Wednesday, March 30, 2011

Marriage Gift Request Letter

solutions to the UIB

jb
have changed the website of the UIB, and access to reviews PAU of the previous years is now:

http://estudis.uib.es/grau/acces/batxiller/Info_materies/


are also the dates of the tests:
7, 8, and 9 June ,
13, 14 and 15 September.

I hope you might help.

jb

Marriage Gift Request Letter

solutions to the UIB

jb
have changed the website of the UIB, and access to reviews PAU of the previous years is now:

http://estudis.uib.es/grau/acces/batxiller/Info_materies/


are also the dates of the tests:
7, 8, and 9 June ,
13, 14 and 15 September.

I hope you might help.

jb

Tuesday, March 29, 2011

Breastfeed Husband At 39 Weeks

nuclear chain reaction

And here again, after a small burden of examination of electromagnetism, several practices and stuff. Today we will see a small demonstration of what a nuclear chain reaction.

As we know, a heavy, unstable atom can fission spontaneously breaking into several pieces, some of these neutrons, which can help other atoms to fission, which releases more neutrons, more atoms to fission .. . The process releases large amounts of energy, which is what we use in our nuclear power plants to produce electricity. Of course, This energy production is controlled so as not to release such amount in such a short space of time can be dangerous.

But what happens if this reaction is controlled. It is customary that if there is a sufficient amount of fissile material, heavily exploited. If there is enough material to explode, the heat released by the reaction is so large that it can melt almost anything it touches.

This level of "what you see from the outside" but sometimes it's a bit difficult to get an idea of \u200b\u200bwhat happens at the atomic level. Okay, we know that an atom fissions and blablabla ... How fast? This is what we will see in the next video.



information: Physical principles of nuclear fission by Migui

Breastfeed Husband At 39 Weeks

nuclear chain reaction

And here again, after a small burden of examination of electromagnetism, several practices and stuff. Today we will see a small demonstration of what a nuclear chain reaction.

As we know, a heavy, unstable atom can fission spontaneously breaking into several pieces, some of these neutrons, which can help other atoms to fission, which releases more neutrons, more atoms to fission .. . The process releases large amounts of energy, which is what we use in our nuclear power plants to produce electricity. Of course, This energy production is controlled so as not to release such amount in such a short space of time can be dangerous.

But what happens if this reaction is controlled. It is customary that if there is a sufficient amount of fissile material, heavily exploited. If there is enough material to explode, the heat released by the reaction is so large that it can melt almost anything it touches.

This level of "what you see from the outside" but sometimes it's a bit difficult to get an idea of \u200b\u200bwhat happens at the atomic level. Okay, we know that an atom fissions and blablabla ... How fast? This is what we will see in the next video.



information: Physical principles of nuclear fission by Migui

Where Can I Buy Goldwell Hair Colour

Item 11: Representation of functions

jb
This topic should be reviewed many concepts from previous years:
is appropriate repaséis the issue of functions or limits of 1 Bachelor

conceptual map of the Unit:



For exercises representation of functions, you can go to that reported in previous years:

¤ Item 11 Representation of functions ¤
Estate, symmetries and periodicity
¤ ¤
Branches infinite singular points
¤ Representation of functions ( I) ¤
Representation of functions (II)
¤ Representation of functions (III)
¤ Representation of functions (IV) ¤
Solutions
item 11
You also have the solutions to exercises.

In Math 2 º Bachillerato you have more resources on this topic. Jb

Where Can I Buy Goldwell Hair Colour

Item 11: Representation of functions

jb
This topic should be reviewed many concepts from previous years:
is appropriate repaséis the issue of functions or limits of 1 Bachelor

conceptual map of the Unit:



For exercises representation of functions, you can go to that reported in previous years:

¤ Item 11 Representation of functions ¤
Estate, symmetries and periodicity
¤ ¤
Branches infinite singular points
¤ Representation of functions ( I) ¤
Representation of functions (II)
¤ Representation of functions (III)
¤ Representation of functions (IV) ¤
Solutions
item 11
You also have the solutions to exercises.

