From: owner-ammf-digest@smoe.org (alt.music.moxy-fruvous digest) To: ammf-digest@smoe.org Subject: alt.music.moxy-fruvous digest V14 #5676 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 Tuesday, January 12 2021 Volume 14 : Number 5676 Today's Subjects: ----------------- You Donât Have to be Alone ["Jucy Date" ] stone carving ["Mr Kin" ] Youâve Been Nominated for inclusion with Whoâs Who⦠["Erica Weinberg" Subject: You Donât Have to be Alone You Donbt Have to be Alone http://obamas.guru/40IH52C0l1yqCeWzTzki7qQq14PBDUMEfMkg0wFyaiFX2CaY http://obamas.guru/CWQwPJCtiHnnilyIjOYrVvd3NVRw6_z8ZOd6zd0elhUI-fEE n radio and telecommunications, the frequency spectrum can be shared among many different broadcasters. The radio spectrum is the part of the electromagnetic spectrum corresponding to frequencies lower below 300 GHz, which corresponds to wavelengths longer than about 1 mm. The microwave spectrum corresponds to frequencies between 300 MHz (0.3 GHz) and 300 GHz and wavelengths between one meter and one millimeter. Each broadcast radio and TV station transmits a wave on an assigned frequency range, called a channel. When many broadcasters are present, the radio spectrum consists of the sum of all the individual channels, each carrying separate information, spread across a wide frequency spectrum. Any particular radio receiver will detect a single function of amplitude (voltage) vs. time. The radio then uses a tuned circuit or tuner to select a single channel or frequency band and demodulate or decode the information from that broadcaster. If we made a graph of the strength of each channel vs. the frequency of the tuner, it would be the frequency spectrum of the antenna signal. In astronomical spectroscopy, the strength, shape, and position of absorption and emission lines, as well as the overall spectral energy distribution of the continuum, reveal many properties of astronomical objects. Stellar classification is the categorisation of stars based on their characteristic electromagnetic spectra. The spectral flux density is used to represent the spectrum of a light-source, such as a sta ------------------------------ Date: Tue, 12 Jan 2021 16:28:52 +0800 From: "Mr Kin" Subject: stone carving Dear distributor We are one of the professional stone carving manufacturers in China.We provide stone carving,stone crafts,tombstones,white marble cravings,stone carving buddha statues etc.,which has good reputation all around the world. If you need these products,please reply us with your requirement details!We will offer you our best price at once! Waiting for your early reply. Thanks & B.regards Mr Kin ------------------------------ Date: Tue, 12 Jan 2021 03:06:35 -0500 From: "Erica Weinberg" Subject: Youâve Been Nominated for inclusion with Whoâs Who⦠Youbve Been Nominated for inclusion with Whobs Whob& http://remedypro.us/hHO5ArjhUaYBDB5EzdMtwdHxQri4LiDU_pnnvtwRIAfbccyl http://remedypro.us/ddSn3OmdHRTG8_hc2DgMx1_yzRAb5xFWmrcb34zLJTZL4CKD he focal length of an optical system is a measure of how strongly the system converges or diverges light; it is the inverse of the system's optical power. A positive focal length indicates that a system converges light, while a negative focal length indicates that the system diverges light. A system with a shorter focal length bends the rays more sharply, bringing them to a focus in a shorter distance or diverging them more quickly. For the special case of a thin lens in air, a positive focal length is the distance over which initially collimated (parallel) rays are brought to a focus, or alternatively a negative focal length indicates how far in front of the lens a point source must be located to form a collimated beam. For more general optical systems, the focal length has no intuitive meaning; it is simply the inverse of the system's optical power. In most photography and all telescopy, where the subject is essentially infinitely far away, longer focal length (lower optical power) leads to higher magnification and a narrower angle of view; conversely, shorter focal length or higher optical power is associated with lower magnification and a wider angle of view. On the other hand, in applications such as microscopy in which magnification is achieved by bringing the object close to the lens, a shorter focal length (higher optical power) leads to higher magnification because the subject can be brought closer to the center of project ------------------------------ Date: Tue, 12 Jan 2021 04:17:43 -0500 From: "Exclusive Reward" Subject: Congrats! You've received an Lowe's reward Congrats! You've received an Lowe's reward http://tinnitusterminator.best/AK099vZbuwiI5NqEcZCzPwzLa01T6OpK_gHEMPEUbxL0p_hS http://tinnitusterminator.best/cRdgK4IMV8i10EE3MDeA50SI7vtw_cVHWQYXInA-Q0nzS5mJ lectromagnetic spectrum refers to the full range of all frequencies of electromagnetic radiation and also to the characteristic distribution of electromagnetic radiation emitted or absorbed by that particular object. Devices used to measure an electromagnetic spectrum are called spectrograph or spectrometer. The visible spectrum is the part of the electromagnetic spectrum that can be seen by the human eye. The wavelength of visible light ranges from 390 to 700 nm. The absorption spectrum of a chemical element or chemical compound is the spectrum of frequencies or wavelengths of incident radiation that are absorbed by the compound due to electron transitions from a lower to a higher energy state. The emission spectrum refers to the spectrum of radiation emitted by the compound due to electron transitions from a higher to a lower energy state. Light from many different sources contains various colors, each with its own brightness or intensity. A rainbow, or prism, sends these component colors in different directions, making them individually visible at different angles. A graph of the intensity plotted against the frequency (showing the brightness of each color) is the frequency spectrum of the light. When all the visible frequencies are present equally, the perceived color of the light is white, and the spectrum is a flat line. Therefore, flat-line spectra in general are often referred to as white, whether they represent light or another type of wave phenomenon (sound, for example, or vibration in a structu ------------------------------ Date: Tue, 12 Jan 2021 02:38:22 -0500 From: "FedEx Opinion Requested" Subject: "Leave your feedback and you could WIN! "Leave your feedback and you could WIN! http://obamas.guru/voEopF-cg7ijIpgPAPLW4d4NhQ8ShpnO9UqAFAWbsEJkUfSB http://obamas.guru/dnpBCz7nOLSJ6cz2VNIIn8kerUkKdrhJ6SMa01-xvfgfc13g t the gallery the Reeds staged nine pieces by William Brough,[n 6] seven by F. C. Burnand,[n 7] and five by W. S. Gilbert,[n 8] whose Ages Ago (1869, with music by Frederic Clay) was the Reeds' longest-running and most frequently revived production, narrowly outdistancing Burnand and Arthur Sullivan's Cox and Box. Other authors whose works were presented there included Shirley Brooks, Henry Chorley, James PlanchC), Robert Reece, T. W. Robertson, Bolton Rowe and Tom Taylor. Among the composers in addition to Reed, Parry, Macfarren, Sullivan, Gabriel and Clay were Alfred Cellier and James Molloy. The Reeds' lease of the gallery expired at the end of July 1873, and the building ceased to be used as a performance space. The programme for the last night there, on 31 July, comprised Mildred's Well; or A Romance of the Middle Ages by Burnand and Reed, Very Catching by Burnand and Molloy, and Our Garden Party by Corney Grain. The Reeds moved to St George's Hall at the opposite end of Regent Street; the gallery became the banqueting hall of the Pall Mall Restaurant, which occupied the site until 1883, when the building was leased by the new Constitutional Cl ------------------------------ Date: Mon, 11 Jan 2021 05:24:32 -0500 From: "Kohls Opinion Requested" Subject: Kohls reward - Open immediately! Kohls reward - Open immediately! http://malecourse.buzz/1fA6o7gjkRM-1y8etwVd-EoWvZfAwvn2yAHWWLQk9LWSwNXc http://malecourse.buzz/r7hKSf_YxjnBhffb5UIRkD7GEoaIovNAr1XB9xlnP-zMzeYj n early December 1984, a Union Carbide India Limited pesticide plant in Bhopal leaked around 32 tons of toxic gases, including methyl isocyanate (MIC) gas which led to the worst industrial disaster in the world to date. The official death toll was initially recorded as around 4,000. A Madhya Pradesh government report stated 3,787 deaths, while other estimates state the fatalities were significantly higher (16,000) from the accident and the medical complications caused by the accident in the weeks and years that followed. The higher estimates have been challenged. The impact of the disaster continues to this day in terms of psychological and neurological disabilities, blindness, skin, vision, breathing, and birth disorders. The soil and ground water near the factory