From: owner-ammf-digest@smoe.org (alt.music.moxy-fruvous digest) To: ammf-digest@smoe.org Subject: alt.music.moxy-fruvous digest V14 #4976 Reply-To: ammf@fruvous.com Sender: owner-ammf-digest@smoe.org Errors-To: owner-ammf-digest@smoe.org Precedence: bulk alt.music.moxy-fruvous digest Saturday, September 19 2020 Volume 14 : Number 4976 Today's Subjects: ----------------- Safely Clean Your Ears with Qgrips ["Qgrips" Subject: Safely Clean Your Ears with Qgrips Safely Clean Your Ears with Qgrips http://bloodpressolution.co/sYvY-TnNnxbHa3woAafSXfFdugWBQ1xhjvVFHAM9fSYIue6q http://bloodpressolution.co/QLNLq2iCYXsqNM-YtE3my_dNrU1fwgHhIvRxvApV_ABWCQ-v mmand module pilot, Worden forged a close, lifelong friendship with the prime crew's CMP, Dick Gordon, with whom he trained. Worden remembered, "Dick was my buddy. We flew together and worked together for a year and a half when he was training for Apollo 12 and I was his backup. We just went everywhere together. We worked really hard but it was also a lot of fun." Gordon and Worden learned navigational techniques for space, so that if communications with Mission Control failed, the CMP could bring the craft home. Worden remembered that the Apollo 12 prime crew, led by Pete Conrad, had a close bond and drove matching black and gold Chevrolet Corvettes at Kennedy Space Center (KSC). In reaction, the backup crew secured a red one for Irwin, white for Worden, and a blue car for Scott, both emphasizing their individuality within the crew, and making them less conspicuous at times when they did not want to be recognized as astronauts, especially since the three cars were rarely seen together. Apollo 15 Preparation and launch Worden in the command module during training Scott, Worden and Irwin were publicly named as the crew of Apollo 15 on March 26, 1970. Apollo 15 was originally scheduled to be an H mission, with a limited stay of 33 hours on the Moon and two moonwalks, but the cancellation of two Apollo missions in mid-1970 meant the flight would be a J mission, with three moonwalks during its three-day stay, the first Lunar Roving Vehicle (LRV), and in the service module (SM) a suite of scientific instruments to probe the Moon. It was Worden's job, as his crewmates walked on the Moon, to operate these devices. For the first time, observations from lunar orbit was made a formal mission objective, and, like the CMPs of Apollo 13 and Apollo 14, Worden worked with geologist Farouk El-Baz during training, learning to interpret what he saw as he flew over the mountains and deserts of the western United States. Worden found El-Baz to be an enjoyable and inspiring teacher. He also accompanied his crewmates on geology training which took them to places where they walked over terrain resembling the Moon's, including sites in Hawaii, Mexico and Iceland. He trained for the possibility he might have to return without Scott and Irwin, or rescue them if the LM launched into the wrong orbit. When he was not busy with that or other training, Worden spent much of his time at North American Rockwell's facilities at Downey, supervising the construction and tes ------------------------------ Date: Fri, 18 Sep 2020 06:09:31 -0400 From: "wood shed plans" Subject: How to build sheds like lego bricks... This email must be viewed in HTML mode. ------------------------------ Date: Fri, 18 Sep 2020 10:04:45 -0400 From: "Massive Male Plus Basic" Subject: Hit This Pressure Point To Increase Your Size by 67% Hit This Pressure Point To Increase Your Size by 67% http://loyalation.buzz/ErxXFUW6tuDjRnMbCtbGmuVTbeFqlRLJOfRGw2_n0hZ29fQ http://loyalation.buzz/ejtG9_HH4TNvGG0RQLQ73zcGgF4Os2gvX9D5xQKLq5XlzQ eriod when the Vedas were composed, the liturgical hymns from some of the Indo-Aryan. The Vedic culture was located in part of north-west India, while other parts of India had a distinct cultural identity during this period. The Vedic culture is described in the texts of Vedas, still sacred to Hindus, which were orally composed in Vedic Sanskrit. The Vedas are some of the oldest extant texts in India. The Vedic period, lasting from about 1500 to 500 BCE, contributed the foundations of several cultural aspects of the Indian subcontinent. In terms of culture, many regions of the Indian subcontinent transitioned from the Chalcolithic to the Iron Age in this period. Vedic society An early 19th century manuscript in the Devanagari script of the Rigveda, originally transmitted orally with fidelity Historians have analysed the Vedas to posit a Vedic culture in the Punjab region and the upper Gangetic Plain. Most historians also consider this period to have encompassed several waves of Indo-Aryan migration into the Indian subcontinent from the north-west. The peepal tree and cow were sanctified by the time of the Atharva Veda. Many of the concepts of Indian philosophy espoused later, like dharma, trace their roots to Vedic antecedents. Early Vedic society is described in the Rigveda, the oldest Vedic text, believed to have been compiled during 2nd millennium BCE, in the northwestern region of the Indian subcontinent. At this time, Aryan society consisted of largely tribal and pastoral groups, distinct from the Harappan urbanisation which had been abandoned. The early Indo-Aryan presence probably corresponds, in part, to the Ochre Coloured Pottery culture in archaeological contexts. At the end of the Rigvedic period, the Aryan society began to expand from the northwestern region of the Indian subcontinent, into the western Ganges plain. It became increasingly agricultural and was socially organised around the hierarchy of the four varnas, or social classes. This social structure was characterised both by syncretising with the native cultures of northern India, but also eventually by the excluding of some indigenous peoples by labeling their occupations impure. During this period, many of the previous small tribal units and chiefdoms began to coalesce into Janapadas (monarc ------------------------------ Date: Thu, 17 Sep 2020 16:02:10 -0400 From: "Painful ear flushing" Subject: Scientists: Tinnitus Has Nothing To Do With Your Ears Scientists: Tinnitus Has Nothing To Do With