Contact

Dr. Urs Mall
Scientist
Phone:+49 551 384 979-152
Email:mall@...
January 2018
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Header Image

The employees of the Department Planets and Comets in July 2012.

Planetary Group Seminar

In the seminars of the Department of Planets, scientists, post-doctoral students, and guests report on discoveries and research results of the missions and projects concerning planets, comets, asteroids, and planetary dust.

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Planetary Group Seminar: Von Mie bis Multiple Scattering-Methoden zur Simulation der Lichtstreuung von Partikeln (T. Wriedt)

  • Date: Jan 25, 2018
  • Time: 11:00 - 12:00
  • Speaker: Thomas Wriedt
  • University of Bremen (Leibniz-Institut für Werkstofforientierte Technologien, IWT)
  • Location: MPS
  • Room: Auditorium
  • Host: Urs Mall

Zur Simulation der Lichtstreuung oder auch der BRDF von komplexen Strukturen und Partikelschichten muss die Lichtstreuung von Einzelpartikeln simuliert werden. In dem Vortrag wird ein Überblick über die zur Verfügung stehenden Theorien gegeben. [more]

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Planetary Group Seminar: Interstellar dust and the heliosphere (V. Sterken)

Interstellar dust (ISD) from the local interstellar cloud traverses the solar system at 26 km/s, owing to the relative motion of the Sun and the cloud. These particles are messengers from interstellar space that can be studied in situ with dust detectors on space missions. In 1993, the first such ISD particles were detected using the Ulysses cosmic dust detector. The mission provided a total of 16 years of ISD data and thus covered almost one Hale cycle. This is important since the dust trajectories are shaped by the solar radiation pressure, gravity and Lorentz force (as they are charged and move through the interplanetary magnetic field that changes throughout the solar cycle). Interpretation of these data is done using monte carlo simulations of dust trajectories, which allows us to constrain the particle properties and it teaches us about the role of the heliosphere. Finally, in 2006, Stardust brought a few samples of interstellar dust material back to Earth, and in 2016, the Cassini mission provided the first time-of-flight mass spectra of 36 ISD impacts on the Cassini Cosmic Dust Analyzer. In this talk, we review the latest developments in the study of “local” interstellar dust with astronomical, in-situ, and sample return techniques. The dynamics of the ISD as it moves through the heliosphere will be explained and finally, we elaborate on what we can gain from computer simulations and spacecraft data for constraining both the ISD properties as well as for studying the heliosphere. [more]

 
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