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Relevant bibliographies by topics / Spire

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Academic literature on the topic 'Spire'

Author: Grafiati

Published: 4 June 2021

Last updated: 17 June 2025

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Journal articles on the topic "Spire"

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Kapustin, Petr, and Elena Bagina. "The spire. Jabbing the sky." проект байкал, no. 83 (April 20, 2025): 60–67. https://doi.org/10.51461/issn.2309-3072/83.2482.

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The spire is a strange, specific architectural detail that has become widespread throughout the world. The origin of this detail and its purpose are not entirely clear. The appearance of spires in the history of European architecture is a symptom of profound changes in the shape formation, in the very view of architecture, and in the image of the building. We have not yet fully realized these changes. The symbolism, mythopoetics, and phenomenology of spires are timeless, like the spire itself, figures of cultural heritage that connect times, ‘stitching’ history into a continuous fabric of meanings and senses.

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Wajda, Eligiusz. "SPIRE." ACM SIGARCH Computer Architecture News 20, no. 1 (1992): 45–54. http://dx.doi.org/10.1145/130823.130825.

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Jia, Ning, Chun Yang, Jing Wang, Dong Tong, and Keyi Wang. "SPIRE." ACM SIGPLAN Notices 48, no. 7 (2013): 1–12. http://dx.doi.org/10.1145/2517326.2451516.

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Lin, Xika, Abhishek Mukherji, Elke A. Rundensteiner, and Matthew O. Ward. "SPIRE." Proceedings of the VLDB Endowment 7, no. 13 (2014): 1653–56. http://dx.doi.org/10.14778/2733004.2733053.

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Li, Chung-Sheng, Lawrence D. Bergman, Yuan-Chi Chang, Vittorio Castelli, and John R. Smith. "SPIRE." ACM SIGMOD Record 29, no. 2 (2000): 598. http://dx.doi.org/10.1145/335191.336583.

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Fogleman, Corey D. "Fallen Spire." Family Medicine 52, no. 6 (2020): 451. http://dx.doi.org/10.22454/fammed.2020.864278.

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Wellington, A., S. Emmons, B. James, et al. "Spire contains actin binding domains and is related to ascidian posterior end mark-5." Development 126, no. 23 (1999): 5267–74. http://dx.doi.org/10.1242/dev.126.23.5267.

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Spire is a maternal effect locus that affects both the dorsal-ventral and anterior-posterior axes of the Drosophila egg and embryo. It is required for localization of determinants within the developing oocyte to the posterior pole and to the dorsal anterior corner. During mid-oogenesis, spire mutants display premature microtubule-dependent cytoplasmic streaming, a phenotype that can be mimicked by pharmacological disruption of the actin cytoskeleton with cytochalasin D. Spire has been cloned by transposon tagging and is related to posterior end mark-5, a gene from sea squirts that encodes a posteriorly localized mRNA. Spire mRNA is not, however, localized to the posterior pole. SPIRE also contains two domains with similarity to the actin monomer-binding WH2 domain, and we demonstrate that SPIRE binds to actin in the interaction trap system and in vitro. In addition, SPIRE interacts with the rho family GTPases RHOA, RAC1 and CDC42 in the interaction trap system. Thus, our evidence supports the model that SPIRE links rho family signaling to the actin cytoskeleton.

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Bae, In-Suk, Koang-Hum Bak, Hyoung-Joon Chun, Je Il Ryu, Sung-Jae Park, and Sung-Jae Lee. "Biomechanical analysis of a newly developed interspinous process device conjunction with interbody cage based on a finite element model." PLOS ONE 15, no. 12 (2020): e0243771. http://dx.doi.org/10.1371/journal.pone.0243771.

