Gotowe bibliografie tematyczne / Visible and near infrared

Gotowa bibliografia na temat „Visible and near infrared”

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Data publikacji: 8 czerwca 2024

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Artykuły w czasopismach na temat "Visible and near infrared"

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Hemmer, James R., Saemi O. Poelma, Nicolas Treat, Zachariah A. Page, Neil D. Dolinski, Yvonne J. Diaz, Warren Tomlinson i in. "Tunable Visible and Near Infrared Photoswitches". Journal of the American Chemical Society 138, nr 42 (18.10.2016): 13960–66. http://dx.doi.org/10.1021/jacs.6b07434.

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Gavrikov, V. F., A. N. Dvoryankin, A. A. Stepanov, A. K. Shmelev i V. A. Shcheglov. "Visible and near-infrared chemical lasers". Journal of Russian Laser Research 15, nr 3 (maj 1994): 177–212. http://dx.doi.org/10.1007/bf02581029.

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BROWN, CHRIS W. "ULTRAVIOLET, VISIBLE, and NEAR-INFRARED SPECTROPHOTOMETERS". Applied Spectroscopy Reviews 35, nr 3 (7.12.2000): 151–73. http://dx.doi.org/10.1081/asr-100101223.

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Hammersley, M. J., P. E. Townsend, G. F. Grayston i S. L. Ranford. "Visible/Near Infrared Spectroscopy of Scoured Wool". Textile Research Journal 65, nr 4 (kwiecień 1995): 241–46. http://dx.doi.org/10.1177/004051759506500409.

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Zhu, Mei, Mingjian Yuan, Xiaofeng Liu, Jialiang Xu, Jing Lv, Changshui Huang, Huibiao Liu, Yuliang Li, Shu Wang i Daoben Zhu. "Visible Near-Infrared Chemosensor for Mercury Ion". Organic Letters 10, nr 7 (kwiecień 2008): 1481–84. http://dx.doi.org/10.1021/ol800197t.

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Fang, Y. "Acid with visible and near-infrared excitations". Journal of Raman Spectroscopy 30, nr 2 (luty 1999): 85–89. http://dx.doi.org/10.1002/(sici)1097-4555(199902)30:2<85::aid-jrs349>3.0.co;2-k.

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Xiao, Qingbo, Haomiao Zhu, Datao Tu, En Ma i Xueyuan Chen. "Near-Infrared-to-Near-Infrared Downshifting and Near-Infrared-to-Visible Upconverting Luminescence of Er3+-Doped In2O3 Nanocrystals". Journal of Physical Chemistry C 117, nr 20 (13.05.2013): 10834–41. http://dx.doi.org/10.1021/jp4030552.

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Ivana, Šestak, Mesić Milan, Zgorelec Željka, Perčin Aleksandra i Stupnišek Ivan. "Visible and near infrared reflectance spectroscopy for field-scale assessment of Stagnosols properties". Plant, Soil and Environment 64, No. 6 (31.05.2018): 276–82. http://dx.doi.org/10.17221/220/2018-pse.

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Spectral data contain information on soil organic and mineral composition, which can be useful for soil quality monitoring. The objective of research was to evaluate hyperspectral visible and near infrared reflectance (VNIR) spectroscopy for field-scale prediction of soil properties and assessment of factors affecting soil spectra. Two hundred soil samples taken from the experiment field (soil depth: 30 cm; sampling grid: 15 × 15 m) were scanned using portable spectroradiometer (350–1050 nm) to identify spectral differences of soil treated with ten different rates of mineral nitrogen (N) fertilizer (0–300 kg N/ha). Principal component analysis revealed distinction between higher- and lower-N level treatments conditioned by differences in soil pH, texture and soil organic matter (SOM) composition. Partial least square regression resulted in very strong correlation and low root mean square error (RMSE) between predicted and measured values for the calibration (C) and validation (V) dataset, respectively (SOM, %: R<sub>C</sub><sup>2</sup> = 0.75 and R<sub>V</sub><sup>2</sup> = 0.74; RMSE<sub>C</sub> = 0.334 and RMSE<sub>V</sub> = 0.346; soil pH: R<sub>C</sub><sup>2</sup> = 0.78 and R<sub>V</sub><sup>2</sup> = 0.62; RMSE<sub>C</sub> = 0.448 and RMSE<sub>V</sub> = 0.591). Results indicated that hyperspectral VNIR spectroscopy is an efficient method for measurement of soil functional attributes within precision farming framework.
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Gerber, H. "Infrared aerosol extinction from visible and near-infrared light scattering". Applied Optics 24, nr 23 (1.12.1985): 4155. http://dx.doi.org/10.1364/ao.24.004155.

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Fu, Tairan, Jiaqi Tang, Kai Chen i Fan Zhang. "Visible, near-infrared and infrared optical properties of silica aerogels". Infrared Physics & Technology 71 (lipiec 2015): 121–26. http://dx.doi.org/10.1016/j.infrared.2015.03.004.

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Rozprawy doktorskie na temat "Visible and near infrared"

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Singh, Baljinder. "Visible and near-infrared spectroscopic analysis of potatoes". Thesis, McGill University, 2005. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=84074.

