4,537 research outputs found

    Transport of magnetic flux and mass in Saturn's inner magnetosphere

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    It is well accepted that cold plasma sourced by Enceladus is ultimately lost to the solar wind, while the magnetic flux convecting outward with the plasma must return to the inner magnetosphere. However, whether the interchange or reconnection, or a combination of the two processes is the dominant mechanism in returning the magnetic flux is still under debate. Initial Cassini observations have shown that the magnetic flux returns in the form of flux tubes in the inner magnetosphere. Here we investigate those events with 10 year Cassini magnetometer data and confirm that their magnetic signatures are determined by the background plasma environments: inside (outside) the plasma disk, the returning magnetic field is enhanced (depressed) in strength. The distribution, temporal variation, shape, and transportation rate of the flux tubes are also characterized. The flux tubes break into smaller ones as they convect in. The shape of their cross section is closer to circular than fingerlike as produced in the simulations based on the interchange mechanism. In addition, no sudden changes in any flux tube properties can be found at the “boundary” which has been claimed to separate the reconnection and interchange-dominant regions. On the other hand, reasonable cold plasma loss rate and outflow velocity can be obtained if the transport rate of the magnetic flux matches the reconnection rate, which supports reconnection alone as the dominant mechanism in unloading the cold plasma from the inner magnetosphere and returning the magnetic flux from the tail

    Subtractive Sets over Cyclotomic Rings:Limits of Schnorr-like Arguments over Lattices

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    We study when (dual) Vandermonde systems of the form VT(âŠș)⋅z⃗=s⋅w⃗{V}_T^{{(\intercal)}} \cdot \vec{z} = s\cdot \vec{w} admit a solution z⃗\vec{z} over a ring R\mathcal{R}, where VT{V}_T is the Vandermonde matrix defined by a set TT and where the slack ss is a measure of the quality of solutions. To this end, we propose the notion of (s,t)(s,t)-subtractive sets over a ring R\mathcal{R}, with the property that if SS is (s,t)(s,t)-subtractive then the above (dual) Vandermonde systems defined by any tt-subset T⊆ST \subseteq S are solvable over R\mathcal{R}. The challenge is then to find large sets SS while minimising (the norm of) ss when given a ring R\mathcal{R}. By constructing families of (s,t)(s,t)-subtractive sets SS of size n=n = poly over cyclotomic rings R=Z[ζpℓ]\mathcal{R} = \mathbb{Z}[\zeta_{p^\ell}] for prime pp, we construct Schnorr-like lattice-based proofs of knowledge for the SIS relation A⋅x⃗=s⋅y⃗ mod q{A} \cdot \vec{x} = s \cdot \vec{y} \bmod q with O(1/n)O(1/n) knowledge error, and s=1s = 1 in case p=p = poly. Our technique slots naturally into the lattice Bulletproof framework from Crypto\u2720, producing lattice-based succinct arguments for NP with better parameters. We then give matching impossibility results constraining nn relative to ss, which suggest that our Bulletproof-compatible protocols are optimal unless fundamentally new techniques are discovered. Noting that the knowledge error of lattice Bulletproofs is Ω(log⁥k/n)\Omega(\log k/n) for witnesses in Rk\mathcal{R}^k and subtractive set size nn, our result represents a barrier to practically efficient lattice-based succinct arguments in the Bulletproof framework. Beyond these main results, the concept of (s,t)(s,t)-subtractive sets bridges group-based threshold cryptography to lattice settings, which we demonstrate by relating it to distributed pseudorandom functions

    Flight Data System

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    The goal of this capstone design project was to design a fully portable sailplane Lift/Drag (L/D) calculator. The system utilizes NMEA format GPS data strings for software data analysis executed by software. Calculated effective L/D results are stored on a removable data storage media (e.g. CompactFlash card) for later data analysis

    Differential item functioning in the Patient Reported Outcomes Measurement Information System Pediatric Short Forms in a sample of children and adolescents with cerebral palsy.

