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Wladimir Lyra
Registrace 30. 08. 2013
MRI with outer dead/active transition.
MRI simulation but with disk started out of equilibrium. Notice the wave that is excited. It propagates outward, hits the boundary and is reflected back. The wave damping boundary should be able to absorb it if it is wide and smooth enough.
zhlédnutí: 29
Video
3D simulations of planet formation by vortex trapping
zhlédnutí 130Před rokem
Talk at Vertical shear instability meeting in (virtual) Copenhagen
ASTR 305 - Class 2 - Video 5 : Heliocentrism and Parallax
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ASTR 305 - Class 2 - Video 5 : Heliocentrism and Parallax
ASTR 305 - Class 2 - Video 4 : Aristotle and Ptolemy
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ASTR 305 - Class 2 - Video 4 : Aristotle and Ptolemy
ASTR 305 - Class 2 - Video 3 : Motions in the sky
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ASTR 305 - Class 2 - Video 3 : Motions in the sky
ASTR 305 - Class 2 - Video 2 : Scientific models
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ASTR 305 - Class 2 - Video 2 : Scientific models
ASTR 305 - Class 2 - Video 1 : The distance to the moon.
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ASTR 305 - Class 2 - Video 1 : The distance to the moon.
ASTR 305 - Class 1 - Video 7: Astrobiology and Biology
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ASTR 305 - Class 1 - Video 7: Astrobiology and Biology
ASTR 305 - Class 1 - Video 6: Astrobiology and Planetary Sciences
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ASTR 305 - Class 1 - Video 6: Astrobiology and Planetary Sciences
ASTR 305 - Class 1 - Video 5: Astronomy and Astrobiology
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ASTR 305 - Class 1 - Video 5: Astronomy and Astrobiology
ASTR 305 - Class 1 - Video 4: Game Changers
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ASTR 305 - Class 1 - Video 4: Game Changers
ASTR 305 - Class 1 - Video 1 - What are we looking for?
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ASTR 305 - Class 1 - Video 1 - What are we looking for?
ASTR 506 - Finite Difference Coefficients
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ASTR 506 - Finite Difference Coefficients
ASTR 506 - Class 20 - Video 3 - Acoustics: Dispersion Relation
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ASTR 506 - Class 20 - Video 3 - Acoustics: Dispersion Relation
ASTR 506 - Class 20 - Video 2 - Acoustics: Wave Solution.
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ASTR 506 - Class 20 - Video 2 - Acoustics: Wave Solution.
ASTR 506 - Class 20 - Video 1 - Acoustics: Linearization
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ASTR 506 - Class 20 - Video 1 - Acoustics: Linearization
ASTR 506 - Class 19 - Extra Video 4 - Index Notation" Example: Double curl via index notation
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ASTR 506 - Class 19 - Extra Video 4 - Index Notation" Example: Double curl via index notation
ASTR 506 - Class 19 - Extra Video 3 - Index Notation: the Levi-Civita symbol
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ASTR 506 - Class 19 - Extra Video 3 - Index Notation: the Levi-Civita symbol
ASTR 506 - Class 19 - Extra Video 2 - Index Notation - Einstein summation notation
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ASTR 506 - Class 19 - Extra Video 2 - Index Notation - Einstein summation notation
ASTR 506 - Class 19 - Extra Video 1 - Index Notation: Intro
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ASTR 506 - Class 19 - Extra Video 1 - Index Notation: Intro
ASTR 506 - Class 19 - Video 11 - Primer on Tensors - Inertia Tensor: all 3 arms off-axes.
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ASTR 506 - Class 19 - Video 11 - Primer on Tensors - Inertia Tensor: all 3 arms off-axes.
ASTR 506 - Class 19 - Video 10 - Primer on Tensors - Inertia Tensor Example - 2: Off-diagonal terms
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ASTR 506 - Class 19 - Video 10 - Primer on Tensors - Inertia Tensor Example - 2: Off-diagonal terms
ASTR 506 - Class 19 - Video 9 - Primer on Tensors - Example of Inertia Tensor - 1 - Mass on axis
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ASTR 506 - Class 19 - Video 9 - Primer on Tensors - Example of Inertia Tensor - 1 - Mass on axis
ASTR 506 - Class 19 - Video 8 - Primer on Tensors - The Inertia Tensor
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ASTR 506 - Class 19 - Video 8 - Primer on Tensors - The Inertia Tensor
ASTR 506 - Class 19 - Video 7 - Primer on Tensors - Example: The Inertia Moment is not a scalar
zhlédnutí 20Před 3 lety
ASTR 506 - Class 19 - Video 7 - Primer on Tensors - Example: The Inertia Moment is not a scalar
Most valuable channel I have ever found on CZcams ❤
Glad to be of help.
looking forward to this playlist
You saved me.. thanks a lot mr.Wladmir.
