221 research outputs found

    Public Policy and Funding the News

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    Illustrates how declining government support and recent regulatory decisions have affected the viability of periodicals and other news outlets. Proposes a policy framework for indirect, content-neutral funding and investment in innovation and new models

    Path dependence: an approach for framing constraints on adaptation in Australian dairy farms

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    Climate change is a salient issue for southern Australia, which has been identified as one of the regions most vulnerable to climate change in the world. The potential impacts of climate change on farms could be profound and may require that producers adapt their farms to a much greater degree than currently undertaken. Generally speaking, it is expected that climate change will require considerable change to agriculture, with the responsibility for this change lying squarely with producers, many of which are small family businesses. In this thesis I explored the capacity of producers to adapt their farms in the face of climate change. Underpinning this exploration was a question regarding the role, if any, for public policy to support producers with managing climate change impacts

    Orbital Phase Variations of the Eccentric Giant Planet HAT-P-2b

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    We present the first secondary eclipse and phase curve observations for the highly eccentric hot Jupiter HAT-P-2b in the 3.6, 4.5, 5.8, and 8.0 ÎŒm bands of the Spitzer Space Telescope. The 3.6 and 4.5 ÎŒm data sets span an entire orbital period of HAT-P-2b (P = 5.6334729 d), making them the longest continuous phase curve observations obtained to date and the first full-orbit observations of a planet with an eccentricity exceeding 0.2. We present an improved non-parametric method for removing the intrapixel sensitivity variations in Spitzer data at 3.6 and 4.5 ÎŒm that robustly maps position-dependent flux variations. We find that the peak in planetary flux occurs at 4.39 ± 0.28, 5.84 ± 0.39, and 4.68 ± 0.37 hr after periapse passage with corresponding maxima in the planet/star flux ratio of 0.1138% ± 0.0089%, 0.1162% ± 0.0080%, and 0.1888% ± 0.0072% in the 3.6, 4.5, and 8.0 ÎŒm bands, respectively. Our measured secondary eclipse depths of 0.0996% ± 0.0072%, 0.1031% ± 0.0061%, 0.071%^(+0.029%)_(-0.013%), and 0.1392% ± 0.0095% in the 3.6, 4.5, 5.8, and 8.0 ÎŒm bands, respectively, indicate that the planet cools significantly from its peak temperature before we measure the dayside flux during secondary eclipse. We compare our measured secondary eclipse depths to the predictions from a one-dimensional radiative transfer model, which suggests the possible presence of a transient day side inversion in HAT-P-2b's atmosphere near periapse. We also derive improved estimates for the system parameters, including its mass, radius, and orbital ephemeris. Our simultaneous fit to the transit, secondary eclipse, and radial velocity data allows us to determine the eccentricity (e = 0.50910 ± 0.00048) and argument of periapse (ω = 188°.09 ± 0°.39) of HAT-P-2b's orbit with a greater precision than has been achieved for any other eccentric extrasolar planet. We also find evidence for a long-term linear trend in the radial velocity data. This trend suggests the presence of another substellar companion in the HAT-P-2 system, which could have caused HAT-P-2b to migrate inward to its present-day orbit via the Kozai mechanism
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