ORAL MUCOSITIS PREVENTION BY LOW-LEVEL LASER THERAPY IN HEAD-AND-NECK CANCER PATIENTS UNDERGOING CONCURRENT CHEMORADIOTHERAPY: A PHASE III RANDOMIZED STUDY

Purpose: Oral mucositis is a major complication of concurrent chemoradiotherapy (CRT) in head-and-neck cancer patients. Low-level laser (LLL) therapy is a promising preventive therapy. We aimed to evaluate the efficacy of LLL therapy to decrease severe oral mucositis and its effect on RT interruptions. Methods and Materials: In the present randomized, double-blind, Phase III study, patients received either gallium-aluminum-arsenide LLL therapy 2.5 J/cm(2) or placebo laser, before each radiation fraction. Eligible patients had to have been diagnosed with squamous cell carcinoma or undifferentiated carcinoma of the oral cavity, pharynx, larynx, or metastases to the neck with an unknown primary site. They were treated with adjuvant or definitive CRT, consisting of conventional RT 60-70 Gy (range, 1.8-2.0 Gy/d, 5 times/wk) and concurrent cisplatin. The primary endpoints were the oral mucositis severity in Weeks 2, 4, and 6 and the number of RT interruptions because of mucositis. The secondary endpoints included patient-reported pain scores. To detect a decrease in the incidence of Grade 3 or 4 oral mucositis from 80% to 50%, we planned to enroll 74 patients. Results: A total of 75 patients were included, and 37 patients received preventive LLL therapy. The mean delivered radiation dose was greater in the patients treated with LLL (69.4 vs. 67.9 Gy, p = .03). During CRT, the number of patients diagnosed with Grade 3 or 4 oral mucositis treated with LLL vs. placebo was 4 vs. 5 (Week 2, p = 1.0), 4 vs. 12 (Week 4, p = .08), and 8 vs. 9 (Week 6, p = 1.0), respectively. More of the patients treated with placebo had RT interruptions because of mucositis (6 vs. 0, p = .02). No difference was detected between the treatment arms in the incidence of severe pain. Conclusions: LLL therapy was not effective in reducing severe oral mucositis, although a marginal benefit could not be excluded. It reduced RT interruptions in these head-and-neck cancer patients, which might translate into improved CRT efficacy. (C) 2012 Elsevier Inc.

Effects of 830 and 670 nm Laser on Viability of Random Skin Flap in Rats

Objective: This study aimed to investigate the effect of 830 and 670 nm diode laser on the viability of random skin flaps in rats. Background data: Low-level laser therapy (LLLT) has been reported to be successful in stimulating the formation of new blood vessels and reducing the inflammatory process after injury. However, the efficiency of such treatment remains uncertain, and there is also some controversy regarding the efficacy of different wavelengths currently on the market. Materials and methods: Thirty Wistar rats were used and divided into three groups, with 10 rats in each. A random skin flap was raised on the dorsum of each animal. Group 1 was the control group, group 2 received 830 nm laser radiations, and group 3 was submitted to 670 nm laser radiation (power density = 0.5 mW/cm(2)). The animals underwent laser therapy with 36 J/cm(2) energy density (total energy = 2.52 J and 72 sec per session) immediately after surgery and on the 4 subsequent days. The application site of laser radiation was one point at 2.5 cm from the flap's cranial base. The percentage of skin flap necrosis area was calculated on the 7th postoperative day using the paper template method. A skin sample was collected immediately after to determine the vascular endothelial growth factor (VEGF) expression and the epidermal cell proliferation index (KiD67). Results: Statistically significant differences were found among the percentages of necrosis, with higher values observed in group 1 compared with groups 2 and 3. No statistically significant differences were found among these groups using the paper template method. Group 3 presented the highest mean number of blood vessels expressing VEGF and of cells in the proliferative phase when compared with groups 1 and 2. Conclusions: LLLT was effective in increasing random skin flap viability in rats. The 670 nm laser presented more satisfactory results than the 830 nm laser.