Glad to hear that
Vaaaaleu, prof!!!!!!!!!!!
De nada ;-)
Thanks for this video and the animation , gives you a much better mental picture of what is happening
This is exactly what I was looking for. Do you provide the hard copy for download of ASTR 506 - Class 19 - Extra videos 1 - 4? If not I'll have to type it all in myself because it is such a great reference.
Of course, here it is: github.com/wlyra/Astro506/blob/main/PrimerOnTensors.ipynb
thanks for the lecture, much love from Brazil
Why I did'nt find your channel before:)
Thank you Very much :D great video :)
6:09 it'd be sin(90-alpha) instead of sin(90+alpha)
No, according to the law of sines applied to the triangle Sun - Galactic Center - Star, it is sin l / R = sin (90+α)/ R0
You are doing great...I am shocked why there are no comments on this vid...keep going man....Love from india
Thanks. I'm glad the video was useful.
i owe you a lot Wladimir Lyra thanks for the video
Best video I found one CZcams to clear my concept
Why does it not hurt to look at all the further away stars then?
Excellent question! Because at some point their angular size in the sky becomes smaller than the resolution of your eye. At this point, the star is just a "pixel" in your eye and the further they are, indeed less energy you get on that pixel. Intensity is a property of angularly resolved sources of radiation.
Why am I only now finding this playlist?! This is so helpful!
Good day sir, thank you for the informative and lucid video. If you don't mind answering a basic question, how is cos(phi) derived?
Glad you found it informative. The cosine of psi is derived in a previous video: ASTR 506 - Class 8 - Video 5 - Hierarchical triples: The Hamiltonian in orbital elements. czcams.com/video/5KFQwiQToEA/video.html
The handwritten notes are in my webpage as well: astronomy.nmsu.edu/wlyra/DynamicsHydrodynamics.html
Most underrated channel out there
is there a link for the notes you wrote?
Yes, in my webpage.
Therefore this also means that all the parallels except the Equator are never the shortest distances.. So for example you could walk parallel to meridians going from north to south but you could never walk parallel to parallels to be the fastest to go east to west (or vice versa), that's interesting
exactly
You have latitude and longitude reversed.
No, I don't.
Thanks a lot, sir🥰
The value of k
do you by any chance keep your handwritten lectures somewhere?
Yes, you can find them in my webpage astronomy.nmsu.edu/wlyra/DynamicsHydrodynamics.html
why didn't you divide by cos(theta)?
I did. It's implicit in the dot product.
Density is the difficult one :D
can you explain the integration of [exp(-P^2/(2mkt) * P^2 dP] in details Pleas
Please explain the process of differentiation in detail
The basic calculus?
Helpful. Text is a bit small to read.
Dear sir, I am doing my thesis but I could not understand transformation between the astronomical coordinate systems, so request you sir plz suggest me the name of best book of astronomical coordinate system transformations.🙏🙏
Check my lecture notes astronomy.nmsu.edu/wlyra/FundamentalAstronomy/Module1_PositionalAstronomy_Notes.pdf
it is very useful for me ,thanks for this knowledge
at 5:29 shouldn't be "crosses the meridian" instead of "horizon" ? (great videos btw, well explained, very clear and precise, excellent pictures and animations )
Correct! When it crosses the meridian. Thanks for catching it :-)
There is an error in dy/d(phi) derivative in Jacobi Matrix. sin(phi) derivative would be cos(phi) not -cos(phi)
Thanks for the correction.
@@wladimirlyra8757 Could I ask you if this approach works for non symmetric case? Can I write ds in cartesian like this: ds=dx+dy+dz And then just transform it into spherical with Jacobian? In most books I have seen some additional angles representing directions theta and phi. d/ds was rewritten with chain rule and in the output there were some direction cosines. I just wonder if both solutions are equivalent and how one can prove it.
What 😳 is that about i don't have a clue 🤔
Very interesting your demonstration. Eratóstenes (BC) already knew this, but in impiricall way.
Can we get the program that can solve a system of n first-order differential equations by the Heun method ( Modified Euler) by FORTRAN
Thanksss for the video
Thanks for sharing this with us
That's a terrific animation for explaining the ecliptic.
Thank you very much. A PhD student in astrophysics
Any chance we could get a text file with the code?
sure, here's the code astronomy.nmsu.edu/wlyra/DynamicsHydrodynamics/euler.f90
also in C++ astronomy.nmsu.edu/wlyra/DynamicsHydrodynamics/euler.cpp
Sir plzzzzz
Sir I am from India
Sir I love your videos
Thank you so much!
spherical astronomy is the hardest astronomy.
Salve Brasil! Muito obrigado pela aula!
It would be better if you make the 2nd diagram bigger ie. the page should be large
GREAT 👍
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Nice presentation and lecture. Please can you email me the Mathematica code or Matlab code I can use to plot these Zero Velocity curves?