High Tunnel Design, Site Development, and Construction

High tunnels are low technology plant growing structures that provide opportunity for season extension, severe weather protection, and modified environments to increase productivity and visual quality of harvested plant products. This publication describes high tunnel components, site selection, development, covering materials, installation, and operation. Experienced specialty plant growers can increase the quality of their products and the duration of their marketing of high- value crops through the use of high tunnels. High tunnels give growers the opportunity to plant earlier and include more sequential planting dates. This can result in early- season, high- dollar returns and the ability to offer their products for longer periods. High tunnels also provide environmental protection, which helps reduce blemishes and discoloration, improving visual appeal. For successful high tunnel crop production, decisions and actions before planting the first crop include choosing a structural design to meet specific needs, identifying the best site for locating the structure, initial soil preparation, and the method of construction

Sustainable Stewardship: The Heuristic-Systemic Approach to Sustainable Attitude-Behavior Gap

Although an increasing number of apparel businesses are striving to exert ecological and social influences that can change consumers’ purchasing behaviors in relation to sustainable products, consumers still feel hesitant about adopting a sustainable lifestyle. Moreover, consumers tend to engage in a complicated decision-making process due to the motivational and practical complexity of sustainable consumption. Given the growing interest among societies and in many industries, comprehending these dynamics can help improve the knowledge level of consumers, and may stipulate further applications of sustainable stewardship. Thus, this study aims (1) to test the systematic conjunction of CSR drives with attitude and sustainable behaviors; and (2) to examine the heuristic influence of eco-labels/indices from the point of vie

X-Ray Ionization of Planet-Opened Gaps in Protostellar Disks

Young planets with masses approaching Jupiter's have tides strong enough to clear gaps around their orbits in the protostellar disk. Gas flow through the gaps regulates the planets' further growth and governs the disks' evolution. Magnetic forces may drive that flow if the gas is sufficiently ionized to couple to the fields. We compute the ionizing effects of the X-rays from the central young star, using Monte Carlo radiative transfer calculations to find the spectrum of Compton-scattered photons reaching the planet's vicinity. The scattered X-rays ionize the gas at rates similar to or greater than the interstellar cosmic ray rate near planets the mass of Saturn and of Jupiter, located at 5 au and at 10 au, in disks with the interstellar mass fraction of sub-micron dust and with the dust depleted a factor 100. Solving a gas-grain recombination reaction network yields charged particle populations whose ability to carry currents is sufficient to partly couple the magnetic fields to the gas around the planet. Most cases can undergo Hall shear instability, and some can launch magnetocentrifugal winds. However the material on the planet's orbit has diffusivities so large in all the cases we examine, that magneto-rotational turbulence is prevented and the non-ideal terms govern the magnetic field's evolution. Thus the flow of gas in the gaps opened by the young giant planets depends crucially on the finite conductivity.Comment: 24 pages, 6 figures. Gap depths are now chosen to match recent hydrodynamical results. Accepted for publication in Ap

The Milky Way satellite velocity function is a sharp probe of small-scale structure problems

Twenty years ago, the mismatch between the observed number of Milky Way satellite galaxies and the predicted number of cold dark matter subhalos was dubbed the "missing satellites problem". Although mostly framed since in terms of satellite counts in luminosity space, the missing satellites problem was originally posed in velocity space. The stellar velocity dispersion function encodes information about the density profile of satellites as well as their abundance. We compare the completeness-corrected MW satellite velocity function down to its ultrafaint dwarfs (L > 340 L$_\odot$) against well-motivated, semi-empirical predictions based on galaxy-halo scaling relations. For our most conservative completeness correction, we find good agreement with a simple CDM model in which massive, classical satellites (M$_{\rm vir} \gtrsim 10^9~$M$_\odot$) have baryon-driven cores, while low-mass, ultrafaint satellites (M$_{\rm vir} \lesssim 10^9~$M$_\odot$) inhabit cuspy halos that are not strongly tidally stripped. This bifurication is required to explain a non-power-law feature in the velocity function at $\sigma_{\rm los}^* \approx 10$ km/s. Intriguingly, this feature could point to a flattening of the stellar-mass--halo-mass relation. Tidal destruction of satellites by the Milky Way's disk must be minimal, or the corrected velocity function exceeds any plausible prediction -- a "too many satellites" problem. We rule out non-core-collapsing self-interacting dark matter models with a constant cross section $\gtrsim$ 0.3 cm$^2$/g. Constraints on warm dark matter are stronger than those based on the luminosity function on account of the velocity function's additional sensitivity to the central densities of subhalos. Reducing uncertainties on stellar kinematics and the amount of tidal stripping experienced by the faintest dwarfs is key to determining the severity of the too many satellites problem.Comment: 19 pages, 13 figures. Key results are summarized in Figure 6. To be submitted to MNRAS. Comments welcome

A Review of Common Drug-Drug and Food-Drug Interactions Associated with Cardiovascular Medications

This home-study CPE activity has been developed to educate pharmacists on the common drug-drug and food-drug interactions associated with cardiovascular medications