Physical Science Under Microgravity: Experiments on Board the SJ-10 Recoverable Satellite
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Towards Understanding the Origin of Cosmic-Ray Electrons
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Precision results on cosmic-ray electrons are presented in the energy range from 0.5 GeV to 1.4 TeV based on 28.1×106 electrons collected by the Alpha Magnetic Spectrometer on the International Space Station. In the entire energy range the electron and positron spectra have distinctly different magnitudes and energy dependences. The electron flux e...
AMS-02 experiment: status and perspectives
The AMS-02 experiment is a cosmic rays observatory installed on the International Space Station for a long duration mission. The results from the first 7 years of data collection are presented and commented.
Neutrinos, dunkle Materie und Co.: von der Entdeckung der kosmischen Strahlung zu den neuesten Ergebnissen der Astroteil...
Claus Grupen erörtert in diesem essential in einem kurzen historischen Abriss die Astroteilchenphysik und beschreibt die neuesten Resultate, ohne ins mathematische Detail zu gehen. Als Einstieg in dieses neue Forschungsgebiet verstanden, gibt er einen Überblick darüber, was sich am Himmel, zwischen den Sternen und zwischen den Galaxien abspielt. Es...
Classifying the Cosmos
Keeping watch in Babylon: the astronomical diaries in context
Geomagnetism, aeronomy and space weather: a journey from the Earth's core to the Sun
11th Cosmic Ray International Seminar : Entering the Era of Multi-Messenger Astronomy (CRIS 2018)
Measurements of the $^3$He and $D$ components in cosmic rays with the AMS-02 experiment
The $^3$He/$^4$He and $D/p$ flux ratios in cosmic rays (CR) are two of the most valuable tools for understanding the propagation of CR in the galaxy and constrain the models that describe it. In this work, two new preliminary measurements of $^3$He/$^4$He and $D/p$ flux ratios are presented, each obtained from the data of the AMS-02 experiment.
Learning about Dark Matter from the Stars
We discuss several novel astrophysical methods for elucidating the nature and the distribution of dark matter in the Universe. First, we argue that subhalos of the Milky Way's dark matter halo traveling through the disk will leave a characteristic imprint in the motion of nearby stars. These "stellar wakes" can be probed using precise astrometric d...
