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What Is a Water Fuel System?

Monday, October 19th, 2009 by www

The entire earth is now effectively being driven by a fossil fuel based economy. The primary Energy supply in the world has been derived mostly from Fossil Fuel and Coal for very many years. Business and trade were much different when all of this started out. On top of that, the technologies that exist at present definately did not exist 100 years ago when the foundation for a fossil fuel based economy was in its early development.

This fossil fuel based economy has evolved into the size that it currently directly or indirectly affects the majority of all business that occurs in the world nowadays. Our reliance on these essential but limited resources has led to dangerous problems, which far go beyond the mere economics of it. Big Oil is a enormously gigantic force with a load of power behind it, but it is not the only power at play.

Nowadays Things Are Changing

Everybody understands that the future of life on our Planet is plainly exposed to exceedingly high risk. In light of acute global consciousness with regard to the state of the ecosystem, it comes as no shock that there has been a considerable effort to turn away from reliance on Fossil Fuels and Coal as the sole sources of our Energy requirements. As a consequence of this, developments in the fields of alternative fuel sources and hybrid vehicles have now unquestionably come of age, despite the dominance of Big Oil. The complex technologies that we now have available are altering the path of our future for the better.

Although there is still global reliance on fossil fuel, and Big Oil is here to provide, let us not disregard that these large companies can, and are, also assisting with the swing towards going green by participating in energy research and development centered around Green alternatives.

What Is a Water Fuel System?

The water fuel system is a highly efficient electro-mechanized system, capable of producing hydrogen and oxygen in sufficient quantity to upgrade the fuel efficiency of internal combustion engines. It is really a conversion system because it does not require removal, modification, or disabling of your cars existing fuel system. This allows you to run your vehicle on either the regular gasoline system or on the water fuel system, where you can simply toggle between either power sources as desired.

How Well Does The System work And What Are The Advantages?

You will not only save gas, you will also increase the life of your vehicle! Water runs clean, and that helps your engine. It essentially cleans your engine while you drive. Your pistons, valves, rings and bearings in particular will all last longer, and that can save you hundreds or thousands of dollars over the life of your car.

A car run by a water fuel cell is theoretically able of traveling from 50 to 300 miles on each gallon of supplemental water, while improving overall fuel efficiency up to 50%. However, as true with any engine, overall results vary depending on factors such as; driving habits, terrain, vehicle weight and shape, and ability to optimize the system.

If you have always wanted to help with the environment and felt guilty at the same time since you have to drive to work to support your household, stop! You do not need to feel guilty anymore.
You can save yourself insane money and help keep the air clean while you drive your current car!

The Water fuel system is quite simple to build and quite simple to install, partiularly compared with other conversion plans on the market. You can save huge money on gasoline, improve your vehicles mileage by making a water fuel cell yourself, and you will be Saving the Planet in the process. Download our Free Report on how to do it here http://www.Earthfriendly-fuel.Com/. The Run Car on Water guide will show you how to do it, step by step.

Portable Drinking Water for Recreation and Disasters

Saturday, September 12th, 2009 by www

You’ve possibly attended public functions where you wished there was free drinking water available. Even if there are sellers selling many different sorts of drinks, there are occasions when all you would like is a good, old-fashioned drinking fountain. Events might be faculty sports occassions, community holidays, family reunions, or any other public occasion where plenty of people come together. Most public event venues don’t have free drinking water available, but even if you are having a superb time, you are finally going to get parched. Wouldit be cool to have a mobile source of cold, clean water available to come to your next group function? There are mobile drinking water trailers available for lease that may do the trick for you.

Companies who operate mobile drinking water trailers travel round the country to various events. These units mix both drinking fountains and faucets where event attendees can fill water bottles. If you are sponsoring an event where you would like to give everyone an opportunity at a cold drink of water, then you can search online for varied firms who lease drinking water trailers.

Now let us take a look at a completely different scenario and consider an emergencysituation which shut down water treatment facilities. In cases like this, folks are unable to get the water they need to survive. That’s’s when another kind of mobile water purification system, a sanitization unit, helps bring clean drinking water to the people. These trailers contain water filtration units capable of decontaminating and disinfecting gallons of safe drinking water using diverse chemical and filtration techniques. Since the whole unit is compact and easily-transportable, it is OK for use in remote areas where larger lorries and sanitation equipment couldn’t access.

Today’s technology is absolutely amazing. It appears to come up with a solution for each problem. Fresh drinking water is important to human life as can be shown in third-world nations where tarnished water sources cause sickness and deaths. FEMA has recognized the important role mobile drinking water trailers can play in maintaining public health in disaster areas, and units have been shipped all over the world. The water treated with these mobile facilities meets government standards for drinking water. It’s hard to think how many lives have been saved due to this modern technology.

