Academic literature on the topic 'HiRISE'

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Journal articles on the topic "HiRISE"

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Sutton, Sarah S., Matthew Chojnacki, Alfred S. McEwen, et al. "Revealing Active Mars with HiRISE Digital Terrain Models." Remote Sensing 14, no. 10 (2022): 2403. http://dx.doi.org/10.3390/rs14102403.

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Many discoveries of active surface processes on Mars have been made due to the availability of repeat high-resolution images from the High Resolution Imaging Science Experiment (HiRISE) onboard the Mars Reconnaissance Orbiter. HiRISE stereo images are used to make digital terrain models (DTMs) and orthorectified images (orthoimages). HiRISE DTMs and orthoimage time series have been crucial for advancing the study of active processes such as recurring slope lineae, dune migration, gully activity, and polar processes. We describe the process of making HiRISE DTMs, orthoimage time series, DTM mosaics, and the difference of DTMs, specifically using the ISIS/SOCET Set workflow. HiRISE DTMs are produced at a 1 and 2 m ground sample distance, with a corresponding estimated vertical precision of tens of cm and ∼1 m, respectively. To date, more than 6000 stereo pairs have been acquired by HiRISE and, of these, more than 800 DTMs and 2700 orthoimages have been produced and made available to the public via the Planetary Data System. The intended audiences of this paper are producers, as well as users, of HiRISE DTMs and orthoimages. We discuss the factors that determine the effective resolution, as well as the quality, precision, and accuracy of HiRISE DTMs, and provide examples of their use in time series analyses of active surface processes on Mars.
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Wang, Yiran, and Bo Wu. "COMPARISON AND CO-REGISTRATION OF DEMS GENERATED FROM HiRISE AND CTX IMAGES." ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences XLI-B4 (June 14, 2016): 511–17. http://dx.doi.org/10.5194/isprs-archives-xli-b4-511-2016.

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Images from two sensors, the High-Resolution Imaging Science Experiment (HiRISE) and the Context Camera (CTX), both on-board the Mars Reconnaissance Orbiter (MRO), were used to generate high-quality DEMs (Digital Elevation Models) of the Martian surface. However, there were discrepancies between the DEMs generated from the images acquired by these two sensors due to various reasons, such as variations in boresight alignment between the two sensors during the flight in the complex environment. This paper presents a systematic investigation of the discrepancies between the DEMs generated from the HiRISE and CTX images. A combined adjustment algorithm is presented for the co-registration of HiRISE and CTX DEMs. Experimental analysis was carried out using the HiRISE and CTX images collected at the Mars Rover landing site and several other typical regions. The results indicated that there were systematic offsets between the HiRISE and CTX DEMs in the longitude and latitude directions. However, the offset in the altitude was less obvious. After combined adjustment, the offsets were eliminated and the HiRISE and CTX DEMs were co-registered to each other. The presented research is of significance for the synergistic use of HiRISE and CTX images for precision Mars topographic mapping.
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Wang, Yiran, and Bo Wu. "COMPARISON AND CO-REGISTRATION OF DEMS GENERATED FROM HiRISE AND CTX IMAGES." ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences XLI-B4 (June 14, 2016): 511–17. http://dx.doi.org/10.5194/isprsarchives-xli-b4-511-2016.

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Images from two sensors, the High-Resolution Imaging Science Experiment (HiRISE) and the Context Camera (CTX), both on-board the Mars Reconnaissance Orbiter (MRO), were used to generate high-quality DEMs (Digital Elevation Models) of the Martian surface. However, there were discrepancies between the DEMs generated from the images acquired by these two sensors due to various reasons, such as variations in boresight alignment between the two sensors during the flight in the complex environment. This paper presents a systematic investigation of the discrepancies between the DEMs generated from the HiRISE and CTX images. A combined adjustment algorithm is presented for the co-registration of HiRISE and CTX DEMs. Experimental analysis was carried out using the HiRISE and CTX images collected at the Mars Rover landing site and several other typical regions. The results indicated that there were systematic offsets between the HiRISE and CTX DEMs in the longitude and latitude directions. However, the offset in the altitude was less obvious. After combined adjustment, the offsets were eliminated and the HiRISE and CTX DEMs were co-registered to each other. The presented research is of significance for the synergistic use of HiRISE and CTX images for precision Mars topographic mapping.
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Li, Yan Chun, Ji Hong Dong, Wei Li, et al. "Detailed Analysis of the HIRISE FPA." Key Engineering Materials 552 (May 2013): 64–68. http://dx.doi.org/10.4028/www.scientific.net/kem.552.64.

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The U.S.A has launched the Mars Orbiter. It brought a high resolution imaging science equipment, and that is the High Resolution Imaging Science Experiment camera(HIRISE). HIRISE is 0.5 m reflecting telescope, which is the highest one ever carried on a deep space mission, and it has a resolution of 1 microradian (μrad), or 0.3 m from an altitude of 300 km. HIRISE can investigate deposits and landforms resulting from geologic and climatic processes and assist in the evaluation of candidate. As a high degree of lightweight ultra-high resolution camera, the design of its FPA is unparalleled .Therefore we should study and learn it carefully. In this article, first of all we discuss and analyze the characters of the HIRISE FPA in terms of the structural layout, material selection, splicing of the CCD, the CCD package, electronics, processing and transmission, and thermal control measures implementation. Next we put forward the design method of highly lightweight space optical remote sensor FPA combined with the characters of the HIRISE FPA, which can provide a reference to the design of the FPA for some space remote sensings.
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Sutton, S. S., A. K. Boyd, R. L. Kirk, et al. "CORRECTING SPACECRAFT JITTER IN HIRISE IMAGES." ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences XLII-3/W1 (July 25, 2017): 141–48. http://dx.doi.org/10.5194/isprs-archives-xlii-3-w1-141-2017.

