April 11, 2008
Hurricanes (Continued)
o While
variations in the total number of hurricanes in the Atlantic Ocean is
interesting, keep in mind that most people only remember the ones that cause
death and destruction on the coast. Many Atlantic hurricanes stay out at sea or
are relatively weak when they make landfall. Those few hurricanes that reach
category 4 and 5, only remain at that strength for
short periods of time, which on average is less than 24 hours. The chance that
one of these monsters will hit the
§
Show link
to a web page that shows the location of all major landfalling
hurricanes to hit the
n Cost of US hurricanes
o Generally
speaking, in the
o Before
Katrina happened, I would present statistics about the effects of hurricanes on
the
§
The damage costs due to
hurricanes in the
Ø
The increasing trend in property damage results
from the fact that much building is occurring along
§ Loss of life associated with hurricanes was decreasing from the early 1900s until Katrina hit in 2005.
Ø
The decreasing loss of life results from two
factors. In the early part of the
century before satellite imagery and sophisticated forecasting methods, people
had little warning of an approaching hurricane, and many were killed. In fact
the
n
Why was
Katrina so deadly?
o Katrina
forces us to reconsider the long-held belief that hurricanes will not cause
many deaths in the
o The
question here is: Even with the ample
warning provided by the
§
See
figure 11.25 to see how well Katrina’s path was forecasted.
o Undoubtedly
the vulnerability of the
o The
one course of action that will always work to save lives is for people to
evacuate the area before the storm hits.
Unfortunately with Katrina many residents remained even though they were
warned in ample time to leave.
§
We can argue about whether this was the
government’s fault or whether the responsibility should be placed on the
individuals who made personal decisions to not evacuate.
§
And no doubt, federal and local government
screwed up in their response to the disaster making it worse than it might have
been.
§
But again, the only sure way to save lives is
for people to evacuate before the storm hits.
Hopefully, Katrina will act as a wake up call for those living in
hurricane-prone areas. Don’t take
chances or at least understand the risk that you and your family take by not
heeding warnings.
§
A Katrina-type disaster was foreseen by many
people. In fact a
Ø
People living in hurricane prone areas need to
understand the devastation that hurricanes can cause, keep informed on
hurricane activity in their area, and be prepared to make intelligent
decisions. People in
Radiation (Chapter 2, pg. 31 forward)
n Radiation is the transfer of energy by electromagnetic wave motion. Electromagnetic energy emitted (or given off) by one object is delivered to another object when it is absorbed by that object.
n Radiation is the most important energy transport process because it is able to travel through empty space (a vacuum), while the other two basic energy transport processes, conduction and convection, both require that matter be present to accomplish the energy transport.
n We will now go through the supplemental reading material to help describe what is meant by an electromagnetic wave, how are different types of radiation distinguished, and several fundamental laws of radiation emission. I believe that the material presented in the supplemental reading will be easier to understand than the material in the textbook.
o The supplemental reading page for electromagnetic radiation is available under the reading link on these class web pages. I strongly suggest that you read over this material before coming to class. It may also be helpful to print the pages so that you have them in front of you when we discuss this material.
n Quick Summary
o Review figure showing electromagnetic spectrum (linked on lecture notes page)
o All objects in the universe emit (or give off) radiation energy. The amount and type of radiation emitted depends strongly on the temperature of the object.
§ The higher the temperature, the more total energy radiated
§ The higher the temperature, the shorter the wavelength of the peak radiation energy emission.
Ø Therefore, the hot sun emits much more radiation energy than the cooler Earth and its peak emission is at a much shorter wavelength than the Earth.
o See figure 2.9. Peak emission for the Sun falls into the visible radiation category, while peak emission for the Earth (and most objects on the Earth) is infrared radiation, which we cannot see with our eyes.
n Photons
o At a very basic level, radiation energy is emitted photon by photon. Billions upon billions upon billions … of photons. We have seen that different types of radiation can be described by the wavelength of its electric and magnetic fields (shorter wavelengths are said to carry more energy). Alternatively, different types of radiation can be described by the energy carried by a single photon. Keep in mind that there exists a continuous spectrum of photon energies in the universe.
§ Because only a small fraction of all the radiation energy emitted from the Sun is in the form of ultraviolet radiation (figure 2.8), we can say that the Sun emits many more visible photons than ultraviolet photons (equating to more visible radiation energy than ultraviolet); however, each ultraviolet photon carries more energy than each visible photon.
o At the very basic level, radiation energy is absorbed photon by photon as well. With respect to human well-being, an important issue here is what happens to a living cell when it absorbs a photon.
§ An ultraviolet photon has enough energy to damage or destroy the DNA in a living cell when it is absorbed.
§ A visible photon does not contain enough energy to damage the cell when it is absorbed.
§ Thus the absorption of many visible photons does not cause a problem, but the absorption of a single ultraviolet photon can cause problems. This is why we must protect ourselves from exposure to ultraviolet radiation (photons).