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Die Hämophilie A und B, die häufigsten plasmatischen Gerinnungsstörungen, beruhen auf dem Defekt des Gerinnungsfaktors VIII bzw. IX. Eine Ausbildung von FVIII- bzw. FIX neutralisierenden Antikörpern (Inhibitoren) ist heute die bedeutendste und schwerwiegendste Nebenwirkung bei der Behandlung der Patienten mit FVIII/FIX-Präparaten. Ungefähr 25-30% der schwer erkrankten Hämophilie A-Patienten (FVIII-Aktivität < 1%) entwickeln Inhibitoren. Bei der Hämophilie B sind nur ca. 1-3% der Patienten von Inhibitoren betroffen. Ziel der Arbeit war es, die Einflußfaktoren der Inhibitorentwicklung zu ermitteln und mit anderen Studien zu vergleichen. Die für die Substitutionstherapie eingesetzten FVIII-Präparate werden entweder aus Spenderplasma gewonnen oder gentechnisch (rekombinant) hergestellt und durch verschiedene Verfahren virusinaktiviert. Eine Charakterisierung der Präparate zeigte leichte, aber unerhebliche Unterschiede zwischen einzelnen Chargen desselben Präparates. Unter Verwendung der FVIII-/FIX-Präparate wurde die Inhibitorwirkung qualitativ und quantitativ nachgewiesen. Es wurde der Verlauf von Inhibitoren zum Schweregrad der Hämophilie, zur Art der verabreichten Präparate, zu der substitutierten Menge- auch bezogen auf das Körpergewicht- und zur Substitutionsfrequenz korreliert. Es konnte gezeigt werden, daß der Mutationstyp, die Dosierung und das Alter der Erstbehandlung die Inhibitorbildung beeinflussen können. Die Intron 22-Inversion verursacht in den meisten Fällen eine schwere Hämophilie A, und dabei werden auch am häufigsten Inhibitoren gebildet. Bei der Hämophilie B verursachen ausschließlich die große Deletion und Nonsensemutationen die Inhibitorentwicklung. Bei einem Vergleich der Inhibitorinzidenzen von r- und pdFVIII-Präparaten konnte kein signifikanter Unterschied gefunden werden, wie auch andere Studien zeigten. Eine Ausnahme stellt eine erst kürzlich vorgetragene retrospektive Studie aus Frankreich dar (Rothschild 2003). Durch Epitopemapping mit rekombinanten FVIII-Fragmenten konnten bestimmte Domänen des Proteines als ,,targetU der neutralisierenden und nicht-neutralisierenden Antikörper identifiziert werden. Auf der schweren Kette des FVIII-Proteines waren die Antikörper gegen die A2- und die Alal-Domänen gerichtet. Auf der leichten Kette waren die Antikörper gegen die C2-, a3A3- und C1-Domänen gerichtet. Zudem konnte gezeigt werden, dass inhibitorische und nicht-inhibitorische Antikörper vorwiegend gegen die schwere Kette (HC) des FVIII-Proteines gerichtet waren. 77 % der untersuchten Patienten zeigten eine Intron 22-Inversion. Dies verdeutlicht, daß diese Mutation einen hohen Risikofaktor hinsichtlich Inhibitor- und Antikörperbildung darstellt.
Heterodyne array receivers are employed in radio astronomy to reduce the observing time needed for mapping extended sources. One of the main factors limiting the amount of pixels in terahertz receivers is the difficulty of generating a sufficient amount of local oscillator power. Another challenge is efficient diplexing and coupling of local oscillator and signal power to the detectors. These problems are attacked in this dissertation by proposing the application of two vacuum electronic terahertz amplifier types for the amplification of the LO-signal and by introducing a new method for finding the defects in a quasioptical diplexer.
A traveling wave tube (TWT) design based on a square helix slow wave structure (SWS) at 825 GHz is introduced. It exhibits a simulated small-signal gain of 18.3 dB and a 3-dB bandwidth of 69 GHz. In order to generate LO-power at even higher frequencies, the operation of an 850-GHz square helix TWT as a frequency doubler has been studied. A simulated conversion efficiency of 7% to 1700 GHz, comparable with the state-of-art solid-state doublers, has been achieved for an input power of 25 mW.
