Relevant bibliographies by topics / Mark galer

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Academic literature on the topic 'Mark galer'

Author: Grafiati
Published: 4 June 2021
Last updated: 11 February 2022

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Journal articles on the topic "Mark galer"

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Wening, Rina Hapsari, Willy Bayuardi Suwarno, Bambang Sapta Purwoko, Indrastuti Apri Rumanti, and Amy Estiati. "Konfirmasi Toleransi Galur-galur Padi terhadap Cekaman Kekeringan secara Molekuler." Jurnal Agronomi Indonesia (Indonesian Journal of Agronomy) 49, no. 2 (September 3, 2021): 105–11. http://dx.doi.org/10.24831/jai.v49i2.36565.

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Seleksi secara fenotipik, terutama terhadap cekaman abiotik, seringkali sulit dilakukan. Kegiatan seleksi secara molekuler diperlukan untuk mengidentifikasi hingga taraf molekuler bahwa suatu sifat toleran terbukti secara genotipik. Tujuan dari penelitian ini ialah untuk mengkonfirmasi sifat toleransi kekeringan galur-galur padi secara molekuler menggunakan marka SSR RM164, RM228, RM248, dan RM328. Penelitian dilaksanakan di Laboratorium Bioteknologi LIPI, Cibinong pada bulan November hingga Desember 2017, menggunakan teknik polymerase chain reaction (PCR). Hasil penelitian menunjukkan bahwa marka RM228 terkait dengan karakter skor menggulung, panjang malai, tinggi tanaman dan umur berbunga, sedangkan RM328 terkait dengan panjang malai, jumlah anakan, jumlah gabah isi per malai, dan produktivitas. Marka tersebut diduga dapat digunakan untuk seleksi toleransi kekeringan. Tujuh dari sepuluh galur yang terindikasi toleran terhadap cekaman kekeringan fase generatif berdasarkan skrining secara artifisial terkonfirmasi secara molekuler berada dalam satu kelompok dengan varietas pembanding toleran ‘Limboto’. Ketujuh galur tersebut ialah B13983E-KA-12-2, B13507E-MR-19, B14366E-KY-50, BP20452e-PWK-0-SKI-1-1, BP20452e-PWK-0-SKI-2-4, BP20452e-PWK-0-SKI-3-3, dan BP29790d-PWK-3-SKI-1-5. Kata kunci: marka, toleransi kekeringan, polymerase chain reaction
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Winandari, Ovi Prasetya, Aris Tjahjoleksono ., and Dwinita Wikan Utami. "IDENTIFIKASI MARKA GEN KETAHANAN HAWAR DAUN BAKTERI PADA GALUR PADI INTRODUKSI DAN GALUR DIHAPLOID." Jurnal Hama dan Penyakit Tumbuhan Tropika 14, no. 2 (June 13, 2014): 101–9. http://dx.doi.org/10.23960/j.hptt.214101-109.

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Identification marker of bacterial leaf blight (BLB) gene resistance on introducted and dihaploid rice germplasm. Bacterial leaf blight (BLB), caused by bacterial pathogen Xanthomonas oryzae pv. oryzae (Xoo), is one of the most devastating diseases in rice. The use of BLB-resistant rice varieties is one of the most efficient ways to protect rice from this disease. BLB-resistant varieties can be produced through the breeding program by using the diverse rice germplasm. The objective of this research was to identify BLB resistance gene on 37 introducted and dihaploid rice lines derived from wide genetic background double crossing from local rice : IR54/Parekaligolara and Bio110/Markuti, by using the molekular markers. As control plant used 23 differential varieties (monogenic lines/IRBB) and TN1 (susceptible). All plants tested were inoculated by 3 selected dominant BLB races (Race III, IV dan VIII). The selected of 19 polymorphism molecular markers used to identify the BLB resistance genes on rice lines tested. The result of this research showed that 4 rice lines were resistance to all BLB races tested. Three molecular markers were specific associated with resistant gene to Race III (Xa7-STS40, Xa1-STS14 and Xa4-STS50); Race IV (Xa1-STS5, Xa4-STS50 and Xa26-STS1), and Race VIII (Xa21-STS6, Xa7-RM20590 and Xa7-STS40). These markers could be utilized for the selection process the developmen of BLB resistance rice lines breeding program.
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Prasetiyono, Joko, Tasliah Tasliah, Nurul Hidayatun, Tintin Suhartini, and Ida H. Soemantri. "Analisis Molekuler dan Uji Daya Hasil Galur-Galur Pup1." Jurnal AgroBiogen 12, no. 1 (February 13, 2018): 1. http://dx.doi.org/10.21082/jbio.v12n1.2016.p1-10.