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Purpose This study aimed to investigate the biomechanical effects of a newly developed interspinous process device (IPD), called TAU. This device was compared with another IPD (SPIRE) and the pedicle screw fixation (PSF) technique at the surgical and adjacent levels of the lumbar spine. Materials and methods A three-dimensional finite element model analysis of the L1-S1 segments was performed to assess the biomechanical effects of the proposed IPD combined with an interbody cage. Three surgical models—two IPD models (TAU and SPIRE) and one PSF model—were developed. The biomechanical effects, such as range of motion (ROM), intradiscal pressure (IDP), disc stress, and facet loads during extension were analyzed at surgical (L3-L4) and adjacent levels (L2-L3 and L4-L5). The study analyzed biomechanical parameters assuming that the implants were perfectly fused with the lumbar spine. Results The TAU model resulted in a 45%, 49%, 65%, and 51% decrease in the ROM at the surgical level in flexion, extension, lateral bending, and axial rotation, respectively, when compared to the intact model. Compared to the SPIRE model, TAU demonstrated advantages in stabilizing the surgical level, in all directions. In addition, the TAU model increased IDP at the L2-L3 and L4-L5 levels by 118.0% and 78.5% in flexion, 92.6% and 65.5% in extension, 84.4% and 82.3% in lateral bending, and 125.8% and 218.8% in axial rotation, respectively. Further, the TAU model exhibited less compensation at adjacent levels than the PSF model in terms of ROM, IDP, disc stress, and facet loads, which may lower the incidence of the adjacent segment disease (ASD). Conclusion The TAU model demonstrated more stabilization at the surgical level than SPIRE but less stabilization than the PSF model. Further, the TAU model demonstrated less compensation at adjacent levels than the PSF model, which may lower the incidence of ASD in the long term. The TAU device can be used as an alternative system for treating degenerative lumbar disease while maintaining the physiological properties of the lumbar spine and minimizing the degeneration of adjacent segments.

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Quinlan, Margot E., Susanne Hilgert, Anaid Bedrossian, R. Dyche Mullins, and Eugen Kerkhoff. "Regulatory interactions between two actin nucleators, Spire and Cappuccino." Journal of Cell Biology 179, no. 1 (2007): 117–28. http://dx.doi.org/10.1083/jcb.200706196.

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Spire and Cappuccino are actin nucleation factors that are required to establish the polarity of Drosophila melanogaster oocytes. Their mutant phenotypes are nearly identical, and the proteins interact biochemically. We find that the interaction between Spire and Cappuccino family proteins is conserved across metazoan phyla and is mediated by binding of the formin homology 2 (FH2) domain from Cappuccino (or its mammalian homologue formin-2) to the kinase noncatalytic C-lobe domain (KIND) from Spire. In vitro, the KIND domain is a monomeric folded domain. Two KIND monomers bind each FH2 dimer with nanomolar affinity and strongly inhibit actin nucleation by the FH2 domain. In contrast, formation of the Spire–Cappuccino complex enhances actin nucleation by Spire. In Drosophila oocytes, Spire localizes to the cortex early in oogenesis and disappears around stage 10b, coincident with the onset of cytoplasmic streaming.

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Jing, Xin, Shu-Peng Ho, Xi Shao, Tung-Chang Liu, Yong Chen, and Xinjia Zhou. "Spire RO Thermal Profiles for Climate Studies: Initial Comparisons of the Measurements from Spire, NOAA-20 ATMS, Radiosonde, and COSMIC-2." Remote Sensing 15, no. 15 (2023): 3710. http://dx.doi.org/10.3390/rs15153710.

