To calculate the distance from the earthquake epicenter based on the difference in arrival times of P-waves and S-waves, we use the fact that P-waves travel faster than S-waves. The average difference in arrival time is approximately 1 minute for every 8 kilometers (5 miles) from the epicenter. Given an arrival time difference of 8 minutes and 40 seconds (which is 8.67 minutes), the distance would be about 69.36 kilometers (or approximately 43.2 miles) from the epicenter.
To determine which observer is farther from an earthquake epicenter, you can compare the arrival times of P-waves (primary waves) and S-waves (secondary waves) at each location. P-waves travel faster than S-waves, so the difference in their arrival times increases with distance from the epicenter. By measuring the time difference between the arrivals of these waves at each observer's location, you can calculate the distance to the epicenter; the observer with the larger time difference will be farther from the epicenter.
To determine which observer is farther from an earthquake epicenter, you can compare the arrival times of P-waves (primary waves) and S-waves (secondary waves). P-waves travel faster than S-waves, so if one location records P-waves significantly earlier than S-waves, it indicates that the observer is closer to the epicenter. By measuring the time difference between the arrival of the P-waves and S-waves at each observer's location, the observer with the greater time difference is farther from the epicenter.
To determine which observer is farther from an earthquake epicenter, you can compare the arrival times of P (primary) waves and S (secondary) waves at each location. P waves travel faster than S waves, so the time difference between their arrivals increases with distance from the epicenter. By analyzing the time difference for each observer, the location with the greater time gap indicates a farther distance from the epicenter. The greater the delay in S wave arrival after the P wave, the farther the observer is from the epicenter.
The time difference between the arrival of P (primary) and S (secondary) waves at a seismic station is directly related to the distance from the earthquake epicenter. In this case, the 8 minutes and 40 seconds delay corresponds to the time it took for the S waves to arrive after the P waves. Using the standard average velocities of P and S waves (about 6 km/s and 3.5 km/s respectively), we can calculate the distance to be approximately 34.6 kilometers from the epicenter.
The frequencies are the same, unless the source is moving relative to the observer.
To determine which observer is farther from an earthquake epicenter, you can compare the arrival times of P-waves (primary waves) and S-waves (secondary waves) at each location. P-waves travel faster than S-waves, so the difference in their arrival times increases with distance from the epicenter. By measuring the time difference between the arrivals of these waves at each observer's location, you can calculate the distance to the epicenter; the observer with the larger time difference will be farther from the epicenter.
To determine which observer is farther from an earthquake epicenter, you can compare the arrival times of P-waves (primary waves) and S-waves (secondary waves). P-waves travel faster than S-waves, so if one location records P-waves significantly earlier than S-waves, it indicates that the observer is closer to the epicenter. By measuring the time difference between the arrival of the P-waves and S-waves at each observer's location, the observer with the greater time difference is farther from the epicenter.
To determine which observer is farther from an earthquake epicenter, you can compare the arrival times of P (primary) waves and S (secondary) waves at each location. P waves travel faster than S waves, so the time difference between their arrivals increases with distance from the epicenter. By analyzing the time difference for each observer, the location with the greater time gap indicates a farther distance from the epicenter. The greater the delay in S wave arrival after the P wave, the farther the observer is from the epicenter.
To determine which of the two observers is farther from the earthquake epicenter, you can compare the arrival times of P (primary) waves and S (secondary) waves at each location. P waves travel faster than S waves, so the difference in their arrival times increases with distance from the epicenter. By calculating the time difference between the arrival of the P and S waves for each observer, the observer with the larger difference is the one farther from the epicenter. This method leverages the known velocities of P and S waves to estimate the distance to the source of the earthquake.
The time difference between the arrival of P (primary) and S (secondary) waves at a seismic station is directly related to the distance from the earthquake epicenter. In this case, the 8 minutes and 40 seconds delay corresponds to the time it took for the S waves to arrive after the P waves. Using the standard average velocities of P and S waves (about 6 km/s and 3.5 km/s respectively), we can calculate the distance to be approximately 34.6 kilometers from the epicenter.
14,4oo km away. i think. check calculations to be sure.
Based on the average speed of a P-wave (6 km/s), if the observer detected the P-wave 8 minutes after the earthquake, they would be approximately 2880 km away from the epicenter. This calculation assumes the P-wave travelled directly through the Earth without any barriers altering its speed.
The frequencies are the same, unless the source is moving relative to the observer.
The path difference is the difference in the physical distance between the two sources to the observer, i.e., the difference in distance travelled from the source to the observer.
Data from one seismometer can give you the distance to an earthquakes epicentre. When data from two stations is available, by plotting the calculated distances as a circle of known radius around the stations, these two circles will intersect in two places. Add in a third station and all three circles will intersect in the same place which is the epicentre.
23.5
An apparent brightness is the brightness of a star as measured by an observer.