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<p>Perbaikan varietas padi untuk daerah yang memiliki masalah dengan ketersediaan P sangat penting dilakukan mengingat harga pupuk P yang semakin mahal, dan ketersediaan P di alam yang semakin sedikit. Lokus <em>Pup1</em> sebagai lokus yang berisi gen-gen yang berperan dalam penangkapan P telah dipetakan dengan baik dan marka-marka untuk seleksi sudah dibuat. Berdasarkan penelitian sebelumnya telah diperoleh galur-galur BC<sub>2</sub>F<sub>8</sub> persilangan Dodokan x Kasalath, Dodokan x NIL-C443, Situ Bagendit x Kasalath, Situ Bagendit x NIL-C443, Batur x Kasalath, dan Batur x NIL-C443. Penelitian ini bertujuan untuk mengevaluasi galur-galur BC<sub>2</sub>F<sub>8</sub> secara molekuler dan melihat potensi hasil pada dua lokasi yang berbeda. Penelitian berlangsung mulai bulan Nopember 2013 s.d. Juni 2014. Penelitian molekuler dilakukan di Laboratorium Biologi Molekuler, Balai Besar Penelitian dan Pengembangan Bioteknologi dan Sumber Daya Genetik Pertanian (BB Biogen), Bogor dan International Rice Research Institue (IRRI), Filipina, sedangkan penelitian lapang dilakukan di KP Taman Bogo, Lampung dan lahan petani di Sukabumi, Jawa Barat. Berdasarkan analisis molekuler diperoleh hasil seluruh galur-galur BC<sub>2</sub>F<sub>8</sub> mengandung lokus <em>Pup1</em><em>, </em>namun ada tiga galur (BC<sub>2</sub>F<sub>8</sub> Situ Bagendit x Kasalath #5, BC<sub>2</sub>F<sub>8</sub> Situ Bagendit x NIL-C443 #2, dan BC<sub>2</sub>F<sub>8 </sub>Batur x NIL-C443 #2) yang mengandung lokus <em>Pup1</em> dalam kondisi heterozigot. Sebagian besar galur-galur <em>Pup1</em> susunan genomnya masih mengikuti genom tetuanya, kecuali BC<sub>2</sub>F<sub>8</sub> Situ Bagendit x Kasalath #7, BC<sub>2</sub>F<sub>8</sub> Batur x NIL-C443 #4, dan #5. Pada percobaan di lapang menunjukkan galur-galur <em>Pup1</em> pada kondisi P tersedianya kurang mengalami pertumbuhan vegetatif jauh lebih besar dibanding dengan pada kondisi yang P nya cukup tersedia. Namun, pada tahap pengisian biji terjadi variasi hasil, dimana masalah tersebut masih diperlukan penelitian lebih lanjut. Galur-galur BC<sub>2</sub>F<sub>8 </sub>Situ Bagendit x Kasalath #2, #3, #6, BC<sub>2</sub>F<sub>8</sub> Situ Bagendit x NIL-C443 #1, #2, BC<sub>2</sub>F<sub>8 </sub>Batur x Kasalath #4, #6, #7, BC<sub>2</sub>F<sub>8</sub> Batur x NIL-C443 #3, #4, dan #5 memiliki potensi untuk dikembangkan di daerah dengan P tersedia sedikit ataupun banyak.<strong></strong></p>
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Tanujaya, Gerald, and Alvin Hadiwono. "GALERI WISATA-MAKNA FOTOGRAFI." Jurnal Sains, Teknologi, Urban, Perancangan, Arsitektur (Stupa) 1, no. 1 (September 9, 2019): 533. http://dx.doi.org/10.24912/stupa.v1i1.3979.