In Math 2 º Bachillerato you have more resources on this topic. Jb

How To Build A Motorcycle Dune



jb
Here solved some problems of the book:

1) The hands of a clock measuring 4 cm and 6 cm, and connecting its ends forms a triangle .
Determines the time between the 12 h and 12 h 30 min in the triangle area is maximum.



2) In a circle of radius r draw the tangent at any point C and a chord AB parallel to this tangent.
obtain thus a triangle ABC whose area we want to be maximized. Shows that for this reason, the distance from C to the rope should be 3 / 2 of the radio.



3) In a semicircle of diameter AB = 2r draw a line CD parallel to AB.
What should be the length of the string so that the area of \u200b\u200bthe trapezoid ABDC is maximum?



4) The figure of the previous problem, we call E the midpoint of the arc CD and draw the pentagon AceDB
a) Calculate rope length CD for the Pentagon area is maximized.
b) Calculate also the value of the maximum area pentagon



jb

How To Build A Motorcycle Dune



jb
Here solved some problems of the book:

1) The hands of a clock measuring 4 cm and 6 cm, and connecting its ends forms a triangle .
Determines the time between the 12 h and 12 h 30 min in the triangle area is maximum.



2) In a circle of radius r draw the tangent at any point C and a chord AB parallel to this tangent.
obtain thus a triangle ABC whose area we want to be maximized. Shows that for this reason, the distance from C to the rope should be 3 / 2 of the radio.



3) In a semicircle of diameter AB = 2r draw a line CD parallel to AB.
What should be the length of the string so that the area of \u200b\u200bthe trapezoid ABDC is maximum?



4) The figure of the previous problem, we call E the midpoint of the arc CD and draw the pentagon AceDB
a) Calculate rope length CD for the Pentagon area is maximized.
b) Calculate also the value of the maximum area pentagon



jb

Saturday, March 26, 2011

Black Hair Blue Eyes Are

A little help to the 3rd Middle


At the request of some spoiled than 3 ° between two guide file to study Powers Luck!



Notes for preparing a test power
resolved Guide powers

Black Hair Blue Eyes Are

A little help to the 3rd Middle


At the request of some spoiled than 3 ° between two guide file to study Powers Luck!



Notes for preparing a test power
resolved Guide powers

Thursday, March 17, 2011

What Does Cm Look Like After Your Period

Welcoming SCHOOL YEAR 2011

Dear children, returning to our school work, greeting wishing them well-deserved success in 2011, remember that academic success alone in their hands. There is no obstacle that can not be overcome with effort and perseverance.

What Does Cm Look Like After Your Period

Welcoming SCHOOL YEAR 2011

Dear children, returning to our school work, greeting wishing them well-deserved success in 2011, remember that academic success alone in their hands. There is no obstacle that can not be overcome with effort and perseverance.

Tuesday, March 15, 2011

Can U Dye An Ivory Dress White

Optimization Problems "L'Hospital L'Hôpital or?

jb
What is the correct spelling: L'Hôpital or L 'Hospital? The

Wikipedia have an explanation on why we wrote the name of two ways, and a summary of his relationship with Johan Bernoulli. Short and interesting it

.

Quoting a famous Aragonese:
"The good, if brief, twice as good, and even worse, if brief, not so bad. "
Baltasar Gracian (1601-1658).


jb

Can U Dye An Ivory Dress White

Optimization Problems "L'Hospital L'Hôpital or?

jb
What is the correct spelling: L'Hôpital or L 'Hospital? The

Wikipedia have an explanation on why we wrote the name of two ways, and a summary of his relationship with Johan Bernoulli. Short and interesting it

.

