Trilogy Productions, Inc. is a full-service Box Office Management and Ticket Company specializing in worry-free ticketing for any organization and superior service for the patron. | |
This web page is not intended to be a marketing tool for, or to "show case" Trilogy Productions products or services. It is used to test css, php, javascript and occasionally to demonstrate ideas to clients. If you come accross this page by chance you may however find it of some interest. | |
The images below are links to the web sites of two of the organizations that Trilogy Productions provides on-going box office management and ticketing services including on-line ticket sales. | |
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The San Francisco Film Society logo is an old version they no longer use. | |
REMOTE_ADDR, server time (uncorrected for drift) and HTTP_USER_AGENT38.107.191.89 Thu, 2 Sep 2010 10:20:15 pm CCBot/1.0 (+http://www.commoncrawl.org/bot.html) | |
Drag me! Close me! HELLO | |
Less we forget how we got here.Which of the first 4 screens below is the easiest to read? Of the 2nd, 3rd and 4th rows of screens below, which is easiest to read - which is easiest on the eyes? The green, amber or paper-white? | |
| Early green, but Arial: | Early green, but Georgia: |
On the shore, dimly seen through the mists of the deep, Where the foe's haughty host in dread silence reposes, What is that which the breeze, o'er the towering steep, As it fitfully blows, half conceals, half discloses? Now it catches the gleam of the morning's first beam, In full glory reflected now shines in the stream: 'Tis the star-spangled banner! Oh long may it wave O'er the land of the free and the home of the brave! | On the shore, dimly seen through the mists of the deep, Where the foe's haughty host in dread silence reposes, What is that which the breeze, o'er the towering steep, As it fitfully blows, half conceals, half discloses? Now it catches the gleam of the morning's first beam, In full glory reflected now shines in the stream: 'Tis the star-spangled banner! Oh long may it wave O'er the land of the free and the home of the brave! |
| Early green, New Courier (close to WYSE terminals): | Early green, but Verdana: |
On the shore, dimly seen through the mists of the deep, Where the foe's haughty host in dread silence reposes, What is that which the breeze, o'er the towering steep, As it fitfully blows, half conceals, half discloses? Now it catches the gleam of the morning's first beam, In full glory reflected now shines in the stream: 'Tis the star-spangled banner! Oh long may it wave O'er the land of the free and the home of the brave! | On the shore, dimly seen through the mists of the deep, Where the foe's haughty host in dread silence reposes, What is that which the breeze, o'er the towering steep, As it fitfully blows, half conceals, half discloses? Now it catches the gleam of the morning's first beam, In full glory reflected now shines in the stream: 'Tis the star-spangled banner! Oh long may it wave O'er the land of the free and the home of the brave! |
| Amber (German), New Courier (close to WYSE terminals): | Amber (German), but Verdana: |
On the shore, dimly seen through the mists of the deep, Where the foe's haughty host in dread silence reposes, What is that which the breeze, o'er the towering steep, As it fitfully blows, half conceals, half discloses? Now it catches the gleam of the morning's first beam, In full glory reflected now shines in the stream: 'Tis the star-spangled banner! Oh long may it wave O'er the land of the free and the home of the brave! | On the shore, dimly seen through the mists of the deep, Where the foe's haughty host in dread silence reposes, What is that which the breeze, o'er the towering steep, As it fitfully blows, half conceals, half discloses? Now it catches the gleam of the morning's first beam, In full glory reflected now shines in the stream: 'Tis the star-spangled banner! Oh long may it wave O'er the land of the free and the home of the brave! |
| European Standard, paper-white/medium contrast, New Courier (close to WYSE terminals): | European Standard, paper-white/medium contrast, but Verdana: |
On the shore, dimly seen through the mists of the deep, Where the foe's haughty host in dread silence reposes, What is that which the breeze, o'er the towering steep, As it fitfully blows, half conceals, half discloses? Now it catches the gleam of the morning's first beam, In full glory reflected now shines in the stream: 'Tis the star-spangled banner! Oh long may it wave O'er the land of the free and the home of the brave! | On the shore, dimly seen through the mists of the deep, Where the foe's haughty host in dread silence reposes, What is that which the breeze, o'er the towering steep, As it fitfully blows, half conceals, half discloses? Now it catches the gleam of the morning's first beam, In full glory reflected now shines in the stream: 'Tis the star-spangled banner! Oh long may it wave O'er the land of the free and the home of the brave! |