Source of slow lithium atoms from Ne or H-2 matrix isolation sublimation

We have studied, via laser absorption spectroscopy, the velocity distribution of Li-7 atoms released from cryogenic matrices of solid neon or molecular hydrogen. The Li atoms are implanted into the Ne or H-2 matrices - grown onto a sapphire substrate - by laser ablation of a solid Li or LiH precursor. A heat pulse is then applied to the sapphire substrate sublimating the matrix together with the isolated atoms. With a NiCr film resistor deposited directly onto the sapphire substrate we are able to transfer high instantaneous power to the matrix, thus reaching a fast sublimation regime. In this regime the Li atoms can get entrained in the released matrix gas, and we were also able to achieve matrix sublimation times down to 10 mu s for both H-2 or Ne matrix, enabling us to proceed with the trapping of the species of our interest such as atomic hydrogen, lithium, and molecules. The sublimation of the H-2 matrix, with its large center-of-mass velocity, provides evidence for a new regime of one-dimensional thermalization. The laser ablated Li seems to penetrate the H-2 matrix deeper than it does in Ne. (C) 2012 American Institute of Physics. [http://dx.doi.org/10.1063/1.4704125]

Influenza delle caratteristiche quali-quantitative della luce da fonti artificiali sulla fisio-morfologia di piante verdi per interior landscaping

La conoscenza delle esigenze luminose (intensità, spettro, durata minima, massima ed ottimale del fotoperiodo di illuminazione) e della tolleranza alle condizioni degli interni delle piante ad uso decorativo, è di fondamentale importanza per una giusta tecnica di progettazione (dimensionamento e dislocazione dei punti luce) dell’indoor plantscaping. Il lungo periodo di condizionamento al quale queste piante vengono sottoposte, caratterizzato principalmente dalla scarsa disponibilità di luce naturale e dagli alti livelli di concentrazione di CO2 determina una forte influenza sui processi morfo-fisiologici. Il presente studio analizza il fattore luminoso ed è articolato su più punti quali; • caratterizzazione della riposta fotosintetica all’intensità luminosa di 21 delle principali specie a fogliame decorativo comunemente utilizzate nella realizzazione degli spazi verdi indoor, per stabilire quali siano i minimi ed ottimali livelli di PAR tali da garantire una fotosintesi netta positiva e nel complesso le condizioni di maggior benessere per le piante; • quantificazione dell’incremento fotosintetico netto dovuto ad una maggior concentrazione di CO2 negli interni rispetto alla concentrazione CO2 atmosferica esterna, all’aumentare dell’ intensità luminosa artificiale sulle precedenti specie; • monitoraggio dell’andamento delle attività fotosintetiche durante il periodo di illuminazione di 8 ore comunemente utilizzato in un interno ad uso lavorativo, a PAR costante e variabile in Ficus elastica e Dieffenbachia picta, al fine di stabilire quali possano essere le durate e le modalità di somministrazione della luce per rendere massima la fotosintesi netta riducendo al minimo i consumi energetici dovuti all’accensione delle lampade; • valutazione della risposta morfo-fisiologica e fotosintetica a modificazioni dello spettro luminoso mediante l’uso di LED monocromatici colorati ad emissione nel bianco, blu e rosso in Ficus benjamina e Iresine herbistii al fine di stabilire se questo tipo di lampade possano essere utilizzate come fonte integrativa e/o sostitutiva nella realizzazione degli spazi verdi interni. Vengono analizzati il punto si compensazione alla luce (g), il punto di saturazione alla luce (s), l’efficienza quantica (AQE), il punto di respirazione al buio (Rd) e la fotosintesi netta massima (A max) per (Aglaonema commutatum, Asplenium nidus, Anthurium andreanum, Begonia rex, Calathea luoise, Calathea veitchiana, Calathea rufibarba, Calathea zebrina, Codiaeum variegatum, Cthenanthe oppenheimiana, Dieffenbakia picta, Ficus benjamina, Ficus elatica, Ficus longifolia, Fittonia verschaffeltii, Iresine herbistii, Philodendron erubescens, Philodendron pertusum, Potos aureus, Spathiphillum wallisi, Syngonium podophillum ) e classificate le specie in funzione di Amax in quattro categorie; A max < 2 µmol CO2 m-2 s-1, A max compresa tra 2 e 4 µmol CO2 m-2 s-1, Amax cpmpresa tra 4 e 6 µmol CO2 m-2 s-1, Amax > 6 µmol CO2 m-2 s-1, al fine di mettere in risalto la potenzialità fotosintetiche di ogni singola specie. I valori di PAR compresi tra (g) ed (s) forniscono le indicazioni sulle quali basarsi per scegliere una giusta lampada o dimensionare un punto luce per ogni singola specie e/o composizione. È stimata l’influenza di due livelli di concentrazione di CO2 ambientale (400 e 800 ppm) all’incrementare dell’intensità luminosa sul processo fotosintetico delle specie precedenti. Per quasi tutte le specie 800 ppm di CO2 non favoriscono nessun incremento all’attività fotosintetica ad eccezione di Ficus benjamina, Ficus elatica e Syngonium podophillum se non accompagnati da una disponibilità luminosa superiore alle 10 µmol m-2 s-1. Viene monitorato l’andamento dell’attività fotosintetica a PAR costante e variabile (intervallando periodi di 8 minuti a PAR 40 e 80) durante 8 ore di illuminazione su Ficus elastica e Dieffenbachia picta al fine di stabilire la miglior modalità di somministrazione della luce. La fotosintesi netta cumulativa per l’intera durata di illuminazione a PAR costante mostra un calo dopo alcune ore dall’attivazione in Dieffenbackia, e un andamento oscillatorio in Ficus. L’illuminazione alternata consente di raggiungere i quantitativi di CO2 organicata a 80 µmol m-2 s-1 di PAR, dopo 5 ore e mezza sia in Ficus che Dieffenbackia sebbene le potenzialità fotosintetiche delle due piante siano molto differenti. È stato valutato l’effetto dell’illuminazione artificiale mediante LED (15W) a luce bianca, blu e rossa monocromatica in rapporto alla luce neon(36W) bianca tradizionale (con differenti abbinamenti tra le lampade) sui principali parametri morfologici e fisiologici, in Ficus benjamin ‘Variegata’ e Iresine herbistii per verificare se tali fonti possono rappresentare una valida alternativa nella sostituzione o integrazione di altre lampade per gli spazi verdi indoor. Tutte le combinazioni LED indagate possono rappresentare un’alternativa di sostituzione alla coltivazione con neon ed un risparmio energetico di oltre il 50%. Una PAR di 20,6 µmol m-2 s-1 della singola lampada LED bianco è sufficiente per mantenere la pianta in condizioni di sopravvivenza con un consumo di 15W a fronte dei 36W necessari per il funzionamento di ogni neon. La combinazione LED bianco + LED blu monocromatico favorisce il contenimento della taglia della pianta, caratteristica gradita nella fase di utilizzo indoor, una maggior produzione di sostanza secca e un’attività fotosintetica più elevata.