The other amplifier type discussed in this work is a 1-THz cascade backward wave amplifier based on a double corrugated waveguide SWS. Specifically, three input/output coupler types between a rectangular waveguide and the SWS are presented. The structures have been realized with microfabrication, and the results of loss measurements at 1 THz will be shown.
Diplexing of the LO- and signal beams is often performed with a Martin-Puplett interferometer. Misalignment and deformation of the quasioptical components causes the polarization state of the output signal to be incorrect, which leads to coupling losses. A ray-tracing program has been developed for studying the influence of such defects. The measurement results of the diplexer of a multi-pixel terahertz receiver operated at the APEX telescope have been analyzed with the program, and the results are presented. The program allows the quasioptical configuration of the diplexer to be corrected in order to obtain higher receiver sensitivity.
"Werden" plays an important role in German, especially as a copula and as an auxiliary verb. It constitutes the analytic (periphrastic) part of the verbal paradigm being used as an auxiliary by encoding the categories of Tense (Future), Mood (Conditional), and Diathesis (Passive).
The original meaning of PIE *uuerth- includes two basic readings – a terminative and an aterminative. Both of them have been used in the process of grammaticalisation of werden in constructions with participles and the infinitive. The terminative reading based on the feature "Change of a State" was originally the categorical marker of "werden" within the opposition "sein" vs. "werden", where "sein" indicated the meaning of "State". As a result of the further development which started in the later OHG period, the aterminative reading of "werden" in constructions with the Participle II mixed with the terminative one by establishing the Passive-Paradigm. This evolution forced "sein"+ Part. II into the periphery of the Diathesis where in NHG it is marked as a resultative (terminative) construction. On the other hand, werden + Participle I (later with Infinitive) did not establish aterminative readings due to the peculiarities of the semantics of the Participle I – form. In connection with the Infinitive the terminativity of werden developed in the process of its auxiliarisation to the prospective I prognostic reading in the future-tense perspective and to the epistemic reading in the perspective of the present tense. In the perspective of the past tense (cf. MHG "ward varen" {became ride}, "was ridden") it disappeared because in this perspective prospective or prognostic readings are impossible.
Aus der Faktenlage ergeben sich folgende Probleme, die derzeit in der einschlägigen Literatur diskutiert werden bzw. bisher noch nicht zur Diskussion gelangt sind und die nun im vorliegenden Beitrag behandelt werden:
(i) Worauf sind Unterschiede in der Kodierung deontischer und epistemischer Lesarten von Modalverben durch (synthetische) Präsens- bzw. Präteritalformen und (analytische bzw. periphrastische) Perfekt- bzw. Plusquamperfektformen zurückzuführen? Worin liegt der genuine Beitrag des (periphrastischen) Perfekts/Plusquamperfekts bei der Manifestierung der kategorialen Funktion von Modalverben?;
(ii) Welches sind die Spezifika der Perfektformen von Modalverben in der Diachronie bzw.welchen kategorialen Wandel erfahren sie im Laufe ihrer Entwicklung?;
(iii) Wie ist die formale und funktionale Konstellation zwischen den Konstruktionen Modalverb + Infinitiv II und der Umschreibung würde + Infinitiv II synchron wie diachron zu beurteilen?;
(iv) Darf vor dem Hintergrund der Formenasymmetrie im Indikativ und Konjunktiv der Umschreibung werden + Inf. I/II (würde + Inf. I/II vs. *wurde + Inf. I/II) von einer "Lücke" im Verbalparadigma gesprochen werden?
In this study, two different methods were applied to derive daily and monthly sunshine duration based on high-resolution satellite products provided by the European Organisation for the Exploitation of Meteorological Satellites (EUMETSAT) Satellite Application Facility on Climate Monitoring using data from Meteosat Second Generation (MSG) SEVIRI (Spinning Enhanced Visible and Infrared Imager). The satellite products were either hourly cloud type or hourly surface incoming direct radiation. The satellite sunshine duration estimates were not found to be significantly different using the native 15-minute temporal resolution of SEVIRI. The satellite-based sunshine duration products give additional spatial information over the European continent compared with equivalent in situ-based products. An evaluation of the satellite sunshine duration by product intercomparison and against station measurements was carried out to determine their accuracy. The satellite data were found to be within ±1 h/day compared to high-quality Baseline Surface Radiation Network or surface synoptic observations (SYNOP) station measurements. The satellite-based products differ more over the oceans than over land, mainly because of the treatment of fractional clouds in the cloud type-based sunshine duration product. This paper presents the methods used to derive the satellite sunshine duration products and the performance of the different retrievals. The main benefits and disadvantages compared to station-based products are also discussed.