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Global Navigation Satellite System (GNSS) Radio Occultation (RO) data play an essential role in improving numerical weather prediction (NWP) and monitoring climate change. The NOAA Commercial RO Purchase Program (CDP) purchased RO data provided by Spire Global Inc. To ensure the data quality from Spire Global Inc. is consistent with other RO missions, we need to quantify their accuracy and retrieval uncertainty carefully. In this work, Spire Wet Profile (wet temperature profile) data from 7 September 2021 to 31 October 2022, processed by the University Corporation for Atmospheric Research (UCAR), and COSMIC-2 (Constellation Observing System for Meteorology, Ionosphere, and Climate-2/Formosa Satellite Mission 7) data are evaluated through comparison with NOAA-20 Advanced Technology Microwave Sounder (ATMS) microwave sounder measurements and collocated RS41 radiosonde measurements. Through the Community Radiative Transfer Model (CRTM) simulation, we convert the Spire and COSMIC-2 RO retrievals to ATMS brightness temperature (BT) at sounding channels CH07 to CH14 (temperature channels), with weighting function peak heights from 8 km to 35 km, and CH19 to CH22 (water vapor channels), with weighting function peak heights ranging from 3.2 km to 6.7 km, and compare the simulations with the collocated NOAA-20 ATMS measurements over ocean. Using ATMS observations as references, Spire and COSMIC-2 BTs agree well with ATMS within 0.07 K for CH07-14 and 0.20 K for CH19-22. The trends between Spire and COSMIC-2 are consistent within 0.07 K/year over the oceans for ATMS CH07-CH13 and CH19-22, indicating that Spire/COSMIC-2 wet profiles are, in general, compatible with each other over oceans. The RO retrievals and RS41 radiosonde observation (RAOB) comparison shows that above 0.2 km altitude, RS41 RAOB matches Spire/COSMIC-2 temperature profiles well with a temperature difference of <0.13 K, and the trends between Spire and COSMIC-2 are consistent within 0.08 K/year over land, indicating that Spire/COSMIC-2 wet profiles are overall compatible with each other through RS41 RAOB measurements over land. In addition, the consistency of Spire and COSMIC-2 based on different latitude intervals, local times, and signal-to-noise ratios (SNRs) through ATMS was evaluated. The results show that the performance of Spire is comparable to COSMIC-2, even though COSMIC-2 has a higher SNR. The high quality of RO profiles from Spire is expected to improve short- and medium-range global numerical weather predictions and help construct consistent climate temperature records.

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Dissertations / Theses on the topic "Spire"

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Grafen, Hansjörg. "Forschungen zur älteren Speyerer Totenbuchüberlieferung : mit einer Textwiedergabe der Necrologanlage von 1273 /." Mainz : Gesellschaft für Mittelrheinische Kirchengeschichte, 1996. http://catalogue.bnf.fr/ark:/12148/cb37689046h.

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Kulling, Edwin Rene. "Human nature in William Golding's The spire." Theological Research Exchange Network (TREN), 1987. http://www.tren.com.

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Spencer, Locke Dean, and University of Lethbridge Faculty of Arts and Science. "Spectral characterization of the Herschel SPIRE photometer." Thesis, Lethbridge, Alta. : University of Lethbridge, Faculty of Arts and Science, 2005, 2005. http://hdl.handle.net/10133/291.

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The European Space Agency's Herschel Space Observatory is comprised of three cryogenically cooled instruments commissioned to explore the far infrared/submillimetre universe. The Spectral and Photometric Imaging REceiver (SPIRE) is one of Herschel's instruments and consists of a three band imaging photometer and a two band imaging spectrometer. Canada is involved in the SPIRE project through provision of instrument development hardware and software, mission flight software, and support personnel. This thesis discusses Fourier transform spectroscopy (FTS) and FTS data processing. A detailed discussion is included on FTS phase correction, with results presented from the optimization of an enhanced Forman phase correction routine developed for this work. This thesis discusses the design, verification, and use of the hardware and software provided by Dr. Naylor's group as it relates to SPIRE verification testing. Results of the photometer characterization are presented. The current status of SPIRE and its future schedule is also discussed.<br>xvii, 239 leaves : ill. (some col.) ; 28 cm.

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Viggh, Herbert E. M. "Surface Prior Information Reflectance Estimation (SPIRE) algorithms." Thesis, Massachusetts Institute of Technology, 2001. http://hdl.handle.net/1721.1/17564.

