Cüvə
Cüvə (also, Cuvə, Güvə, and Dzhuva) is a village and municipality in the Agdash Rayon of Azerbaijan. It has a population of 496.
References
3C-2V
3C-2V is commonly marked on low cost coaxial cable used for domestic TV signals.
It is one of the options of the Japanese cable standard JIS C 3501.
Nominal loss at 100 MHz is 42 dB/km.
With its narrow core it is similar to RG-59 cable; RG-6 coax cable is better shielded and has lower losses.
References
External links
Internet slang
Internet slang (Internet shorthand, Cyber-slang, netspeak, or chatspeak) refers to a variety of slang languages used by different people on the Internet. It is difficult to provide a standardized definition of Internet slang due to the constant changes made to its nature. However, it can be understood to be a type of slang that Internet users have popularized, and in many cases, have coined. Such terms often originate with the purpose of saving keystrokes or to compensate for small character limits. Many people use the same abbreviations in texting and instant messaging, and social networking websites. Acronyms, keyboard symbols and abbreviations are common types of Internet slang. New dialects of slang, such as leet or Lolspeak, develop as ingroup internet memes rather than time savers.
Creation and evolution
Origins
Internet slang originated in the early days of the Internet with some terms predating the Internet. Internet slang is used in chat rooms, social networking services, online games, video games and in the online community. Since 1979, users of communications networks like Usenet created their own shorthand.
C/2015 V2
C/2015 V2 (JOHNSON) is a Parabolic Comet discovered on 3 November 2015 by Jess A. Johnson (Catalina Sky Survey) at an apparent magnitude of 17.1 using a 0.68-meter (27 in) Schmidt–Cassegrain telescope.
References
C/1948 V1
The Eclipse Comet of 1948, formally known as C/1948 V1, was an especially bright comet discovered during a solar eclipse on November 1, 1948. Although there have been several comets that have been seen during solar eclipses, the Eclipse Comet of 1948 is arguably the best-known; it was however, best viewed only from the Southern Hemisphere.
When it was first discovered during totality, it was already quite bright, at magnitude -2; as it was near perihelion, this was its peak brightness. Its visibility during morning twilight improved as it receded outward from the Sun; it peaked near zero magnitude, and at one point displayed a tail roughly 30 degrees in length, before falling below naked eye visibility by the end of December.
References
Comet Ikeya–Murakami
Comet Ikeya–Murakami (P/2010 V1) is a short-period comet with period of approximately 5.4 years first identified independently by the two Japanese amateur astronomers Kaoru Ikeya and Shigeki Murakami on November 3, 2010. Ikeya identified the comet using a 25-centimeter (10-inch) reflector at 39×, while Murakami used a 46 cm (18-inch) reflector at 78×. Photographic confirmation of the comet was obtained by Ernesto Guido and Giovanni Sostero using a Global-Rent-a-Scope (GRAS) telescope in New Mexico. Both Ikeya and Murakami discovered the comet using manual observation through optical telescopes. Such visual discoveries have become rare in recent years.
At the start of November 2010, a few weeks past perihelion passage, it was discovered the comet had undergone a major outburst between October 31 and November 3. After the 2010 perihelion passage, the comet only had about an 80-day observation arc.
The recovery of P/2010 V1 on December 31, 2015, at magnitude 20 was announced on January 2, 2016, and designated as P/2015 Y2. A secondary fragment (B) was confirmed and announced on January 5, 2016. The comet is now composed of component A and B with two different comas, envelopes and tails. Around January 11, 2016, two fainter potential fragments, designated P/2010 V1-C and P/2010 V1-D have been located, both likely having been fragmented from P/2010 V1-B. As of January 29, fragments B and D have nearly entirely desintegrated, and C is undergoing an outburst, making it as bright as P/2010 V1-A
