Protons in cosmic rays strike the Earth’s upper atmosphere at an average rate of 1200 protons per square meter per second. What total is the current (in Coulombs per second, or Amperes) does the Earth receive from these cosmic rays? (For the radius of the Earth, use R^E = 6.38 x 10^6 meters.)
Protons in cosmic rays strike the Earth’s upper atmosphere at an average rate of 1200 protons...
5. Protons in cosmic rays strike the Earth's upper atmosphere at an average rate of 1200 protons per square meter per second. What total current (in Coulombs per second, or Amperes) does the Earth receive from these cosmic rays? (For the radius of the Earth, use Re- 6.38 x 10s meters.)
Earth's atmosphere is constantly bombarded by cosmic ray protons that originate somewhere in space. If the protons all passed through the atmosphere, each square meter of Earth's surface would intercept protons at the average rate of 1800 protons per second. What would be the electric current in amperes intercepted by a 14 x 107 km2 area on the planet?
Muons are formed high in the atmosphere by the interaction of cosmic rays with atomic nuclei in the upper atmosphere. They have an average lifetime of about two millionth of a second and according to classical physics should decay before reaching the sea level. However, measurements show a large number of muons reach the Earth’s surface. Give an explanation how this is possible with respect to the earth and muon’s reference frames using ideas of time dilation and length contraction.
Question 9 Earth's atmosphere is constantly bombarded by cosmic ray protons that originate somewhere in space. If the protons all passed through the atmosphere, each square meter of Earth's surface would intercept protons at the average rate of 1900 protons per second. ha would be the electric current nam ere ntercepte b a 2· km2 area on the planet? ' Number the tolerance is +/-590 Click if you would like to Show Work for this question: Units Open Show Work
1. Subatomic particles called muons can be created in the upper atmosphere by collisions of cosmic rays (energetic particles coming from astrophysical sources). As we shall see in a few lectures, muons quickly decay (in 2.2 microseconds on average) into other particles. Consider a muon that was created at a height the same as the top of a nearby mountain, traveled straight down towards the Earth through the atmosphere at 0.9 times the speed of light, and then decayed at...
If the Earth’s atmosphere is considered to extend from the
surface to 20 km, the earth’s radius is 6,200 km, and the
atmosphere is partitioned into cells spaced 0.5 km apart, how many
floating‐point calculations will be required to run one iteration
of a global weather simulation, assuming that each cell requires
200 floating‐point operations? If it requires 20 cycles
(iterations) of simulation to calculate the weather over the next
24 hours, and a forecast is needed in 30 minutes,...
(15%) Problem 8: Suppose a cosmic ray colliding with a nucleus in the Earth's upper atmosphere produces a muon that has speed v = 0.92c. The muon then travels at constant speed and lives 1.5 us as measured in the muon's frame of reference. (You can imagine this as the muon's internal clock.) Randomized Variables y = 0.92 c t = 1.5 us > * 33% Part (a) How long does the muon live in seconds) as observed on the...
The following ANOVA model is for a multiple regression model
with two independent variables:
Degrees
of
Sum
of
Mean
Source
Freedom
Squares
Squares
F
Regression
2
60
Error
18
120
Total
20
180
Determine the Regression Mean Square (MSR):
Determine the Mean Square Error (MSE):
Compute the overall Fstat test statistic.
Is the Fstat significant at the 0.05 level?
A linear regression was run on auto sales relative to consumer
income. The Regression Sum of Squares (SSR) was 360 and...