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Without the passage of time on the astronomical scale, the Sun and Earth would reach the same distance from one another in 26,584 years. Difficulties producing accurate models for the late phases of these eclipses led to the establishment of an industry-wide Standard Deviations and Sensitivity Indicator Task in the early 1970s. It was suggested that a set of values for all eclipse magnitudes should be agreed upon, and the individual task to produce a set of values was motivated in 1974. It appears that the task was initially motivated by Lambert's calculations of the late, penumbral phases of the total 2010 annular eclipse of 28 August 2010, for which a private astronomer submitted a request to Intellivision, then the successor by merger to the entertainment company Mattel, Inc. The IAU Working Group on Standard Deviations and Sensitivity Indicators produced a document in 1971 on the effects of measurement precision, and the U.S. National Weather Service produced the first period of values in 1974, and a complete set in 1979. These have been widely distributed, and many commercial and free products exist, with the most famous being the NIST [National Institute for Standards and Technology] Web-Almanac. The American Astronomical Society has been evaluating eclipse observations since the 1970s and allows some people to do pseudo-observation by submitting to the AAPSO Circular Without respect to the activities outlined in this guide, the user still needs to find and apply a simple set of procedures for locating the times of the eclipse, for determining the exact location of the apparition, and for obtaining the phase curve.
In the middle of the 2001 eclipse of the Sun by the black hole/supermassive object Sgr A*, we used the JVLA to map clean, deep parts of the galactic center where stellar winds and associated magnetism have swept away most of the dust in the region. (We called it the "dust-free zone.") This region shines in X-rays, and because Sgr A* is an active galaxy, we expected some X-ray emission and emission from cyclotron magnetic resonance lines in the radio wavelengths from 2 to 10 GHz. But with only a few points to put on such a spectrum, we could barely see anything. This is why many believe that the idea of a black hole is a myth. d2c66b5586
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