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Mechanical oscillations or vibrations on spacecraft, also called pointing jitter, cause geometric distortions and/or smear in high resolution digital images acquired from orbit. Geometric distortion is especially a problem with pushbroom type sensors, such as the High Resolution Imaging Science Experiment (HiRISE) instrument on board the Mars Reconnaissance Orbiter (MRO). Geometric distortions occur at a range of frequencies that may not be obvious in the image products, but can cause problems with stereo image correlation in the production of digital elevation models, and in measuring surface changes over time in orthorectified images. The HiRISE focal plane comprises a staggered array of fourteen charge-coupled devices (CCDs) with pixel IFOV of 1 microradian. The high spatial resolution of HiRISE makes it both sensitive to, and an excellent recorder of jitter. We present an algorithm using Fourier analysis to resolve the jitter function for a HiRISE image that is then used to update instrument pointing information to remove geometric distortions from the image. Implementation of the jitter analysis and image correction is performed on selected HiRISE images. Resulting corrected images and updated pointing information are made available to the public. Results show marked reduction of geometric distortions. This work has applications to similar cameras operating now, and to the design of future instruments (such as the Europa Imaging System).
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Otten, G. P. P. L., A. Vigan, E. Muslimov, et al. "Direct characterization of young giant exoplanets at high spectral resolution by coupling SPHERE and CRIRES+." Astronomy & Astrophysics 646 (February 2021): A150. http://dx.doi.org/10.1051/0004-6361/202038517.

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Studies of atmospheres of directly imaged extrasolar planets with high-resolution spectrographs have shown that their characterization is predominantly limited by noise on the stellar halo at the location of the studied exoplanet. An instrumental combination of high-contrast imaging and high spectral resolution that suppresses this noise and resolves the spectral lines can therefore yield higher quality spectra. We study the performance of the proposed HiRISE fiber coupling between the direct imager SPHERE and the spectrograph CRIRES+ at the Very Large Telescope for spectral characterization of directly imaged planets. Using end-to-end simulations of HiRISE we determine the signal-to-noise ratio (S/N) of the detection of molecular species for known extrasolar planets in H and K bands, and compare them to CRIRES+. We investigate the ultimate detection limits of HiRISE as a function of stellar magnitude, and we quantify the impact of different coronagraphs and of the system transmission. We find that HiRISE largely outperforms CRIRES+ for companions around bright hosts like β Pictoris or 51 Eridani. For an H = 3.5 host, we observe a gain of a factor of up to 16 in observing time with HiRISE to reach the same S/N on a companion at 200 mas. More generally, HiRISE provides better performance than CRIRES+ in 2 h integration times between 50 and 350 mas for hosts with H < 8.5 and between 50 and 700 mas for H < 7. For fainter hosts like PDS 70 and HIP 65426, no significant improvements are observed. We find that using no coronagraph yields the best S/N when characterizing known exoplanets due to higher transmission and fiber-based starlight suppression. We demonstrate that the overall transmission of the system is in fact the main driver of performance. Finally, we show that HiRISE outperforms the best detection limits of SPHERE for bright stars, opening major possibilities for the characterization of future planetary companions detected by other techniques.
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Hou, Yifan, Xun Geng, Shuai Xing, Yonghe Tang, and Qing Xu. "RADIOMETRIC CALIBRATION OF MARS HiRISE HIGH RESOLUTION IMAGERY BASED ON FPGA." ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences XLI-B4 (June 13, 2016): 405–9. http://dx.doi.org/10.5194/isprs-archives-xli-b4-405-2016.

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Due to the large data amount of HiRISE imagery, traditional radiometric calibration method is not able to meet the fast processing requirements. To solve this problem, a radiometric calibration system of HiRISE imagery based on field program gate array (FPGA) is designed. The montage gap between two channels caused by gray inconsistency is removed through histogram matching. The calibration system is composed of FPGA and DSP, which makes full use of the parallel processing ability of FPGA and fast computation as well as flexible control characteristic of DSP. Experimental results show that the designed system consumes less hardware resources and the real-time processing ability of radiometric calibration of HiRISE imagery is improved.
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Hou, Yifan, Xun Geng, Shuai Xing, Yonghe Tang, and Qing Xu. "RADIOMETRIC CALIBRATION OF MARS HiRISE HIGH RESOLUTION IMAGERY BASED ON FPGA." ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences XLI-B4 (June 13, 2016): 405–9. http://dx.doi.org/10.5194/isprsarchives-xli-b4-405-2016.