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Penulisan Laporan kali ini bertujuan menginformasikan tentang sebuah seni dalam perkembangan teknologi yang sangat pesat di era globalisasi saat ini yaitu fotografi, hampir diseluruh dunia yang serba digital kali ini fotografi mengambil peran penting di berbagai aspek kehidupan dan dapat menjadi sebuah jembatan antar bahasa bagi seluruh dunia, sehingga sangat bersinergi dengan media informasi dan platform media sosial yang sangat marak di era digital dan market place online. Fotografi memiliki perkembangan yang cukup pesat dan dampak yang sangat besar salah satunya dalam aspek pariwisata architourism. banyaknya eksistensi perlombaan fotografi sebagai salah satu cara marketing di era digital ini, dan juga daya beli kamera yang terus meningkat menunjukan bahwa Indonesia menerima dengan baik teknologi fotografi itu sendiri, berkaca dari kemajuan bidang fotografi yang pesat, khususnya di kota metropolitan Jakarta yang menjadikan titik acuan prospek strategis untuk menampung kegiatan praktik fotografi yang sangat kompleks dan cukup dapat mewarnai atmosfer dunia seni, pendidikan, perdagangan konvensional dan digital, parawisata, dan media lain dituangkan ke dalam suatu wadah galeri fotografi.
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Yendra, Sasferi. "Museum dan Galeri (Tantangan dan Solusi)." JURNAL TATA KELOLA SENI 4, no. 2 (August 2, 2019): 103–8. http://dx.doi.org/10.24821/jtks.v4i2.3088.

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Abstrak Latar belakang penelitian ini adalah fenomena masyarakat luas yang terlihat kesadaran untuk berkunjung ke museum, terlihat pada akun sosial media masyarakat zaman sekarang yang semakin marak. Ruang pamer museum merupakan sebuah wadah aktivitas yang dilakukan pengguna dalam museum yang berfungsi sebagai elemen utama visualisasi, ruang sebagai program, dan ruang sebagai susunan tata letak. Sering ditemukannya ruang pamer yang tidak sesuai harapan dan lemahnya interaksi museum terhadap pengunjung, kegagalan kepuasan pengunjung terhadap ruang pamer dapat menjadi kendala menurunnya minat untuk datang kembali. Abstract The background of this study is a phenomenon of the wider community that shows awareness to visit the museum, seen in the social media accounts of today's society which are increasingly prevalent. The museum exhibition room is a place of activity carried out by users in the museum which functions as the main element of visualization, space as a program, and space as an arrangement of layout. Often found showrooms that do not match expectations and weak museum interaction with visitors, the failure of visitor satisfaction to the showroom can be an obstacle to the decline in interest in coming back.
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Pardal, Saptowo J., V. R. Rahayu, K. Nugroho, and Suharsono Suharsono. "Analisis Keragaman Genetik Galur Kedelai Transgenik Toleran Cekaman Aluminium dan Varietas Non-Trasngenik Berdasarkan Marka SSR." Jurnal Penelitian Pertanian Tanaman Pangan 4, no. 3 (December 14, 2020): 171. http://dx.doi.org/10.21082/jpptp.v4n3.2020.p171-177.

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Pardal, Saptowo J., V. R. Rahayu, K. Nugroho, and Suharsono Suharsono. "Analisis Keragaman Genetik Galur Kedelai Transgenik Toleran Cekaman Aluminium dan Varietas Non-Trasngenik Berdasarkan Marka SSR." Jurnal Penelitian Pertanian Tanaman Pangan 4, no. 3 (December 14, 2020): 171. http://dx.doi.org/10.21082/jpptp.v4n3.2020.p171-177.

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Riddle, John M. "Mark Grant. Galen on Food and Diet. x + 214 pp., bibl., index. New York/London: Routledge, 2000. $85 (cloth); $27.95 (paper)." Isis 94, no. 3 (September 2003): 518. http://dx.doi.org/10.1086/380677.

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Chaerani, Chaerani, DW Utami, N. Hidayatun, B. Abdullah, and B. Suprihatno. ""Asosiasi antara marka SSR dengan ketahanan terhadap wereng batang coklat pada varietas dan calon galur harapan padi." Jurnal Entomologi Indonesia 11, no. 1 (April 21, 2014): 43–52. http://dx.doi.org/10.5994/jei.11.1.43.

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Nutton, Vivian. "Mark Grant, Galen on food and diet, London and New York, Routledge, 2000, pp. ix, 214, illus., £15.99 (paperback 0415-23233-3)." Medical History 45, no. 4 (October 2001): 562–63. http://dx.doi.org/10.1017/s0025727300068654.

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Dissertations / Theses on the topic "Mark galer"

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L'Haridon, Jonas. "Diagenetic processes on Mars : analysis by the ChemCam instrument on the Curiosity rover." Thesis, Nantes, 2018. http://www.theses.fr/2018NANT4087/document.

