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Beginning in 2002, episodes of the original The Twilight Zone were adapted for radio, with Stacy Keach taking Serling's role as narrator and produced by Carl Amari of Falcon Picture Group. Each episode features a current Hollywood celebrity, including Jason Alexander, Blair Underwood, Lou Gossett, Jr., Michael York, Jim Caviezel, Jane Seymour, Don Johnson, Sean Astin, Luke Perry and others in the title roles. The series is broadcast on hundreds of radio stations from coast to coast and over Sirius/XM. The station list and episodes for download, including 3 Free episodes are available at the official website at www.twilightzoneradio.com

Many Treehouse Of Horror episodes of The Simpsons also reference the show. These include "Treehouse of Horror" (where the family are abducted by aliens, "Hungry Are The Damned"), "Treehouse of Horror III" (which features an evil Krusty The Clown doll, "Clown Without Pity") and "Treehouse of Horror IV" (where Bart sees a gremlin on the side of the school bus, "Terror at 5 1/2 Feet"). Homer also references the show in the "Homer3" segment of "Treehouse of Horror VI," when, upon entering the 3rd dimension, he says "It's like something out of that twilighty show about that zone".[59][60][61][62][63]

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The Twilight Zone (marketed as Twilight Zone for its final two seasons) is an American science fiction horror anthology television series created and presented by Rod Serling, which ran for five seasons on CBS from October 2, 1959, to June 19, 1964.[1] Each episode presents a standalone story in which characters find themselves dealing with often disturbing or unusual events, an experience described as entering "the Twilight Zone", often with a surprise ending and a moral. Although predominantly science-fiction, the show's paranormal and Kafkaesque events leaned the show towards fantasy and horror. The phrase "twilight zone", inspired by the series, is used to describe surreal experiences.

For example, some fish use an adaptation called counterillumination to keep from being seen by potential predators. Since light in the twilight zone comes from above, many predators look up to search for prey silhouetted against the surface. Consequently, some small prey fish have rows of organs called photophores along their bellies that emit light similar in intensity and color to the light of the surface water above, making them nearly invisible when viewed from below.

During World War II, U.S. Navy sonar operators looking for enemy submarines were puzzled when sonar images seemed to show the seafloor changing its depth, from about a quarter mile down during the day, to near the surface after dark. What appeared to be a shifting seafloor turned out to be plankton, fish, and other twilight-zone animals making a nightly migration to and from the surface to find food.

Another fast track for carbon into deeper water is through the daily migration of twilight zone animals that feed near the surface at night then bring the carbon in their food back down into the twilight zone during the day.

About 90 percent of the carbon that gets into the twilight zone remains there, but a small percentage of it sinks to down into the deep ocean when animals die or expel carbon-rich fecal matter. Once there, it can remain isolated from the atmosphere for hundreds or even thousands of years.

Open-water fisheries far from land are currently largely unregulated, and we do not yet know enough to ensure that potential extraction of fisheries from the twilight zone would be sustainable. Nevertheless, countries including Norway and Pakistan have already issued licenses to begin fishing the twilight zone. Work began in 2018 under the United Nations Law of the Sea Convention to promote the preservation and sustainable use of marine biodiversity in areas beyond national jurisdiction, but efforts so far have focused on improving the conservation of surface-water fisheries and the genetic resources of the seabed, not of the twilight zone and its important ecosystem services, which are not well understood.

In 2018, WHOI launched an ambitious mission to explore and understand the ocean twilight zone, with initial funding of $35 million from the Audacious Project. The effort is drawing on the expertise of a team of scientists and engineers, combining research, new technologies, and broad public engagement.

By combining these and other new technologies with more traditional methods such as ship-based sonar and net tows, WHOI scientists and engineers hope to rapidly advance our understanding of the twilight zone and the animals living in it.