Produkte der solaren kosmischen Strahlung in Meteoriten

In dieser Arbeit wurde der Aufbau und der Einsatz einer Laser-Extraktionsanlage für Edelgase dargestellt. Diese neue Anlage stellt eine Erweiterung eines bereits bestehenden Edelgas-Massenspektrometers dar. Ein Großteil der Arbeit befasste sich mit dem Aufbau und der Abschätzung der Einsatzmöglichkeiten. Erste Untersuchungen waren Tiefenprofile an Meteoriten. Dabei stand die Unterscheidung der zwei Komponenten der kosmischen Strahlung im Mittelpunkt. Es ist erstmalig gelungen einen Beitrag zur Produktion von stabilen Nukliden durch die 'solare kosmische Strahlung' direkt nachzuweisen. Ebenfalls konnten die zwei unterschiedlichen Komponenten gegeneinander abgeschätzt und eine zweistufige Bestrahlung belegt werden. An Hand eines zweistufigen Modells wurde gezeigt, dass der Nachweis eines SCR-Beitrags durch Radionuklide deutlicher ausfallen muss, als der über stabile Nuklide. Der direkte Nachweis durch die Analyse der Neon-Isotope ist somit bei einer 'ungewöhnlichen' Bestrahlungsgeschichte erfolgt. Die empirischen Produktionsraten (Eugster) wurden so interpretiert, dass sie eine Superposition der Produkte aus galaktischer- und solarer kosmischer Strahlung darstellen, welche von den 'theoretischen' Modellen vorhergesagt werden.