Quoting a famous Aragonese:
"The good, if brief, twice as good, and even worse, if brief, not so bad. "
Baltasar Gracian (1601-1658).


jb

Whipped Woman Scenes In Movies

Item 10: Applications of the derivative

jb
To start the issue: didactic



Programming Exercises Derive

Evaluation Criteria

A global look at the unit: concept map



For exercises on limits, you can go to the published years previous:

¤

Topic 10 Applications of the derivative.

¤ Applications of the derivative (II)

¤ Applications of the derivative (III) Optimization

¤ L'Hôpital rule -Bernoulli.

¤ Rolle theorem and the mean value.

¤ Applications (VI) Solutions and theoretical questions.

¤ Review items 9 and 10

Exercises functions, continuity and differentiability, the selectivity of the Illes Balears University (from 2001 to 2008)

Functions 1 Functions 2


Functions 3 Functions 4

's statements here reviews

open files with Internet Explorer (does not work with Mozilla) and if you get a warning:


must allow scripts to run (Allow content blocked ...) You also have the

solutions to the exercises in the book. In

Math 2 º Bachillerato you have more resources on this topic.

an interesting chapter in the history of mathematics:
"L'Hôpital Controversy - Bernoulli." Jb

Whipped Woman Scenes In Movies

Item 10: Applications of the derivative

jb
To start the issue: didactic



Programming Exercises Derive

Evaluation Criteria

A global look at the unit: concept map



For exercises on limits, you can go to the published years previous:

¤

Topic 10 Applications of the derivative.

¤ Applications of the derivative (II)

¤ Applications of the derivative (III) Optimization

¤ L'Hôpital rule -Bernoulli.

¤ Rolle theorem and the mean value.

¤ Applications (VI) Solutions and theoretical questions.

¤ Review items 9 and 10

Exercises functions, continuity and differentiability, the selectivity of the Illes Balears University (from 2001 to 2008)

Functions 1 Functions 2


Functions 3 Functions 4

's statements here reviews

open files with Internet Explorer (does not work with Mozilla) and if you get a warning:


must allow scripts to run (Allow content blocked ...) You also have the

solutions to the exercises in the book. In

Math 2 º Bachillerato you have more resources on this topic.

an interesting chapter in the history of mathematics:
"L'Hôpital Controversy - Bernoulli." Jb

Saturday, March 12, 2011

Testicles Checked By Female Doctors




Caturday
And again, this time with a special guest: a Ocelot, or lolcelot, as is known. The ocelot is the next pet after Narval Ubuntu, announced recently. To which we, poem catlike / cat / on the ocelot (^_^)


In the dim room where there is no light you can always find

some other quiet silent


few steps you can reveal the hidden corner

is protected


A lonely cat feline
an ocelot tranquil dream dreaming

future while the present
walks past
and last, that, has left behind


at least you hope so you understand now what am I nops (^_^) Happy Caturday.

Testicles Checked By Female Doctors




Caturday
And again, this time with a special guest: a Ocelot, or lolcelot, as is known. The ocelot is the next pet after Narval Ubuntu, announced recently. To which we, poem catlike / cat / on the ocelot (^_^)


In the dim room where there is no light you can always find

some other quiet silent


few steps you can reveal the hidden corner

is protected


A lonely cat feline
an ocelot tranquil dream dreaming

future while the present
walks past
and last, that, has left behind


at least you hope so you understand now what am I nops (^_^) Happy Caturday.

Thursday, March 10, 2011

Denise Milani Tight Scats

Light Dark Side Of The Universe

This morning, framed in discussions of the cycle Appointment With Science, Professor Gabriela Barenboim has given us a lecture entitled The Dark Side Of The Universe, from which I will try make a short summary so we can all enjoy it. So, without further delay.

Dark Side Of The Universe by Gabriela Barenboim

To begin, we started, where it usually starts (^_^) What we see when we look at the sky? We can see stars if you look hard enough, we can see that are grouped in a structure which we call galaxy, our galaxy, the Milky Way.