Need more information on portable water filtration? If you’re looking for water filtration companies you can trust to deliver quality service and equipment, visit SeparmaticSystems.com for all your water purification needs including diatomaceous earth filters and portable water purification systems.

Guide to Miami museum of science

Thursday, September 10th, 2009 by www

The Miami museum of science educates the visitors about the physical and natural sciences, astrology, technology and the state’s unique ecology and offers both permanent and traveling exhibitions Whether you have young children or are a kid at heart yourself, there is a little of something for everyone.Plan your trip to the Miami Childrens Museum in advance as there is a lot to see and to do at the museum.

If you are planning to go to the Miami Museum of Science as a large group, you might want to consider making an event of your group, hence making it one of the most flexible places to visit. The museum hosts special events for groups between ten and one thousand.

If you don’t want to join a large event or host a birthday party event, going to the museum is a great way to just relax. The Miami Museum of Science is open seven days a week with the exceptions of Thanksgiving and Christmas Day. Before you go to the Miami Museum of Science, dont forget to check the museum’s calender for special events and exhibits.The museum sponsors many different traveling exhibitions, including those created by prestigious museums like the Smithsonian National Museum of Natural History. However, these exhibitions change fairly frequently, so it is important that you plan your visit on a day where the exhibition you wish to see is running.

The Miami science museum also has shows and demonstrations planned for certain parts of each day. When you go to the museum, you will want to check what times events are running and make sure you are at the right place at the right time to see the demonstrations or shows that you are interested in.

If you have gone to the Miami Museum of Science and enjoyed your visit, you may want to consider supporting the museum. The Miami Science Museum has been nurtured by a legion of tireless volunteers and generous contributors. As the cost of acquiring new exhibits is quite high, ever little bit helps. If you do not have a lot of money, but live near the Miami Museum of Science, you may want to consider donating your time. Volunteers help support the museum in many ways including tours. If you plan on volunteering, most museums require a certain amount of time committed to help cover the investment of training the volunteers.

Miami museum of science offers children and adults alike an entertaining, educational experience. It’s a great place to visit, whether you’re on vacation, a school field trip or a weekend family outing.

Peter S. Museer

Basic Information On Fuel Cells

Friday, July 31st, 2009 by www

Fuel cells are electrochemical devices that combine hydrogen and oxygen in order to produce electricity.

During the power generation cycle, water and heat are produced as a by-products. This is a far more ideal byproduct than the unclean emissions which are created by other methods of generating electricity.

They will operate and generate power so long as fuel is supplied. Since the conversion of the fuel to energy takes place via an electrochemical process, and not by combustion, the process is clean, quiet, and highly efficient - two to three times more efficient than ordinary combustion, such as that done by gasoline in a generator.

Fuel cell technology is unique as a power technology - no other energy generation technology offers the combination of benefits that these devices do. While they produce extremely low (or zero) emissions (depending on the type used), other benefits include:

• Multi-fuel capability
• High efficiency and reliability
• Scalability
• Durability
• Ease of maintenance

Since they generate power through a chemical process, they operate silently. Thus, they reduce noise pollution, as well as air pollution. Heat generated by the cells, in the process of generating electricity can be captured and used to provide hot water or space heating for a home or office, in larger applications.

Another key aspect of this technology is that the cells can be scaled to any size required, without difficulty. Small cells can be produced which will power mobile phones for up to thirty days, or operate laptops for twenty hours or more. Larger versions can be produced to operate as power plants, in order to provide electricity for small cities. And of course, there are many sizes in between.

The most notable use of fuel cells currently being developed is as a replacement for the combustion engine. It is very likely that cars and other vehicles will be powered by fuel cells in the not too distant future.

In light of the above, the U.S. Department of Energy (COE) is running a program in order to research and develop this technology further. The DOE considers this to be an important enabling technology for the hydrogen economy. It states that they have the potential to revolutionize the way we power our nation, by offering cleaner and more highly efficient alternatives to the combustion of gasoline and other hazardous fossil fuels.

The DOE also considers that these devices have the potential to replace internal-combustion engines in vehicles, and to provide power in stationary and portable power applications because they are energy-efficient, clean, and fuel-flexible.

Currently the DOE is working closely with its national laboratories, universities, and industry partners across the United States, in order to overcome critical technical barriers to the commercialization of fuel cell technology. It is currently focused on the development of reliable, low-cost, high-performance fuel cell system components, for transportation and buildings applications.

The first fuel-cell operated cars are currently being piloted. The first commercially available cars of this make are predicted to reach the consumer market by the year 2012.

