Landschaftspläne in Europa: Status quo und Perspektiven konzeptioneller Landschaftspläne im europäischen Vergleich: Zusammenfassendes Ergebnispapier: Inspirierender Expertenaustausch über Landschaftsplanung: Expertenworkshop des BfN vom - 17.- 20.09.2008 an der Internationalen Naturschutzakademie Insel Vilm

Die Vortragenden wurden im Vorfeld gebeten folgende Aspekte zu berücksichtigen: 1. Wie sind "Landschaftspläne" in das Planungssystem ihres Landes eingebunden, d. h. wie ist ihr Verhältnis zur Raum-, Naturschutz-, Kultur- und Umweltplanung? 2. Was sind wichtige Inhalte a) der Analyse sowie b) der Entwicklungskonzeption der Pläne? Zugleich wurden die Referenten gebeten, einen guten oder erfolgreichen Landschaftsplan ihres Landes auszuwählen und diesen auf dem Workshop vorzustellen und zugänglich zu machen

X-ray full field microscopy at 30 KeV

In our X-ray full field microscopy experiments, we demonstrated a resolution better than 260 nm over the entire field of view of 80 μm x 80 μm at 30 keV. Our experimental setup at PETRA III, P05, had a length of about 5 m consisting of an illumination optics, an imaging lens and a detector. For imaging, we used a compound refractive lens (CLR) consisting of mr-L negative photo resist, which was fabricated by deep X-ray lithography. As illumination optics, we choose a refractive rolled X-ray prism lens, which was adapted to the numerical aperture of the imaging lens

Simulation of Ablating Hypersonic Vehicles with Finite-Rate Surface Chemistry

Peer Reviewedhttps://deepblue.lib.umich.edu/bitstream/2027.42/140434/1/6.2014-2124.pd

Efeitos de diferentes níveis de desfolha nos estádios vegetativo e reprodutivo sobre desenvolvimento da cultura da soja.

JIPE 2013

Eficiência de inseticidas, quando aplicados nas sementes de soja, associados ou não com produtos aplicados na parte aérea, no controle de pragas foliares na cultura.

JIPE 2013

Transit Timing Analysis in the HAT-P-32 system

We present the results of 45 transit observations obtained for the transiting exoplanet HAT-P-32b. The transits have been observed using several telescopes mainly throughout the YETI network. In 25 cases, complete transit light curves with a timing precision better than $1.4\:$min have been obtained. These light curves have been used to refine the system properties, namely inclination $i$, planet-to-star radius ratio $R_\textrm{p}/R_\textrm{s}$, and the ratio between the semimajor axis and the stellar radius $a/R_\textrm{s}$. First analyses by Hartman et al. (2011) suggest the existence of a second planet in the system, thus we tried to find an additional body using the transit timing variation (TTV) technique. Taking also literature data points into account, we can explain all mid-transit times by refining the linear ephemeris by 21ms. Thus we can exclude TTV amplitudes of more than $\sim1.5$min.Comment: MNRAS accepted; 13 pages, 10 figure

Transit Timing Analysis in the HAT-P-32 System

We present the results of 45 transit observations obtained for the transiting exoplanet HATP- 32b. The transits have been observed using several telescopes mainly throughout the YETI (Young Exoplanet Transit Initiative) network. In 25 cases, complete transit light curves with a timing precision better than 1.4 min have been obtained. These light curves have been used to refine the system properties, namely inclination i, planet-to-star radius ratio Rp/Rs, and the ratio between the semimajor axis and the stellar radius a/Rs. First analyses by Hartman et al. suggests the existence of a second planet in the system, thus we tried to find an additional body using the transit timing variation (TTV) technique. Taking also the literature data points into account, we can explain all mid-transit times by refining the linear ephemeris by 21 ms. Thus, we can exclude TTV amplitudes of more than ∼1.5min