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Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Electrical Engineering and Computer Science, 2001.<br>Includes bibliographical references (p. 393-396).<br>In this thesis we address the problem of estimating changes in surface reflectance in hyperspectral image cubes, under unknown multiplicative and additive illumination noise. Rather than using the Empirical Line Method (ELM) or physics-based approaches, we assumed the presence of a prior reflectance image cube and ensembles of typical multiplicative and additive illumination noise vectors, and developed algorithms which estimate reflectance using this prior information. These algorithms were developed under the additional assumptions that the illumination effects were band limited to lower spatial frequencies and that the differences in the surface reflectance from the prior were small in area relative to the scene, and have defined edges. These new algorithms were named Surface Prior Information Reflectance Estimation (SPIRE) algorithms. Spatial SPIRE algorithms that employ spatial processing were developed for six cases defined by the presence or absence of the additive noise, and by whether or not the noise signals are spatially uniform or varying. These algorithms use high-pass spatial filtering to remove the noise effects. Spectral SPIRE algorithms that employ spectral processing were developed and use zero-padded Principal Components (PC) filtering to remove the illumination noise. Combined SPIRE algorithms that use both spatial and spectral processing were also developed. A Selective SPIRE technique that chooses between Combined and Spectral SPIRE reflectance estimates was developed; it maximizes estimation performance on both modified and unmodified pixels. The different SPIRE algorithms were tested on HYDICE airborne sensor hyperspectral data, and their reflectance estimates were compared to those from the physics-based ATmospheric REMoval (ATREM) and the Empirical Line Method atmospheric compensation algorithms. SPIRE algorithm performance was found to be nearly identical to the ELM ground-truth based results. SPIRE algorithms performed better than ATREM overall, and significantly better under high clouds and haze. Minimum-distance classification experiments demonstrated SPIRE's superior performance over both ATREM and ELM in cross-image supervised classification applications. The taxonomy of SPIRE algorithms was presented and suggestions were made concerning which SPIRE algorithm is recommended for various applications.<br>by Herbert Erik Mattias Viggh.<br>Ph.D.

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Asboth, Viktoria. "Studying dusty star-forming galaxies with Herschel-SPIRE." Thesis, University of British Columbia, 2015. http://hdl.handle.net/2429/55041.

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Observations suggest that almost half of the total light emitted by stars in the Universe is absorbed by dust, and the emission is re-radiated at far-infrared and submillimeter wavelengths. Dusty star-forming galaxies play a significant role in the stellar mass build-up at high redshift, but their contribution to the cosmic star formation rate density at z > 4 is still unknown, due to the currently limited availability of statistically significant high-redshift dusty galaxy samples. In this thesis we analyze data from two large area surveys, the HerMES Large Mode Survey (HeLMS) and the Herschel Stripe 82 Survey (HerS), observed with the Herschel-SPIRE instrument at far-infrared wavelengths of 250, 350 and 500 μm. We describe the process of constructing maps from detector data that provide an unbiased estimate of the sky signal, then we use a map-based detection method to assemble a large catalog of candidate z > 4 dusty star-forming galaxies detected in HeLMS. The large area of the survey allows us to detect a significant number of sources and we are able to determine the differential number counts of these galaxies at 500 μm. We find an excess of such high-redshift galaxies compared to model predictions, and our counts suggest strong evolution in their properties. We examine the properties of our sources at different wavelengths. Follow-up observations with ALMA, SCUBA-2 and ACT strengthen our initial assumption that the detected population consists of high-z dusty galaxies with their spectrum dominated by thermal dust emission, best fitted with an optically thick modified blackbody. These follow-up observations also allow us to examine the biasing effects in our number counts due to blending of nearby sources. We also investigate the mean dusty star formation activity in moderate redshift massive galaxy clusters detected by the Atacama Cosmology Telescope. We find that, on average, there is an excess of far-infrared emission in the line of sight of these clusters. Finding dusty star-forming galaxies in massive clusters implies that the environment can affect the star formation activity in galaxies.<br>Science, Faculty of<br>Physics and Astronomy, Department of<br>Graduate

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Buckee, Fiona G. "Reconstructing a Latina temple spire : Temple 45, Sanchi." Thesis, Cardiff University, 2010. http://orca.cf.ac.uk/54362/.