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Due to the large data amount of HiRISE imagery, traditional radiometric calibration method is not able to meet the fast processing requirements. To solve this problem, a radiometric calibration system of HiRISE imagery based on field program gate array (FPGA) is designed. The montage gap between two channels caused by gray inconsistency is removed through histogram matching. The calibration system is composed of FPGA and DSP, which makes full use of the parallel processing ability of FPGA and fast computation as well as flexible control characteristic of DSP. Experimental results show that the designed system consumes less hardware resources and the real-time processing ability of radiometric calibration of HiRISE imagery is improved.
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Tao, Y., J. P. Muller, K. Willner, et al. "3D Data Products and Web-GIS for Mars Rover Mission for Seamless Visualisation from Orbit to Ground-level." ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences XL-4 (April 23, 2014): 249–56. http://dx.doi.org/10.5194/isprsarchives-xl-4-249-2014.

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This paper presents a wide range of research and processing results in the area of multi-resolution orbital data co-registration, multiresolution ground 3D reconstruction, and orbit-to-ground data fusion, achieved within the EU-FP7 PRoVisG and PRoViDE project. We focus on three NASA rover missions, MER-A, MER-B, and MSL, to provide examples of automated methods for producing coregistered, multi-resolution 3D products. We highlight the mis-registration discovered between current HiRISE to HRSC datasets, CTX to HRSC and HiRISE to CTX co- results, wide baseline stereo reconstruction results of rover imagery, ground-to-orbit coregistration, i.e. reconstructed wide baseline ground ORI and HiRISE ORI co-registration, and extensive exploitation of the coregistered datasets in visualisation and interactive web-GIS.
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Wang, Y., and B. Wu. "IMPROVED LARGE-SCALE SLOPE ANALYSIS ON MARS BASED ON CORRELATION OF SLOPES DERIVED WITH DIFFERENT BASELINES." ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences XLII-3/W1 (July 25, 2017): 155–61. http://dx.doi.org/10.5194/isprs-archives-xlii-3-w1-155-2017.

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The surface slopes of planetary bodies are important factors for exploration missions, such as landing site selection and rover manoeuvre. Generally, high-resolution digital elevation models (DEMs) such as those generated from the HiRISE images on Mars are preferred to generate detailed slopes with a better fidelity of terrain features. Unfortunately, high-resolution datasets normally only cover small area and are not always available. While lower resolution datasets, such as MOLA, provide global coverage of the Martian surface. Slopes generated from the low-resolution DEM will be based on a large baseline and be smoothed from the real situation. In order to carry out slope analysis at large scale on Martian surface based low-resolution data such as MOLA data, while alleviating the smoothness problem of slopes due to its low resolution, this paper presents an amplifying function of slopes derived from low-resolution DEMs based on the relationships between DEM resolutions and slopes. First, slope maps are derived from the HiRISE DEM (meter-level resolution DEM generated from HiRISE images) and a series of down-sampled HiRISE DEMs. The latter are used to simulate low-resolution DEMs. Then the high-resolution slope map is down- sampled to the same resolution with the slope map from the lower-resolution DEMs. Thus, a comparison can be conducted pixel-wise. For each pixel on the slope map derived from the lower-resolution DEM, it can reach the same value with the down-sampled HiRISE slope by multiplying an amplifying factor. Seven sets of HiRISE images with representative terrain types are used for correlation analysis. It shows that the relationship between the amplifying factors and the original MOLA slopes can be described by the exponential function. Verifications using other datasets show that after applying the proposed amplifying function, the updated slope maps give better representations of slopes on Martian surface compared with the original slopes.
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Dissertations / Theses on the topic "HiRISE"

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Ayoub, François. "Suivi de changements morphologiques de surface à partir d'images aériennes et satellitaires, sur Terre et Mars." Toulouse 3, 2014. http://thesesups.ups-tlse.fr/2621/.

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Les progrés en télédétection permettent désormais une mesure dense et précise des déplacements de la surface terrestre à partir de l'analyse fine d'images satellitaires acquises à différentes dates. Ces méthodes permettent de détecter et de quantifier par exemple la déformation co-sismique du sol, l'avancée ou le recul de glacier, la migration de dunes, ou les glissements de terrain, survenus entre les dates d'acquisition des images. Au cours de cette thèse nous étudions 1) l'extension des méthodes de traitement d'images satellitaires aux images aériennes et 2) l'applicabilitée des méthodes satellitaires terrestres en planétologie, en particulier pour l'étude des processus éoliens sur mars. L'imagerie aérienne, dont les premières acquisitions datent d'avant l'ère satellitaire et offrant de meilleures résolutions spatiales, constitue une source d'images intéressante pour le suivi des processus de surface terrestre. Nous proposons une méthode de traitement d'images aériennes, basée sur les méthodes satellitaires et prenant en compte les spécificités des images aériennes d'archive acquises sur film notamment. Le potentiel (e. G. , mesure de déplacement de quelques centimètres, revisite d'évènements passés, extension de séries temporelles) et limites (e. G. , déformation du film, défauts de numérisation) de ce type d'imagerie sont caractérisés. La méthode est appliquée à la mesure de l'ouverture du rift de Krafla en Icelande (1975-1984) à partir de deux série d'images aériennes (1957, 1990), d'une image espion déclassifiée et d'une image satellitaire. En seconde partie, nous appliquons ces techniques sur mars via l'analyse d'une paire d'images HIRISE pour le suivi d'activité d'un champ de dunes. Après adaptation des méthodes terrestres au capteur HiRISE (e. G. , géométrie de l'instrument, projection cartographique martienne), nous mesurons la migration des rides de sable couvrant les dunes et estimons un flux de sable associé, qui s'avère être d'intensité comparable à celui de certains champs de dunes terrestres. L'analyse est étendue à une série temporelle de 10 images HiRISE, permettant ainsi de caractériser la variation saisonnière du flux au cours d'une année martienne. Cette variation saisonnière est ensuite utilisée conjointement avec une prédiction de flux issue d'une simulation atmosphérique pour calibrer la contrainte en cisaillement du sable sur mars<br>The analysis of satellites imagery acquired at different dates allows the measurement of Earth surface displacement (earthquake ground deformation, glacier advance and retreat, sand dunes migration, slow-moving landslide,. . . ) that occured between the images acquisitions. In this thesis we investigate 1) the extension of the processing techniques established for satellite imagery to aerial imagery, and 2) the applicability of Earth-based technique to monitor eolian surface processes on Mars. Aerial imagery, whose first acquisition dates back decades before the satellite era, and whose ground resolution is higher than satellite one, can be relevant to monitor Earth surface displacement. We present a methodological extension of the satellite technique to aerial imagery. Potential and limitations are investigated. Application to the Krafla rift opening in Iceland (1975-1984), using aerial imagery, declassied spy imagery, and modern satellite imagery is presented. Next, we applied the method to Mars imagery taking advantage of the high resolution HiRISE instrument. A pair of HiRISE images is processed to monitor the activitys of a dune field. We measured sand ripple migration and inferred a sand flux comparable to some the Earth dune fields sand flux. We then expand our processing to a time-series of 10 HiRISE images, and characterized the seasonal variability of the sand flux throughout the year. This seasonal sand flux variability is used jointly with a sand flux prediction from atmospheric simulations to constrain the sand mobility threshold
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Re, Cristina. "THREE-DIMENSIONAL RECONSTRUCTION OF PLANETARY SURFACES FROM STEREO SATELLITE IMAGES." Doctoral thesis, Università degli studi di Padova, 2014. http://hdl.handle.net/11577/3424553.