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The potential of different spectroscopic techniques for evaluating potato (Solanum tuberosum L.) quality was investigated. Spectral data in the wavelength range of 400-1750 nm were used to develop quality prediction models. The Partial Least Squares (PLS) regression was used for predicting the water content in potato samples. Water content was predicted with R2 ≥ 0.938.
A further study was conducted to find the best wavelengths for predicting water content using two methods, PLS and multiple linear regression. Wavelength ranges of 910-1020, 1129-1211, 1363-1403 nm were selected for samples without skin, while 700-900, 930-1050, 1100-1300, 1400-1550 nm were selected for samples with-skin. Weight prediction models were established using the predicted water content.
Visible spectroscopy was used for classifying shriveled and non-shriveled potatoes. The wavelength ranges best suited to such a classification were those of 442-452, 456-466, 641-651, and 684-694 nm, with accuracies as high as 94.28% and as low as 80%.
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Abdel-Nour, Nicolas. "Chicken egg quality assessment from visible/near infrared observations". Thesis, McGill University, 2009. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=32396.

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Egg is a fragile component within the human diet. Important changes occur in egg during storage. Prediction of these changes is critical in order to grade the eggs upon their quality and freshness. The objectives of this study were to evaluate the application of visible and near infrared spectroscopy as a non-destructive method for the assessment of egg quality and freshness. Therefore, visible and near infrared transmittance spectral data ranging from 350 to 2500 nm was collected with the help of a radiospectrometer on 360 freshly laid eggs. A partial least squares model was built in order to link the spectral data with the most widely used destructive methods, namely Haugh Units and albumen pH in terms of egg quality and the number of storage days in terms of egg freshness. The ability of maximum R2 method to select the relevant wavelengths in order to build a partial least squares (PLS) predictive model was investigated in the first part of the study. The results showed that this method improved the predictive ability of the model. Coefficient of determination (R2) and root mean square error of cross validation (RMSECV) were calculated in order to select sets of wavelengths to build the model with the best predictive ability. The second part of the study was based on building calibration models for predicting egg freshness in terms of number of storage day and egg quality in terms of Haugh Units and albumen pH. The results showed that the models had good predictive ability and R2 for number of storage days, Haugh Units and albumen pH were 0.89, 0.79 and 0.90, respectively. RMSECV for these three parameters were 1.65, 5.05 and 0.06, respectively.
L'oeuf est un composant fragile dans le regime alimentaire humain. Des changements importants arrivent dans loeuf pendant le stockage. La prediction de ces changements eat ctitique pour classer les oeufs selon leur qualité et leur fraîcheur. Les objectifs de cette étude étaient d'évaluer l'application méthode basée sur la spectroscopie visible et infra-rouge proche comme une method non destructive pour l'évaluation de la qualité et la fraîcheur des oeufs. Donc, la transmission visible et infra rouge proche des données spectrales aux limites de 350 à 2500 nm ont été exécutées à l'aide d'un radiosectromètre sur 360 oeufs récemment pondus. Un modèle des moindres carrées partiels (MCP) a été construit afin de lier les données soectrakes avec les méthodes destructives les plus utilisées, à savoir Unité de Haugh at le pH d'albumen en termes de qualité d'oeufs et le nombre de jours de stoclage en termees de fraîcheur d'oeufs. La première étude a traité de la capacité de la méthode maximum R2 à choisir les longueurs d'onde appropriées afin d'établir un modèle des moindres carrés partiels (MCP). Les résultats ont révélé combien cette méthode a été un bon outil dans le choix des longueurs d'onde instructives et dans l'amélioration de la capacité prédictive du modèle. Le coefficient de détermination (R2) et les erreurs de la racine carrée moyenne (ERCM) ont été calculés afin de choisir des ensembles de longueurs d'onde, lesquels aident le mieux à construire le modèle qui possède la meilleure capacité prédictive. La seconde étude a visé l'établissement des modèles prédictifs de la fraîcheur d'oeufs en fonction du n
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Klesman, Alison J. (Alison June) 1981. "Comet-asteroid differentiation using visible and near-infrared spectroscopy". Thesis, Massachusetts Institute of Technology, 2004. http://hdl.handle.net/1721.1/28610.

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Thesis (S.M.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 2004.
Includes bibliographical references (leaves 40-42).
Comets have historically been defined as objects that experience the formation of a "head" (coma) or "tail" as ice and other volatiles that comprise their chemical makeup vaporize when they near the sun. Comets can lose this ability to form a coma or tail, however, through a variety of dynamical processes, creating objects that could chemically be comets but that do not fit the traditional definition. Thus, a new challenge has arisen to correctly define the properties that differentiate comets and asteroids. In this study, a number of cometary candidates were observed in visible and infrared wavelengths in an attempt to correctly classify them as asteroids or dormant or extinct comets. From this data, two groups of objects were identified: one group of possible cometary candidates, and one group of likely outer asteroid belt origin objects. From this and other studies, a broader picture of solar system dynamics can be achieved that will give much insight into not only the current dynamical processes that control interplanetary bodies, but also processes that were important in the formation and stratification of the solar system at its birth.
by Alison J. Klesman.
S.M.
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Balkenhol, Michelle Rose. "Visible and near infrared reflectance spectroscopy of irregular solids /". Thesis, Connect to this title online; UW restricted, 1992. http://hdl.handle.net/1773/8493.

