#SOLAR ECLIPSE MAESTRO KESTREL DOWNLOAD#

To subscribe : send an E-mail to the end of August 2007, the third Solar Eclipse Conference (SEC 2007) was held at the Griffith Observatory in Los Angeles, California, USA. If you want to keep in touch with everything to do with Solar Eclipses you should consider subscribing to the Solar Eclipse Mailing List (SEML).

Solar Eclipse Mailing List & Solar Eclipse Conferences and Workshops (adapted from Fred Espenak and Jean Meeus Five Millennium Canon) View the 204 Saros GIF animations by Dan McGlaun

#SOLAR ECLIPSE MAESTRO KESTREL DOWNLOAD#

Sorry, your browser doesn’t support embedded videos, but you can download it and watch it with your favorite video player! Mount Vinson (4,897 m), Antarctica 2008įive Millennium Animated GIFs of Saros Cycles.Having a look at the solar activity cycle is interesting to know if there is a chance to have sunspots and also know the general shape of the solar corona.

Know more about deltaT (ΔT) and leap seconds. Or explore the Five Millennium (-1999 to +3000) Canon of Solar Eclipses and its 11,898 eclipses to help you prepare your eclipse journeys or study historical events. The interactive Google maps or the Google Earth kmz files let you explore the path of totality and compute local circumstances of contemporary eclipses. You can also subscribe to a mailing list to stay posted. A time exposure calculator is there to help you choose your camera settings. You can use this solar eclipse calculator to compute the local circumstances of an eclipse, and the solar eclipse timer notifies the beginning of the various events. Those who want to concentrate on observing the event visually can rely on Solar Eclipse Maestro to automatically take pictures for them. Choosing your viewing location according to the phenomena you want to observe is equally important. You don’t want to find yourself in such inconvenient situation. This is why observing such a glorious and majestic event must be well planned in advance as shown in those various scouting trips or airborne when required. A total eclipse of the Sun occurs on average every 18 months (often in hardly reachable locations), but is only visible from a small band - the Path of Totality - and with an average duration of three minutes (maximum duration just over seven minutes). Chasing total solar eclipses is not only an addiction, but an affliction and a way of life that sometimes poses complex logistical, technical and financial problems. Those who were forunate enough to witness a total solar eclipse, in an unusual surroundings with clear sky, can testify of the outstanding beauty of such an event that also attracts celebrities. There is a special case where the apparent diameter of the Moon is smaller than that of the Sun at the beginning of the eclipse, then bigger (around the maximum) and then smaller again, the eclipse is then called a total-annular eclipse or hybrid eclipse as the one on April 8, 2005.

There are two types of central eclipses: total, when the apparent diameter of the Moon is bigger than that of the Sun (the Sun is fully eclipsed), and annular when the apparent diameter of the Moon is smaller than that of the Sun. When the Earth crosses the axis of the Moon’s umbra we have a central solar eclipse. When the Earth only crosses the penumbra of the Moon, we have a partial eclipse of the Sun. Solar eclipses occur during the New Moon, when the Earth enters the penumbra and then possibly the umbra of the Moon.

Solar eclipse maestro kestrel