There are many forms of alternative energy being researched, developed, and utilized around the world. There is solar power, wind power, hydro-kinetic power, biomass, ocean wave power, tidal power, and the list goes on and on. A key factor in reducing our uses of polluting fossil fuels will be to determine which alternative energy resources work best under which circumstances and in which locations. A full understanding of all clean alternative energy sources is necessary.

Fuels cells play a big role in helping clean up our environment.

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Anna Williams educates others on alternative, renewable, and clean energy forms, on her blog, Alternative and Renewable Energy.

For further information on the different uses of fuel cells, please visit How Fuel Cells can be Used.

Source Article: Fuel Cells - Basic Information

Make Telescopes Of Your Own!

Wednesday, July 29th, 2009 by www

An investigation into early telescopes makes for interesting reading. In 1722, John Hadley, an English mathematician, completed a form of reflector for the telescope in the style of Newton in which the mirror evidently was suitably figured. This instrument attracted considerable attention, and presently other makers were turning out Newtonian reflectors, following Hadley’s technique, which consisted of removing the spherical aberration as it was revealed by the extra-focal diffraction rings of a star image.

Hadley then turned his attention to a design by James Gregory and in 1726 he began to make a telescope slightly over 2″ in diameter and 12″ in focal length. Observatories purchased his larger instruments, a tribute to his skill, and the smaller ones were marketed chiefly among the aristocracy and amateur astronomers.

The principal attraction to make telescope%s according to the Gregorian design was the erect image it gave, which made it suitable for terrestrial use. This circumstance influenced its preference over the Newtonian, notwithstanding the fact that its images must have been pretty dull. Well into the 19th century, however, the Gregorian rode a wave of popularity that no type of telescope has known, until overwhelmed in comparatively recent years by the flood of amateurs who have flocked to Newton’s design.

From the time of the invention of the telescope, and the startling discoveries of Jupiter’s moons and the rings of Saturn, interest in astronomy had become something infectious. Many began to make telescopes or become interested in astronomy as a hobby. Each new discovery was accorded the widest publicity, stimulating a desire among those of learning to gain at first hand a glimpse of these celestial wonders. Those whose means permitted bought telescopes, and envied was the gentleman who possessed one of three or four inches aperture, by an “exclusive” artist. But, judged by present-day standards, many of those reflectors were tiny. There is one (maker unknown) in the Fugger Collection at Augsburg, barely 1″ in diameter and 6″ in focal length, that was concealed in a walking stick! Eyepiece lenses of 1/6″ or less in focal length were quite common.

To facilitate the work, the comparatively thin disks were cast to the approximate curve, the backs also being curved to give uniform thickness and equalization of temperature effects. Grinding was done on convex iron tools of similar radius, using emery, and sometimes sand. Polishing was done on a pitch lap, with rouge.

Manufacturers usually devised their own machines to do the work of grinding and polishing. Except where the utmost perfection was imperative, figuring seems to have consisted for the most part of a final brief variation of the stroke, in an unguided attempt to concentrate the polishing at the center. In reflective ability, speculum was only about 60 per cent efficient, and the surface tarnished rapidly, effecting a further serious light loss. This meant frequent repolishing, and repolishing meant refiguring.

It is interesting to inquire into the prices that were asked for telescopes in that period, the latter half of the 18th century. The early telescopes were certainly gaining popularity by this time and amateur telescope making was beginning to take off.

See the Stars! Make Telescopes

Tuesday, July 28th, 2009 by www

For those who decide to make telescope%s it is a fascinating hobby. Telescopes are usually designed to perform particular kinds of work. In general, for visual work, low-ratio telescopes with their wide fields are useful for comet seeking, variable star work, and the like. The higher ratios are used in planetary study, double star observations, and in other fields where high powers and fine definition are required. Anyone can make telescopes though, don’t be scared off by technical terms.

From the experience gained by those involved in amateur telescope making, it has been found that the most practical and popular instrument for amateur use is the 6-inch f/8 Newtonian reflector. Its concave mirror is 6″ in diameter and its focal length 48″. The delicate task of parabolizing the mirror, while not easy, is not beyond the ability of a careful worker. The 4-foot focal length makes for comfortable observing, and with a low-power eyepiece, the field of view is a trifle over one degree in diameter - more than twice that of the full moon. When you make telescopes the benefits are extremely rewarding.

The magnifications that may be employed permit of a modest size of mounting, which can be made portable. Such a telescope should reveal stars of magnitude 12.8, as compared with the 6th-magnitude limit of the unaided eye, and the 9th-magnitude limit of the average small binocular.