The aim of this study is a better understanding of radiation processes in regional climate models (RCMs) in order to quantify their impact and to reduce possible errors. A first important task in finding an answer to this question was to examine the accuracy of the components of the radiation budget in regional climate simulations. To this end, the simulated radiation budgets of two regional climate simulations for Europe were compared with a satellite-based reference. In the simulations with the RCM COSMO-CLM there were some serious under- and overestimations of short- and long-wave net radiation in Europe. However, taking into account the differences in the reference datasets, the results of the COSMO-CLM were quite satisfactory.
Using statistical methods, the influence of potential sources of uncertainties was estimated. Uncertainties in the cloud cover and surface albedo had a significant impact on uncertainties in short-wave net radiation, the explained variance of uncertainties in cloud cover was two to three times higher than that of uncertainties in surface albedo. Uncertainties in the cloud cover resulted in significant errors in the net long-wave radiation. However, the influence of uncertainties in soil temperature on errors in the long-wave radiation budget was low or even negligible. These results were confirmed in a comparison with simulations of the REMO and ALADIN regional climate models. It is reasonable to expect that a better parameterization of relatively simple parameters such as cloud cover and surface albedo is a means of significantly improving the simulation of radiation budget components in the COSMO-CLM.
An important question for the application of RCMs is to examine whether the results of radiation uncertainties and their impact factors are comparable if the model is applied in a region that is not the one for which it was originally created. Comparisons of the simulated radiation budgets of different RCMs for West Africa showed that problems in the simulation of short- and long-wave radiation fluxes were a widespread problem. Most of the tested models showed some considerable under- or overestimation of the short- and long-wave radiation fluxes.
Similar to Europe uncertainties in cloud cover were also in the simulations for Africa a significant factor affecting uncertainties in the simulated radiation fluxes. However, for the African simulations uncertainties in the parameterization of surface albedo were much more important than in Europe. On average, overland uncertainties in the cloud cover and surface albedo were of similar importance. Uncertainties in soil temperature simulations were of higher importance in Africa, and reached overland similar values of the mean explained variance (R2 ≈ 0.2) such as uncertainties in the cloud cover. This indicates a geographical dependence of the model error. This study confirmed the assumption that an improved parameterization of relatively simple parameters such as the surface albedo in RCMs leads to a significant improvement in the modeled radiation budget, particularly in Africa.
The influence of errors in the simulated radiation budget components on the simulation of climate processes, such as the West-African monsoon (WAM), was investigated in a next step. The evaluation of ERA-Interim and ECHAM5 driven COSMO-CLM simulations for Africa showed that the main features of the WAM were well reproduced by the model, but there were only slight improvements compared to the driving data. The index of convective activity in the model simulations was much too high and precipitation was underestimated in large parts of tropical Africa. The partly considerable differences between the ERA-Interim and ECHAM5 driven simulations demonstrated the sensitivity of the RCM to the boundary conditions and in particular to the sea surface temperature. An excessive northwards shift of the monsoon in the model was influenced by the land-sea temperature gradient and the strength of the Saharan heat low. Consequently, a part of the error was due to the driving data and the model itself produced another part.
By modifying the parameterization of the bare soil albedo the errors in the radiation budget and 2 m temperature in the Sahara region were significantly reduced. Similarly, the overesti-mation of precipitation and convection has been reduced in the Sahel. The effect of this modifi-cation on the examined WAM area was low. This confirmed that especially in desert regions, errors in the surface albedo were a driving factor for errors in the radiation budget. However, there are other important factors not yet sufficiently understood that have a strong influence on the quality of the simulation of the WAM.
The analysis of the actual state, the quantification of error sources and the highlighting of connections made it possible to find means to reduce uncertainties in the simulated radiation in RCMs and to have a better understanding of radiation processes. However, the magnitude of the errors found, the number of possible influencing factors, and the complexity of interactions, indicate that there is still a need for further research in this area.