@book{OPUS4-56791,
  title     = {Aus der m{\"a}rkischen Streusandb{\"u}chse in die Welt hinein},
  series = {Schriften der Landesgeschichtlichen Vereinigung f{\"u}r die Mark Brandenburg ; Neue Folge, 14 Einzelver{\"o}ffentlchungen des Brandenburgischen Landeshauptarchivs; 28},
  journal   = {Schriften der Landesgeschichtlichen Vereinigung f{\"u}r die Mark Brandenburg ; Neue Folge, 14 Einzelver{\"o}ffentlchungen des Brandenburgischen Landeshauptarchivs; 28},
  editor    = {Engel, Felix and Ruffert, Elisabeth and Seeger, Anke and Str{\"a}ßner, Ulrike},
  publisher = {Lukas Verlag f{\"u}r Kunst- und Geistesgeschichte},
  address   = {Berlin},
  isbn      = {978-3-86732-423-6},
  pages     = {344},
  year      = {2022},
  abstract  = {Frank G{\"o}se, Hochschullehrer und apl. Professor f{\"u}r Landesgeschichte an der Universit{\"a}t Potsdam, dem der vorliegende Band anl{\"a}sslich seines 65. Geburtstages gewidmet ist, setzt sich seit Jahrzehnten epochen{\"u}bergreifend und vergleichend mit der Geschichte seines Heimatlandes Brandenburg und der daran gekn{\"u}pften Mythen auseinander. Mit seiner dezidiert quellenges{\"a}ttigten, thematisch und methodisch stets offenen Forschung legt er neue Perspektiven auf »Land und Leute« frei. Denn nicht nur die Betrachtung Brandenburgs und Preußens, sondern ebenso der Blick auf das benachbarte Sachsen und die Herstellung internationaler Kontexte zeichnen Frank G{\"o}se aus, sodass die hier versammelten Beitr{\"a}ge seiner Sch{\"u}lerinnen und Sch{\"u}ler sowie Wegbegleiterinnen und Wegbegleiter die viel­f{\"a}ltigen Interessen des Jubilars spiegeln.},
  language  = {de}
}
@book{OPUS4-9756,
  title     = {Brennpunkte kultureller Begegnungen auf dem Weg zu einem modernen Europa : Identit{\"a}ten und Alterit{\"a}ten eines Kontinents},
  editor    = {Klettke, Cornelia and Pr{\"o}ve, Ralf},
  publisher = {V \& R Unipress},
  address   = {G{\"o}ttingen},
  isbn      = {978-3-89971-877-5 (print)},
  publisher      = {Universit{\"a}t Potsdam},
  pages     = {277},
  year      = {2011},
  language  = {de}
}
@misc{Kraemer2015,
  author    = {Kr{\"a}mer, Raimund},
  title     = {Polen in Europa},
  series = {WeltTrends : Zeitschrift f{\"u}r internationale Politik},
  volume    = {2015},
  journal   = {WeltTrends : Zeitschrift f{\"u}r internationale Politik},
  number    = {100},
  publisher = {WeltTrends},
  address   = {Babelsberg},
  issn      = {0944-8101},
  pages     = {144},
  year      = {2015},
  abstract  = {Bei unseren {\"o}stlichen Nachbarn werden derzeit mehrere Jubil{\"a}en zelebriert: 25 Jahre politischer Umbruch, 15 Jahre Mitgliedschaft in der NATO und 10 Jahre in der EU. WeltTrends nimmt diese geballte Zahlenmagie zum Anlass, Polen zum Thema zu machen. Heft 100 gew{\"a}hrt einen Einblick in die aktuellen außenpolitischen Diskurse in Polen: Sei es zum Verh{\"a}ltnis zur EU, zu den USA oder zu Russland. Nat{\"u}rlich geht es dabei stets auch um das Verh{\"a}ltnis zu Deutschland und ob die Anfang der 1990er Jahre proklamierte „strategische Interessengemeinschaft" zu einer tats{\"a}chlichen Partnerschaft geworden ist.},
  language  = {de}
}
@article{PostbergGruenHoranyietal.2011,
  author    = {Postberg, Frank and Gr{\"u}n, Eberhard and Horanyi, Mihaly and Kempf, Sascha and Krueger, Harald and Schmidt, J{\"u}rgen and Spahn, Frank and Srama, Ralf and Sternovsky, Zoltan and Trieloff, Mario},
  title     = {Compositional mapping of planetary moons by mass spectrometry of dust ejecta},
  series = {Planetary and space science},
  volume    = {59},
  journal   = {Planetary and space science},
  number    = {14},
  publisher = {Elsevier},
  address   = {Oxford},
  issn      = {0032-0633},
  doi       = {10.1016/j.pss.2011.05.001},
  pages     = {1815 -- 1825},
  year      = {2011},
  abstract  = {Classical methods to analyze the surface composition of atmosphereless planetary objects from an orbiter are IR and gamma ray spectroscopy and neutron backscatter measurements. The idea to analyze surface properties with an in-situ instrument has been proposed by Johnson et al. (1998). There, it was suggested to analyze Europa's thin atmosphere with an ion and neutral gas spectrometer. Since the atmospheric components are released by sputtering of the moon's surface, they provide a link to surface composition. Here we present an improved, complementary method to analyze rocky or icy dust particles as samples of planetary objects from which they were ejected. Such particles, generated by the ambient meteoroid bombardment that erodes the surface, are naturally present on all atmosphereless moons and planets. The planetary bodies are enshrouded in clouds of ballistic dust particles, which are characteristic samples of their surfaces. In situ mass spectroscopic analysis of these dust particles