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Howell, Ellen Susanna. "Probing asteroid composition using visible and near-infrared spectroscopy". Diss., The University of Arizona, 1995. http://hdl.handle.net/10150/187372.

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The compositional distribution of asteroids provides clues to understanding solar system formation and evolutionary processes in the asteroid belt. The surface mineralogy and distribution of volatiles on asteroids is determined using visible and near-infrared spectroscopy. A revised asteroid taxonomy is developed which incorporates compositional information from the near-infrared asteroid spectra. A search is conducted for organic compounds on distant asteroids, thought to be most volatile-rich in composition. Our near-infrared spectroscopy of outer belt asteroids shows a trend of increasing red continuum slope with heliocentric distance. I interpret this trend as a compositional change, possibly due to increasing abundance of complex organic compounds on these more distant objects. I do not observe a CN absorption band near 2.2 $\mu$m, and conclude that the organics present are not primarily CN-bearing solids. The 3-$\mu$m water absorption band is not detected on distant D asteroids, but is seen on main belt D asteroids. This observation is consistent with the idea that D asteroids are volatile-rich, but the object must be heated in order to transform the silicates into hydrated minerals. No evidence of clay minerals is seen on any of the distant asteroids observed. The majority of the Jupiter Trojan asteroids have a uniform spectral appearance in spite of collisional processing, which implies that the dark red surface material is not a thin surface coating, but is representative of the bulk composition. Observations of near-Earth asteroids indicates a wide range of compositions, suggesting a variety of source regions. Two objects are detected which may contain hydrated minerals, a valuable resource in space. Three near-Earth asteroids are studied in detail, revealing a range of pyroxene chemistry and olivine content inconsistent with ordinary chondrite composition. The occurrence of spectral variability, and implied compositional inhomogeneity is approximately 20%, and on spatial scales as small as tens of meters. This observation implies that asteroids are geologically complex, not chemically uniform, as is often assumed in meteorite studies.
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Font, Aragonès Xavier. "Visible, near infrared and thermal hand-based image biometric recognition". Doctoral thesis, Universitat Politècnica de Catalunya, 2013. http://hdl.handle.net/10803/117685.

