![]() ![]() While Charles Bolden is a real NASA official, he issued no report or announcement about "15 days of darkness." Moreover, Newswatch33 web site was not a legitimate news outlet, but a fake news site that began darkening the doorstep of social media networks shortly after the nearly identical NewsWatch28 fake news site shut down in mid-2015. This bit of fake news was lifted from an older (debunked) viral rumor that had already been around the online block several times before and has long since become an "evergreen" online hoax - a jape that is typically resurrected a few times a year by dubious web sites that simply update the time span for the alleged "period of darkness" and send it winging around the Internet again. According to officials, the "November Black Out" event will be caused by another astronomical event between Venus and Jupiter.Ĭharles Bolden, who was appointed to head of NASA by President Obama, issued a 1000 page document explaining the event to the White House. ![]() and will end on Monday, Novemat 4:15 p.m. The event, according to NASA, hasn't occurred in over 1 Million years.Īstronomers from NASA have indicated that the world will remain in complete darkness starting on Sunday, Novemat 3 a.m. During an unprecedented 1-year mission to the International Space Station, scientists are studying how astronauts bodies respond to long-duration space travel. NASA has confirmed that the Earth will experience 15 days of total darkness between November 15 and November 29, 2015. Please read the corrigendum first before accessing the article.Back in July 2015, the fake news web site Newswatch33 published an article titled "NASA Confirms Earth Will Experience 15 Days of Complete Darkness in November 2015," reporting that: We note that in these specific case studies, the linear particle depolarization ratio for smoke and dust-dominated aerosol are more similar at 355 nm than at 532 nm, having possible implications for using the particle depolarization ratio at a single wavelength for aerosol typing. The depolarization in the smoke case may be explained by the presence of coated soot aggregates. The smoke layer has the opposite spectral dependence, with the peak of 0.24 at 355 nm, decreasing to 0.09 and 0.02 at 5 nm, respectively. President Ronald Reagans State of the Union Address directs NASA to build an international space station within the next 10 years. The cause of the maximum at 1064 nm is inferred to be very large particles that have not settled out of the dust layer. A case of aerosol containing locally generated wind-blown North American dust has a maximum of 0.38 at 1064 nm, decreasing to 0.37 and 0.24 at 532 and 355 nm, respectively. ET on Wednesday morning, with the agency’s most powerful rocket ever kicking off a nearly month-long journey. A case of transported Saharan dust has a spectral dependence with a peak of 0.30 at 532 nm with smaller particle depolarization ratios of 0.27 and 0.25 at 1064 and 355 nm, respectively. Key Points NASA launched the Artemis I mission from Florida at 1:47 a.m. Participants will be: Kirt Costello, deputy chief scientist, International Space Station Program Science Office, NASA’s Johnson Space Center. NASA Television will provide live coverage, as well as streaming Internet coverage. These cases have partial analogs in earlier HSRL-1 depolarization measurements at 5 nm and in literature, but the availability of three wavelengths gives additional insight into different scenarios for non-spherical particles in the atmosphere. 2: An ISS Science, Research and Technology briefing will be held at Kennedy’s Press Site at 1 p.m. The three measurement cases presented here include two cases of dust-dominated aerosol and one case of smoke aerosol. UTC 15 - Mar - 2015 14:00 Tropical Cyclone Nathan's Winds March 15-16, 2015 as seen. The HSRL-2 instrument measures depolarization at three wavelengths: 355, 532, and 1064 nm. in the news NASA's ISS - RapidScat Wind Data Proving Valuable for. Particle depolarization ratio from lidar is an indicator of non-spherical particles and is sensitive to the fraction of non-spherical particles and their size. Linear particle depolarization ratio is presented for three case studies from the NASA Langley airborne High Spectral Resolution Lidar-2 HSRL-2). ![]()
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