Web colors:Which of the 6 rows of screens below is easiest to read - which is easiest on the eyes? | |
Astrophysics and the Pauli exclusion principle Astronomy provides spectacular demonstration of the Pauli exclusion principle, in the form of white dwarf stars and neutron stars. For both such bodies, their usual atomic structure is disrupted by large gravitational forces, leaving the constituents supported by "degeneracy pressure" alone. This exotic form of matter is known as degenerate matter. In white dwarfs, the atoms are held apart by the electron degeneracy pressure. In neutron stars, which exhibit even more intense gravitational forces, the electrons have merged with the protons to form neutrons. Neutrons are capable of producing an even higher degeneracy pressure albeit over a shorter range. This can stabilize neutron stars from further collapse but at a smaller size and higher density than a white dwarf. Neutrons are the most "rigid" objects known - their Young modulus (or more accurately, bulk modulus) is 20 orders of magnitude larger than that of diamond. Even this enormous rigidity can still be overcome by the gravitational field of a massive star or by the pressure of a supernova, leading to the formation of a black hole. | Astrophysics and the Pauli exclusion principle Astronomy provides spectacular demonstration of the Pauli exclusion principle, in the form of white dwarf stars and neutron stars. For both such bodies, their usual atomic structure is disrupted by large gravitational forces, leaving the constituents supported by "degeneracy pressure" alone. This exotic form of matter is known as degenerate matter. In white dwarfs, the atoms are held apart by the electron degeneracy pressure. In neutron stars, which exhibit even more intense gravitational forces, the electrons have merged with the protons to form neutrons. Neutrons are capable of producing an even higher degeneracy pressure albeit over a shorter range. This can stabilize neutron stars from further collapse but at a smaller size and higher density than a white dwarf. Neutrons are the most "rigid" objects known - their Young modulus (or more accurately, bulk modulus) is 20 orders of magnitude larger than that of diamond. Even this enormous rigidity can still be overcome by the gravitational field of a massive star or by the pressure of a supernova, leading to the formation of a black hole. |
Astrophysics and the Pauli exclusion principle Astronomy provides spectacular demonstration of the Pauli exclusion principle, in the form of white dwarf stars and neutron stars. For both such bodies, their usual atomic structure is disrupted by large gravitational forces, leaving the constituents supported by "degeneracy pressure" alone. This exotic form of matter is known as degenerate matter. In white dwarfs, the atoms are held apart by the electron degeneracy pressure. In neutron stars, which exhibit even more intense gravitational forces, the electrons have merged with the protons to form neutrons. Neutrons are capable of producing an even higher degeneracy pressure albeit over a shorter range. This can stabilize neutron stars from further collapse but at a smaller size and higher density than a white dwarf. Neutrons are the most "rigid" objects known - their Young modulus (or more accurately, bulk modulus) is 20 orders of magnitude larger than that of diamond. Even this enormous rigidity can still be overcome by the gravitational field of a massive star or by the pressure of a supernova, leading to the formation of a black hole. | Astrophysics and the Pauli exclusion principle Astronomy provides spectacular demonstration of the Pauli exclusion principle, in the form of white dwarf stars and neutron stars. For both such bodies, their usual atomic structure is disrupted by large gravitational forces, leaving the constituents supported by "degeneracy pressure" alone. This exotic form of matter is known as degenerate matter. In white dwarfs, the atoms are held apart by the electron degeneracy pressure. In neutron stars, which exhibit even more intense gravitational forces, the electrons have merged with the protons to form neutrons. Neutrons are capable of producing an even higher degeneracy pressure albeit over a shorter range. This can stabilize neutron stars from further collapse but at a smaller size and higher density than a white dwarf. Neutrons are the most "rigid" objects known - their Young modulus (or more accurately, bulk modulus) is 20 orders of magnitude larger than that of diamond. Even this enormous rigidity can still be overcome by the gravitational field of a massive star or by the pressure of a supernova, leading to the formation of a black hole. |