This telescope will show the divisions in Saturn’s rings; surface markings on the moon little more than a mile across should also be visible. Amazing what suddenly opens for you when you decide to make telescopes!

The purchase price of such an instrument of professional make is necessarily high, and many an amateur feels compelled to do without it. Of course, many engaged in amateur telescope making feel that their mirrors are inferior to the professionals’, but this is not necessarily true. It has been frequently demonstrated that mirrors of professional make will seldom stand up to a test, because it is impossible for the professional optician to spend sufficient time on the mirror without losing money, whereas the amateur can, if he will, devote all the time and care necessary to produce a mirror of admirable figure.

Upkeep is slight for those who chose to make telescopes at home. The reflective aluminum coating of the mirrors of a reflector is subject to deterioration from dust and the elements admitted by the open tube, but given the same protection when not in use that is accorded a refractor, at least two years of service should be realized before the aluminizing job need be repeated.

For those involved in amateur telescope making, the task is time consuming but extremely rewarding. Good luck! Go for it- make a telescope!

Make Telescopes: The Perfect Machine

Tuesday, July 28th, 2009 by www

The development of building a telescope was greatly aided by the construction of the achromatic lens.In 1733, the achromatic lens was invented by Chester Moore Hall, an English barrister. This helped to give better instructions to those intending to make a telescope.

Dollond’s efforts led to a demand for clearer glasses of more varied densities and of less equal dispersions, needed to improve achromatism, and chemists pursued experiments in learning how to control the refractive indices of melts, and in the pouring of large disks of limpid, homogeneous glass.

Dollond began make telescopes of the refractory variety (spyglasses) with single-lens objectives as early as 1742, his price for a 2-foot telescope then being 7s 6d. In comparison, in 1762 he sold a 2-foot telescope with a two-lens objective (achromat) for 2 guineas. The lens diameters in each case were just under 2″.

In 1783, with a view to combining the benefits of the wide field of Huygens’ eyepiece with a means of making micrometric measurements of an image in the focal plane, Jesse Ramsden, an English optician, designed the compound eyepiece. building a telescope was becoming more like the process undertaken today. It can be seen that a measuring device, such as adjustable parallel wires, set in the focal plane would be magnified along with the image. With the advent of the achromatic lens, the erecting or terrestrial eyepiece assumed considerable importance. In the early part of the 19th century, small achromatic refractors were being manufactured by several concerns. For those not having the means to buy achromats, telescopes with single-lens objectives continued to be made. Enterprising opticians were also offering lens sets that could be assembled into simple refractors.

The method of chemically depositing silver on glass discovered about 1840 by Justus von Liebig, of Nuremberg, was successfully applied to a small glass telescope mirror in 1856 by Karl Steinheil, a German physicist, and independently in the following year by Jean Foucault, the famous French physicist.

Various processes of plating glass with metal for the making of mirrors had been known and practiced for centuries, but for one reason or another, the coatings were unsuited for front-surface reflection.

Then, in 1858, Foucault announced the development of his amazingly delicate and simple test for a concave reflecting surface, using an illuminated pinhole and a straightedge placed in the vicinity of the center of curvature of the mirror. The pinhole and straightedge were the outgrowth of earlier experiments in which simultaneous microscopic comparison was made of a pin point, likewise placed at the center of curvature of a mirror, and its reflected image, which was caused to fall alongside.

Silver-on-glass mirrors replaced the more expensive and difficult-to-work speculum.

After this point in history a telescope was becoming closer to being constructed in the style we know it today. You can also make telescopes at home that is similar is style and functionality to the telescoped made by histories great astronomers.

Make Telescopes: Understand Amateur Telescopes

Thursday, July 23rd, 2009 by www

In the past there has been considerable discussion by those inclined to make telescopes on the relative merits of reflector and refractor. From the standpoint of professional astronomers, there is no serious competition between them, as each type supplements the other in a well-rounded observing program. An amateur who plans to make a telescope and to use them for general observing has other factors to take into consideration. Let us first look at some of the optical characteristics of reflectors and refractors.

Very early in the 19th century, when advocates of the speculum mirror began to feel the challenge of the refractor, Dr. Nevil Maskelyne, English Astronomer Royal, ventured the opinion “that the aperture of a common reflecting telescope, in order to show objects as bright as the achromat, must be to that of an achromatic telescope as 8 to 5.”

The relative inefficiency of the reflector of that day was due to the fact that, even under most favorable circumstances, barely 40 per cent of the original light escaped absorption by the metal mirrors, the greatest losses occurring in the short and medium wave lengths. Even silver-on-glass mirrors are subject to considerable deterioration, especially under certain conditions of the atmosphere.