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    AIM: The present study examined the Patient Reported Outcomes Measurement Information System (PROMIS) Mobility, Fatigue, and Pain Interference Short Forms (SFs) in children and adolescents with cerebral palsy (CP) for the presence of differential item functioning (DIF) relative to the original calibration sample. METHOD: Using the Graded Response Model we compared item parameter estimates generated from a sample of 303 children and adolescents with CP (175 males, 128 females; mean age 15y 5mo) to parameter estimates from the PROMIS calibration sample, which served as the reference group. DIF was assessed in a two-step process using the item response theory-likelihood ratio-differential item functioning detection procedure. RESULTS: Significant DIF was identified for four of eight items in the PROMIS Mobility SF, for two of eight items in the Pain Interference Scale, and for one item out of 10 on the Fatigue Scale. Impact of DIF on total score estimation was notable for Mobility and Pain Interference, but not for Fatigue. INTERPRETATION: Results suggest differences in the responses of adolescents with CP to some items on the PROMIS Mobility and Pain Interference SFs. Cognitive interviews about the PROMIS items with adolescents with varying degrees of mobility limitations would provide better understanding of how they are interpreting and selecting responses to the PROMIS items and thus help guide selection of the most appropriate way to address this issue

    Does Osmotic Stress Affect Natural Product Expression in Fungi?

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    Acknowledgments: Russell Kerr acknowledges the assistance of Nadia Prigoda-Lee, Marius Grote, Kate McQuillan and Stephanie Duffy, and generous financial support from NSERC, the Canada Research Chair program, the Jeanne and Jean-Louis LĂ©vesque Foundation and the Atlantic Canada Opportunities Agency. Ka-Lai Pang thanks the president of National Taiwan Ocean University, Ching-Fong Chang, for a special fund to attend the workshop held in Charlottetown, Canada in 2014 where this work was discussed. Rob Capon and Zhuo Shang acknowledge support from the University of Queensland, and the UQ Institute for Molecular Bioscience. Zhuo Shang acknowledges the provision of an International Postgraduate Research Scholarship (IPRS) and a Centennial Scholarship by the University of Queensland. Catherine Roullier acknowledges the assistance of Marie-Claude Boumard and Thibaut Robiou du Pont, and support from Region Pays de la Loire, FrancePeer reviewedPublisher PD

    Exploring Efficient Irrigation Methods for the Pueblo of Santa Ana

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    The goal of this project was to assist the Pueblo of Santa Ana Water Division’s efforts to increase irrigation efficiency by proposing an irrigation plan for the newly acquired Northern Field. We designed multiple layouts for the field to try to optimize the area of the field, water efficiency, as well as monetary cost to implement an irrigation system on the Northern Field. We provided a breakdown of the monetary costs for each irrigation layouts we designed for the Northern Field, and also designed a new platform for communication between the farmers and the Mayordomo to help scheduling and to eliminate wasteful irrigation practices. Finally, we used our analysis to provide recommendations that would best fit the Pueblo’s cultural values and practical needs

    Mass Transfer, Transiting Stream and Magnetopause in Close-in Exoplanetary Systems with Applications to WASP-12

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    We study mass transfer by Roche lobe overflow in close-in exoplanetary systems. The planet's atmospheric gas passes through the inner Lagrangian point and flows along a narrow stream, accelerating to 100-200\kms velocity before forming an accretion disk. We show that the cylinder-shaped accretion stream can have an area (projected in the plane of the sky) comparable to that of the planet and a significant optical depth to spectral line absorption. Such a "transiting cylinder" may produce an earlier ingress of the planet transit, as suggested by recent HST observations of the WASP-12 system. The asymmetric disk produced by the accretion stream may also lead to time-dependent obscuration of the star light and apparent earlier ingress. We also consider the interaction of the stellar wind with the planetary magnetosphere. Since the wind speed is subsonic/sub-Alfvenic and comparable to the orbital velocity of the planet, the head of the magnetopause lies eastward relative to the substellar line (the line joining the planet and the star). The gas around the magnetopause may, if sufficiently compressed, give rise to asymmetric ingress/egress during the planet transit, although more works are needed to evaluate this possibility.Comment: 6 pages with 2 figures. Accepted in ApJ. Small changes (add discussion on asymmetric disks
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