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We began with a problem (we have too much light at night) and a related question (how much artificial light at night is appropriate?). We now have the origins, context, and detailed definition in hand for the concept of light pollution. With this, we can return to the question of framing outlined in Section 2, and scrutinize the ethical significance of increasingly relying on light pollution for policy decision-making; we can assess the answer light pollution provides for our question. Increased regulation and alternative design approaches will be necessary to address the myriad of undesired effects uncovered in contemporary research. And, light pollution offers a framing to orient responses. Furthermore, in it’s broad understanding of causes and effects, light pollution accommodates a variety of interpretations, allowing for a multiplicity of regulatory and technical solutions. Dark sky ordinances and new laws already exist, which often include detailed technical specifications.99. Morgan-Taylor (2014 Morgan-Taylor, M. (2014). Regulating light pollution in Europe: Legal challenges and ways forward. In J. Meier, U. Hasenöhrl, K. Krause, & M. Pottharst (Eds.), Urban lighting, light pollution and society (pp. 159–176). New York, NY: Taylor & Francis. [Google Scholar]) provides a brief analysis of current regulatory efforts in Europe. France is cited as having perhaps the strongest law to date, which requires non-residential buildings to switch off exterior lights and window displays between 1am and 7am. Other examples cited include regions of Italy that have taken a technical approach, prohibited lights above a specific brightness to project above the horizontal. Additionally, an online appendix to the article by Kyba et al. (2014 Kyba, C., Hänel, A., & Hölker, F. (2014). Redefining efficiency for outdoor lighting. Energy & Environmental Science, 7, 1806–1809.10.1039/C4EE00566J[Crossref], [Web of Science ®] [Google Scholar]) lists all known regulations and ordinances that are currently in place, as well as their motivations and targets.View all notes However, it is pertinent to reflect on the framework in which these decisions were made, and to consider how light pollution will shape future initiatives. When you report a faulty street light we will inspect it as soon as possible. We normally repair them within 5 working days but where lights are not working because of supply cable faults this could take longer. Central to Dorst’s frame creation model (2015 Dorst, K. (2015). Frame innovation: Create new thinking by design. Cambridge: The MIT Press. [Google Scholar]) is the great length that designers go to assess the frameworks through which problems are approached. Complex problems—such as the impacts of artificial nighttime lighting—are often caused by underlying value conflicts, and the inability of current frameworks to adequately address said values. By looking into the origins and history of the problem, the key driving issue, and the current context, a more comprehensive picture of the problem and underlying values emerge. And simultaneously the possibility of new approaches, or frames, will also emerge (Dorst, 2015 Dorst, K. (2015). Frame innovation: Create new thinking by design. Cambridge: The MIT Press. [Google Scholar]). However, for our present purposes we will not search for a new or radically different approach, but rather ask how the coalescing frame of light pollution is responding to our problem. We have our core issue present in the novel challenge described above. The next steps are to examine the origins and current context in turn, so see how light pollution can be improved as an effective frame. Senator Bernie Sanders took the spotlight Monday in a live-streamed town hall focused on inequality. The event came a couple of days after an op-ed in The Guardian in which he criticized “corporate media” for ignoring the rise of oligarchy in the US. 8. Gallaway et al. (2010 Gallaway, T., Olsen, R., & Mitchell, D. (2010). The economics of global light pollution. Ecological Economics, 69, 658–665.10.1016/j.ecolecon.2009.10.003[Crossref], [Web of Science ®] [Google Scholar]) utilize the threshold criteria established by Cinzano et al. (2001 Cinzano, P., Falchi, F., & Elvidge, C. D. (2001). The first world Atlas of the artificial night sky brightness. Monthly Notices of the Royal Astronomical Society, 328, 689–707.10.1046/j.1365-8711.2001.04882.x[Crossref], [Web of Science ®] [Google Scholar]) for considering an area ‘polluted’ by light. These criteria ‘consider the night sky polluted when the artificial brightness of the sky is greater than 10% of the natural sky brightness above 45° of elevation’ (Gallaway et al., 2010 Gallaway, T., Olsen, R., & Mitchell, D. (2010). The economics of global light pollution. Ecological Economics, 69, 658–665.10.1016/j.ecolecon.2009.10.003[Crossref], [Web of Science ®] [Google Scholar], p. 660). A study presented at the American Geophysical Union meeting in San Francisco found that light pollution destroys nitrate radicals thus preventing the normal night time reduction of atmospheric smog produced by fumes emitted from cars and factories.[82][83] The study was presented by Harald Stark from the National Oceanic and Atmospheric Administration. In another example, the city of Calgary has recently replaced most residential street lights with models that are comparably energy efficient.[98] The motivation is primarily operation cost and environmental conservation. The costs of installation are expected to be regained through energy savings within six to seven years. Nighttime illumination, once scarce, is now possessed in abundance and unavoidably ubiquitous. As a result, though, an interrelated shift in perception and valuation emerged—a shift that is critical to present discourse. With this abundance and ubiquity, a renewed attention was given to what is hindered by light. Darkness became, as Hasenöhrl notes, a valorized and ‘sought-after luxury’ of our electrified nights (2014 Hasenöhrl, U. (2014). Lighting conflicts from a historical perspective. In J. Meier, U. Hasenöhrl, K. Krause, & M. Pottharst (Eds.), Urban lighting, light pollution, and society (pp. 105–124). New York, NY: Taylor & Francis. [Google Scholar], p. 119). As a result, our taken-for-granted infrastructure of artificial nighttime lighting has been re-noticed, but in a new light. Concerns are increasingly articulated through a sense of loss—a loss of connection to starlight, or an aspect of nature, or the sublime, or a piece of our humanity—brought about by the loss of dark or ‘natural’ nights (e.g. Bogard, 2013 Bogard, P. (2013). The end of night: Searching for natural darkness in an age of artificial light. New York, NY: Back Bay Books. [Google Scholar]). The physics of fluorescent lights can’t be changed, but coatings inside the bulbs can be so they produce a warmer, less blue light. LED lights are more efficient than fluorescent lights, but they also produce a fair amount of light in the blue spectrum. Richard Hansler, a light researcher at John Carroll University in Cleveland, notes that ordinary incandescent lights also produce some blue light, although less than most fluorescent lightbulbs. Unfortunately, white LED lighting also tends to transmit high levels of blue light, which can pose potential health hazards. Few creationists have aggressively pursued solution one. The reasoning for this solution has been that if the distances of astronomical objects are not known that well, then astronomical bodies may be far closer than generally thought, and hence there is no light travel time problem. This solution amounts to defining the problem away, but there are additional problems with this solution. First, creationists who have suggested this solution do correctly point out that trigonometric parallax, the only direct method of measuring stellar distances, yields distances that at most are only a few hundred light years. So this could explain why we see all the stars for which we have directly determined distances. One might further reason that since the distance determination methods that give very great distances that cause the light travel time problem today are indirect, those indirect methods are somehow suspect. However, one cannot dismiss the indirect methods so easily. Most of these methods are based upon well understood physical principles, and many of the indirect methods are calibrated to trigonometric parallax. See Faulkner (2013) for a discussion of distance determination methods. Second, this solution relies upon the incorrectly formulated light travel time problem. While today we can see stars such as Alpha Centauri, the closest star similar to the sun, with this solution it would not have been visible to Adam at the conclusion of the Creation Week, because it is 4.3 light years away. For this solution to work, even the well determined trigonometric parallax method must be abandoned, but this is not physically supported. Maxman deseo Testo Ultra power up premium Celuraid Muscle BeMass power up premium VigRX Plus eracto power up premium