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Astrophysics and Astrononmy
IAC Investiga - Física Solar
Natural Sciences (Astrophysics and Astrononmy)
SOLARNET - High Resolution Solar Physics Network
Date of upload:
28.08.2015
Caption:
Video on Solar Physics at the IAC with English Subtitles
El IAC cuenta sus líneas de investigación en cinco vídeos. "Física Solar" es el primero de los audiovisuales producidos por este centro astrofísico con financiación del programa Severo Ochoa.
Before the Big Bang: What Happened? - Space
Natural Sciences (Astrophysics and Astrononmy)
Date of upload:
28.09.2015
Caption:
The universe was born 13.7 billion years ago with the Big Bang. But what was there before? Scientists are starting to get an answer thanks to the time-travelling Planck mission.
Made by euronews, the most watched news channel in Europe, euronews knowledge gives YouTubers amazing access into the scientists labs and research fields, including the origins of the universe!
Promotional Video about the EST project
Natural Sciences (Astrophysics and Astrononmy)
SOLARNET - High Resolution Solar Physics Network
Date of upload:
26.08.2015
Co-author:
The EST Consortium
Caption:
The European Solar Telescope (EST) is of major interest for all the European Solar Community, since it will help to maintain Europe on the top of science, Solar Physics, and technology.
The EST design study was funded by the European Commission's 7th Framework Programme under contract number FP7-212482.
The G320-G330 sector of the Galaxy in atomic and molecular gas
Natural Sciences (Astrophysics and Astrononmy)
Date of upload:
30.09.2015
Co-author:
Catherine Braiding
Caption:
G320-330: A comparison along the sector of the Galactic Plane from l=320°-330° of the atomic hydrogen from the SGPS (top; McClure-Griffiths et al. 2005), $^{12}$CO from our Mopra CO survey (middle; Braiding et al. 2015) and $^{12}$CO from the original Dame et al. (2001) survey (bottom). The effect of the improvement in resolution, a factor of ~10 angular and spectral dimensions, is dramatic.
Slipping reconnection - Movie 1
Natural Sciences (Astrophysics and Astrononmy)
Date of upload:
26.10.2015
Caption:
Slipping reconnection model
Dynamic evolution of $\beta=1$-layer in the solar atmosphere
Natural Sciences (Astrophysics and Astrononmy)
Date of upload:
20.03.2015
Caption:
The contour shows the dynamic evolution of the $\beta=1$ layer in the strongly magnetized solar atmosphere.
The GREGOR Solar Telescope
Natural Sciences (Astrophysics and Astrononmy)
SOLARNET - High Resolution Solar Physics Network
Date of upload:
26.08.2015
Co-author:
produced by IAC Videos
Caption:
Promotional video produced by the Instituto de Astrofíscia de Canarias on Tenerife about the new German solar telescope GREGOR.
Manuel Collados Vera - GREGOR telescope
Natural Sciences (Astrophysics and Astrononmy)
SOLARNET - High Resolution Solar Physics Network
Date of upload:
26.08.2015
Caption:
Manuel Collados Vera talking about the GREGOR telescope
Mopra_CMZ_12CO_13CO_P-V
Natural Sciences (Astrophysics and Astrononmy)
Date of upload:
11.12.2015
Caption:
Video of the current Mopra CMZ 12CO and 13CO in position-velocity space, as shown at the UNSW December 2015 Mopra Workshop.
Magneto-acoustic wave propagation in the solar atmosphere: vertical magnetic field ($\theta=30^°$), disturbance $\delta B$
Natural Sciences (Astrophysics and Astrononmy)
Date of upload:
13.03.2015
Co-author:
M. Roth, O. Steiner
Caption:
Magnetic field perturbations, $\delta B/B_0$, for di fferent time steps and for the scenario of a vertical magnetic fi eld. The magneto-acoustic wave propagates from the source (piston) located at (x; z) = (1000;-750) km. The horizontal line shows the equipartition level, where the sound speed equals the Alfven speed, $c_\mathrm{s}=c_\mathrm{A}$. The vertical lines represent magnetic field lines.
Magneto-acoustic wave propagation in the solar atmosphere: vertical magnetic field, disturbance $\delta B$
Natural Sciences (Astrophysics and Astrononmy)
Date of upload:
13.03.2015
Co-author:
M. Roth, O. Steiner
Caption:
Magnetic field perturbations, $\delta B/B_0$, for
di fferent time steps and for the scenario of a vertical magnetic fi eld. The
magneto-acoustic wave propagates from the source (piston) located at (x; z) =
(1000;-750) km. The horizontal line shows the equipartition level, where the sound speed equals the Alfven speed, $c_\mathrm{s}=c_\mathrm{A}$. The vertical lines represent magnetic field lines.
Life On Mars? ExoMars Experts Answer - Space
Natural Sciences (Astrophysics and Astrononmy)
Date of upload:
28.08.2015
Caption:
euronews knowledge brings you a fresh mix of the world's most interesting know-hows, directly from space and sci-tech experts.\\
Made by euronews, the most watched news channel in Europe.
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