Thomas Steindl
Thomas Steindl
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More pulsation modes

The spherical harmonics of even more pulsation modes.

The pulsation modes of oscillating stars are a combination of spherical harmonics $ Y^m_l $ together with a time dependence $exp(i\omega t$). This page shows the resulting modes for different values of the spherical degree $l$ and azimuthal order $m$. Please contact me if you want to use any of my artwork. Higher resolution or specific $l$-$m$ combinations are available on request.
$l=0$
$m=0$
$l=1$
$m=-1$
$l=1$
$m=0$
$l=1$
$m=1$
$l=2$
$m=0$
$l=2$
$m=1$
$l=2$
$m=2$
$l=3$
$m=-3$
$l=3$
$m=-2$
$l=3$
$m=-1$
$l=3$
$m=0$
$l=4$
$m=0$
$l=4$
$m=2$
$l=5$
$m=-3$
$l=5$
$m=0$
$l=6$
$m=-4$
$l=7$
$m=5$
$l=8$
$m=0$
$l=9$
$m=2$
$l=10$
$m=7$
$l=11$
$m=10$
$l=12$
$m=-6$
$l=13$
$m=-9$

About me

Thomas Steindl MSc

PhD student at the Institute for Astro- and Particle physics at the University Innsbruck

Research Group of Univ. Prof. Mag. Dr. Konstanze Zwintz

Links
  • Universität Innsbruck
  • Institute for Astro- and Particle Physics
  • Konstanze Zwintz
  • TESS
  • BRITE constellation
Tools & Software
  • MESA
  • GYRE
  • SMURFS
  • Phoebe
Location

Technikerstraße 25 | 6020 Innsbruck | Room: 8/07

+43 512 507 52031

thomas.steindl@uibk.ac.at