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The dissertation is related to the work of the team involved in the development of a STereo Camera (STC) for the ESA-JAXA mission BepiColombo to Mercury (Cremonese et al, 2009) and is focused on validation of the STC 3D reconstruction process and software development for DTM generation. STC will provide the images for the global mapping in stereo mode of the entire Hermean surface. In order to estimate and characterize the actual stereo reconstruction capabilities of STC, an indoor Stereo Validation Setup (SVS) has been developed and tested in laboratory with a functional breadboard. The stereo validation concept has been proven by comparing the DTMs produced by the Dense Matcher software (DM), developed at University of Parma, from a series of rock samples stereo pairs with the ones produced by an high resolution laser scanning system. The same procedure will be therefore applied to the STC flight model. Originally developed for use in close range photogrammetry, the DM program, in these years, has been optimized to cope with very high resolution images provided by the most recent missions (LROC NAC and HiRISE). Efforts have been mainly directed to the improvement of the image correlation kernel and of the process automation. More specifically, important changes have been made to the correlation kernel, still maintaining its high performance in terms of precision and accuracy by implementing an advanced version of the Least Squares Matching (LSM) algorithm. An iterative algorithm has been developed to adapt the geometric transformation in image resampling using different shape functions. Commonly an affine transformation is used as geometric transformation in the area-based matching algorithms implemented in the Least Squares Optimization; however, perspective changes due to rough terrain morphology are difficult to accommodate by an area-based stereo correlator with such model only. Many authors (Sutton & al., 1988) (Bruck & al., 1989) (Lu & Cary, 2000) found that the use of a simplified shape function requires less computational load but yields lower accuracy when significant changes in the terrain curvature occurs. Also Bethmann (Bethmann & al., 2010) showed that using different shape functions to model the geometric transformation in LSM can bring higher accuracy and solve, in some cases, numerical problems like pixel-locking (Stein, Andreas, & Larry, 2006). In this context, the new DM software uses, rather than the common affine transformation, alternative functional models in the geometrical transformation involved during LSM to handle perspective differences. The evaluation of the alternative models has been carried out in terms of accuracy and evaluating statistically the quality of the solution convergence. The test scenarios have been organized considering many processing variables and different set of images, in order to identify the difficulties in the matching phase. Furthermore, the performance of the image correlation kernel of the program has been evaluated through comparisons with DTMs generated by other well established software like Socet Set by Bae System and Ames Stereo Pipeline (NASA) on HiRISE stereo pairs. Comparisons have been also made with the DTMs produced with NAC stereo-pairs by the VICAR software by DLR (German Aerospace Center), as well as against the LOLA altimeter tracks. The results look very promising and represent a concrete proof of the capability of Dense Matcher software in dealing with HiRISE and LROC images, two of the most significant examples of high resolution orbital imagers.<br>Questo lavoro di tesi è connesso alle attività del team coinvolto nello sviluppo della Stereo Camera (STC) per la missione ESA-JAXA Bepicolombo su Mercurio (Cremonese et al, 2009) ed è focalizzato alla validazione del processo di ricostruzione tridimensionale di STC insieme allo sviluppo del software per la generazione di DTM. STC fornirà le immagini per la mappatura globale dell’intera superficie di Mecurio in modalità stereo. Al fine di caratterizzare le effettive capacità di ricostruzione stereo di STC, un Setup di Validazione Stereo (SVS) è stato sviluppato e testato in laboratorio tramite un apposito breadboard. Il concetto di validazione stereo è stato collaudato confrontando i DTM (Digital Terrain Model) prodotti con Dense Matcher software (DM), sviluppato all’Università di Parma, rispetto al modello tridimansionale acquisito con un sistema laser ad alta risoluzione. La stessa procedura verrà applicata al modello di volo. Originariamente sviluppato per l’ambito della fotogrammetria dei vicini, il DM, in queesti anni è stato ottimizzato per gestire le immagini ad alta risoluzione fornite dalle più recenti missioni spaziali (LROC NAC and HiRISE). A questo scopo molti sforzi sono stati diretti al miglioramento del kernel connesso al processo di correlazione di immagine e anche allo sviluppo dell’automazione dell’intero processo. Più specificatamente, sono stati attuati una serie di miglioramenti algoritmici con l’implementazione di una versione avanzata dell’algorimo ai minimi quadrati (LSM) cercando di mantenere le elevate prestazioni in termini di precisione ed accuratezza già caratterizzanti il pacchetto software. L’algorimo che è stato introdotto permette di adattare la trasformazione geometrica coinvolta nel ricampionamento dell’immagine in maniera iterativa usando diverse funzioni di forma. Gli algoritmi di matching area-based che implementano ottimizzazioni ai minimi quadrati, impiegano come traformazione geometrica nel modello funzionale, la trasformazione Affine; tuttavia, i cambiamenti prospettici coinvolti in presenza di morfologie superficiali complesse, sono difficili da descrivere attraverso un algoritmo di correlazione che implementa tale modello a soli 6 parametri. Molti autori (Sutton & al., 1988) (Bruck & al., 1989) (Lu & Cary, 2000) sostengono che l’uso di modelli di semplici come l’Affine richiedano meno sforzo computazionale portando tuttavia all’ottenimento di accuratezze più basse qualora si incontrino complessità superficiali elevate. Anche Bethmann (Bethmann & al., 2010) dimostra che usare funzioni di forma di grado superiore per modellare le trasformazioni geometriche nel LSM può portare ad accuratezze superiori e si risolvono, in alcuni casi, problemi numerici come il cosiddetto “pixel-locking” (Stein, Andreas, & Larry, 2006). In questo contesto, il nuovo DM usa, piuttosto che la comune trasformazione Affine, modelli funzionali alternativi per la definizione delle trasformazioni geometriche coinvolte durante la stima ai minimi quadrati finalizzata ad modellare le differenze prospettiche tra le immagini. La valutazione dei modelli alternativi implementati nell’algoritmo di matching di DM è stata svolta in termini di accuratezza e analizzando statisticamente la qualità e il comportamento della convergenza alla soluzione. Lo scenario dei test ha previsto lo studio di diverse variabili di processamento e sono state impiegati diversi tipi di immagini al fine di identificare precisamente le difficoltà della fase di matching. Le performance del nuovo algoritmo di matching implementato nel programma DM è stato valutato anche eseguendo una serie di confronti tra i DTM generati e quelli ottenuti mediante altri pacchetti software ben collaudati come Socet Set della Bae System e Ames Stereo Pipeline (NASA) processando le coppie stereo di HiRISE. Per quanto riguarda una serie di immagini acquisite dalla camera NAC, una serie di confronti sono stati svolti con il software VICAR del DLR e anche le traccie fornite dal laser altimetro sono state impiegate come dato di riferimento. I risultati ottenuti dai confronti quali-quantitativi tra i vari modelli tridimensionali possono essere considerati una prova delle capacità di DM gestire le immagini ad altissima risoluzione fornite dalle camere HiRISE e LROC.
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Kesek, Helga, and Nilsson Frida. "Hiring Audit Assistants : 'Do not be late if you want to hire a graduate'." Thesis, Umeå universitet, Företagsekonomi, 2017. http://urn.kb.se/resolve?urn=urn:nbn:se:umu:diva-137150.