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Biometric Recognition refers to the automatic identification of a person based on his or her anatomical characteristic or modality (i.e., fingerprint, palmprint, face) or behavioural (i.e., signature) characteristic. It is a fundamental key issue in any process concerned with security, shared resources, network transactions among many others. Arises as a fundamental problem widely known as recognition, and becomes a must step before permission is granted. It is supposed that protects key resources by only allowing those resources to be used by users that have been granted authority to use or to have access to them. Biometric systems can operate in verification mode, where the question to be solved is Am I who I claim I am? or in identification mode where the question is Who am I? Scientific community has increased its efforts in order to improve performance of biometric systems. Depending on the application many solutions go in the way of working with several modalities or combining different classification methods. Since increasing modalities require some user inconvenience many of these approaches will never reach the market. For example working with iris, face and fingerprints requires some user effort in order to help acquisition. This thesis addresses hand-based biometric system in a thorough way. The main contributions are in the direction of a new multi-spectral hand-based image database and methods for performance improvement. The main contributions are: A) The first multi-spectral hand-based image database from both hand faces: palmar and dorsal. Biometric database are a precious commodity for research, mainly when it offers something new like visual (VIS), near infrared (NIR) and thermography (TIR) images at a time. This database with a length of 100 users and 10 samples per user constitute a good starting point to check algorithms and hand suitability for recognition. B) In order to correctly deal with raw hand data, some image preprocessing steps are necessary. Three different segmentation phases are deployed to deal with VIS, NIR and TIR images specifically. Some of the tough questions to address: overexposed images, ring fingers and the cuffs, cold finger and noise image. Once image segmented, two different approaches are prepared to deal with the segmented data. These two approaches called: Holistic and Geometric define the main focus to extract the feature vector. These feature vectors can be used alone or can be combined in some way. Many questions can be stated: e.g. which approach is better for recognition?, Can fingers alone obtain better performance than the whole hand? and Is thermography hand information suitable for recognition due to its thermoregulation properties? A complete set of data ready to analyse, coming from the holistic and geometric approach have been designed and saved to test. Some innovative geometric approach related to curvature will be demonstrated. C) Finally the Biometric Dispersion Matcher (BDM) is used in order to explore how it works under different fusion schemes, as well as with different classification methods. It is the intention of this research to contrast what happen when using other methods close to BDM like Linear Discriminant Analysis (LDA). At this point, some interesting questions will be solved, e.g. by taking advantage of the finger segmentation (as five different modalities) to figure out if they can outperform what the whole hand data can teach us.
El Reconeixement Biomètric fa referència a la identi cació automàtica de persones fent us d'alguna característica o modalitat anatòmica (empremta digital) o d'alguna característica de comportament (signatura). És un aspecte fonamental en qualsevol procés relacionat amb la seguretat, la compartició de recursos o les transaccions electròniques entre d'altres. És converteix en un pas imprescindible abans de concedir l'autorització. Aquesta autorització, s'entén que protegeix recursos clau, permeten així, que aquests siguin utilitzats pels usuaris que han estat autoritzats a utilitzar-los o a tenir-hi accés. Els sistemes biomètrics poden funcionar en veri cació, on es resol la pregunta: Soc jo qui dic que soc? O en identi cació on es resol la qüestió: Qui soc jo? La comunitat cientí ca ha incrementat els seus esforços per millorar el rendiment dels sistemes biomètrics. En funció de l'aplicació, diverses solucions s'adrecen a treballar amb múltiples modalitats o combinant diferents mètodes de classi cació. Donat que incrementar el número de modalitats, representa a la vegada problemes pels usuaris, moltes d'aquestes aproximacions no arriben mai al mercat. La tesis contribueix principalment en tres grans àrees, totes elles amb el denominador comú següent: Reconeixement biometric a través de les mans. i) La primera d'elles constitueix la base de qualsevol estudi, les dades. Per poder interpretar, i establir un sistema de reconeixement biomètric prou robust amb un clar enfocament a múltiples fonts d'informació, però amb el mínim esforç per part de l'usuari es construeix aquesta Base de Dades de mans multi espectral. Les bases de dades biomètriques constitueixen un recurs molt preuat per a la recerca; sobretot si ofereixen algun element nou com es el cas. Imatges de mans en diferents espectres electromagnètics: en visible (VIS), en infraroig (NIR) i en tèrmic (TIR). Amb un total de 100 usuaris, i 10 mostres per usuari, constitueix un bon punt de partida per estudiar i posar a prova sistemes multi biomètrics enfocats a les mans. ii) El segon bloc s'adreça a les dues aproximacions existents en la literatura per a tractar les dades en brut. Aquestes dues aproximacions, anomenades Holística (tracta la imatge com un tot) i Geomètrica (utilitza càlculs geomètrics) de neixen el focus alhora d'extreure el vector de característiques. Abans de tractar alguna d'aquestes dues aproximacions, però, és necessària l'aplicació de diferents tècniques de preprocessat digital de la imatge per obtenir les regions d'interès desitjades. Diferents problemes presents a les imatges s'han hagut de solucionar de forma original per a cadascuna de les tipologies de les imatges presents: VIS, NIR i TIR. VIS: imatges sobre exposades, anells, mànigues, braçalets. NIR: Ungles pintades, distorsió en forma de soroll en les imatges TIR: Dits freds La segona àrea presenta aspectes innovadors, ja que a part de segmentar la imatge de la ma, es segmenten tots i cadascun dels dits (feature-based approach). Així aconseguim contrastar la seva capacitat de reconeixement envers la ma de forma completa. Addicionalment es presenta un conjunt de procediments geomètrics amb la idea de comparar-los amb els provinents de l'extracció holística. La tercera i última àrea contrasta el procediment de classi cació anomenat Biometric Dispersion Matcher (BDM) amb diferents situacions. La primera relacionada amb l'efectivitat respecte d'altres mètode de reconeixement, com ara l'Anàlisi Lineal Discriminant (LDA) o bé mètodes com KNN o la regressió logística. Les altres situacions que s'analitzen tenen a veure amb múltiples fonts d'informació, quan s'apliquen tècniques de normalització i/o estratègies de combinació (fusió) per millorar els resultats. Els resultats obtinguts no deixen lloc per a la confusió, i són certament prometedors en el sentit que posen a la llum la importància de combinar informació complementària per obtenir rendiments superiors.
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Karlsson, Jonas. "FPGA-Accelerated Dehazing by Visible and Near-infrared Image Fusion". Thesis, Mälardalens högskola, Akademin för innovation, design och teknik, 2015. http://urn.kb.se/resolve?urn=urn:nbn:se:mdh:diva-28322.

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Fog and haze can have a dramatic impact on vision systems for land and sea vehicles. The impact of such conditions on infrared images is not as severe as for standard images. By fusing images from two cameras, one ordinary and one near-infrared camera, a complete dehazing system with colour preservation can be achieved. Applying several different algorithms to an image set and evaluating the results, the most suitable image fusion algoritm has been identified. Using an FPGA, a programmable integrated circuit, a crucial part of the algorithm has been implemented. It is capable of producing processed images 30 times faster than a laptop computer. This implementation lays the foundation of a real-time dehazing system and provides a significant part of the full solution. The results show that such a system can be accomplished with an FPGA.
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Costa, Posada Carlos Rufino. "The topographic effect in visible and near infrared satellite imagery". Thesis, University of Cambridge, 1998. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.624720.

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Karkoschka, Erich. "Saturn's atmosphere in the visible and near-infrared, 1986-1989". Diss., The University of Arizona, 1990. http://hdl.handle.net/10150/185074.