Beremboim Professor has now to comment on the life of Edwin Hubble, who considered the Father of Cosmology: not very good student law degree, later Professor, PhD in Physics and then finally, the discovery that there is one galaxy in the universe. In fact, he finds many galaxies, and even more: it measures your speed, and discover that the universe is expanding and also the speed of the galaxies are fit to call "Hubble's Law" in which the rate is proportional to the distance to the galaxy.


But these ideas of an expanding universe do not seem to be accepted as well by the scientific community, but the case is qeu if they were, and to understand, we need to discuss what led to the revolution of Relativity. En este momento, pasamos a comentar las Leyes de Maxwell y sus diferencias con las Transformaciones de Galileo, si la una era correcta, la otra no, y viceversa. En principio, se consideró que eran las Leyes de Maxwell las que necesitarían una corrección, hasta que llegó Einstein con la Teoría de la Relatividad y postuló que en realidad lo que estaba mal eran los 200 años de mecánica que se habían hecho hasta entonces. Pero ahora tenemos que demostrar que la Teoría de la Relatividad es correcta, para ello, podemos utilizar el resultado de que la propia luz sería desviada por el paso cercano a una gran masa. Para ello, necesitamos una gran masa: el Sol, y la luz de una estrella distante, y que pase al lado del sol, and that the sun does not bother the measures: we also need a total solar eclipse, of course, it was found that the relativity worked.

Now, we can apply the theory of relativity to the entire known universe, with two outcomes: Either the universe is expanding or shrinking. And as mentioned a little earlier, Hubble proved that the universe is expanding. This has interesting consequences, but first let's make a distinction between radiation and matter. We say that the first has a rate comparable to that of light, and the second much lower. Now, with our expanding universe model, we can see that radiation should be "diluted", which is known as redshifted making its wavelength is longer.

With these data, we try to predict what will happen to the universe in the future: will expand, and what happened in the past: it contracts. And besides, we can try to estimate the age of the universe: about 14 billion (14 billion) years.

At this point, we turn to discuss the composition (known at that time) of the universe. On the one hand we have fermions, with which we can build things that occupy space, and on the other bosons, with which we can collect things and no space. Both types of particles form what is called standard model of particle.

But ... How do I know it's all there is? It is known that there is more matter must interact gravitationally, so we can make a map of the gravitational field. To this end, calls can use gravitational lensing: mass concentrations at several galaxies, near which passes the light of a galaxy that is behind, and with which, by analyzing the images generated in the galaxy can deduce the mass distribution, concluding that there is a large amount of mass in stars and galaxies we see, but there is a uniform distribution of mass below of which we know nothing: dark matter. Do you really know nothing? No, already had obtained information about their existence when Vera Rubin, considered by Prof. Barenboim as the first lady of cosmology, studied about the speed of rotation of galaxies and discovering that there should be more mass than actually see.


But to measure this dark matter, we must separate from matter 'normal'. To do this, we can monitor the sky waiting for a collision between large clusters of galaxies, where dark matter comes from the opposite side without interacting with anything, and stuff 'normal' interacts each other, so that lags behind dark matter, so they are separated.

Using the Chandra telescope, found the event and confirmed the existence of dark matter. But ... Is there anything else?


Now our challenge is to weigh the universe, so we must measure the rate of expansion or deceleration of the universe. For this we need a standard distance, from which we may offer the Supernovae 1A standard candles in astrophysics at what distance can be estimated with precision. With all this, we reach the universe is expanding ... rapidly.

There must be something to neutralize the effect of gravity, a sort of negative gravity or repulsive force. To explain this we suggest the existence of something we call dark energy, which must have the following characteristics: still exists even when empty, is uniformly distributed in the universe, has a constant density, and is invisible. And by count, we find that at present, dark energy constitutes about 70% of the universe, dark matter 25% and 5% ordinary matter remaining.

Again, we try to make predictions about future and the past of the universe: in the past, the dark energy density was much lower, and in the future will be much higher.