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The auditing profession is a popular career choice among business graduates, and the Big N firms hire large cohorts of audit assistants every year. The auditing profession is special in the way that it has a defined career ladder, as well as a high employee turnover rate. The hiring process involves contact both with the HR department and auditors from the operating business. Since the audit assistants are not expected to have great technical knowledge at the beginning of their employment, other things than the actual auditing skills must be tested during the hiring process.   In prior research, studies have been conducted from the perspective of the applicant, rather than the organizational perspective. There has been relatively little research on the recruitment of auditors, and most research has been conducted in another context than a Swedish one. The research question used for this thesis is: How do audit firms hire entry-level audit assistants, and what profile is desired by the HR department and the operating business?   The main purposes of this study are to explore the hiring process and what profile is desired, from both the HR department’s perspective and the operating business’ perspective. The study is qualitative, and the data was collected through semi-structured interviews with delegates from the largest audit firms in Sweden. The sample consisted of eleven informants including seven auditors and four recruiters.  The empirical findings suggest that the Big N firms in Sweden hire through a centralized HR-department, with a standardized process that is similar among all the firms. A lot of responsibility lies with the HR-department, but the auditors make the final determination if the applicant will fit into the group. The most important characteristics desired of an audit assistant are found to be social skills, team ability, and dedication, and these are assessed at the different steps of the hiring process. Finally, the findings suggest that the HR department and the delegates from the operating business of the HR firms agree on what profile they are looking for, however, there is no formal way of evaluating the hiring process in any of the firms. The contributions of this thesis can be of use for various actors, for example audit firms when developing their hiring strategies, regulatory authorities when discussing the development of the industry and educational bodies and students when preparing for a career within auditing. From an academic perspective, this study can be used as a point of departure for future research.
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Hiris, Lori E. "Atlantis unbound." Thesis, Montana State University, 2009. http://etd.lib.montana.edu/etd/2009/hiris/HirisL0509.pdf.