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This work describes observations of Saturn's atmosphere in the visible and near infrared (450-1000 nm) including four hydrogen quadrupole lines, 17 methane absorption bands ranging over three orders of magnitude in absorption strength, an ammonia absorption band, and the absolute calibrated continuum spectrum. All observations have complete coverage of Saturn's disk, in latitude as well as in center-to-limb position. The accuracy of the data is comparable or better than previous data. This data set gives a quite complete description of Saturn's atmosphere in the visible and near infrared at the spatial resolution of ground based observations. While the main data were acquired in 1988, small changes between 1986 and 1989 were determined also. An atmospheric model is given which fits all observations within estimated errors. It has clear gas at the top of the atmosphere, an extended haze layer and a reflective cloud at the bottom. Pressure levels and the haze optical depth were determined as a function of latitude. The single scattering albedo spectrum of the particles (most likely ammonia ice crystals) is also given for each latitude. The methane mixing ratio is (3.0 ± 0.6) x 10⁻³, the ammonia mixing ratio is (1.2 + 0.8/-0.6) x 10⁻³ below the ammonia condensation level. Room temperature methane absorption spectra do not fit the observed spectra for any cloud structure. A cold temperature methane absorption spectrum is determined under the assumption that methane band strengths are temperature invariant, but not necessarily the absorption coefficients at each location across the band. It indicates that the absorption coefficients are typically 20-30 per cent stronger in the center of a band and up to a factor of two weaker in the wings. This spectrum should be useful in the interpretation of methane observations of all the giant planets and Titan.
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Amat, Genís Albert. "Effect of visible and near-infrared light on adenosine triphosphate (atp)". Doctoral thesis, Universitat Rovira i Virgili, 2005. http://hdl.handle.net/10803/8715.

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L' ATP es una molecula clau en el metabolisme cel.lular, actuant com a donador d'energia lliure i acoplant reaccions endergoniques i exergoniques. L'ATP es sintetitzat a la mitocondria en un proces anomenat fosforil.lacio oxidativa despres d'una serie de reaccions a la cadena de citocroms que es troba en la membrana interna de l'organel.la. La font d'energia necessaria per aquesta sintesi s'obte en les cel.lules animals dels nutrients de l'ingestio, i de la llum solar en les plantes. Existeix una via alternativa de sintesi d'ATP extramitocondrial, la glicolisi, que s'inicia amb la fosforilacio de la glucosa per l'enzim hexokinasa.
Interaccio llum-materia
L'energia electromagnetica l'ona de la qual oscil.la en una longitud d'ona de nanometres es anomenada llum. En aquestes frequencies, l'energia promou excitacio electronica de certs atoms i molecules. Existeix una interaccio diferent de la llum amb molecules, produida per el camp electromagnetic que per definicio la llum provoca en qualsevol medi. El camp electric resultant desplaca els electrons dels enllacos quimics produint una polaritzacio del medi sense que existeixi absorcio de l'energia. Aquest es un mecanisme interactiu que existeix sempre, i es l'unic que es dona en molecules que son transparents (no absorbeixen) per a una determinada frequencia de la llum, com es el cas de l'ATP per l'energia visible i infravermella propera.
Experiments, resultats i discussio
Quan l'ATP es excitat amb fotons ultraviolats, es produiex una fluorescencia en longituts d'ona visibles. L'io magnesi s'ha utilitzat per estudiar com la llum visible i infravermella propera produiex un desplacament de carregues electriques a la molecula d'ATP.
La construccio d'un interferometre de Michelson ha servit per observar l'interaccio no absortiva de la llum i l'ATP. La mesura directa de l'index de refraccio d'una solucio d'ATP dona informacio sobre les caracteristiques electriques del medi. L'observacio de que aquest index canvia despres d'irradiar la solucio amb longituds d'ona visibles i infravermelles properes, confirmen que la llum provoca canvis electrics significatius en l'ATP.
En aquest treball tambe s'ha estudiat el comportament bioquimic de l'ATP irradiat quant forma part de dues reaccions quimiques diferents: la de la luciferina-luciferasa i la de la hexoquinasa. En tots dos casos, l'us d'aquest ATP irradiat ha produit una alteracio dels parametres cinetics estudiats, V0 i k en la reaccio de la luciferina-luciferasa, i km i vmax en la reaccio de l'hexoquinasa.
Conclusions
Aquesta interaccio no absortiva de la llum amb l'ATP es la primera descrita per a una biomolecula. El mecanisme aporta noves dades per explicar els efectes observats en el metabolisme cel.lular despres de l'irradiacio d'organismes, teixits i cultius cel.lulars amb llum visible i infravermella propera.
ATP is a key molecule in cellular metabolism. In this thesis, I examined the effects of visible (635 and 655 nm) and near-infrared (810 and 830 nm) light on ATP in solution. I also examined were the biochemical behavior of light-exposed ATP in the luciferine-luciferase reaction and hexokinase reaction, the initial step in glycolysis that begins extra mithocondrial ATP synthesis. Irradiated groups in the luciferine-luciferase reaction showed an improvement in the kinetic parameters V0 and k, and more ATP molecules reacted with the enzyme when they were excited by light. When irradiated ATP was added to the hexokinase reaction, the experimental groups showed significant differences in the Michaelis-Menten kinetic parameters (km for ATP and vmax) and the rate of product synthesis was greater. Changes in both reactions were wavelength and dose dependant.
When ATP was excited with UV photons, it fluoresced. This fluorescence decreased when Mg2+ was added, probably because the ion binds the phosphates, which are the part of the molecule responsible for light emission. Irradiating the ATP-Mg2+ solution with 655 nm and 830 nm light increased the fluorescence resulting from a displacement of charges in the phosphor-oxygen bond that repels Mg2+.
The refraction of light in an ATP solution was observed by the Michelson interferometer and by directly measuring the refractive index. The refractive index changed after red and near-infrared light interaction due to a change in the electrical permittivity of the medium.
Since ATP in water is transparent to visible and near-infrared light, and is therefore not a chromophore for those wavelengths, I conclude that the observed light interaction with ATP is not due to photon absorption but to the electromagnetic disturbance produced by the light, which leads to a polarization of the dielectric molecule that is ATP.
This interaction of visible and near-infrared electromagnetic energy with ATP offers new perspectives for explaining light interaction at subcellular level.
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Książki na temat "Visible and near infrared"

