Is the "solar wind" an actual wind? ? If it is, why doesn't it blow away our space probes?
"Wind" is an analogy term used to help us understand the impact of the electromagnetic fields and particles similar to physical wind in the atmosphere.
The solar "wind" is a flow of electromagnetic energy and particles that originates from the sun; it does interact physically with our planet, as evidenced by the Aurora Borealis, but not all definitions used, even in science, are exactly the same or necessarily intended to explicitly describe the entire effect of some phenomena.
It DOES affect other objects in space, including earth satellites, but not enough to have a significant short-term impact on their orbital mechanics. This is because the type of energy and mass transfer is very different from atmospheric "wind".
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The name "solar wind" is a bit misleading because it's not like wind on Earth; it's made up of charged particles, mostly protons and electrons, that are ejected from the Sun's upper atmosphere at high speeds. It's not a typical wind, but it can still exert pressure on objects in space, including spacecraft; space probes are made to be resistant to the effects of the solar wind by positioning sensitive components away from direct exposure and using protective shielding; further away from the Sun, the solar wind has less of an impact.
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When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
- Given the following, calculate the total power radiated by the Sun. Calculate the rms values of the electric and magnetic fields of by the Sun. What is the net force of sunlight on Saturn?
- Approximately how long does it take the photons released in nuclear reactions in the core of the sun to exit the sun?
- How can photons have momentum?
- How does the sun atmosphere differ from its interior?
- How is helioseismology used to model the sun?
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