The reflectivity of aluminum, however, is more-or-less constant, and from a standpoint of image brightness, it placed the reflector on a more equal footing with the refractor. In fact, until the quite recent development of anti-reflection lens coatings, an aluminized mirror has had the same efficiency, in light-transmitting qualities, as an air-spaced achromatic objective lens of equal aperture.

Coming down to figures - due to reflection there occurs in an untreated lens a light loss of slightly more than four per cent at each of its surfaces.

With reflection losses to be accounted for, plus an absorption loss in the substance of the glass (amounting to about two per cent for lenses of moderate size), it is evident that about 82 per cent of the original light is transmitted. In the reflector, after first deducting that area of the mirror’s surface obscured by the diagonal, an equal percentage of the original light is found to be transmitted.

Of course, this transmitted light is subject to another reflection by the diagonal, but the refractor will probably employ a star diagonal, the function of which is similar to that of the diagonal or prism of the Newtonian, so an equivalent loss may occur there. Therefore, for those engaged in amateur telescope making, with either instrument, the same amount of light reaches the eyepiece.

It was discovered, however, in the latter part of the last century by those who make telescopes, that some lenses which had been tarnished by the elements transmitted more light than ones that were newly polished; it was found that this resulted from lessened reflections at the tarnished surfaces. Various processes of producing an artificial tarnish were attempted. At present, in the most satisfactory method, metallic salts (such as magnesium fluoride) are evaporated in a high vacuum onto the glass. Ideally, the refractive index of an anti-reflection fluoride coating should vary from that of glass at the glass-fluoride surface to that of air at the fluoride-air surface, in which case no reflection would occur.

Practically, the index of the coating should be equal to the square root of the index of the glass, and its thickness equal to a quarter of a wave length of yellow-green light. Only the light at opposite ends of the visible spectrum is then reflected, amounting in general to less than one per cent of that of the whole, and is detected by the purplish color given to the reflection.
From the standpoint of an introduction to the optician’s trade, the experience of thousands of amateurs has shown that one’s teeth should first be cut on at least one good mirror. Then, if a refractor is contemplated, additional experience can be gained by making the optical flat that is so essential in the testing and figuring of the objective lens.

For beginners it would seem that the first step to make telescopes is to make a reflector.

Make Telescopes: Make Them, Use Them

Thursday, July 23rd, 2009 by www

The history of the telescope makes for interesting reading from a theoretical perspective, but also from the perspective of someone interested in beginning to make a telescope. During the development of the telescope, practical experiments with reflectors had already begun in 1639, but it was not until 1663 that they gained any prominence.

The Gregorian Telescope

High magnification could be had with this instrument, the second reflection amplifying the focal length of the primary in the ratio of fs to Fs.

He began to make telescopes, but whatever chance it may have had of performing creditably was lost by polishing the speculum on a cloth lap - putty (tin oxide) being used as the polishing agent. The Cassegrainian Telescope Sieur Cassegrain, a Frenchman, in 1672 designed a second compound reflector, differing from Gregory’s in that it employed a convex secondary, to be of hyperboloidal figure, placed inside of the focus of the paraboloidal primary .

The Newtonian Telescope

The history of the telescope takes an interesting turn at this point. In the same year, Newton designed and began to make telescopes that had two small reflectors, of the type so popular with amateur astronomers today and which still bears his name. They were not large, as we know telescopes today, the effective apertures of the concave specula being about 1 1/3″. Their focal length was 6″, making the focal ratio f/4.5.6

Newton, according to his Opticks (1704), polished his specula on pitch, using putty as the polishing agent. It might be concluded that if the center of the mirror were properly deepened, that is, given a shorter radius, or if the radii of the outer zones were progressively lengthened, or if a little of each were done, all the reflected rays could be brought to a common focus. The standard practice is to deepen the spherical mirror so that, for a 6-inch f/8 mirror, the glass removed in the operation is but half a wave length of light in thickness at the center. The field lens, like Galileo’s concave lens, is placed before the focal plane of the objective.

Ever since Galileo took a Dutch invention and adapted it to astronomical use, astronomical telescope making has been an evolving discipline. Many astronomers after the time of Galileo built their own telescopes out of necessity, but the advent of amateurs in the field building telescopes for their own enjoyment and education seems to have come into prominence in the 20th century.

Today telescopes of the size and technicality used by NASA experts are out of an amateurs grasp (and price range), but an amateur can easily begin to make telescopes of the kinds mentioned above both inexpensively and easily.

How Globe For Energy Can Economize You Thousands on Your Power Bill - Earth 4 Energy Bonus

Tuesday, May 19th, 2009 by www

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