1

International, Strategic Directions, red. Visible, UV-visible, and near infrared instruments in the U.S. Los Angeles, CA: Strategic Directions International, 1997.

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Cutler, Paul M. Visible and near-infrared reflectivities in a mid-latitude glacier basin. Ottawa: National Library of Canada = Bibliothèque nationale du Canada, 1991.

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Lowe, Andrew Timothy. Estimation of visible and near-infrared reflectivity for Peyto Glacier Basin usinf satellite data. Ottawa: National Library of Canada, 1993.

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Zijlstra, Willem G. Visible and near infrared absorption spectra of human and animal haemoglobin: Determination and application. Utrecht: VSP, 2000.

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Elhinney, John Mc. Direct quality measurement of flour and discrimination of selected meats by visible, near and mid-infrared spectroscopy. Dublin: University College Dublin, 1998.

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Larason, Thomas C. Spectroradiometric detector measurements: Part 1-ultraviolet detectors and part II-visible to near-infrared detectors. Gaithersburg, MD: U.S. Dept. of Commerce, Technology Administration, National Institute of Standards and Technology, 1998.

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Liggins, E. P. A critique of exposure limits for non-ionizing radiation in the visible and near-infrared. London: HMSO, 1999.

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Wiggan, C. F. Visible and near-infrared spectroscopic investigations for the non-invasive determination of foetal blood pH THESIS. Manchester: UMIST, 1988.

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Smith, Gilbert R. Visible and near-infrared channel calibration of the GOES-6 VISSR using high-altitude aircraft measurements. Moffett Field, Calif: National Aeronautics and Space Administration, Ames Research Center, 1989.

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R, Smith Gilbert, i Ames Research Center, red. Visible and near-infrared channel calibration of the GOES-6 VISSR using high-altitude aircraft measurements. Moffett Field, Calif: National Aeronautics and Space Administration, Ames Research Center, 1989.

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Części książek na temat "Visible and near infrared"

1

Kobayashi, Hisataka. "Theranostic Near-Infrared Photoimmunotherapy". W Make Life Visible, 219–25. Singapore: Springer Singapore, 2019. http://dx.doi.org/10.1007/978-981-13-7908-6_22.

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Masunaga, Hirohiko. "Visible/Near-Infrared Imaging". W Satellite Measurements of Clouds and Precipitation, 171–92. Singapore: Springer Nature Singapore, 2022. http://dx.doi.org/10.1007/978-981-19-2243-5_8.

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Masunaga, Hirohiko. "Visible/Near-Infrared Imaging". W Satellite Measurements of Clouds and Precipitation, 171–92. Singapore: Springer Nature Singapore, 2022. http://dx.doi.org/10.1007/978-981-19-2243-5_8.

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Brown, Chris W. "Ultraviolet, Visible, Near-Infrared Spectrophotometers". W Ewing’s Analytical Instrumentation Handbook, Fourth Edition, 117–28. Fourth edition / [edited by] Nelu Grinberg, Sonia Rodriguez. | Boca Raton : CRC Press, Taylor & Francis Group, 2019.: CRC Press, 2019. http://dx.doi.org/10.1201/9781315118024-5.

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Chauhan, Mamta, i Prakash Chauhan. "Visible and Near-Infrared Spectroscopy". W Encyclopedia of Lunar Science, 1–6. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-319-05546-6_174-1.

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Chauhan, Mamta, i Prakash Chauhan. "Visible and Near-Infrared Spectroscopy". W Encyclopedia of Lunar Science, 1239–44. Cham: Springer International Publishing, 2023. http://dx.doi.org/10.1007/978-3-319-14541-9_174.

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Beckwith, Steven V. W. "The visible and near-infrared domain". W Observing Photons in Space, 121–37. New York, NY: Springer New York, 2013. http://dx.doi.org/10.1007/978-1-4614-7804-1_6.

