Archive for July, 2009

July 28th, 2009

Passwords

Passwords come in many flavors and types. There are weak passwords, medium strength passwords, strong passwords, and passwords so secure, not even you can remember them.

A weak password is a terrible thing to have, as it can be easily broken, and is like having a screen door on a submarine. Weak passwords have no special features, are short, and are just alphabetic characters.

Some examples are: password, birthday, cats

A medium password is like having closed, but unlocked doors. They will keep out most people, but anyone with a modicum of talent, or time can crack the code. Medium passwords are short, and have alphanumeric characters.

Some examples are: Tac0B3LL, 1337Haxx0R, 0xDeadBEEF

A strong password is a good thing to have, much like an iron door. Strong passwords are random strings of alphanumeric and special characters. They are long, and use a mixture of lower and upper case letters. Cracking them is almost impossible.

Some examples are: e$S130Skoo), r*sk8vrt9(3, and te#dthu(86

To generate special passwords, please visit this MSN article, and download the HTA program it has. This program has an easy to use GUI, and is very secure, with a long period random number generator.

July 25th, 2009

Garbage Manners

Last Wednesday, my driver and I collected 15.89 tons of garbage in a rather quick ten and a half hours. Another two hundred and ten pounds, and we would have had an amazing sixteen tons, aka, 36,000 lbs (about 8,000 kg). For our particular truck, the maximum gross vehicular weight is 54,000 lbs (26 tons), with our truck itself taking up a svelte 16,000 lbs (8 tons).

Thursday, I went on a bulk trash run, and in the span of twelve and a half hours, my driver and myself picked up 14.25 tons, however, two tons of that came from the first three stops we had.

Tuesday, I was back on regular trash duty, and collected an amazing eighteen tons. It was a foul day, as there was a lot of loose garbage lying around. There was a lot of glass, dirty food, and maggots. Now, I know trash is normally disgusting, but this was something else. Even though Allied Waste (whom I work through, via Labor Ready) gives out a do and don’t list for garbage, people seem mentally unavailable/ unwilling to follow the list. Thus, I come home almost every night stinking like hell.

Thus, I present: How not to piss off your garbage man

  1. Put your trash in garbage bags. Garbage men don’t pick up loose trash.
  2. If you have several bags, or loose animals in your neighborhood, put the bags in the trash bin. Garbage men don’t pick up loose trash, and we might miss a loose bag. Cans are much harder to miss.
  3. Keep your bins under fifty pounds. An extremely heavy trash bin is the number one cause of injuries. If you can’t lift your bin at least four feet into the air, why should we?
  4. Bag your glass. Broken glass is very dangerous, and is the second most common cause of injuries.
  5. Balance your bins. One super-heavy bin and three light bins is worse to lift then four medium heavy bins.
  6. Drain all liquids before you toss them. Spoilt drink breeds maggots faster then food, and it stinks worse.
  7. Do NOT put your yard waste with your trash. In most places, this is a big no-no. Yard waste is really, really heavy, it soaks up water, and is a breeding place for flies, and other such lovelies. I mark any houses that do this, that way, they can be charged extra on their next bill.
  8. Use strong bags. Flimsy bags are worthless, and just cause trash to get scattered all over the ground. Flimsy bags just piss me off, and when I get pissed, trashcans get rattled.

If you follow these simple rules, you ought to have no problems with your garbage men, and they will not have any problems with you.



July 23rd, 2009

Some Interesting Equations

Here’s a collection of random, important equations in advanced physics. Find one you like, and read up on it.

Einstein’s Field Theory

G_{\mu\nu} + \Lambda g_{\mu\nu} = \frac{8 \pi G_N}{c^4} T_{\mu\nu}

Maxwell’s equations

\frac{4\pi}{c}j^\beta = \partial_{\alpha}F^{\alpha\beta} + \Gamma^{\alpha}_{\mu\alpha}F^{\mu\beta} + \Gamma^{\beta}_{\mu\alpha}F^{\alpha\mu}

0 = \partial_{\gamma}F_{\alpha\beta} + \partial_{\beta}F_{\gamma\alpha} + \partial_{\alpha}F_{\beta\gamma}