Your Ears http://naturalmedi.co/O4GR6XWZnmxq_MIGaj5fyRYecFrtcIfCRnUYCyBt7VlulZvL http://naturalmedi.co/TuEflXC2EPAHlPjCH3FLXd45CY2ke2VDRNg-s3sPTY9CafBL Without an atmosphere, a small star would have an apparent size, an "Airy disk", in a telescope image determined by diffraction and would be inversely proportional to the diameter of the telescope. However, when light enters the Earth's atmosphere, the different temperature layers and different wind speeds distort the light waves, leading to distortions in the image of a star. The effects of the atmosphere can be modeled as rotating cells of air moving turbulently. At most observatories, the turbulence is only significant on scales larger than r0 (see belowbthe seeing parameter r0 is 10b20 cm at visible wavelengths under the best conditions) and this limits the resolution of telescopes to be about the same as given by a space-based 10b20 cm telescope. The distortion changes at a high rate, typically more frequently than 100 times a second. In a typical astronomical image of a star with an exposure time of seconds or even minutes, the different distortions average out as a filled disc called the "seeing disc". The diameter of the seeing disk, most often defined as the full width at half maximum (FWHM), is a measure of the astronomical seeing conditions. It follows from this definition that seeing is always a variable quantity, different from place to place, from night to night, and even variable on a scale of minutes. Astronomers often talk about "good" nights with a low average seeing disc diameter, and "bad" nights where the seeing diameter was so high that all observations were worthless. Slow motion movie of the image seen at a telescope when looking at a star at high magnification (negative images). The telescope used had a diameter of about 7r0 (see definition of r0 below, and example simulated image through a 7r0 telescope). The star breaks up into multiple blobs (speckles) -- entirely an atmospheric effect. Some telescope vibration is also noticeable. The FWHM of the seeing disc (or just "seeing") is usually measured in arcseconds, abbreviated with the symbol (?). A 1.0? seeing is a good one for average astronomical sites. The seeing of an urban environment is usually much worse. Good seeing nights tend to be clear, cold nights without wind gusts. Warm air rises (convection), degrading the seeing, as do wind and clouds. At the best high-altitude mountaintop observatories, the wind brings in stable air which has not previously been in contact with the ground, sometimes providing seeing as good as 0.4". r0 and t0 The astronomical seeing conditions at an observatory can be conveniently described by the parameters r0 and t0. For telescopes with diameters smaller than r0, the resolution of long-exposure images is determined primarily by diffraction and the size of the Airy pattern and thus is inversely proportional to the telescope diameter. For telescopes with diameters larger than r0, the image resolution is determined primarily by the atmosphere and is independent of telescope diameter, remaining constant at the value given by a telescope of diameter equal to r0. r0 also corresponds to the length-scale over which the turbulence becomes significant (10b20 cm at visible wavelengths at good observatories), and t0 corresponds to the time-scale over which the changes in the turbulence become significant. r0 determines the spacing of the actuators needed in an adaptive optics system, and t0 determines the correction speed required to compensate for the effects of the atmosphere. ------------------------------ Date: Fri, 18 Sep 2020 10:47:50 -0400 From: "CV-19 Survivors" Subject: The New 'Miracle' Medicine That's Sweeping The USA The New 'Miracle' Medicine That's Sweeping The USA http://crisplinks.co/g03V-eAuQ1AfA46WbFsYB_ooYNGkq1xZrtuPBEoZFrc_YV_p http://crisplinks.co/wYW2RqRYudd1FBFCaTqgpW4EBWWxD3uVGwlFQtKXV0S4wXq4 An optical telescope gathers and focuses light mainly from the visible part of the electromagnetic spectrum (although some work in the infrared and ultraviolet). Optical telescopes increase the apparent angular size of distant objects as well as their apparent brightness. In order for the image to be observed, photographed, studied, and sent to a computer, telescopes work by employing one or more curved optical elements, usually made from glass lenses and/or mirrors, to gather light and other electromagnetic radiation to bring that light or radiation to a focal point. Optical telescopes are used for astronomy and in many non-astronomical instruments, including: theodolites (including transits), spotting scopes, monoculars, binoculars, camera lenses, and spyglasses. There are three main optical types: The refracting telescope which uses lenses to form an image. The reflecting telescope which uses an arrangement of mirrors to form an image. The catadioptric telescope which uses mirrors combined with lenses to form an image. A Fresnel Imager is a proposed ultra-lightweight design for a space telescope that uses a Fresnel lens to focus light. Beyond these basic optical types there are many sub-types of varying optical design classified by the task they perform such as astrographs, comet seekers and solar telescopes. Radio telescopes The Very Large Array at Socorro, New Mexico, United States. Main articles: Radio telescope and Radio astronomy Radio telescopes are directional radio antennas that typically employ a large dish to collect radio waves. The dishes are sometimes constructed of a conductive wire mesh whose openings are smaller than the wavelength being observed. Unlike an optical telescope, which produces a magnified image of the patch of sky being observed, a traditional radio telescope dish contains a single receiver and records a single time-varying signal characteristic of the observed region; this signal may be sampled at various frequencies. In some newer radio telescope designs, a single dish contains an array of several receivers; this is known as a focal-plane array. ------------------------------ End of alt.music.moxy-fruvous digest V14 #4976 **********************************************