Kalorimetrische Tieftemperaturdetektoren für niederenergetische (E 1 MeV/amu) Schwerionen und ihr erster Einsatz in der Beschleuniger-Massenspektrometrie zur Spurenanalyse von 236 U

Im Rahmen der vorliegenden Arbeit wurden zum ersten Mal kalorimetrische Tieftemperatur-Detektoren in der Beschleuniger-Massenspektrometrie (Accelerator Mass Spectrometry AMS), einer Standard-Methode zur Bestimmung kleinster Isotopenverhältnisse, eingesetzt, um das Isotopenverhältnis von 236U zu 238U zu bestimmen. Das Uran-Isotop 236U entsteht in der Neutroneneinfang-Reaktion 235U(n,gamma)236U und kann daher als Monitor-Nuklid für Neutronenflüsse verwendet werden. Die Detektoren bestehen aus einem Saphir-Absorber, auf den ein supraleitender Aluminium-Film aufgedampft ist, der als Thermistor dient. Ein energetisches Schwerion deponiert seine kinetische Energie als Wärme im Absorber, dessen Temperaturänderung durch die Widerstandsänderung des Supraleiters nachgewiesen wird. Mit solchen Detektoren konnte in vorhergehenden Experimenten bei GSI in einem Energiebereich von E = 5 - 300 MeV/amu für eine Vielzahl von Ionen von Neon bis Uran eine relative Energieauflösung von (1 - 4) E-3 erreicht werden. Der für die Beschleuniger-Massenspektrometrie typische Energiebereich liegt bei E = 0.1 - 1 MeV/amu. Im ersten Schritt wurde daher die systematische Untersuchung der Detektoreigenschaften auf diesen Energiebereich ausgedehnt. Diese Untersuchungen sowie die AMS-Messungen wurden am Tandem-Beschleuniger VERA des Instituts für Isotopenforschung und Kernphysik der Universität Wien durchgeführt. In einem Energiebereich von 10 - 60 MeV konnte für verschiedene Ionen (13C, 197Au, 238U) zunächst eine relative Energieauflösung von DeltaE/E = 7 E-3 erreicht werden. Dies übertrifft die Auflösung konventioneller Ionisations-Detektoren um ca. eine Größenordnung. Durch eine Verbesserung thermischer und elektronischer Rauschbeiträge konnte in einem zweiten Experiment für Uran der Energie 17 MeV die Auflösung auf DeltaE/E = 4.6 E-3 verbessert werden. Die Energie-Response des Detektors war linear über den gesamten beobachteten Energiebereich und unabhängig von der Ionenmasse; bis auf ein Niveau von 0.1 % wurde kein Pulshöhendefekt beobachtet. Diese Ergebnisse zeigen, daß solche Detektoren ein wertvolles Werkzeug in der Schwerionenphysik im Bereich relativ niedriger Ionenenergien darstellen. Mit der erreichten Energieauflösung war es möglich, für mehrere Proben aus natürlichem Uran das Isotopenverhältnis 236U/238U zu bestimmen: Um einen Material-Standard für Uran in der AMS zu etablieren, wurde das Isotopenverhältnis 236U/238U für zwei Proben aus der Mine ''K.u.K. Joachimsthal'' möglichst präzise bestimmt. Die Ergebnisse in der vorliegenden Arbeit stimmen gut mit früheren Messungen überein, die mit einem konventionellen Detektorsystem durchgeführt wurden. Sowohl der statistische als auch der systematische Fehler konnten deutlich reduziert werden. Für eine weitere Probe, extrahiert aus dem Wasser einer Uran-haltigen Quelle in Bad Gastein, wurde ein Isotopenverhältnis von 6.1 E-12 gemessen. Dies stellt das kleinste bislang für 236U/238U gemessene Isotopenverhältnis dar und bedeutet eine Steigerung der Sensitivität um eine Größenordnung. Die erreichte Energieauflösung ermöglicht es außerdem, die Detektoren zur direkten Massenidentifikation von schweren Ionen mittels einer kombinierten Energie-Flugzeit-Messung einzusetzen. In ersten Test-Messungen im Rahmen der vorliegenden Arbeit wurde eine Massenauflösung von DeltaM/M = (8.5 - 11.0) E-3 erreicht. In einem ersten Test für den Einsatz dieser Detektoren zum Nachweis sog. ''superschwerer Elemente (Z >= 112)'' erlaubte der große dynamische Bereich, die Reaktionsprodukte und ihre nachfolgenden Alpha-Zerfälle mit hoher Energieauflösung simultan und zeitaufgelöst nachzuweisen.