Schrodinger Equation

-\frac{\hbar^2}{2m} \nabla^2 \Psi (\vec{r},t) + U(\vec{r}) \Psi (\vec{r},t) = i\hbar \frac{\partial}{\partial t} \Psi (\vec{r},t)

i\hbar \partial_t |\Psi\rangle = H|\Psi\rangle

More Quantum Mechanical Equations

1 = \int \Psi^{*}\Psi dV =  \langle\Psi|\Psi\rangle = \Psi_i \Psi^i

|\Psi\rangle = Ae^{i(\vec{r}\cdot\vec{k} - \omega t)}

Hawking Radiation
T = \frac{\hbar c^3}{8 \pi G_N M_{BH} k_B}

P = \frac{\hbar c^6}{15360 \pi G^{2}_{N} M^{2}_{BH}}

Feynman integral in curved spacetime

\langle q_{j+1} | \exp\left( {- {i \over \hbar } \hat H \delta t} \right) |q_j\rangle = \exp\left( {- {i \over \hbar } V \left( q_j \right) \delta t} \right) \int { dp \over 2\pi } \exp\left( {- {i \over \hbar } { { p}^2 \over 2m} \delta t} -{i\over \hbar} p \left( q_{j+1} - q_{j} \right) \right)

July 22nd, 2009

It isn’t about the People

I’m Gordon – a different Gordon. While Gordon is away he asked me to send over a post today. I keep my own blog and I’m also a professor at the University of Washington. I’m an experimental physicist working on the ALTAS and DZERO experiments. But I’m not going to talk about those. :-)

So – who’s been following the Apollo 8th’s 40th anniversary? NASA has put together a pretty cool web site with lots of great resources. The Apollo mission was truly one of our crowning technological achievements. And at a time like this you can’t help but look forward at the same time you look forward. And you run right into the same questions as always: can America afford space exploration? What should the program look like in the near and long-term future?

Ignoring the moral factor for the country, the science case for exploration is pretty strong in my view. There is a lot we don’t know about our own earth, about the moon, and, especially, about near-by planets. Telescopes that are out of the earth’s atmosphere have unique advantages when it comes to deep space exploration. We have a lot yet to discover about the planet we currently live on and on the solar system, galaxy, and universe we inhabit. I’m always in favor of more knowledge. Can we afford it. The USA? Certainly! I can’t think of many crises in the USA that would warrant totally canceling the space program (or any other science program for that matter). No country can survive without a balance in how it spends money – on the present as well as the near and far futures. The global warming crisis has already taught us how important it is to know where we live and how we are affecting the environment around us (no matter which side of the debate you are on!).

So what should be space program look like? I think it should look more like this:

and less like this:

The reason is bang-for-the-buck. I think it is pretty hard to deny that sending people up into space is amazingly expensive right now. You have to get them up, and you have to get them back. You have to supply life support. Escape hatches. Lots of space you might fill with equipment is people and oxygen and etc. People are amazingly good at improvising. Something goes wrong – your buggy gets stuck on a rock or similar – people can adapt. That is where they really beat out a robot. We can get an idea of something that needs to be done, and quickly come up with a plan that balances all the risk factors, the obstacles, and still achieves the goal. Heck, if on the way to accomplishing the plan something interesting distracts us – well, that is useful too – perhaps we made one of those serendipitous discoveries; whatever: we can quickly evaluate the interesting thing and decide if it is just a rock reflecting light or some form of Martian currency. Finally, because we have to bring back the humans, bringing back that discovery has very little additional cost (other than biohazard containment!).

Robots have different strengths. Many of the things I’ve listed above robots aren’t so good at. On the other hand, they can stay on a planet for months or years. Need no life support – so getting them there is a lot cheaper. We are getting good enough at creating these exploration robots that we can given them simple tasks and they can take care of themselves. Since they are there for months or years at a time, it doesn’t matter if they aren’t extraordinarily efficient, we can just have them repeat the exercise several times until they get it right. And, perhaps because we don’t have to carry all the support equipment for humans out there, we can stuff an extra scientific instrument or two on the device and get that much more information out.