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The initial aim of this thesis is to reconstruct, through drawings, the original design of the spire from Temple 45, a ruined Latina temple from the Buddhist, World Heritage Site of Sanchi in Madhya Pradesh. The hundreds of un-analysed architectural fragments from the temple that survive on site are the primary data for this project: a veritable three-dimensional jigsaw puzzle of pieces waiting to be studied and reassembled. In order to turn the mass of architectural data collected at Sanchi into a virtual reconstruction of the spire from Temple 45, an authentic and detailed method of Latina spire design must be used. Finding such a method, one ratified by the Vastusasastras, by the shape of surviving Latina superstructures, and by the proportions of Temple 45 and its spire courses, forms the second, broader research question of the thesis. Although Latina temples are a seminal feature of North Indian temple architecture, scholars' explanations of how they were designed are inconsistent, incomplete and often unconvincing. In pursuit of this design method, therefore, the thesis explores the origination and development of the Latina temple form across Central India. It interrogates contemporary scholars' theories of Latina spire design and investigates the role that the Vastusasdstras may have played in the practises of early temple architects. Vastusasastric descriptions of Latina spire design are turned into drawings of spire elevations in order to assess their credibility, and in doing so a particular method of spire design is ratified and additional design details are suggested in order to provide a working explanation. Using this method, four sets of spire proportions given in a West Indian text called the DiparUava are validated. These are shown to create convincing Latina elevations with proportions that are borne out by surviving Central Indian Latina temples, by an engraving of a half Latina spire carved into the hallway of the Harihara 2 Temple in Osian, and by the proportions of Temple 45 its fragmented remains. Drawing from these findings, and returning to the initial aim of the thesis, the thesis proposes a detailed and convincing elevation of the spire from Temple 45.

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Chiou, Stefanie Chiawhei 1980. "SPIRE : systems for plan recovery in intelligent environments." Thesis, Massachusetts Institute of Technology, 2004. http://hdl.handle.net/1721.1/27095.

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Thesis (M. Eng. and S.B.)--Massachusetts Institute of Technology, Dept. of Electrical Engineering and Computer Science, 2004.<br>Includes bibliographical references (leaves 29-30).<br>As intelligent spaces have become more prevalent, the need for diagnosis and recovery from failures in these spaces has also grown. In an effort to make these types of spaces more useable for people who neither care about nor want to understand the underlying technology, encapsulation of high-level ideas into plans is being explored. Unfortunately, these plans are not always executed flawlessly. To deal with these failures, we have developed a system for plan recovery in intelligent spaces called a desktop multi-player virtual simulation game. In Charles River City, students work in teams to SPRIE. SPRIE is an automated system that uses a two-stage process for recovery from plan execution failures. In the first stage, the failure is diagnosed using Bayesian networks. In the second stage, a alternate plan is selected to recover from the failure. By automating the recovery process, the burden of understand the underlying architecture of the intelligent space is removed from the user.<br>by Stefanie Chiawhei Chiou.<br>M.Eng.and S.B.

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Rykala, Adam. "Star formation studies using the Herschel-SPIRE Imaging FTS." Thesis, Cardiff University, 2011. http://orca.cf.ac.uk/19702/.