Finally, we can summarize what is currently cosmology. So far, we have Einstein's general relativity, the Standard Model of Particles and an inventory of the components of the universe. We still have to link quantum mechanics with relativity, know what dark matter and know what dark energy. And here we can make watching the universe with probes like Planck and Fermi, and interrogating the universe with experiments like the LHC.

And, as recent details, Professor Barenboim tells us that "The Dark Side of the force is the interesting" We plant a picture of Darth Vader and says that of "May the force be with you" (^_^) I hope you enjoyed the summary If something needs to be clarified, either because they do not understand or because I have expressed avisáis wrong and corrects me when I can.

Denise Milani Tight Scats

Light Dark Side Of The Universe

This morning, framed in discussions of the cycle Appointment With Science, Professor Gabriela Barenboim has given us a lecture entitled The Dark Side Of The Universe, from which I will try make a short summary so we can all enjoy it. So, without further delay.

Dark Side Of The Universe by Gabriela Barenboim

To begin, we started, where it usually starts (^_^) What we see when we look at the sky? We can see stars if you look hard enough, we can see that are grouped in a structure which we call galaxy, our galaxy, the Milky Way.

Beremboim Professor has now to comment on the life of Edwin Hubble, who considered the Father of Cosmology: not very good student law degree, later Professor, PhD in Physics and then finally, the discovery that there is one galaxy in the universe. In fact, he finds many galaxies, and even more: it measures your speed, and discover that the universe is expanding and also the speed of the galaxies are fit to call "Hubble's Law" in which the rate is proportional to the distance to the galaxy.


But these ideas of an expanding universe do not seem to be accepted as well by the scientific community, but the case is qeu if they were, and to understand, we need to discuss what led to the revolution of Relativity. En este momento, pasamos a comentar las Leyes de Maxwell y sus diferencias con las Transformaciones de Galileo, si la una era correcta, la otra no, y viceversa. En principio, se consideró que eran las Leyes de Maxwell las que necesitarían una corrección, hasta que llegó Einstein con la Teoría de la Relatividad y postuló que en realidad lo que estaba mal eran los 200 años de mecánica que se habían hecho hasta entonces. Pero ahora tenemos que demostrar que la Teoría de la Relatividad es correcta, para ello, podemos utilizar el resultado de que la propia luz sería desviada por el paso cercano a una gran masa. Para ello, necesitamos una gran masa: el Sol, y la luz de una estrella distante, y que pase al lado del sol, and that the sun does not bother the measures: we also need a total solar eclipse, of course, it was found that the relativity worked.

Now, we can apply the theory of relativity to the entire known universe, with two outcomes: Either the universe is expanding or shrinking. And as mentioned a little earlier, Hubble proved that the universe is expanding. This has interesting consequences, but first let's make a distinction between radiation and matter. We say that the first has a rate comparable to that of light, and the second much lower. Now, with our expanding universe model, we can see that radiation should be "diluted", which is known as redshifted making its wavelength is longer.

With these data, we try to predict what will happen to the universe in the future: will expand, and what happened in the past: it contracts. And besides, we can try to estimate the age of the universe: about 14 billion (14 billion) years.

At this point, we turn to discuss the composition (known at that time) of the universe. On the one hand we have fermions, with which we can build things that occupy space, and on the other bosons, with which we can collect things and no space. Both types of particles form what is called standard model of particle.

But ... How do I know it's all there is? It is known that there is more matter must interact gravitationally, so we can make a map of the gravitational field. To this end, calls can use gravitational lensing: mass concentrations at several galaxies, near which passes the light of a galaxy that is behind, and with which, by analyzing the images generated in the galaxy can deduce the mass distribution, concluding that there is a large amount of mass in stars and galaxies we see, but there is a uniform distribution of mass below of which we know nothing: dark matter. Do you really know nothing? No, already had obtained information about their existence when Vera Rubin, considered by Prof. Barenboim as the first lady of cosmology, studied about the speed of rotation of galaxies and discovering that there should be more mass than actually see.