The thing is – the science case is overwhelmingly in favor of the robots right now. Check out the poster-child for this – the Mars Rover Missions. 5 years of exploration and science. Less than one billion bucks. What did putting a man on the moon cost? I can’t find firm numbers – but it isn’t uncommon to see numbers like 100 billion. Now, I don’t think going back to the moon would be that expensive – it usually is cheaper the second time around. Mars, which was Bush’s stated goal, would probably be that or close to it. For that kind of cost you could littler Mars with rovers and send a few to other planets.

Maybe these commercial endeavors getting people into space cheaply will change the cost/benefit equation. If successful they may well change my opinion of things like the space station – things in low earth orbit. If you could fly the parts up there cheaply and ferry people back and forth – then it might just be another expensive government lab where micro-gravity experiments could be done (in isolation too). But getting people further out to the Moon or Mars would still be very expensive – I doubt I’d be convinced.

Besides, the more experience we have with sending objects up the better prepared we will be when the aliens arrive. ;-)

July 12th, 2009

Elbow Relief

As some of you may know, I have been unemployed for some time. I have recently taken a day labor job at our local Labor Ready ™ to help with the bills.

For the past few weeks, I have been running garbage for the local municipal garbage companies. However, the past couple of days, my left elbow has been hurting whenever I move my arm, and I seem to lose power when I try and pick up anything heavy.

It all started when some fool tried to cheat the rules, and put yard waste in with his garbage, a big no-no. Because of him, I got hurt, and I can’t afford to take time off to heal.

SO, I am appealing to you, my readers for assistance. Does anyone have any advice for me, so I can help my elbow heal as fast as possible? I cannot afford health insurance, so seeing a doctor is out of the question.

Any advice would be helpful.

July 8th, 2009

Maxwell’s Equations in Free Space

Solving Maxwell’s Equations in Free Space

Before, I had enumerated Maxwell’s Equations

Consider a region of space with no free charges, so Maxwell’s equations simplify to:

\nabla\times\vec{E} = \frac{-\partial\vec{B}}{\partial{t}}

\nabla\times\vec{B} =\mu_{0}\epsilon_{0}\frac{\partial\vec{E}}{\partial{t}}

\nabla\cdot\vec{E} = 0

\nabla\cdot\vec{B} = 0

We then select a direction by taking the curl of our first equation
\nabla\times\vec{E} = \frac{-\partial\vec{B}}{\partial{t}} to get the second order equation

\nabla\times(\nabla\times\vec{E}) = \nabla\times(\frac{-\partial\vec{B}}{\partial{t}})

This yields

\nabla^{2}\vec{E} - \frac{\partial^{2}\vec{E}}{\partial{t^2}} = 0.

The interested reader is encouraged to verify this fact. It may be wise to make use of the definition of the cross product, and that the electric and magnetic fields are perpendicular. If you have questions about direction, please remember the right hand rule.

The solution to the equation is E=E_{0} \sin(\frac{2\pi x\pm vt}{\lambda}). Here, x is the position of our wave, t is the time, and v is the speed of propagation. Again, check this; use f(x)=x\pm vt, E=E_{0}e^{f(x)} and E=E_{0}e^{if(x)}, and remember Ae^{if(x)} = A\cos(f(x)) + Ai\sin(f(x)) if you need it.

Note that there are two solutions, f(x+vt) and f(x-vt). The two solutions are identical in everything but time. That is, one solutions is a wave moving forward in time, and the other is a wave moving backward. Without loss of generality, a physicist can toss the unneeded solution away.

Checking that the solution by double differentiation works if, and only if v2 is \frac{1}{\mu_0 \epsilon_0}. Since both \mu_0 and \epsilon_0 are constants, that implies v is also a constant. It turns out v is almost 3.0 \times 10^8 \frac{m}{s}, which is the speed of light. Thus, v is c, the speed of light, and hence, light is an electromagnetic disturbance.

July 5th, 2009

A slight problem

Dear Users:

Over the 4th of July weekend, the /gcsgz5 directory was corrupted, and unfortunately, everything had to be reinstalled.

I was able to recover the old posts, but the MySQL databases were hosed.  This means that all users must re-register, both for the blog and the bulletin board.

I am really sorry this had to happen.

-Gordon

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