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The study of low mass star formation in our local Galaxy is particularly suited to HERSCHEL. The SPIRE spectrometer and photometer aboard the spacecraft operate in the ~ 200 - 600�m range and are well suited to probe the cold, dusty environments in molecular clouds where prestellar cores reside. The SPIRE FTS spectrometer is an interferometer, and this instrument design has strengths and weaknesses which are im- portant to understand when using data from the instrument. Herschel is set to continue groundbreaking work in the infrared, building upon earlier work from ISO, IRAS, and SPITZER, probing deep into star forming regions and improving our knowledge of the processes within. In this PhD thesis, we outline the current body of knowledge in low mass star formation. We examine the properties of the SPIRE FTS as a spectrometerusing a small, laboratory designed desktop FTS. We study the intrinsic properties of the instrument, as a way of understanding issues we are likely to see when using the SPIRE FTS in ight. With these issues firmly in mind, we examine the creation and use of SLIDE - an interactive IDL-based tool for processing SPIRE FTS data. SLIDE can extract line and continuum information from SPIRE FTS SEDs. We outline the creation, testing and use of SLIDE and provide examples of the use of SLIDE in astronomy with some examples from the literature. We then use the line information we extract from a variety of sources with the spectrometer, to examine how SED fitting from photometer data could be affected by line contamination. We simulate a wide range of greybodies with noise and line con- tamination and examine how SED fitting is affected. Our simulations conclude that line contamination is not enough to affect the recovery of temperature and spectral index B significantly. Finally we use the information we have deduced to examine SPIRE FTS SEDs of L1689B - a prestellar core located in Ophiuchus. Our SED fitting of the core confirms that this core is starless with no internal heating source, and the spectral index profile over the core morphology is consistent with an increasing density of fractal aggregrate grains towards the centre. The increase in grain density and spectral index profile is also in agreement with previous CO depletion data. Fractal grain growth of this nature is consistent with dust grain models.

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Dahlgaard, Katja. "The role of Cappuccino and Spire in Drosophila axis specification." Thesis, University of Cambridge, 2008. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.611859.

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Sibthorpe, Bruce. "Characterisation and optimisation of the Herschel-SPIRE imaging through simulations." Thesis, Cardiff University, 2007. http://orca.cf.ac.uk/54580/.

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The Spectral and Photometric Imaging Receiver (SPIRE) is one of the three instruments on-board the European Space Agency's Herschel Space Observatory, due for launch in 2008. SPIRE is a dual instrument comprising a photometer, and imaging Fourier transform spectrometer. This thesis deals with the design and operation of a software simulator for the SPIRE photometer. The simulator architecture and modelling methods are described, and the fidelity of its output verified. This simulation software is then used to optimise and characterise data from the SPIRE photometer. The optimum observing parameters are derived, in order to maximise observing efficiency, and data quality. The impact of uncorrelated 1/f noise on the extraction of sources of arbitrary scale is assessed, and quantified. This work is also extended to include the impact of uncorrected 1/f noise on observations of sources in a confused environment. These results provide important information regarding the quality of SPIRE photometer data for the planning of large survey observations. The simulator is also an active tool within the SPIRE Instrument Control Centre team, and its use in the selection of the SPIRE map making algorithm is described. This thesis also contains an analysis of observations of the Cassiopeia A supernova remnant made with the Balloon-borne Large Aperture submillimetre Telescope (BLAST), an instrument based on the SPIRE photometer design. This analysis assesses the hypothesis that supernovae might be a significant dust formation mechanism in the universe, as proposed in recent literature. Results from this study suggest that this hypothesis may be correct, but that evidence from previous observations might in fact be upper limits to the total mass of dust, rather than an absolute measurement.

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Books on the topic "Spire"

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Patterson, Richard North. The spire. Center Point Pub., 2009.

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Patterson, Richard North. The spire. St. Martin's Paperbacks, 2010.

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(Firm), Ian Ritchie Architects. The Spire =: Túr solais. Categorical Books, 2004.

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Cordell, Bruce R. The sinister spire: Adventure. Wizards of the Coast, 2007.

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Cordell, Bruce R. The sinister spire: Adventure. Wizards of the Coast, 2007.

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Cordell, Bruce R. The sinister spire: Adventure. Wizards of the Coast, 2007.

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National Arboretum (U.S.). Gardens Unit., ed. Euonymus japonicus 'Green spire'. [Gardens Unit, U.S. National Arboretum, U.S. Dept. of Agriculture, Agricultural Research Service, 1999.

