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M48 Kommando Survival Rescue Axe UC2820 Sign in Cart 0 Product Products (empty) No products Free shipping! This law enforcement quality badge is master crafted; with a durable high luster finish and a strong clip attachment on the back.
You must have JavaScript enabled in your browser to utilize the functionality of this website. A total eclipse of the Sun has not been seen in the continental USA for nearly two generations. Although people may opt for the longer durations in eastern regions of the USA, poorer weather prospects here suggest going west. Prudence may suggest observing from regions of good weather prospects with shorter durations than locations with longer durations that have higher probabilities of not seeing the eclipse at all. Currently maximum total eclipse durations are declining with the 2009 July eclipse longest of the 21st Century. Finally, maximum duration of a total solar eclipse occurs only on the center line of the eclipse path about mid-way between its ends.
Read about the Eclipse at Madras, Oregon including circumstance of the eclipse in Part  4. Extended capacity, Ruger factory markings, and guaranteed performance make this Mini-14 magazine a must have for any fan of the Mini-14.
Travel anywhere out west and you will see farmers and ranchers with their Mini-14 rifles in their trucks.
A seven minute duration will not happen again until 2150 June (7m14s) while a total eclipse with a duration near maximum is nearly two centuries in the future.

Not until 2078 will total eclipse durations begin to increase when Saros cycle 139 begins to bring eclipses of longer and longer durations. This position may often be difficult to access as it was, for example, during the 2012 November Australia eclipse. Look at the world events in Paris, France and you will see the French National Police using the Mini-14 for security applications. Although eclipse durations have their maximum values along points on the central line, these durations diminish with increasing distance from the central line. Almost half are approximately three minutes or less (as will be with the 2017 August eclipse). This will not happen until the remarkable 2186 July total eclipse (7m29s), the longest duration of totality during the years -2000 to +4000. For this eclipse, maximum duration was 4m02s over the central Pacific Ocean and not the Australian mainland. This versatile rifle fills the void where a tactical rifle that does not look miltary in nature is desired, while the military-style performance is not sacrificed.For years Ruger refused to manufacture magazines that held more than 10-rounds which left production to aftermarket companies. Annular eclipses occur when the Moon's disk is not large enough to hide the entire solar disk at maximum eclipse. Unfortunately, this long duration will take place about 400 mi (640 km) east of South America in the Atlantic Ocean, 500 mi (800 km) north of the equator.
Fortunately, greatest duration for the 2017 August eclipse does occur over the mainland USA. For awhile now this policy has changed at Ruger and the quality of the magazines being produced is phenomenal.

Totality is a two minute eclipse on the West Coast with the east coast having 34 seconds more. Thus, western location may again have an advantage since summer storms tend to build during afternoon hours, a common occurrence during summer months. The duration of totality decreases slowly at first with the distance from the central line of totality then increases rapidly. Although much less spectacular than total solar eclipses, central durations are often much longer.
This 30-round magazine is no exception with the fit, feel, and performance being what you would expect from the Ruger factory - perfection in all areas. The approximate range in altitude of the Sun in degrees during the eclipse is also shown for both west and east regions. For example, at a distance of 60% away from the central line to the edge of totality, the duration is still 80% of maximum. Even if the fractional distance from the central line is one half, the loss in duration is only about 15%. Hence, observers usually do not need to be exactly on the central line to experience most of the duration of totality.

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