scholarly journals Relative functional and optical absorption cross-sections of PSII and other photosynthetic parameters monitored in situ, at a distance with a time resolution of a few seconds, using a prototype light induced fluorescence transient (LIFT) device

2017 ◽  
Vol 44 (10) ◽  
pp. 985 ◽  
Author(s):  
Barry Osmond ◽  
Wah Soon Chow ◽  
Rhys Wyber ◽  
Alonso Zavafer ◽  
Beat Keller ◽  
...  

The prototype light-induced fluorescence transient (LIFT) instrument provides continuous, minimally intrusive, high time resolution (~2 s) assessment of photosynthetic performance in terrestrial plants from up to 2 m. It induces a chlorophyll fluorescence transient by a series of short flashes in a saturation sequence (180 ~1μs flashlets in <380 μs) to achieve near-full reduction of the primary acceptor QA, followed by a relaxation sequence (RQA; 90 flashlets at exponentially increasing intervals over ~30 ms) to observe kinetics of QA re-oxidation. When fitted by the fast repetition rate (FRR) model (Kolber et al. 1998) the QA flash of LIFT/FRR gives smaller values for FmQA from dark adapted leaves than FmPAM from pulse amplitude modulated (PAM) assays. The ratio FmQA/FmPAM resembles the ratio of fluorescence yield at the J/P phases of the classical O-J-I-P transient and we conclude that the difference simply is due to the levels of PQ pool reduction induced by the two techniques. In a strong PAM-analogous WL pulse in the dark monitored by the QA flash of LIFT/FRR φPSIIWL ≈ φPSIIPAM. The QA flash also tracks PQ pool reduction as well as the associated responses of ETR QA → PQ and PQ → PSI, the relative functional (σPSII) and optical absorption (aPSII) cross-sections of PSII in situ with a time resolution of ~2 s as they relax after the pulse. It is impractical to deliver strong WL pulses at a distance in the field but a longer PQ flash from LIFT/FRR also achieves full reduction of PQ pool and delivers φPSIIPQ ≈ φPSIIPAM to obtain PAM-equivalent estimates of ETR and NPQ at a distance. In situ values of σPSII and aPSII from the QA flash with smaller antenna barley (chlorina-f2) and Arabidopsis mutants (asLhcb2–12, ch1–3 Lhcb5) are proportionally similar to those previously reported from in vitro assays. These direct measurements are further validated by changes in antenna size in response to growth irradiance. We illustrate how the QA flash facilitates our understanding of photosynthetic regulation during sun flecks in natural environments at a distance, with a time resolution of a few seconds.

1997 ◽  
Vol 475 ◽  
Author(s):  
T. Duden ◽  
E. Bauer

ABSTRACTUltrathin epitaxial Co layers grown on Au(111) show strong perpendicular magnetic aniso-tropy resulting in out-of-plane magnetization in thin films. With increasing Co thickness the increasing contribution of the shape anisotropy leads to a reorientation transition of the magnetization which has already been subject of many other studies. In the dynamic in-situ experiments reported here bulk Au(111) is replaced by epitaxially grown Au(111)/W(110). The high time resolution (0.05 ML Co deposition per acquisition cycle) allows to extract several mechanisms which occur during the spin reorientation transition.


2006 ◽  
Vol 6 (6) ◽  
pp. 12671-12700
Author(s):  
R. J. Leigh ◽  
G. K. Corlett ◽  
U. Frieß ◽  
P. S. Monks

Abstract. A novel system using the technique of concurrent multi-axis differential optical absorption spectroscopy system has been developed and applied to the measurement of nitrogen dioxide in an urban environment. Using five fixed telescopes, slant columns of nitrogen dioxide, ozone, water vapour, and the oxygen dimer, O4, are simultaneously retrieved in five vertically separated viewing directions. The application of this remote sensing technique in the urban environment is explored. Through, the application of several simplifying assumptions a tropospheric concentration of NO2 is derived and compared with an urban background in-situ chemiluminescence detector. The remote sensing and in-situ techniques show good agreement. Owing to the high time resolution of the measurements, the ability to image and quantify plumes within the urban environment is demonstrated. The CMAX-DOAS measurements provide a useful measure of overall NO2 concentrations on a city-wide scale.