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National Arboretum (U.S.). Gardens Unit, ed. Euonymus japonicus 'Green spire'. [Gardens Unit, U.S. National Arboretum, U.S. Dept. of Agriculture, Agricultural Research Service, 1999.

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Cordell, Bruce R. The sinister spire: Adventure. Wizards of the Coast, 2007.

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National Arboretum (U.S.). Gardens Unit., ed. Euonymus japonicus 'Green spire'. U.S. National Arboretum Elite Plant, Gardens Unit, U.S. National Arboretum, U.S. Dept. of Agriculture, Agricultural Research Service, 1999.

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Book chapters on the topic "Spire"

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Ben-Shahar, Tal. "The SPIRE of Happiness." In Happiness Studies. Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-64869-5_3.

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Cappaert, Jeroen. "The Spire Small Satellite Network." In Handbook of Small Satellites. Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-20707-6_93-1.

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Cappaert, Jeroen. "The Spire Small Satellite Network." In Handbook of Small Satellites. Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-36308-6_93.

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Spire-Uran, Marie-Brunette. "Thérèse Marix-Spire (1898-1987)." In La bibliothèque de la Sorbonne. Éditions de la Sorbonne, 2021. http://dx.doi.org/10.4000/12itj.

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Sumner, Rosemary. "THe Spire: Summaries And Critical Commentary." In Macmillan Master Guides The Spire By William Golding. Macmillan Education UK, 1986. http://dx.doi.org/10.1007/978-1-349-08221-6_2.

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Qi, Chenyang, Zhengzhong Tu, Keren Ye, et al. "SPIRE: Semantic Prompt-Driven Image Restoration." In Lecture Notes in Computer Science. Springer Nature Switzerland, 2024. http://dx.doi.org/10.1007/978-3-031-73661-2_25.

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Sumner, Rosemary. "What The Spire Is About: A Conversation." In Macmillan Master Guides The Spire By William Golding. Macmillan Education UK, 1986. http://dx.doi.org/10.1007/978-1-349-08221-6_3.

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Jones, A. Richard. "Norwich Cathedral Spire: Why it Still Stands." In Medieval and Early Modern Art, Architecture and Archaeology in Norwich. Routledge, 2024. http://dx.doi.org/10.4324/9781003580386-13.

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Gindin, James. "The Metaphor: Pincher Martin, Free Fall and The Spire." In Macmillan Modern Novelists: William Golding. Palgrave Macmillan UK, 1988. http://dx.doi.org/10.1007/978-1-349-18987-8_4.

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Sumner, Rosemary. "William Golding: Life And Background." In Macmillan Master Guides The Spire By William Golding. Macmillan Education UK, 1986. http://dx.doi.org/10.1007/978-1-349-08221-6_1.

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Conference papers on the topic "Spire"

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Zhang, Jiahua, Jan-Peter Weiss, and John Braun. "Exploring Spire GNSS Reflections for Global Soil Moisture Monitoring." In IGARSS 2024 - 2024 IEEE International Geoscience and Remote Sensing Symposium. IEEE, 2024. http://dx.doi.org/10.1109/igarss53475.2024.10642541.

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Jia, Ning, Chun Yang, Jing Wang, Dong Tong, and Keyi Wang. "SPIRE." In the 9th ACM SIGPLAN/SIGOPS international conference. ACM Press, 2013. http://dx.doi.org/10.1145/2451512.2451516.

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Li, Chung-Sheng, Lawrence D. Bergman, Yuan-Chi Chang, Vittorio Castelli, and John R. Smith. "SPIRE." In the 2000 ACM SIGMOD international conference. ACM Press, 2000. http://dx.doi.org/10.1145/342009.336583.

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Gorea, Adriana, Felicia Bello, and Raquel Ventura. "Spire to Wear." In Pivoting for the Pandemic. Iowa State University Digital Press, 2020. http://dx.doi.org/10.31274/itaa.11982.

