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Die Kometenmission Rosetta
DOI: 10.1002/piuz.201601453 Bibcode: 2016PhuZ...47..274K

Krüger, Harald

Die Rosetta-Mission ist ein Meilenstein in der Erforschung der Kometen und ihrer Entstehung. Eine der größten üerraschungen war die unregelmäßge hantelförmige Gestalt des Zielkometen 67P/Tschurjumow-Gerassimenko. Er besteht wahrscheinlich aus zwei Einzelkörpern, die durch ihre Schwerkraft aneinander gehalten werden. Seine Oberfläche ist sehr rau u…

2016 Physik in unserer Zeit
Rosetta 0
Cassini detects interstellar dust grains
Bibcode: 2016Sci...352Q.304S

Smith, Keith T.

2016 Science
Cassini 0
The Strategy and Implementation of the Rosetta Communication Campaign
Bibcode: 2016CAPJ...19....5B

Bauer, M.; McCaughrean, M.; Landeau-Constantin, J.

The communication campaign for Rosetta has been the biggest success in the history of European Space Agency outreach, resulting in global awareness for the agency. The mission itself is an extraordinary operational and scientific success, but communicating only the operational and scientific firsts would likely not have brought the Rosetta orbiter…

2016 Communicating Astronomy with the Public Journal
Rosetta 0
Analyzing the interstellar neutral He bulk flow parameters with IBEX-Lo
Bibcode: 2016PhDT........67L

Leonard, Trevor W.

Our Sun is immersed in a local galactic environment which is composed of a warm, dilute, and partially ionized gas. Due to the Sun's motion relative to this environment, the interstellar neutral (ISN) gas flows through the heliosphere providing the opportunity to perform in-situ observations of the ISN gas from Earth's orbit. The Interstellar Boun…

2016 Ph.D. Thesis
Ulysses 0
Inflow Generated X-Ray Corona around Supermassive Black Holes and a Unified Model for X-Ray Emission
DOI: 10.3847/0004-637X/817/2/99 Bibcode: 2016ApJ...817...99W

Cen, Renyue; Wang, Lile

Three-dimensional hydrodynamic simulations are performed, which cover the spatial domain from hundreds of Schwarzschild radii to 2 pc around the central supermassive black hole of mass {10}8{M}, with detailed radiative cooling processes. The existence of a significant amount of shock heated, high temperature (≥slant {10}

2016 The Astrophysical Journal
INTEGRAL 0
Building the analytical response in frequency domain of AC biased bolometers. Application to Planck/HFI
DOI: 10.1007/s10686-016-9514-1 Bibcode: 2016ExA....42..361S

Montier, Ludovic; Sauvé, Alexandre

Context: Bolometers are high sensitivity detector commonly used in Infrared astronomy. The HFI instrument of the Planck satellite makes extensive use of them, but after the satellite launch two electronic related problems revealed critical. First an unexpected excess response of detectors at low optical excitation frequency for ν < 1 Hz, and se…

2016 Experimental Astronomy
Planck 0
Refinement of Stereo Image Analysis Using Photometric Shape Recovery as AN Alternative to Bundle Adjustment
DOI: 10.5194/isprs-archives-XLI-B4-565-2016 Bibcode: 2016ISPAr41B4..565G

Mall, U.; Wöhler, C.; Grumpe, A. +3 more

Topographic mapping, e.g. the generation of Digital Elevation Models (DEM), is of general interest to the remote sensing community and scientific research. Commonly, photogrammetric methods, e.g. stereo image analysis methods (SIAM) or bundle adjustment methods (BAM), are applied to derive 3D information based on multiple images of an area. These …

2016 ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences
Rosetta 0
An Historic Encounter: Reviewing the Outreach around ESA's Rosetta Mission
Bibcode: 2016CAPJ...19...44L

Lorenzen, D.

The Rosetta mission is a milestone in terms of science and public outreach. The European Space Agency and the Deutsches Zentrum für Luft- und Raumfahrt in particular did a marvellous job of sparking global public interest, driven by various events throughout the mission. In contrast, the actions of the Max Planck Society research group in charge o…

2016 Communicating Astronomy with the Public Journal
Rosetta 0
Observations of long-period oscillations of the solar active regions in the visible and UV spectral intervals
DOI: 10.1134/S001679321607015X Bibcode: 2016Ge&Ae..56..872T

Tlatov, A. G.; Dormidontov, D. V.; Chernov, Ya. O.

The variation of intensity in spectral line wings, which was obtained from observations of the patrol telescope at the Kislovodsk Mountain Astronomical Station of the Pulkovo Observatory, Russian Academy of Science (KMAS) and the Interface Region Imaging Spectrograph (IRIS) space observatory, are considered. A series of observations lasting a few …

2016 Geomagnetism and Aeronomy
IRIS 0
Spectral energy distribution, radio maps and polarization of Cygnus X-1: a lepto-hadronic model
Bibcode: 2016BAAA...58..240V

Romero, G. E.; Vila, G. S.; Pepe, C.

The microquasar Cygnus X-1 is one of the most studied astrophysical sources. Several radiative models for the non-thermal broadband emission of Cygnus X-1 are available. For the jet emission in particular, only leptonic models have been considered despite the observational evidence of the presence of hadrons in the jets of other microquasars. In t…

2016 Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
INTEGRAL 0