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The data derived from the study of the hereditary traits in Drosophila-Melanogaster remind the viewer of the tremendous potential in technology and genetic engineering. My Installation is witness to this ever-changing technology and how it shapes our culture, history, and politics. Dreams and nightmares coexist in this installation and my intent is merely to invite the viewer to consider the consequences. Inheritance in the age of database culture and the sovereignty of the Algorithm conspires to envision utopia - a New Atlantis: Bound and Unbound.
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Hall, Gerrit. "Startup hiring practices." Thesis, Massachusetts Institute of Technology, 2014. http://hdl.handle.net/1721.1/90217.

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Thesis: M.B.A., Massachusetts Institute of Technology, Sloan School of Management, 2014.<br>Cataloged from PDF version of thesis.<br>An exploratory qualitative study of hiring practices at technology startups in Silicon Valley and the USA.<br>by Gerrit Hall.<br>M.B.A.
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Gholston, Sylvia. "Developing Strategies for Hiring Managers: A Case Study on Hiring Employees." ScholarWorks, 2015. https://scholarworks.waldenu.edu/dissertations/1890.

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Gaining information about competency within hiring practices is critical for hiring managers seeking to hire skilled workers, improve employee fit, and lower hiring cost. Employee replacement cost ranges from 30% of an entry-level engineering or aeronautical employee's salary to 400% for a high-level employee in those fields. Guided by the transformational leadership theory and the decision-making theory, the purpose of this qualitative exploratory case study was to explore the hiring strategies used by 4 hiring managers to hire employees for organizational fit. The managers work within the aeronautics and engineering fields within the Southeast region of the United States, which included metro Atlanta, Georgia, and South Carolina. Data came from semistructured interviews with the hiring managers and company documents. Member checking was employed as a means of reinforcing credibility and trustworthiness. The data were analyzed and coded and 5 themes emerged: job descriptions and job requirements, resume review and interview matrices, practical demonstrations, leadership training, and compensation and benefits. By implementing practices that management supports, hiring managers can succeed in hiring employees for organizational fit. The findings may influence social change in that if hiring managers select the right workers, the business may sustain operations in the community and thus contribute to the prosperity of the employees, their families, the community, and the economy.
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Emendack, Yves Yatou. "Drought performance of millet (Panicum miliaceum) and sorghum (Sorghum bicolor (L.) Moench)." Berlin dissertation.de, 2007. http://www.dissertation.de/buch.php3?buch=5025.

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Connelly, Camryn. "Hiring Leaders in Catholic Schools." Thesis, Loyola Marymount University, 2014. http://pqdtopen.proquest.com/#viewpdf?dispub=3638153.

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<p>In the Archdiocese of Los Angeles, principals are often ill prepared for the demands of the job. According to Baxter (2012), every year in the Archdiocese approximately 30 principal vacancies are filled. Many of the Pastors who hire for these vacancies do not have an educational background, nor do they have much experience in hiring practices. With the increase of lay educators leading Catholic schools, not only are competent principals needed, but principals who can be Pastoral, educational, and managerial leaders (Manno, 1985). To increase the probability of hiring strong candidates for the principal vacancies in schools across the Archdiocese of Los Angeles, a hiring protocol is needed to standardize the process, while encouraging collaboration and input from multiple stakeholders. This case study implemented and evaluated a hiring protocol at one school site within the Archdiocese of Los Angeles. The protocol was designed to help Catholic schools hire qualified principals, and its development was guided by previous research on effective hiring procedures for such positions. The case-study data collected provides insight into the benefits and of using this specialized hiring protocol while also identifying potential changes to further strengthen the protocol. The results of the case study will be shared with the Department of Catholic Schools in the Archdiocese of Los Angeles to provide a framework for a principal hiring protocol that can be used at all school sites.
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Connelly, Camryn Marie. "Hiring Leaders in Catholic Schools." Digital Commons at Loyola Marymount University and Loyola Law School, 2014. https://digitalcommons.lmu.edu/etd/198.

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In the Archdiocese of Los Angeles, principals are often ill prepared for the demands of the job. According to Baxter (2012), every year in the Archdiocese approximately 30 principal vacancies are filled. Many of the Pastors who hire for these vacancies do not have an educational background, nor do they have much experience in hiring practices. With the increase of lay educators leading Catholic schools, not only are competent principals needed, but principals who can be Pastoral, educational, and managerial leaders (Manno, 1985). To increase the probability of hiring strong candidates for the principal vacancies in schools across the Archdiocese of Los Angeles, a hiring protocol is needed to standardize the process, while encouraging collaboration and input from multiple stakeholders. This case study implemented and evaluated a hiring protocol at one school site within the Archdiocese of Los Angeles. The protocol was designed to help Catholic schools hire qualified principals, and its development was guided by previous research on effective hiring procedures for such positions. The case-study data collected provides insight into the benefits and of using this specialized hiring protocol while also identifying potential changes to further strengthen the protocol. The results of the case study will be shared with the Department of Catholic Schools in the Archdiocese of Los Angeles to provide a framework for a principal hiring protocol that can be used at all school sites.
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Carlsson, Magnus. "Essays on discrimination in hiring /." Växjö : Växjö University Press, 2009. http://urn.kb.se/resolve?urn=urn:nbn:se:vxu:diva-5864.