But to measure this dark matter, we must separate from matter 'normal'. To do this, we can monitor the sky waiting for a collision between large clusters of galaxies, where dark matter comes from the opposite side without interacting with anything, and stuff 'normal' interacts each other, so that lags behind dark matter, so they are separated.

Using the Chandra telescope, found the event and confirmed the existence of dark matter. But ... Is there anything else?


Now our challenge is to weigh the universe, so we must measure the rate of expansion or deceleration of the universe. For this we need a standard distance, from which we may offer the Supernovae 1A standard candles in astrophysics at what distance can be estimated with precision. With all this, we reach the universe is expanding ... rapidly.

There must be something to neutralize the effect of gravity, a sort of negative gravity or repulsive force. To explain this we suggest the existence of something we call dark energy, which must have the following characteristics: still exists even when empty, is uniformly distributed in the universe, has a constant density, and is invisible. And by count, we find that at present, dark energy constitutes about 70% of the universe, dark matter 25% and 5% ordinary matter remaining.

Again, we try to make predictions about future and the past of the universe: in the past, the dark energy density was much lower, and in the future will be much higher.

Finally, we can summarize what is currently cosmology. So far, we have Einstein's general relativity, the Standard Model of Particles and an inventory of the components of the universe. We still have to link quantum mechanics with relativity, know what dark matter and know what dark energy. And here we can make watching the universe with probes like Planck and Fermi, and interrogating the universe with experiments like the LHC.

And, as recent details, Professor Barenboim tells us that "The Dark Side of the force is the interesting" We plant a picture of Darth Vader and says that of "May the force be with you" (^_^) I hope you enjoyed the summary If something needs to be clarified, either because they do not understand or because I have expressed avisáis wrong and corrects me when I can.

Tuesday, March 8, 2011

Custom Made Dashboards

How behaves Fire In Zero Gravity?

all know how fire behaves in space: It does not. All those action movies are wrong. The fire needs oxygen, and oxygen is not abundant outside the earth's atmosphere. Fire can occur within a closed environment and oxygenated in space, but do not behave the same way as they do on Earth. The Earth's gravity imposes many conditions on the fire, which do not exist in microgravity or zero-g. For this is why astronauts can not light a candle at both ends. [Pun on the real meaning of burn a candle at Both ENDS, and meaning as much cliché working late nights]


Gravity is a compendium of good and bad. Yes, it helps maintain muscle tone and bone density, and allows us to eat the soup in a bowl without causing a mess. Unfortunately, it also tries to kill us, making us stumble and pulling heavy objects on us. Apparently not content with beating with hard objects, gravity also trying to kill us by the fire. When a fire starts, warms the surrounding air. This causes that particular section of air becomes less dense. This section less dense air is directed upwards because gravity is pulling everything, and sections of cold, dense air displaces up on their way to a position closer to the ground. The fire is in luck, because the only reason for the hot air is because the fire was consuming oxygen. When the thin air is pushed upward by oxygen-rich air, the fire gets a new shipment of fresh oxygen to burn.

This does not happen in zero gravity. The air is heated by the fire expands, but as there is no gravity to pull the denser air into this space, just ... stays there. Meanwhile, the fire continues to consume oxygen and returning carbon dioxide until it suffocates itself. Space travel is very complicated, with many problems taking drastic consequences, fire is one of the few ways in which the astronauts have a break. Unless there is some kind of airflow feeding the fire, giving fresh oxygen, a fire in a spacecraft will turn itself off. This is not the same as saying not have to be careful with fire.

Some flames, eg candles, also change color in space. When the wick of a candle burns, is being undone molecule by molecule. This separation absorbs heat. However, when molecules, in this case, long chains of carbon, are pushed upward, as coal burning and shining with yellow. In zero gravity, the carbon chains are not consumed, and the flame is blue, cooler and more tenuous.

Found and translated, more or less, io9