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Griffin, Matthew J., Bruce M. Swinyard, and Laurent Vigroux. "The Herschel-SPIRE instrument." In SPIE Astronomical Telescopes + Instrumentation, edited by John C. Mather. SPIE, 2004. http://dx.doi.org/10.1117/12.552695.

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Griffin, Matthew J., Bruce M. Swinyard, and Laurent G. Vigroux. "SPIRE instrument for FIRST." In Astronomical Telescopes and Instrumentation, edited by James B. Breckinridge and Peter Jakobsen. SPIE, 2000. http://dx.doi.org/10.1117/12.393958.

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Swinyard, Bruce M., Kjetil Dohlen, Didier Ferand, et al. "Imaging FTS for Herschel SPIRE." In Astronomical Telescopes and Instrumentation, edited by John C. Mather. SPIE, 2003. http://dx.doi.org/10.1117/12.461529.

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Woodcraft, Adam L., Hien Nguyen, James Bock, et al. "Understanding the Herschel-SPIRE bolometers." In SPIE Astronomical Telescopes + Instrumentation, edited by William D. Duncan, Wayne S. Holland, Stafford Withington, and Jonas Zmuidzinas. SPIE, 2008. http://dx.doi.org/10.1117/12.788789.

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Falcao, Eduardo, Matteus Silva, Ariel Luz, and Andrey Brito. "Supporting Confidential Workloads in SPIRE." In 2022 IEEE International Conference on Cloud Computing Technology and Science (CloudCom). IEEE, 2022. http://dx.doi.org/10.1109/cloudcom55334.2022.00035.

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Reichert, Beatriz M., and Rafael R. Obelheiro. "IT-SPIRE: Improving the Resilience of the SPIFFE/SPIRE Architecture with an Intrusion-Tolerant Server." In LADC 2024: 13th Latin-American Symposium on Dependable and Secure Computing. ACM, 2024. https://doi.org/10.1145/3697090.3697108.

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Reports on the topic "Spire"

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Campbell, Murray. EPI-SPIRE: A Bio-Surveillance Prototype. Defense Technical Information Center, 2005. http://dx.doi.org/10.21236/ada435473.

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Stevens, Sam N., and Augustin J. Calapristi. Evaluation of Spatial Paradigm for Information Retrieval and Exploration (SPIRE) Technology for Trauma Data Analysis. Defense Technical Information Center, 1997. http://dx.doi.org/10.21236/ada359248.

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Neitzel, D., T. Frest, and Washington Univ., Seattle, WA (USA)). Survey of Columbia River Basin Streams for Giant Columbia River Spire Snail Fluminicola columbiana and Great Columbia River limpet Fisherola nuttalli. Office of Scientific and Technical Information (OSTI), 1989. http://dx.doi.org/10.2172/5473804.

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Hall, Katelyn. Shoulder Spike. Iowa State University, Digital Repository, 2014. http://dx.doi.org/10.31274/itaa_proceedings-180814-1035.

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Cleary, Kevin. Periscopic Spine Surgery. Defense Technical Information Center, 2002. http://dx.doi.org/10.21236/ada402363.

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Cleary, Kevin R. Periscopic Spine Surgery. Defense Technical Information Center, 2005. http://dx.doi.org/10.21236/ada433062.

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Cleary, Kevin R. Periscopic Spine Surgery. Defense Technical Information Center, 2005. http://dx.doi.org/10.21236/ada434394.

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Cleary, Kevin R. Periscopic Spine Surgery. Defense Technical Information Center, 2008. http://dx.doi.org/10.21236/ada510225.

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Pritchard, Joy, H. R. Whay, and A. Brown. Withers/spine lesions. Brooke, 2011. http://dx.doi.org/10.46746/gaw.2020.abi.les.wspin.

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Ozair, Ahmad. Advancing spine evidence synthesis: North American Spine Society (NASS) Guidelines. World Evidence-based Healthcare Day, 2024. http://dx.doi.org/10.70253/ukwl6380.

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