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Solar Eclipse 2015 - Table of figures |
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6: Table of figures and websites used at this document Here, I list all images and websites used down the submenue astronomy. All pictures on this website, which are marked with "own image", are subject to my copyright. They may not be copied or used in individual parts without my consent. Pictures with foreign copyright are listed below, too. I have received a permit for use. To the end Fig. 1: My telescope; own image Back Fig. 2: First moonpicture; own image Back Fig. 2a: First moonpicture - large picture; own image Back Fig. 3: Second moonpicture; own image Back Fig. 3a: Second moonpicture - large picture; own image Back Fig. 4: Third moonpicture; own image Back Fig. 4a: Third moonpicture - large picture; own image Back Fig. 5: Destroyed wavefronts; own image Back Fig. 6: Run time error at the mirror; own image Back Fig. 7: Distorted glass surface as well as their simplification; own image Back Fig. 8: Distorted wave front by different propagation speed in the glass; own image Back Fig. 9: The projection method; own image Back Fig. 10: The observation crew; own image Back You will get a manual to buidt your own solar filter at: http://astrosolar.com/en/information/how-to/ Back to: "Sunobservation by direct observation with filters" Back to: "Sunobservation at solar eclipse 2015 chapter preliminary remarks " Fig. 11: Projection of Sun; own image Back Fig. 12: The "Sun egg"; own image Back Fig. 13: Transit of Mercury at May 07 2003; own image Back Fig. 13a: Transit of Mercury at May 07 2003 - large picture; own image Back Fig. 14: Mercury in front of Sun, May 07 2003; own image Back Fig. 14a: Mercury in front of Sun, May 07 2003 - large picture; own image Back Fig. 15: Construction of the centre of Sun; own image Back Fig. 16: Construction of the centre of Sun, application in the photo; own image Back Fig. 17: Sun-filter mounting; own image Back Fig. 18: Mounting the camera; own image Back Fig. 19: Transit of Venus at 11:36 o’clock; own image Back Fig. 19a: Transit of Venus at 11:36 o’clock - large picture; own image Back Fig. 20: Transit of Venus at 12:44 o’clock; own image Back Fig. 20a: Transit of Venus at 12:44 o’clock - large picture; own image Back Fig. 21: Transit of Venus, 'contact 3'; own image Back Fig. 21a: Transit of Venus, 'contact 3' - large picture; own image Back Fig. 22: Half Venus in front of Sun; own image Back Fig. 22a: Half Venus in front of Sun - large picture; own image Back Fig. 23: Apparent diameter of the Venus; own image Back When determining the astronomical unit (German language) look at: http://www.av-ortenau.de/archiv/venus2004/AE/ae.php (Copyright by Christian Flick) Back to: "Orbit data evaluation of Venus" Fig. 24: Transit of Venus, merged positions; own image Back Fig. 25: Computation of the Venus orbit; own image Back Fig. 26: the observer of Venus; own image Back Fig. 27: function f(Sv); own image Back Fig. 30: Central Zone of the solar eclipse on March 20, 2015 (Saros cycle 120) Created with Win-Eclipse 3.7 by Heinz Scsibrany and courtesy of Sonnenfinsternis.org(http://www.sofi2015.de). Times of contact: at Frankfurt, Germany, are found at the site: http://www.sofi2015.de/mitteleuropa.htm Go back to: "Where and at what time the event will take place?" Go back to: "Determining the degree of occultation of Sun" Fig. 31: Camera is ready; own image Go back Fig. 32: Sunbathing with safety goggles; own image. In courtesy of my daughter Go back to: "My observations" Go back to: "My experiences and results" Instructions for building your own solar filter are found at: http://astrosolar.com/de/informationen/know-how/ Go back to: "Solar filter, chapter Preliminary remark" Fig. 33: Image sequence eclipse history; own image Go back to: "My experiences" Go back to: "My results" Fig. 34: Compilation of my image sequence; own image Go back to: "My experiences and results" Go back to: "Compilation of my image sequence" Fig. 35: Graphical center-design of Sun and Moon; own image Go back Fig. 36: Graphical determining the degree of occultation of the Sun; own image Go back Fig. 37: Occultation [%] of Sun on March 20, 2015 from 9:30 to 11:30 CET; own image Go back German-power-net-survives-solar-eclipse: (© Deutsche Welle at: http://www.dw.de/german-power-net-survives-solar-eclipse/a-18331190) Go back Fig. 38: Daily results of solar power in Dresden on March 20, 2015 (Occultation Dresden: 71.5%) Wikimedia Commons: http://commons.wikimedia.org/wiki/File:Sonnenfinsternis_2015_Einstrahlung.svg; © Creative Commons CC0 Go back Fig. 39: Comparison of solar power in Dresden with my data of occultation; own image Go back Fig. 40: Inclination of the lunar orbit to the ecliptic. In courtesy of "Sternfreunde Bad Salzuflen e.V." Go back to: "Lunar orbit determination" Go back to: "Why don't solar eclipse turn up every month?" Fig. 41: Graphical determination of lunar orbital inclination using my image sequence; own image Go back to: "Inclination of the lunar orbit" Go back to: "Error analysis" Die Animation der Mondphasen: (© Andi Boesch) findet man unter: http://www.cybervisuals.ch/moon/moon.html, Go back With the online calculator (© Özgür Aydin) I calculated the data to: azimuth, elevation of Sun and Moon and distance in the range of my observation time at: http://www.kostenlose-online-rechner.de/entfernung-zur-sonne Go back Fig. 42: Emergence of a solar eclipse. In courtesy of "Sternfreunde Bad Salzuflen e.V." Go back Fig. 43: Emergence of a lunar eclipse. In courtesy of "Sternfreunde Bad Salzuflen e.V." Go back Lunar orbit und Saros cycle (© Ulf Unbehaun): http://www.astronomie.de/bibliothek/artikel-und-beitraege/der-erdmond/mondbahn-und-saroszyklus/ Go back Fig. 44: The variable apparent Moon diameter for different distances to Earth, © Thomas Hebbeker (see: http://www.spektrum.de/wissen/das-mysterium-supermond/1304167). In courtesy Thomas Hebbeker, Department of Physics, RWTH Aachen University Go back to: "Why Sun and Moon appear to us at the same size?" Go back to: "Why do we observe annular solar eclipses seldom?" Fig. 45: covering the sun at 09:28 CET; own image Go back Fig. 46: covering the sun at 09:35 CET; own image Go back Fig. 47: covering the sun at 09:48 CET; own image Go back Fig. 48: covering the sun at 10:01 CET; own image Go back Fig. 49: covering the sun at 10:17 CET; own image Go back Fig. 50: covering the sun at 10:29 CET; own image Go back Fig. 51: covering the sun at 10:38 CET; own image Go back Fig. 52: covering the sun at 10:54 CET; own image Go back Fig. 53: covering the sun at 11:09 CET; own image Go back Fig. 54: covering the sun at 11:20 CET; own image Go back Fig. 55: covering the sun at 11:33 CET; own image Go back Fig. 56: covering the sun at 12:03 CET; own image Go back Go back to: "Why do we observe annular solar eclipses seldom?" Back to directory | |
| Copyright by Hans Joachim Ilgen since 1950 | |