Ein neuartiges Interferometer zur Messung magneto-optischer Effekte an L-Absorptionskanten von ferromagnetischen Metallen mit linearpolarisierter Undulatorstrahlung

Am Mainzer Mikrotron MAMI wurde ein neuartiges Interferometer entwickelt und getestet, mit dem magneto-optische Effekte an dünnen, freitragenden Folien von 3d-Übergangsmetallen wie Eisen, Kobalt oder Nickel an den L_{2,3}-Absorptionskanten (im Spektralbereich der weichen Röntgenstrahlung) gemessen werden können. Es handelt sich um eine Weiterentwicklung eines an MAMI erprobten Interferometers, das im wesentlichen aus einer kollinearen Anordnung zweier identischer Undulatoren, zwischen die die dünne Probefolie eingebracht wird, und einem Gitterspektrometer besteht. Aus den als Funktion des Abstands der Undulatoren beobachtbaren Intensitätsoszillation lassen sich das Dekrement des Realteils δ und der Absorptionskoeffizient β des komplexen Brechungsindex bestimmen.rnIm Rahmen der vorliegenden Arbeit wurde die Apparatur derart weiterentwickelt, dass auch die magnetisch zirkulare Doppelbrechung Δδ und der magnetisch zirkulare Dichroismus Δβ an den L_{2,3}-Absorptionskanten von Übergangsmetallen gemessen werden können. Der zweite Undulator wurde um die Elektronenstrahlachse um den Winkel Ψ = ±107° drehbar gemacht. Damit dient er auch als Analysator der aus der Folie austretenden elliptisch polarisierten weichen Röntgenstrahlung, für die - wie bei der Faraday-Rotation - die Polarisationsebene gedreht ist. Weiterhin kann die Spaltbreite der 10-poligen Hybrid-Undulatoren mit einer Periodenlänge von 12 mm und damit der Undulatorparameter über eine Antriebsmechanik kontinuierlich variiert werden, wodurch eine optimale Anpassung der Amplituden der Undulatorstrahlung aus den beiden Undulatoren möglich wird. Der maximale Undulatorparameter beträgt K = 1.1. Auch das Spektrometer, das auf einem selbstfokussierenden Gitter mit variierter Liniendichte (im Mittel 1400 Linien / mm) basiert, wurde weiterentwickelt. Als Detektor kommt jetzt eine fensterlose CCD mit 1024 x 1024 Pixeln und einer Pixelgröße von 13 μm x 13 μm zum Einsatz, die im Bildmodus betrieben wird, was die gleichzeitige Messung eines Energieintervalls von ca. 50 eV ermöglicht. Die totale Linienbreite wurde bei einer vertikalen Strahlfleckausdehnung von σ_y = 70 μm (rms) am Neon 1s-3p Übergang bei (867.18 ±0.02) eV zu Δħω = (0.218 ±0.002) eV (FWHM) gemessen. Das hohe Auflösungsvermögen von 4000 und die Möglichkeit der Eichung gegen den 1s-3p Übergang von Neon wurden ausgenutzt, um die Energie der Maxima an den Absorptionskanten von Nickel (weiße Linien) neu zu bestimmen. Die Ergebnisse E_{L_2}=(869.65_{-0.16}^{+0.27}) eV und E_{L_3}=(852.37_{-0.11}^{+0.16}) eV stellen eine Verbesserung früherer Messungen dar, die große Streuungen aufwiesen.rnAus systematischen Messungen als Funktion des Abstandes der Undulatoren und des Drehwinkels Ψ wurden die magnetisch zirkulare Doppelbrechung Δδ im Energiebereich 834 eV ≤ ħω ≤ 885 eV an einer freitragenden, bis zur Sättigung magnetisierten Nickelfolie der Dicke von (96.4 ±2.7) nm gemessen. Sowohl das Auflösungsvermögen als auch die Genauigkeit der Messungen für Δδ übersteigen bekannte Literaturangaben signifikant, so dass eine bisher nicht bekannte Feinstruktur gefunden werden konnte. Außerdem wurde der Betrag des magnetisch zirkularen Dichroismus |Δβ| im Bereich des Maximums an der L_3-Absorptionskante mit hoher Genauigkeit gemessen.rn