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Sasaki, Yoichi, Nobuhiro Yanai i Nobuo Kimizuka. "Near-Infrared-to-Visible Photon Upconversion". W Emerging Strategies to Reduce Transmission and Thermalization Losses in Solar Cells, 29–48. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-70358-5_3.

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da Silva Terra, Fabrício, Rodnei Rizzo, Eyal Ben Dor i José A. M. Demattê. "Soil Sensing by Visible and Infrared Radiation". W Handbook of Near-Infrared Analysis, 839–68. Wyd. 4. Fourth edition. | Boca Raton : Taylor and Francis, 2021. |: CRC Press, 2021. http://dx.doi.org/10.1201/b22513-46.

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Adriani, A., G. Bellucci, L. Gambicorti, M. Focardi, E. Oliva, M. Farina, A. M. Di Giorgio i in. "The visible and near infrared module of EChO". W EChO - Exoplanet Characterisation Observatory, 71–87. Dordrecht: Springer Netherlands, 2014. http://dx.doi.org/10.1007/978-94-024-0837-9_5.

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Streszczenia konferencji na temat "Visible and near infrared"

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Yasuoka, Yoshifumi, Masao Naka i Yuji Miyachi. "Advanced visible near-infrared radiometer (AVNIR)". W Satellite Remote Sensing II, redaktorzy Hiroyuki Fujisada i Martin N. Sweeting. SPIE, 1995. http://dx.doi.org/10.1117/12.228563.

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Murguia, James E., Toby D. Reeves, Jonathan M. Mooney, William S. Ewing, Freeman D. Shepherd i Andrzej K. Brodzik. "Compact visible/near-infrared hyperspectral imager". W AeroSense 2000, redaktorzy Eustace L. Dereniak i Robert E. Sampson. SPIE, 2000. http://dx.doi.org/10.1117/12.391760.

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Nedelcu, Tudor, Shejin Thavalengal i Peter Corcoran. "Hybrid sensor visible + near infrared demosaicing". W 2015 IEEE 5th International Conference on Consumer Electronics - Berlin (ICCE-Berlin). IEEE, 2015. http://dx.doi.org/10.1109/icce-berlin.2015.7391249.

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Byard, Paul L. "Dual-channel near-infrared/visible imaging systems". W Astronomical Telescopes & Instrumentation, redaktor Albert M. Fowler. SPIE, 1998. http://dx.doi.org/10.1117/12.317334.

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de Lima, J. J. I., A. A. Souza Lins, A. M. Menezes Alexandre, P. S. Filho i V. F. Rodriguez-Esquerre. "Visible and Near Infrared Broadband Plasmonic Absorber". W Frontiers in Optics. Washington, D.C.: OSA, 2021. http://dx.doi.org/10.1364/fio.2021.jth5a.139.

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Knadel, Maria, Yi Peng, Cecilie Hermansen, Trine Norgaard, Rene Gislum, Lis Wollesen de Jonge, Per Moldrup i Mogens Humlekrog Gerve. "Determining the clay/organic carbon ratio by visible near infrared spectroscopy". W 17th International Conference on Near Infrared Spectroscopy. Foz do Iguaçu - PR, Brazil: Galoa, 2015. http://dx.doi.org/10.17648/nir-2015-34197.

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Millar-Blanchaer, Max, Dae-Sik Moon, James R. Graham i Michael Escuti. "Polarization gratings for visible and near-infrared astronomy". W SPIE Astronomical Telescopes + Instrumentation, redaktorzy Ramón Navarro, Colin R. Cunningham i Allison A. Barto. SPIE, 2014. http://dx.doi.org/10.1117/12.2056998.

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Reininger, Francis M. "Near-ultraviolet visible infrared mapping spectrometer (NU-VIMS)". W Garmisch - DL tentative, redaktorzy Guy Cerutti-Maori i Philippe Roussel. SPIE, 1994. http://dx.doi.org/10.1117/12.185266.

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Zeller, John W., Caitlin Rouse, Harry Efstathiadis, Pradeep Haldar, Jay S. Lewis, Nibir K. Dhar, Priyalal Wijewarnasuriya, Yash R. Puri i Ashok K. Sood. "Development of silicon-germanium visible-near infrared arrays". W SPIE Commercial + Scientific Sensing and Imaging, redaktorzy Nibir K. Dhar i Achyut K. Dutta. SPIE, 2016. http://dx.doi.org/10.1117/12.2229650.

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Piegari, Angela, Anna K. Sytchkova, Ilaria Di Sarcina i Jiri Bulir. "Visible and near-infrared filters for miniaturized spectrometers". W SPIE Astronomical Telescopes + Instrumentation, redaktorzy Eli Atad-Ettedgui i Dietrich Lemke. SPIE, 2008. http://dx.doi.org/10.1117/12.789189.

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Raporty organizacyjne na temat "Visible and near infrared"

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Taylor, B. Ultraviolet-visible-near infrared spectra of 50 samples. Office of Scientific and Technical Information (OSTI), sierpień 1988. http://dx.doi.org/10.2172/67460.

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Shell, James R., Schott II i John R. Quantifying Polarized Clutter in the Visible to Near-Infrared. Fort Belvoir, VA: Defense Technical Information Center, luty 2005. http://dx.doi.org/10.21236/ada430395.

