Operational challenges of retinal prostheses.

Two computational models for research on retinal implants are presented. In the first model, the electric field produced by a multi-electrode array in a uniform retina is calculated. It is shown how cross talk of activated electrodes and the resulting bunching of field lines in monopole and dipole activation prevent high resolution imaging with retinal implants. Furthermore, it is demonstrated how sequential stimulation and multipolar stimulation may overcome this limitation. In the second model a target volume, i.e., a probe cylinder approximating a bipolar cell, in the retina is chosen, and the passive Heaviside cable equation is solved inside this target volume to calculate the depolarization of the cell membrane. The depolarization as a function of time indicates that shorter signals stimulate better as long as the current does not change sign during stimulation of the retina, i.e., mono-phasic stimulation. Both computational models are equally applicable to epiretinal, subretinal, and suprachoroidal vision implants.

Comparison of protocols for DNA extraction from long-term preserved formalin fixed tissues.

The current study compared the applicability of protocols to extract DNA from formalin fixed heart tissues that have been preserved for more than 50 years. Ten methods were tested: a cetyltrimethylammonium bromide (CTAB) standard protocol, seven variants of this standard protocol, and two commercial kits. In the case of younger specimens (fixed in 1951, 1934, or 1914), extracts with DNA concentrations ≥ 10.0 ng/µl were obtained with the standard CTAB protocol, two variants of the standard protocol including prolonged tissue digestion (72 h instead of 1-2h), and a commercial kit particularly recommended for DNA extraction from formalin fixed paraffin embedded tissues (FFPE Kit). With the FFPE Kit, DNA could also be extracted from older tissues (fixed in 1893, 1850/1851, or before 1820). In general, the purity of the DNA extracts, assessed from the ratio of the absorbance at 260 and 280 nm, was not very high. In spite of their rather low purity, the DNA extracts could, however, be used to amplify a 122-bp sequence and, in most cases, also a 171-bp sequence of the gene coding for human albumin by the polymerase chain reaction (PCR).

QCM array for on-line-monitoring of composting procedures.

Six QCM resonators forming a sensor array were coated with different molecularly imprinted polymers for the on-line monitoring of composting procedures. Four key analytes are traced, namely water, 1-propanol, ethyl acetate and limonene. Trendlines obtained on-line by the sensor during measurements in a commercial composter give a distinct pattern: the signal for the alcohols first decreases according to an increase in ethyl acetate concentration, and increases again, when obviously no more acetic acid is formed. Limonene is detected in later stages of composting. Similar trends could also be observed by GC-MS. Additionally, chromatographic and sensor data for limonene could be correlated with each other.

Assignment of quinone derivatives as the main compound class composing 'interstellar' grains based on both polarity ions detected by the 'Cometary and Interstellar Dust Analyser' (CIDA) onboard the spacecraft STARDUST.

The 'Cometary and Interstellar Dust Analyser' (CIDA) is a particle impact time-of-flight mass spectrometer onboard the NASA spacecraft STARDUST. A series of positive and negative ion mass spectra from the impact of (apparently) interstellar dust particles has been collected since 1999. In the meantime laboratory work has been performed to better understand the ion formation processes of organic grains impacting at those speeds (>15 km/s) and to relate them to some other ion formation methods. The key ion types were the negative ions, with some additional information from the positive ions. Here, first the principal ion formation rules are briefly reviewed. Secondly, the common substance class is inferred mainly by the application of exclusion principles, and appears to be partly condensed aromatic and quinonoid compounds with high oxygen and low nitrogen content. Oxygen appears to be present in quinone-type structures with condensed aromatic rings, possibly with furan substructures and some hydroxyl moieties. Some nitrogen may be present in pyrrole- or quinoline-type structures. Considerations of thermodynamics and radiation physics of these dust particles within the solar system are consistent with this interpretation. Quinoenzyme cofactors such as the known compound pyrroloquinoline-quinone (PQQ) and its subconstituents would be expected to yield similar mass spectra.