The Genesis Solar Wind Concentrator: Flight and Post-Flight Conditions and Modeling of Instrumental Fractionation

The Genesis mission Solar Wind Concentrator was built to enhance fluences of solar wind by an average of 20x over the 2.3 years that the mission exposed substrates to the solar wind. The Concentrator targets survived the hard landing upon return to Earth and were used to determine the isotopic composition of solar-wind—and hence solar—oxygen and nitrogen. Here we report on the flight operation of the instrument and on simulations of its performance. Concentration and fractionation patterns obtained from simulations are given for He, Li, N, O, Ne, Mg, Si, S, and Ar in SiC targets, and are compared with measured concentrations and isotope ratios for the noble gases. Carbon is also modeled for a Si target. Predicted differences in instrumental fractionation between elements are discussed. Additionally, as the Concentrator was designed only for ions ≤22 AMU, implications of analyzing elements as heavy as argon are discussed. Post-flight simulations of instrumental fractionation as a function of radial position on the targets incorporate solar-wind velocity and angular distributions measured in flight, and predict fractionation patterns for various elements and isotopes of interest. A tighter angular distribution, mostly due to better spacecraft spin stability than assumed in pre-flight modeling, results in a steeper isotopic fractionation gradient between the center and the perimeter of the targets. Using the distribution of solar-wind velocities encountered during flight, which are higher than those used in pre-flight modeling, results in elemental abundance patterns slightly less peaked at the center. Mean fractionations trend with atomic mass, with differences relative to the measured isotopes of neon of +4.1±0.9 ‰/amu for Li, between -0.4 and +2.8 ‰/amu for C, +1.9±0.7‰/amu for N, +1.3±0.4 ‰/amu for O, -7.5±0.4 ‰/amu for Mg, -8.9±0.6 ‰/amu for Si, and -22.0±0.7 ‰/amu for S (uncertainties reflect Monte Carlo statistics). The slopes of the fractionation trends depend to first order only on the relative differential mass ratio, Δ m/ m. This article and a companion paper (Reisenfeld et al. 2012, this issue) provide post-flight information necessary for the analysis of the Genesis solar wind samples, and thus serve to complement the Space Science Review volume, The Genesis Mission (v. 105, 2003).

Noble gas, CFC and other geochemical evidence for the age and origin of the Bath thermal waters, UK

The city of Bath is a World Heritage site and its thermal waters, the Roman Baths and new spa development rely on undisturbed flow of the springs (45 °C). The current investigations provide an improved understanding of the residence times and flow regime as basis for the source protection. Trace gas indicators including the noble gases (helium, neon, argon, krypton and xenon) and chlorofluorocarbons (CFCs), together with a more comprehensive examination of chemical and stable isotope tracers are used to characterise the sources of the thermal water and any modern components. It is shown conclusively by the use of 39Ar that the bulk of the thermal water has been in circulation within the Carboniferous Limestone for at least 1000 years. Other stable isotope and noble gas measurements confirm previous findings and strongly suggest recharge within the Holocene time period (i.e. the last 12 kyr). Measurements of dissolved 85Kr and chlorofluorocarbons constrain previous indications from tritium that a small proportion (<5%) of the thermal water originates from modern leakage into the spring pipe passing through Mesozoic valley fill underlying Bath. This introduces small amounts of O2 into the system, resulting in the Fe precipitation seen in the King’s Spring. Silica geothermometry indicates that the water is likely to have reached a maximum temperature of between 69–99 °C, indicating a most probable maximum circulation depth of ∼3 km, which is in line with recent geological models. The rise to the surface of the water is sufficiently indirect that a temperature loss of >20 °C is incurred. There is overwhelming evidence that the water has evolved within the Carboniferous Limestone formation, although the chemistry alone cannot pinpoint the geometry of the recharge area or circulation route. For a likely residence time of 1–12 kyr, volumetric calculations imply a large storage volume and circulation pathway if typical porosities of the limestone at depth are used, indicating that much of the Bath-Bristol basin must be involved in the water storage.

