Recent content by Logarythmic

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    High & Low Resistivity Effects on Magnetic Field Lines

    Yeah Faraday's law holds, so maybe \frac{\eta}{\mu_0} \nabla^2 \vec{B} - (\nabla \cdot \vec{v})\vec{B} - \frac{\partial \vec{B}}{\partial t} = 0 is a correct answer? But what about the behaviour of the field lines? Could one say that for high resistivity the current is zero and the magnetic...
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    High & Low Resistivity Effects on Magnetic Field Lines

    Homework Statement Two of the MHD equations can be formulated as \vec{E} + \vec{v} \times \vec{B} = \eta \vec{J} \nabla \times \vec{B} = \mu_0 \vec{J} where [itex]\eta[/tex] is the resistivity of the plasma. a.) Derive an equation for the magnetic field at very high resistivity and...
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    Show that a longitudinal wave is electrostatic

    Sometimes I feel so smart that I don't know what to do with myself. ;) Thanks!
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    Show that a longitudinal wave is electrostatic

    I tried with \vec{B} = B_0 \sin{[i(kx-\omega t)]} so \nabla \times \vec{E} = i \omega B_0 \cos{[i(kx-\omega t)]} But that doesn't really help me.
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    Show that a longitudinal wave is electrostatic

    Homework Statement Show that all longitudinal waves must be electrostatic by using Faraday's law. Homework Equations Faraday's law: \frac{\partial \vec{B}}{\partial t} = - \nabla \times \vec{E} The Attempt at a Solution Where should I start??
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    Calculating Solar Wind Density at Jupiter: Formula and Assumptions Explained"

    Homework Statement I'm trying to solve a problem related to the solar wind pressure at Jupiter but I'm stuck at calculating the density. It is stated that the solar wind has a density of 5 [itex]cm^{-3}[/tex] and a speed of 400 km/s at the orbit of the Earth, and that it should be assumed...
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    Solving Complex Integrals: Can I Treat i as Any Other Constant?

    Got it, so w(x) = \int_{-u_0}^{u_0} i2 \pi v e^{i2 \pi vx} dv = \frac{1}{\pi x^2} \left[ 2 \pi u_0 x \cos{(2 \pi u_0 x)} - \sin{(2 \pi u_0 x)} \right]
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    Solving Complex Integrals: Can I Treat i as Any Other Constant?

    \int f(v) e^{iavx} dv = \int f(v) \left( \cos{avx} + i \sin{avx} \right) dv = = \int f(v) \cos{avx} dv + i \int f(v) \sin{avx} dv Maybe?
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    Solving Complex Integrals: Can I Treat i as Any Other Constant?

    How do I solve an integral of the type \int f(v) e^{iavx} dv ? Can I just treat i as any other constant?
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    What is the relationship between Rayleighs and counts in a CCD?

    I'm using that paper, my problem is that I'm not really sure about the definition of counts.
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    What is the relationship between Rayleighs and counts in a CCD?

    How can I find the number of Rayleighs per count if I know the column emission rate, radiance, irradiance, #photons per pixel and #photoelectrons per pixel? I'm totally lost in this one, please help!
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    How Can Heat Conduction Be Modeled in a Cylindrical CanSat?

    Hey everyone! I am currently on a project building a small CanSat. This is a small satellite of the size of a coke can which will be launched together with a balloon and then descend from an altitude of 35 000 m. My problem now is to work out the heat conduction to see if our insulation is...
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    Determine the force in z-direction on the gyrocenter of a charged particle

    I did it with the Lorentz Force on the guiding center and got the equation given by Astronuc but with a plus sign. I guess that the sign is dependent on the charge.
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    How Do You Calculate the Wavelength of Particle Motion in Parametric Equations?

    I thought about that too, but it's stated in the problem that the motion is periodic with period \Omega. Anyway, my question still remains.
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    How Do You Calculate the Wavelength of Particle Motion in Parametric Equations?

    I have two parametric equations for the speed of a particle in a plane: \dot{x}(t) = A \left( 1 - cos{\Omega t} \right) \dot{y}(t) = A sin{\Omega t} The period is equal to \Omega. How do I find the wavelength of the motion? The wavelength is just \lambda = \Omega v , where v =...
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