12/9/2023 0 Comments Unlabeled lunar eclipse diagram![]() I share cloud statistics along the eclipse path compiled by Jay Anderson, the foremost eclipse meteorologist. I discuss aspects of EPO based on my experiences at the 60 solar eclipses I have seen. I discuss ongoing plans and discussions for EPO and scientific observing of the 21 August 2017 total solar eclipse. Preparing for and Observing the 2017 Total Solar Eclipse In 2023, the path of annularity of an annular eclipse will cross Mexico, the United States, and Canada, with partial phases visible throughout those countries. The next total solar eclipse path crossing the U.S. It is timely, given that a total solar eclipse will cross the continental United States on August 21, 2017. This Resource Letter provides a guide to the available literature, listing selected books, articles, and online resources about scientific, cultural, and practical issues related to observing solar eclipses. Resource Letter OSE-1: Observing Solar Eclipses A variety of investigations of the Sun and of the response of the terrestrial atmosphere and ionosphere to the abrupt solar cutoff can be carried out at the future eclipses, making the Antarctic observations scientifically useful. On behalf of the Working Group on Solar Eclipses of the IAU, the poster showed the solar eclipses visible from Antarctica and this article shows a subset (see for the full set). Partial phases as high as 87% coverage were visible and were imaged in Antarctica on 2011 November 25, and in addition to partial phases of the total and annular eclipses listed above, partial phases were visible in Antarctica on 2001 July 2011, 2002 DecemApSeptemSeptember 11, and 2009 January 26, and will be visible on 2015 SeptemSeptemFebruFebruary 15, and 2020 December 14. Totality crossing Antarctica included the eclipse of 2003 November 23, and will next occur on 2021 December 4 annularity crossing Antarctica included the eclipse of 2008 February 7, and will next occur on 2014 April 29. Aspects of the solar corona are still best observed during totality of solar eclipses, and other high-resolution observations of coronal active regions can be observed with radio telescopes by differentiation of occultation observations, as we did with the Jansky Very Large Array for the annular solar eclipse of 2012 May 20 in the US.
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