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Zhu, Jinyu, Mun Y. Choi, George W. Mulholland i Louis A. Gritzo. Soot Scattering Measurements in the Visible and Near-Infrared Spectrum. Fort Belvoir, VA: Defense Technical Information Center, sierpień 2000. http://dx.doi.org/10.21236/ada455427.

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Powell, J. W., E. G. Potter, V. Tschirhart, J. B. Percival, S. Mount, B. McEwan, R. Ashley i K. Wheatley. Quantifying fertile alteration in the Patterson Lake corridor, Saskatchewan, through visible-near infrared-shortwave infrared spectroscopy. Natural Resources Canada/ESS/Scientific and Technical Publishing Services, 2019. http://dx.doi.org/10.4095/313671.

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Sheehe, Suzanne Marie Lanier, i Scott I. Jackson. Identification of Species from Visible and Near-Infrared Spectral Emission of a Nitromethane-Air Diffusion Flame. Office of Scientific and Technical Information (OSTI), kwiecień 2019. http://dx.doi.org/10.2172/1508530.

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Peter, J. M., D. Layton-Matthews, M. G. Gadd, S. Gill, S. Baker, S. Plett i S. Paradis. Application of visible-near infrared and short wave infrared spectroscopy to sediment-hosted Zn-Pb deposit exploration in the Selwyn Basin, Yukon. Natural Resources Canada/ESS/Scientific and Technical Publishing Services, 2015. http://dx.doi.org/10.4095/296336.

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Augustoni, Arnold L. Laser selection based on maximum permissible exposure limits for visible and middle-near infrared repetitively pulsed lasers. Office of Scientific and Technical Information (OSTI), marzec 2004. http://dx.doi.org/10.2172/918747.

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CIE. CIE 250:2022 Spectroradiometric Measurement of Optical Radiation Sources. International Commission on Illumination, czerwiec 2022. http://dx.doi.org/10.25039/tr.250.2022.

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Streszczenie:
This Technical Report provides basic measurement principles and practical guidance on spectroradiometry of optical radiation sources in the ultraviolet, visible and near-infrared regions of the electromagnetic spectrum in the wavelength range from 200 nm to 2 500 nm. The document primarily deals with spectral measurements of irradiance, radiance, radiant intensity, radiant flux and derivative quantities. The document provides a detailed overview of relevant terminology and basic measurement principles, including those for instrument calibration. It provides practical guidance for identifying, understanding and quantifying relevant measurement uncertainty components. This document replaces CIE 063-1984. Additional details on measurement principles not covered in this document can be found in CIE 214:2014. The document is written in English, with a short summary in French and German. It consists of 94 pages with 41 figures and 3 tables and is readily available from the CIE Webshop or from the National Committees of the CIE.
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Lee Spangler, Ross Bricklemyer i David Brown. Cropland Field Monitoring: MMV Page 1 Montana Cropland Enrolled Farm Fields Carbon Sequestration Field Sampling, Measurement, Monitoring, and Verification: Application of Visible-Near Infrared Diffuse Reflectance Spectroscopy (VNIR) and Laser-induced Breakdown Spectroscopy (LIBS). Office of Scientific and Technical Information (OSTI), marzec 2012. http://dx.doi.org/10.2172/1037876.

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Letcher, Theodore, Julie Parno, Zoe Courville, Lauren Farnsworth i Jason Olivier. A generalized photon-tracking approach to simulate spectral snow albedo and transmittance using X-ray microtomography and geometric optics. Engineer Research and Development Center (U.S.), czerwiec 2023. http://dx.doi.org/10.21079/11681/47122.

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A majority of snow radiative transfer models (RTMs) treat snow as a collection of idealized grains rather than an organized ice–air matrix. Here we present a generalized multi-layer photon-tracking RTM that simulates light reflectance and transmittance of snow based on X-ray micro- tomography images, treating snow as a coherent 3D structure rather than a collection of grains. The model uses a blended approach to expand ray-tracing techniques applied to sub-1 cm3 snow samples to snowpacks of arbitrary depths. While this framework has many potential applications, this study’s effort is focused on simulating reflectance and transmittance in the visible and near infrared (NIR) through thin snow- packs as this is relevant for surface energy balance and remote sensing applications. We demonstrate that this framework fits well within the context of previous work and capably reproduces many known optical properties of a snow surface, including the dependence of spectral reflectance on the snow specific surface area and incident zenith angle as well as the surface bidirectional reflectance distribution function (BRDF). To evaluate the model, we compare it against reflectance data collected with a spectroradiometer at a field site in east-central Vermont. In this experiment, painted panels were inserted at various depths beneath the snow to emulate thin snow. The model compares remarkably well against the reflectance measured with a spectroradiometer, with an average RMSE of 0.03 in the 400–1600 nm range. Sensitivity simulations using this model indicate that snow transmittance is greatest in the visible wavelengths, limiting light penetration to the top 6 cm of the snowpack for fine-grain snow but increasing to 12 cm for coarse-grain snow. These results suggest that the 5% transmission depth in snow can vary by over 6 cm according to the snow type.
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