Author(s):  
Sophia Ruiz-Vásquez ◽  
Carlos Roldán ◽  
Vicky Cheng

Con el fin de apoyar de manera sostenible los múltiples sistemas de energía, las estrategiasde mejoramiento de sistemas de eficiencia energética implican la integración y aplicación deherramientas de análisis de energía urbanas. Los sistemas de energía, como la energía solarintermitente, requieren investigación sobre la capacidad de adaptación entre la demanda y laproducción. El análisis de coincidencia de energía requiere de fuentes de error mínimas, con elfin de obtener resultados más puntuales.En ciertas aplicaciones de simulación de energía, el intervalo de tiempo de uso común es deuna hora, sin embargo, estudios han demostrado que esto puede ser una fuente significativade error. Por ende, para la identificación del impacto que tiene la frecuencia temporal en lassimulaciones, se crearon modelos holísticos en alta resolución. Con estos modelos, se pretendela representación y obtención de resultados más precisos y exactos.El modelo de producción de energía fotovoltaica generada in-situ, se basa en un modelodesarrollado por el grupo de investigación Energy Effcient and Smart Cities (EESC). Datospertinentes, tales como la radiación incidente y la radiación global se obtuvieron del softwareMeteonorm. Para la elaboración del modelo de alta resolución de la demanda eléctricadoméstica, el modelo desarrollado por Centre for Renewable Energy Systems Technology ofLoughborough University, fue utilizado y modificado usando información pertinente de CostaRica.Estos modelos, implican módulos fotovoltaicos con producción energética in-situ y representanadecuadamente la demanda de electricidad doméstica. Por lo tanto, el cálculo de los análisisde la capacidad de adaptación de energía pudo ser efectuado. Dichos cálculos involucran losíndices OEF y OEM, que se refieren a la fracción de energía in situ y la coincidencia de energíaen las instalaciones, respectivamente. Mediante estos cálculos, se mostró que el uso de lasresoluciones más gruesas en el análisis de energía conduce a la sobreestimación, y a su vez elporcentaje de error incrementa.


2015 ◽  
Vol 14 (8) ◽  
pp. vzj2014.11.0169 ◽  
Author(s):  
Laura Gangi ◽  
Youri Rothfuss ◽  
Jerôme Ogée ◽  
Lisa Wingate ◽  
Harry Vereecken ◽  
...  

2020 ◽  
Vol 27 (5) ◽  
pp. 1339-1346 ◽  
Author(s):  
Silja Flenner ◽  
Malte Storm ◽  
Adam Kubec ◽  
Elena Longo ◽  
Florian Döring ◽  
...  

Hard X-ray nanotomography enables 3D investigations of a wide range of samples with high resolution (<100 nm) with both synchrotron-based and laboratory-based setups. However, the advantage of synchrotron-based setups is the high flux, enabling time resolution, which cannot be achieved at laboratory sources. Here, the nanotomography setup at the imaging beamline P05 at PETRA III is presented, which offers high time resolution not only in absorption but for the first time also in Zernike phase contrast. Two test samples are used to evaluate the image quality in both contrast modalities based on the quantitative analysis of contrast-to-noise ratio (CNR) and spatial resolution. High-quality scans can be recorded in 15 min and fast scans down to 3 min are also possible without significant loss of image quality. At scan times well below 3 min, the CNR values decrease significantly and classical image-filtering techniques reach their limitation. A machine-learning approach shows promising results, enabling acquisition of a full tomography in only 6 s. Overall, the transmission X-ray microscopy instrument offers high temporal resolution in absorption and Zernike phase contrast, enabling in situ experiments at the beamline.


2016 ◽  
Vol 819 (2) ◽  
pp. 126 ◽  
Author(s):  
U. Mall ◽  
K. Altwegg ◽  
H. Balsiger ◽  
A. Bar-Nun ◽  
J.-J. Berthelier ◽  
...  

2007 ◽  
Vol 7 (18) ◽  
pp. 4751-4762 ◽  
Author(s):  
R. J. Leigh ◽  
G. K. Corlett ◽  
U. Frieß ◽  
P. S. Monks

Abstract. A novel system using the technique of concurrent multi-axis differential optical absorption spectroscopy system has been developed and applied to the measurement of nitrogen dioxide in an urban environment. Using five fixed telescopes, slant columns of nitrogen dioxide, ozone, water vapour, and the oxygen dimer, O4, are simultaneously retrieved in five vertically separated viewing directions. The application of this remote sensing technique in the urban environment is explored. Through the application of several simplifying assumptions a tropospheric concentration of NO2 is derived and compared with an urban background in-situ chemiluminescence detector. Trends derived from remote sensing and in-situ techniques show agreement to within 15 to 40% depending on conditions. Owing to the high time resolution of the measurements, the ability to image and quantify plumes within the urban environment is demonstrated. The CMAX-DOAS measurements provide a useful measure of overall NO2 concentrations on a city-wide scale.


1994 ◽  
Vol 144 ◽  
pp. 431-434
Author(s):  
M. Minarovjech ◽  
M. Rybanský

AbstractThis paper deals with a possibility to use the ground-based method of observation in order to solve basic problems connected with the solar corona research. Namely:1.heating of the solar corona2.course of the global cycle in the corona3.rotation of the solar corona and development of active regions.There is stressed a possibility of high-time resolution of the coronal line photometer at Lomnický Peak coronal station, and use of the latter to obtain crucial observations.


2000 ◽  
Vol 179 ◽  
pp. 197-200
Author(s):  
Milan Minarovjech ◽  
Milan Rybanský ◽  
Vojtech Rušin

AbstractWe present an analysis of short time-scale intensity variations in the coronal green line as obtained with high time resolution observations. The observed data can be divided into two groups. The first one shows periodic intensity variations with a period of 5 min. the second one does not show any significant intensity variations. We studied the relation between regions of coronal intensity oscillations and the shape of white-light coronal structures. We found that the coronal green-line oscillations occur mainly in regions where open white-light coronal structures are located.


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