We give an
experimental example by directly measuring the transverse spatial wavefunction
of a single photon, a task not previously realized by any method. We show that
the concept is universal, being applicable both to other degrees of freedom of
the photon (e.g. polarization, frequency, etc.) and to other quantum systems
(e.g. electron spin-z quantum state, SQUIDs, trapped ions, etc.). Consequently,
this method gives the wavefunction a straightforward and general definition in
terms of a specific set of experimental operations. We expect it to expand the
range of quantum systems scientists are able to characterize and initiate new
avenues to understand fundamental quantum theory
Abstention, Protest, and Residual Votes in the 2016 Election
Objective: We analyze the significant increase in the residual vote rate in the 2016 presidential election. The residual vote rate, which is the percentage of ballots cast in a presidential election that contain no vote for president, rose nationwide from 0.99 to 1.41 percent between 2012 and 2016.
Method: We use election return data and public opinion data to examine why the residual vote rate increased in 2016.
Results: The primary explanation for this rise is an increase in abstentions, which we argue results primarily from disaffected Republican voters rather than alienated Democratic voters. In addition, other factors related to election administration and electoral competition explain variation in the residual vote rates across states, particularly the use of mail/absentee ballots and the lack of competition at the top of the ticket in nonbattleground states. However, we note that the rise in the residual vote rate was not due to changes in voting technologies.
Conclusion: Our research has implications for the use of the residual vote as a metric for studying election administration and voting technologies
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