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Books on the topic "HiRISE"

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Hawthorne, Nathaniel. The custom-house: The scarlet letter ; The hirise of the seven gables ; The Blithedale romance ; The marble faun. Peerage Books, 1986.

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1922-, Okamura Shigeru, Hirose Kyokusō 1807-1863, and Hirose Tansō 1782-1856, eds. Hirose Tansō, Hirose Kyokusō. Iwanami Shoten, 1991.

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Takahashi, Masahiko. Hirose Tansō. Ōita-ken Kyōiku Iinkai, 2014.

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editor, Inoue Toshiyuki 1942, ed. Hirose Tansō. Shibunkaku Shuppan, 2016.

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Hayashida, Shinnosuke1932. Hirose Tansō. Kenbun Shuppan, 2005.

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Gakkai, Nihon Rekish, ed. Hirose Tansō. Yoshikawa Kōbunkan, 1987.

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Collection, Hirose. Hirose Collection. Hirose Shūji, 2017.

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A, Landgrebe D., National Science Foundation (U.S.), and United States. National Aeronautics and Space Administration., eds. HIRIS performance study. School of Electrical Engineering, Purdue University, 1989.

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O'Hanlon, Michael. Hiring fairs & farm workers in North-West Ireland. Guildhall Press, 1992.

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Nakamura, Yukihiko. Hirose Senken Bunko mokuroku. Hakkō Hirose Senken Bunko, 1995.

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Book chapters on the topic "HiRISE"

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Soare, Richard. "Latitude-Dependent Mantle (in HiRISE) (with No Stratigraphically Associated Periglacial Landforms)." In Encyclopedia of Planetary Landforms. Springer New York, 2014. http://dx.doi.org/10.1007/978-1-4614-9213-9_626-1.

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Soare, Richard. "Latitude-Dependent Mantle (in HiRISE) (with No Stratigraphically Associated Periglacial Landforms)." In Encyclopedia of Planetary Landforms. Springer New York, 2022. http://dx.doi.org/10.1007/978-1-4614-9213-9_220-2.

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Soare, Richard. "Latitude-Dependent Mantle (in HiRISE) (with No Stratigraphically Associated Periglacial Landforms)." In Encyclopedia of Planetary Landforms. Springer New York, 2015. http://dx.doi.org/10.1007/978-1-4614-3134-3_626.

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Bährle-Rapp, Marina. "Hirse." In Springer Lexikon Kosmetik und Körperpflege. Springer Berlin Heidelberg, 2007. http://dx.doi.org/10.1007/978-3-540-71095-0_4768.

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Chun, Julia, Tyler Tingley, and William Lidwell. "Hiring." In The Elements of Education for School Leaders. Routledge, 2022. http://dx.doi.org/10.4324/9780429321641-22.

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Jakobus, Benjamin, Pedro Henrique Lobato Sena, and Claudio Souza. "Hiring." In Leadership Paradigms for Remote Agile Development. Apress, 2022. http://dx.doi.org/10.1007/978-1-4842-8719-4_4.

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Praz. "Hiring." In Link Technology to Your Long-Term Business Goals. Apress, 2022. http://dx.doi.org/10.1007/978-1-4842-8208-3_2.

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Sunderland, Alexandra. "Hiring." In Remote Engineering Management. Apress, 2022. http://dx.doi.org/10.1007/978-1-4842-8584-8_1.

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Shuster, Stephen M., and Michael J. Wade. "Hiring Selection." In Feminism and Evolutionary Biology. Springer US, 1997. http://dx.doi.org/10.1007/978-1-4615-5985-6_7.

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McCuller, Patrick. "Hiring Decisions." In How to Recruit and Hire Great Software Engineers. Apress, 2012. http://dx.doi.org/10.1007/978-1-4302-4918-4_8.

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Conference papers on the topic "HiRISE"

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Priyadharshini, J. Mary Hanna, C. Chrisil David, M. Jaikrish, and M. Aswin. "Leveraging Large Vision Models for Terrain Classification in HiRISE Mars Orbital Images." In 2024 15th International Conference on Computing Communication and Networking Technologies (ICCCNT). IEEE, 2024. http://dx.doi.org/10.1109/icccnt61001.2024.10725508.

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Heckman, Stephen M. "Stop Hiring Bad Employees!" In Paint and Coatings Expo (PACE) 2007. SSPC, 2007. https://doi.org/10.5006/s2007-00039.

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Abstract A shrinking pool of quality employee candidates has made it increasingly difficult to hire good people for your business. A band of inferior hopefuls stand outside your door, hoping to gain entry and wreak havoc in your business – you represent the only barrier that keeps them from coming through. Being able to see through their smoke and mirrors will improve the odds of hiring someone that will represent you and your company well.
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Mishra, Archana, and Kapesh Subhash Raghatate. "Blockchain for Safe Credential Checking in Hiring." In 2025 International Conference on Intelligent Control, Computing and Communications (IC3). IEEE, 2025. https://doi.org/10.1109/ic363308.2025.10957402.