site have been contaminated by the toxic wastes. The Bhopal disaster continues to be the part of the socio-political debate; the clean-up of environmental contamination and rehabilitation of those affected continues to challenge the people of Bhopal. Compensation to families of the victims - The Centre is seeking a direction to Union Carbide and other firms for Rs 78.44 billion additional amount over and above the earlier settlement amount of USD 470 million in 1989 for paying compensation to the gas tragedy victim ------------------------------ Date: Mon, 11 Jan 2021 06:38:33 -0500 From: "Preventing Barking" Subject: The Solution to Annoying Barking The Solution to Annoying Barking http://newfund.buzz/2Zd5K3R-u8ZFq2IqLQwtBkUPyorVbafFHcUN6uiz16FmCvZq http://newfund.buzz/FFLUUwq-Qy4AAbsZq8CYgwQv9L0Znvwg7UYZhW6p4mIx2-rU hopal has a humid subtropical climate, with cool, dry winters, a hot summer and a humid monsoon season. Summers start in late March and go on till mid-June, the average temperature being around 30 B0C (86 B0F), with the peak of summer in May, when the highs regularly exceed 40 B0C (104 B0F) Extreme high in May was 46.7 B0C on 19 May 2016 and in June it was 45.9 B0C on 7 June 2019. The monsoon starts in late June and ends in late September. These months see about 40 inches (1020 mm) of precipitation, frequent thunderstorms and flooding. The average temperature is around 25 B0C (77 B0F) and the humidity is quite high. Temperatures rise again up to early November when winter starts, which lasts up to early March. Winters in Bhopal are cool, and not very much comfortable like summers, with average daily temperatures around 16 B0C (61 B0F). The winter peaks in January when temperatures may drop close to freezing on some nights. Lowest temperature ever recorded was 0.3 B0C. Total annual rainfall is about 1146 mm (46 inch ------------------------------ Date: Sun, 10 Jan 2021 09:21:56 -0500 From: "Massive Male Plus" Subject: Any man out there add length and girth in under one minute... Any man out there add length and girth in under one minute... http://pocketinsurance.buzz/kT4Ro5oc5ciPD7ZZI5OqBtBlcogsIb1qF5JchjjG2JH_-eHx http://pocketinsurance.buzz/jv5nq6cjRAFK-y8Tp_4ElvI_DZc7UUeE7sKlueMJA6Q-SL-l rate pool for each series b the Wild Card games, the Division Series, the League Championship Series, and the World Series. The players' bonus pool is funded with 60% of the gate receipts for each of the Wild Card games, the first three games of each Division Series, the first four games of each LCS and the first four games of the World Series; limiting the funding for the pool to these games, the minimum number in each series, removes incentive to extend the series for merely fiscal sake. The value of the gate is determined by the size of the venues, the amount of high-priced premium seating in the venues, the number of games played in the series and whether the games sell out. Ticket prices for each series are set by MLB, not the home teams, so they are relatively uniform across baseball. How much the winner and loser receives from each pool The World Series winner gets 36%, the World Series loser gets 24%, both League Championship Series losers get 12%, the four Division Series losers get 3.25%, and the two Wild Card playoff losers get 1.5%. In 2020, the eight Wild Card Series losers got 0.375%. How the team's share of the pool is divided The division of the team's share of the pool is voted upon by the players who have been on the team during the entire regular season, in a meeting chaired by their union representative. This meeting follows the trade deadline on July 31. Players who have been with the team for the full season automatically receive a full share. At the meeting, the full-season players vote on whether anyone elsebincluding players who have not been with the team for the full season, coaches, and trainersbis to be granted a full share, less than a full share, a cash award, or no share. After the World Series, the pool of money is split according to the shares determined in the vote. There is no limit to the number of shares that may be granted, but a greater number of shares dilutes the value of each share, and consequently the amount each player is awarded. As an example, playoff-pool full-share holders for the St. Louis Cardin ------------------------------ End of alt.music.moxy-fruvous digest V14 #5676 **********************************************