Astrophysics and the Pauli exclusion principle Astronomy provides spectacular demonstration of the Pauli exclusion principle, in the form of white dwarf stars and neutron stars. For both such bodies, their usual atomic structure is disrupted by large gravitational forces, leaving the constituents supported by "degeneracy pressure" alone. This exotic form of matter is known as degenerate matter. In white dwarfs, the atoms are held apart by the electron degeneracy pressure. In neutron stars, which exhibit even more intense gravitational forces, the electrons have merged with the protons to form neutrons. Neutrons are capable of producing an even higher degeneracy pressure albeit over a shorter range. This can stabilize neutron stars from further collapse but at a smaller size and higher density than a white dwarf. Neutrons are the most "rigid" objects known - their Young modulus (or more accurately, bulk modulus) is 20 orders of magnitude larger than that of diamond. Even this enormous rigidity can still be overcome by the gravitational field of a massive star or by the pressure of a supernova, leading to the formation of a black hole. | Astrophysics and the Pauli exclusion principle Astronomy provides spectacular demonstration of the Pauli exclusion principle, in the form of white dwarf stars and neutron stars. For both such bodies, their usual atomic structure is disrupted by large gravitational forces, leaving the constituents supported by "degeneracy pressure" alone. This exotic form of matter is known as degenerate matter. In white dwarfs, the atoms are held apart by the electron degeneracy pressure. In neutron stars, which exhibit even more intense gravitational forces, the electrons have merged with the protons to form neutrons. Neutrons are capable of producing an even higher degeneracy pressure albeit over a shorter range. This can stabilize neutron stars from further collapse but at a smaller size and higher density than a white dwarf. Neutrons are the most "rigid" objects known - their Young modulus (or more accurately, bulk modulus) is 20 orders of magnitude larger than that of diamond. Even this enormous rigidity can still be overcome by the gravitational field of a massive star or by the pressure of a supernova, leading to the formation of a black hole. |
Which of the following have degenerate matter: white dwarf star, neutron star, black hole? The probability of a correct answer is partially dependent on which of the screens above you read. | |
Commonly used navigation links.For enlightenment, follow the two links below. | |
 The philosophical vein of various kinds of skepticism contains many kinds of doubt and rejection of the various bases upon which logic rests, such as the idea of logical form, correct inference, or meaning, typically leading to the conclusion that there are no logical truths. Observe that this is opposite to the usual views in philosophical skepticism, where logic directs skeptical enquiry to doubt received wisdoms, as in the work of Sextus Empiricus. Friedrich Nietzsche provides a strong example of the rejection of the usual basis of logic: his radical rejection of idealisation led him to reject truth as a "mobile army of metaphors, metonyms, and anthropomorphisms-in short ... metaphors which are worn out and without sensuous power: coins which have lost their pictures and now matter only as metal, no longer as coins". His rejection of truth did not lead him to reject the idea of either inference or logic completely, but rather suggested that "logic [came] into existence in man's head [out] of illogic, whose realm originally must have been immense. Innumerable beings who made inferences in a way different from ours perished". Thus there is the idea that logical inference has a use as a tool for human survival, but that its existence does not support the existence of truth, nor does it have a reality beyond the instrumental: "Logic, too, also rests on assumptions that do not correspond to anything in the real world". | |
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The Critical Path:Critical path analysis or critical path method (CPM), is a valuable scheduling tool used in project management. It's very simple conceptually and in application. | |