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Valkanova, Kremena, and Pencho Yordanov. "Irrelevant Alternatives Bias Large Language Model Hiring Decisions." In Findings of the Association for Computational Linguistics: EMNLP 2024. Association for Computational Linguistics, 2024. http://dx.doi.org/10.18653/v1/2024.findings-emnlp.405.

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Mollay, Martin H., Deepak S. Sharma, Aryan G. Kale, Pankajkumar Anawade, and Shailesh Gahane. "Smart Hiring: Leveraging AI for Effective Employee Selection." In 2024 2nd DMIHER International Conference on Artificial Intelligence in Healthcare, Education and Industry (IDICAIEI). IEEE, 2024. https://doi.org/10.1109/idicaiei61867.2024.10842754.

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Satwik, Ch, K. L. Sailaja, Nambur Akhil Babu, and Vejendla Chaturya Sri. "Job Hunt Mobile Application for Hiring Skilled Labour." In 2024 1st International Conference on Advanced Computing and Emerging Technologies (ACET). IEEE, 2024. http://dx.doi.org/10.1109/acet61898.2024.10729921.

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Akhtar, MD Samir, Gauri Mathur, and Jimmy Singla. "An Intelligent System for Hiring Employees in Organizations." In 2024 9th International Conference on Communication and Electronics Systems (ICCES). IEEE, 2024. https://doi.org/10.1109/icces63552.2024.10859993.

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Zhang, Kechi, Ge Li, Huangzhao Zhang, and Zhi Jin. "HiRoPE: Length Extrapolation for Code Models Using Hierarchical Position." In Proceedings of the 62nd Annual Meeting of the Association for Computational Linguistics (Volume 1: Long Papers). Association for Computational Linguistics, 2024. http://dx.doi.org/10.18653/v1/2024.acl-long.735.

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Kumar, Shubham, Nikhil Rajput, Varsha Mishra, and Gunjan Aggarwal. "Intelligent Hiring Software- Job Recommendation System and Profile Builder." In 2025 First International Conference on Advances in Computer Science, Electrical, Electronics, and Communication Technologies (CE2CT). IEEE, 2025. https://doi.org/10.1109/ce2ct64011.2025.10941622.

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Golombek, Matthew. "HOW HIRISE CHANGED MARS EXPLORATION." In GSA Annual Meeting in Phoenix, Arizona, USA - 2019. Geological Society of America, 2019. http://dx.doi.org/10.1130/abs/2019am-336503.

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Reports on the topic "HiRISE"

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Hunt, Will, and Jacqueline O'Reilly. Rapid Recruitment in Retail: Leveraging AI in the hiring of hourly paid frontline associates during the Covid-19 Pandemic. Digital Futures at Work Research Centre, 2022. http://dx.doi.org/10.20919/alnb9606.

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Increased demand due to the Coronavirus pandemic created the need for Walmart to onboard tens of thousands of workers in a short period. This acted as a catalyst for Walmart to bring forward existing plans to update the hiring system for store-level hourly paid associates in its US stores. The Rapid Recruitment project sought to make hiring safer, faster, fairer and more effective by removing in-person interviews and leveraging machine learning and predictive analytics. This working paper reports on a case study of the Rapid Recruitment project involving semi-structured qualitative interviews with members of the project team and hiring staff at five US stores. The research finds that while implementation of the changes had been successful and the changes were largely valued by hiring staff, lack of awareness and confidence in some changes threatened to undermine some of the objectives of the changes. Reservations about the pre-employment assessment and the algorithm’s ability to predict quality hires led someusers reviewing more applications than perhaps necessary and potentially undermining prediction of 90-day turnover. Concerns about the ability to assess candidates over the phone meant that some users had reverted to in-person interviews, raising the riskof Covid transmission and potentially undermining the objective of removing the influence of human bias linked to appearance and other factors unrelated to performance. The impact of awareness and confidence in the changes to the hiring system are discussed in relation to the project objectives
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Kippen, Karen Elizabeth. We are hiring. Office of Scientific and Technical Information (OSTI), 2018. http://dx.doi.org/10.2172/1481967.

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Hoffman, Mitchell, Lisa Kahn, and Danielle Li. Discretion in Hiring. National Bureau of Economic Research, 2015. http://dx.doi.org/10.3386/w21709.

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Kippen, Karen Elizabeth. We are hiring. Office of Scientific and Technical Information (OSTI), 2016. http://dx.doi.org/10.2172/1331255.

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Lazear, Edward. Hiring Risky Workers. National Bureau of Economic Research, 1995. http://dx.doi.org/10.3386/w5334.

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Meyerhofer, David Dietrich. We Are Hiring. Office of Scientific and Technical Information (OSTI), 2020. http://dx.doi.org/10.2172/1595628.

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Weiss, Andrew, and Henry Landau. Validating Hiring Criteria. National Bureau of Economic Research, 1987. http://dx.doi.org/10.3386/w2167.

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Li, Danielle, Lindsey Raymond, and Peter Bergman. Hiring as Exploration. National Bureau of Economic Research, 2020. http://dx.doi.org/10.3386/w27736.

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Halverstadt, Ashleigh Halverstadt. Hiring an External Evaluator. S. D. Bechtel, Jr. Foundation, 2018. http://dx.doi.org/10.15868/socialsector.37453.

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Tobin, Bob Tobin. Hiring a Communications Consultant. S. D. Bechtel, Jr. Foundation, 2018. http://dx.doi.org/10.15868/socialsector.37459.

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