impacting onto a detector of an orbiting spacecraft reveals their composition. Recent instrumental developments and tests allow the chemical characterization of ice and dust particles encountered at speeds as low as 1 km/s and an accurate reconstruction of their trajectories. Depending on the sampling altitude, a dust trajectory sensor can trace back the origin of each analyzed grain with about 10 km accuracy at the surface. Since the detection rates are of the order of thousand per orbit, a spatially resolved mapping of the surface composition can be achieved. Certain bodies (e.g., Europa) with particularly dense dust clouds, could provide impact statistics that allow for compositional mapping even on single flybys. Dust impact velocities are in general sufficiently high at orbiters about planetary objects with a radius > 1000 km and with only a thin or no atmosphere. In this work we focus on the scientific benefit of a dust spectrometer on a spacecraft orbiting Earth's Moon as well as Jupiter's Galilean satellites. This 'dust spectrometer' approach provides key chemical and isotopic constraints for varying provinces or geological formations on the surfaces, leading to better understanding of the body's geological evolution.},
  language  = {en}
}
@article{KempfSramaGruenetal.2012,
  author    = {Kempf, Sascha and Srama, Ralf and Gr{\"u}n, Eberhard and Mocker, Anna and Postberg, Frank and Hillier, Jon K. and Horanyi, Mihaly and Sternovsky, Zoltan and Abel, Bernd and Beinsen, Alexander and Thissen, Roland and Schmidt, J{\"u}rgen and Spahn, Frank and Altobelli, Nicolas},
  title     = {Linear high resolution dust mass spectrometer for a mission to the Galilean satellites},
  series = {Planetary and space science},
  volume    = {65},
  journal   = {Planetary and space science},
  number    = {1},
  publisher = {Elsevier},
  address   = {Oxford},
  issn      = {0032-0633},
  doi       = {10.1016/j.pss.2011.12.019},
  pages     = {10 -- 20},
  year      = {2012},
  abstract  = {The discovery of volcanic activity on Enceladus stands out amongst the long list of findings by the Cassini mission to Saturn. In particular the compositional analysis of Enceladus ice particles by Cassini's Cosmic Dust Analyser (CDA) (Srama et al., 2004) has proven to be a powerful technique for obtaining information about processes below the moon's ice crust. Small amounts of sodium salts embedded in the particles' ice matrices provide direct evidence for a subsurface liquid water reservoir, which is, or has been, in contact with the moon's rocky core (Postberg et al., 2009, 2011b). Jupiter's Galilean satellites Ganymede, Europa, and Callisto are also believed to have subsurface oceans and are therefore prime targets for future NASA and ESA outer Solar System missions. The Galilean moons are engulfed in tenuous dust clouds consisting of tiny pieces of the moons' surfaces (Kruger et al., 1999), released by hypervelocity impacts of micrometeoroids, which steadily bombard the surfaces of the moons. In situ chemical analysis of these grains by a high resolution dust spectrometer will provide spatially resolved mapping of the surface composition of Europa. Ganymede, and Callisto, meeting key scientific objectives of the planned missions. However, novel high-resolution reflectron-type dust mass spectrometers (Sternovsky et al., 2007; Srama et al., 2007) developed for dust astronomy missions (Gran et al., 2009) are probably not robust enough to be operated in the energetic radiation environment of the inner Jovian system. In contrast, CDA's linear spectrometer is much less affected by harsh radiation conditions because its ion detector is not directly facing out into space. The instrument has been continuously operated on Cassini for 11 years. In this paper we investigate the possibility of operating a CDA-like instrument as a high resolution impact mass spectrometer. We show that such an instrument is capable of reliably identifying traces of organic and inorganic materials in the ice matrix of ejecta expected to be generated from the surfaces of the Galilean moons. These measurements are complementary, and in some cases superior, compared to other traditional techniques such as infrared remote sensing or in situ ion or neutral mass spectrometers.},
  language  = {en}
}
@article{Klettke2014,
  author    = {Klettke, Cornelia},
  title     = {Verzauberung (Madame de Sta{\"e}l)},
  series = {Rom r{\"u}ckw{\"a}rts : europ{\"a}ische {\"U}bertragungsschicksale},
  journal   = {Rom r{\"u}ckw{\"a}rts : europ{\"a}ische {\"U}bertragungsschicksale},
  editor    = {Kasper, Judith and Wild, Cornelia},
  publisher = {Fink},
  address   = {M{\"u}nchen},
  isbn      = {978-3-7705-5849-0},
  pages     = {210 -- 214},
  year      = {2014},
  language  = {de}
}