Cool Glacial Temperatures and Changes in Moisture Source Recorded in Oman Groundwaters

Concentrations of atmospheric noble gases (neon, argon, krypton, and xenon) dissolved in groundwaters from northern Oman indicate that the average ground temperature during the Late Pleistocene (15,000 to 24,000 years before present) was 6.5° ± 0.6°C lower than that of today. Stable oxygen and hydrogen isotopic groundwater data show that the origin of atmospheric water vapor changed from a primarily southern, Indian Ocean source during the Late Pleistocene to a dominantly northern, Mediterranean source today. The reduced northern water vapor source is consistent with a drier Last Glacial Maximum through much of northern Africa and Arabia.

NonViral Gene Delivery of Growth and Differentiation Factor 6 (GDF6) to whole bovine Intervertebral Disc

Question: Low back pain is an increasing global health problem, which is associated with intervertebral disc (IVD) damage and de- generation. Major changes occur in the nucleus pulposus (NP), with the degradation of the extracellular matrix (ECM) [1]. Further studies showed that growth factors from the transforming growth factor (TGF) and bone morphogenic proteins (BMP) family may induce chondrogenic differentiation of mesenchymal stem cells (MSC) [2]. Focusing on non-viral gene therapies and their possible translation into the clinics, we investigated if GDF6 (syn. BMP13 or CDMP2) can induce regeneration of degraded NP. We hypothesized that IVD transfected with plasmid over-expressing GDF6 also up-regulates other NP- and chondrogenic cell markers and enhances ECM deposition. Methods: Bovine IVD cells were isolated by pronase/collagenase II overnight digestion. After monolayer expansion up to passage 3, cells were transfected with the plasmid pGDF6 (RG211366, Origene, SF) or with green fluorescence protein (GFP) control using the NeonÒ transfection system (Invitrogen, Basel), both equipped with a Cy- tomegalovirus (CMV) promotor to induce over-expression. We tested a range of yet unpublished parameters for each of the primary disc cells to optimize efficiency. To test a non-viral gene therapy applied directly to 3D whole organ culture, bovine IVDs were harvested from fresh tails obtained from the abattoir within 5 h post-mortem [3]. Discs were then pre-incubated for 24 h in high glucose Dulbecco’s Modified Eagle Medium and 5 % fetal calf serum. Each disc was transfected by injection of 5 lg of plasmid GDF6 (Origene, RG211366) into the center by 25G needle and using Hamilton sy- ringe. Electroporation was performed using 2-needle array electrode or tweezertrodes; 8 pulses at 200mv/cm with an interval of 10 ms were applied using ECM830 Square Wave Electroporation System (Harvard Apparatus, MA) (Fig. 1). After transfection discs were cultured for 72 h to allow expression of GFP or GDF6. Discs were then fixed, cryosectioned and analysed by immunofluorescence against GDF6. Results: We successfully transfected bovine NP and AF cells in monolayer culture with the two plasmids using a 1,400 V, 20 ms and 2 pulses with a *25 % efficiency using 0.15 M cells and 3 lg DNA (Fig. 1). Organ IVD culture transfection revealed GFP6 positive staining in the centre of the disc using 2-needle array electrode. Results from tweezertrodes did not show any GFP posi- tive cells. Conclusions: We identified novel parameters to successfully transfect primary bovine IVD cells. For transfection of whole IVD explants electroporation parameters need to be further optimized. Acknowledgments: This study was supported by the Lindenhof Foundation ‘‘Forschung und Lehre’’ (Project no. 13-02-F). References 1. Roughly PJ (2004) Spine (Phila) 29:2691–2699 2. 3. Clarke LE, McConell JC, Sherratt MJ, Derby B, Richardson SM, Hoyland JA (2014) Arthritis Res Ther 16:R67 Chan SC, Gantenbein-Ritter B (2012) J Vis Exp 60(60):e3490