Cosmic Radiation - how is our sun's speed calculated?

In summary, the velocity of an object can be calculated through the use of the anisotropic dipole of the CMB. This is done by observing the Doppler effect on the radiation, which appears blueshifted in the direction of motion and redshifted in the opposite direction. By comparing the frequency of the dipole radiation to the non-dipole radiation, the speed of the object can be determined. This method requires the assumption that the radiation is isotropic and can accurately determine velocities down to a level of one part in 105.
  • #1
lenfromkits
107
0
From the anisotropic dipole of the CMB, they are able to calculate our velocity through space relative to this radiation. How exactly is this done - in general terms. What assumptions are they needing to make ab out this radiation to deduce our speed from it?

I don't understand the connection between observing the radiation and identifying our speed relative to it.

Thanks!
 
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  • #2
The connection is basically just the Doppler effect. The radiation will appear blueshifted in the direction of motion and redshifted in the opposite direction. That's why there is a dipole in the first place. This can tell you the velocity relative to a frame of reference in which the radiation appears isotropic (down to a level of one part in 105 of course :wink:)
 
  • #3
cepheid said:
The connection is basically just the Doppler effect. The radiation will appear blueshifted in the direction of motion and redshifted in the opposite direction. That's why there is a dipole in the first place. This can tell you the velocity relative to a frame of reference in which the radiation appears isotropic (down to a level of one part in 105 of course :wink:)

Oh... I think I'm getting it now. It sounds like you mean they are comparing the frequency of the dipole radiation to the frequency of the non-dipole radiation. The difference in frequency represents the speed at which we are traveling (ie, based on the doppler shift of this frequency that is)?

Thanks for the explanation.
 

1. What is cosmic radiation?

Cosmic radiation refers to high-energy particles that originate from outer space and constantly bombard the Earth's atmosphere. These particles come from various sources, including our own sun, other stars, and even distant galaxies.

2. How is cosmic radiation measured?

Cosmic radiation is measured using specialized instruments such as particle detectors, spectrometers, and telescopes. These instruments can detect and measure the energy, direction, and type of the incoming particles.

3. How is the speed of our sun calculated?

The speed of our sun is calculated using a combination of observations and mathematical models. Astronomers use telescopes to measure the sun's position and velocity relative to other stars and objects in the galaxy. They also use mathematical equations to calculate the sun's speed based on its mass and the gravitational forces acting upon it.

4. What factors affect the speed of our sun?

The speed of our sun is affected by several factors, including its mass, gravitational forces from other objects in the galaxy, and the distribution of matter within the sun. Additionally, the sun's speed can also be influenced by external events such as solar flares and interactions with other stars.

5. How does cosmic radiation impact our planet?

Cosmic radiation can have both positive and negative impacts on our planet. On one hand, it plays a crucial role in the formation and evolution of life on Earth. On the other hand, excessive exposure to cosmic radiation can be harmful to living organisms, causing damage to cells and DNA. Fortunately, the Earth's atmosphere and magnetic field provide some protection against cosmic radiation, but astronauts and frequent flyers are at a higher risk of exposure.

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