Not exact matches
«Long ago and far away there was a dot that expanded rapidly into the universe...» that in itself is a leap in logic my friend... many assumptions made
about cosmic
background radiation that we know very little
about.
How
about cosmic microwave
background radiation, time dilation in supernovae light curves, the Hubble deep field, the Sunyaev - Zel «dovich effect, the Integrated Sachs - Wolfe effect, the hom.ogeneity of stars and galaxies, etc, etc...
Taking into account natural
background radiation, medical procedures and other sources, people in the U.S. encounter an average of
about 6.5 millisieverts per year.
Embedded in this cosmic microwave
background (CMB)
radiation are hints aplenty
about the universe in its infancy.
Called the cosmic microwave
background (CMB)
radiation, this afterglow was produced
about 370,000 years after the big bang when the first atoms formed and has been studied in great detail by satellites, such as NASA's WMAP probe.
The fliers in this nebula, which appear as two red blobs against a pale green
background of
radiation, seem to be moving fast enough —
about 100,000 miles per hour — to fit Balick's original theory, but they also have backward - pointing bow shocks, as though an even faster wind were coming from behind and pushing past them.
According to standard physics, cosmic rays created outside our galaxy with energies greater than
about 1020 electronvolts (eV) should not reach Earth at those energies: as they travel over such vast regions of space they should lose energy because of collisions with photons of the cosmic microwave
background (CMB), the
radiation left over from the big bang.
A typical nuclear medicine procedure may impart a
radiation dose to the patient comparable to
about one to four years of natural
background radiation depending on the type of study.1 As with X-rays, the value of diagnostic imaging is great and the risks are negligible compared to the health benefits of having the procedure.
While we may not be able to do much
about air pollution or
background radiation, let's look at the factors we can control in more detail.
The additional exposures received by most Japanese people in the first year and subsequent years due to the radioactive releases from the accident are less than the doses received from natural
background radiation (which is
about 2.1 mSv per year).
The cosmic
background radiation is
about 3K so without somehow shading a surface against the warm glow left over from the big bang that's as cold as it gets.
The biggest increase in
background radiation levels world wide was during the peak of atmospheric weapons testing during the 1960s raising the level by
about 5 %.
He was right
about so many things — the
background nineteenth - century CO2 concentration level and its increase over the twentieth century; the importance of high - quality temperature data and the warming trend observed over much of his lifetime; the infrared spectroscopy of CO2 and its effect on «sky
radiation»; and more.
But, if we leave the fission products alone for a few hundred years, they will decay to normal
background levels of
radiation (Safe enough we don't need to worry
about them as much).
And remember, we are talking
about an additional
radiation exposure in the realm of 0.0002 mSv for those living near a nuclear power plant, versus a
background level of 2 to 4 mSv (depending on where you live) due to everything from cosmic rays to ground - derived radon emission to eating bananas (this last one gives you more
radiation than the NPP).