Sequence alignments unambiguously distinguish between protein pairs of similar and non-similar structure when the pairwise sequence identity is high (>40% for long alignments). The signal gets blurred in the twilight zone of 20-35% sequence identity. Here, more than a million sequence alignments were analysed between protein pairs of known structures to re-define a line distinguishing between true and false positives for low levels of similarity. Four results stood out. (i) The transition from the safe zone of sequence alignment into the twilight zone is described by an explosion of false negatives. More than 95% of all pairs detected in the twilight zone had different structures. More precisely, above a cut-off roughly corresponding to 30% sequence identity, 90% of the pairs were homologous; below 25% less than 10% were. (ii) Whether or not sequence homology implied structural identity depended crucially on the alignment length. For example, if 10 residues were similar in an alignment of length 16 (>60%), structural similarity could not be inferred. (iii) The 'more similar than identical' rule (discarding all pairs for which percentage similarity was lower than percentage identity) reduced false positives significantly. (iv) Using intermediate sequences for finding links between more distant families was almost as successful: pairs were predicted to be homologous when the respective sequence families had proteins in common. All findings are applicable to automatic database searches.

Possible instrument combinations: OSIRIS TZ observations can be run on LRIS, HIRES, OSIRIS and MOSFIRE nights. NIRC2 TZ observations can be run on DEIMOS, KCWI, NIRC2, NIRES and NIRSPEC nights. TZ observations during twilights are more suited for nights when the classically-scheduled program uses an optical instrument (LRIS, HIRES, DEIMOS or KCWI).

The ocean is divided into three zones based on depth and light level. The upper 200 meters of the ocean is called the euphotic, or "sunlight," zone. This zone contains the vast majority of commercial fisheries and is home to many protected marine mammals and sea turtles.

The aphotic zone exists in depths below 1,000 meters. Sunlight does not penetrate to these depths and the zone is bathed in darkness. The aphotic zone is further subdivided into the bathypelagic zone (or midnight zone) between 1,000 and 4,000 meters, the abyssopelagic (or the abyss) between 4,000 and 6,000 meters, and the hadopelagic zone (or hadal zone) 6,000 meters and deeper.

The W.M. Keck Observatory has implemented a cadence observing program for observations conducted during twilight - periods that are not otherwise utilized by the classically-scheduled observers due to limitations on the sky brightness. We initiated observations with NIRC2 NGS-AO during semester 18A as a pilot program to monitor spatially resolved, temporal phenomena on Solar System objects. The observations are performed when the classically-scheduled observers on Keck II using optical spectrometers DEIMOS or KCWI surrender the twilight time, because the sky is too bright to obtain any useful data at visible wavelengths. The observations can be executed by the Keck Observing Assistants (OAs). To facilitate the work of the OAs, web-based planning tools, observation scripts, and instructions ( ) were developed by N. Molter, with contributions from K. de Kleer, in the framework of the Keck Visiting Scholars program. The twilight observing program has already proven very successful, with observations carried out on 26 different nights within the last year, leading to a science publication (Molter et al. 2018, submitted) and to a considerable gain on telescope time utilization. Due to the success of the pilot twilight observing program, cadence twilight observing is included in our call for proposals starting in semester 18B. The twilight observing program is open to the four major W. M. Keck Observatory constituents; UC, CIT, NASA and UH. Each institution is limited to one program, where programs designed for a duration of 1 to 2 years have priority. The main guiding principles of this program are (1) voluntary participation by classically-scheduled PI and OA, and (2) execution of observations completely at the discretion of the classically-scheduled PI and OA. Any PI proposing a cadence twilight observing program is required to develop the appropriate tools for the OAs to conduct the observations autonomously. Specifically, PIs are required to (1) develop target and observation managers, (2) develop, test and debug observation scripts, (3) employ simple instrument configurations, and (4) dissect the observations in short individual integrations (

This organic matter forms the base of the marine food web, which basically means that these microscopic plants serve as food for tiny marine animals called zooplankton, which are eaten by larger marine organisms and so on up to larger animals, like the fish that humans consume. Many of these animals come up from the twilight zone at night, using the cover of darkness to feed in surface waters and then disappear come daybreak. This is, in fact, the largest animal migration on Earth and happens around the globe every day, and we barely know it happens. ff782bc1db