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L’exploration de la surface de Mars par le rover Curiosity, au niveau du cratère Gale, a permis de révéler la présence de conditions habitables par le passe, a travers l’observation de dépôts sédimentaires fluvio-lacustres attestant d'une activité hydrologique prolongée. Ces roches portent également les stigmates de l’évolution complexe des sédiments lors de la diagenèse, sous forme de veines, nodules et concrétions s'etant formes par la circulation de fluides en sub-surface. A bord du rover, la spectroscopie de plasma induit par laser (LIBS) de l’instrument ChemCam permet une mesure chimique a petite échelle, particulièrement adaptée a l'analyse de tels éléments géologiques. Cette étude démontre que les veines de Ca-sulfate, observées dans toutes les unités géologiques traversées par le rover, présentent des enrichissements ponctuels en Fe témoignant de conditions de formation oxydantes lors de la diagenèse tardive. Par ailleurs, l’une des structures sédimentaires du cratère est caractérisée par des signatures spectrales d’hématite depuis l'orbite, suggérant que sa formation est en partie liée a des processus d'oxydo-reduction, pendant et/ou après le dépôt des sédiments. A cet endroit, ChemCam a mis en évidence la mobilité du Fe lors de la diagenèse, ainsi que la formation d'oxyde de Fe en association avec les veines de Ca-sulfate. Pour conclure, ces travaux montrent l'importance des interactions fluides-roches, comme les réactions d’oxydoreduction, lors de l’enfouissement des sédiments martiens, processus devant être pris en compte pour éviter des erreurs d’interprétation sur l’environnement de dépôt et l’intérêt exo-biologique des sédiments étudiés
The exploration of the Martian surface by the rover Curiosity, at Gale crater, has unveiled past habitable conditions on the planet with evidences for sustained period of surface aqueous activity recorded in fluvio-lacustrine sedimentary deposits. In addition, the rocks also bear traces of the complex post-depositional evolution of the sediments during diagenesis, in the form of small-scale fracture-fills, nodules, and concretions that formed by sub-surface fluid circulations. On board, the rover, the Laser-Induced Breakdown Spectroscopy (LIBS) performed by the ChemCam instrument provide remote fine-scale chemical measurements, especially suited to the analysis of such geological items. This study demonstrates that the Ca-sulfate-bearing veins, observed across all geological terrains, show enrichments in Fe at specific locations along the rover traverse, tracing localized oxidizing conditions at the time of their formation in the later stages of diagenesis. Additionally, a key sedimentary structure in Gale crater is characterized by hematite spectral signatures from orbit, suggesting the involvement of redox-driven processes in its formation, either related to primary deposition or post-depositional conditions. There, in situ ChemCam observations highlight the mobility of Fe during diagenesis and the authigenic formation of Fe-oxide in association with Ca-sulfate bearing features. As such, this work attests of significant fluid interactions, and notably redox-driven chemical reactions, affecting the Martian sediments after their deposition and burial, which need to be taken into account in order to avoid any misinterpretations on the environment of deposition and its habitability
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Galek, Marek [Verfasser]. "M2C-Converter auf Basis von MOS-Transistoren für Niederspannungsnetze / Marek Galek." Aachen : Shaker, 2016. http://d-nb.info/112086447X/34.

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Horvath, David G., and Jeffrey C. Andrews-Hanna. "Reconstructing the past climate at Gale crater, Mars, from hydrological modeling of late-stage lakes." AMER GEOPHYSICAL UNION, 2017. http://hdl.handle.net/10150/625822.

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The sedimentary deposits in Gale crater may preserve one of the best records of the early Martian climate during the Late Noachian and Early Hesperian. Surface and orbital observations support the presence of two periods of lake stability in Gale craterprior to the formation of the sedimentary mound during the Late Noachian and after the formation and erosion of the mound to its present state in the Early Hesperian. Here we use hydrological models and late-stage lake levels at Gale, to reconstruct the climate of Mars after mound formation and erosion to its present state. Using Earth analog climates, we show that the late-stage lakes require wetter interludes characterized by semiarid climates after the transition to arid conditions in the Hesperian. These climates are much wetter than is thought to characterize much of the Hesperian and are more similar to estimates of the Late Noachian climate.
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Achilles, C. N., R. T. Downs, D. W. Ming, E. B. Rampe, R. V. Morris, A. H. Treiman, S. M. Morrison, et al. "Mineralogy of an active eolian sediment from the Namib dune, Gale crater, Mars." AMER GEOPHYSICAL UNION, 2017. http://hdl.handle.net/10150/626447.

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The Mars Science Laboratory rover, Curiosity, is using a comprehensive scientific payload to explore rocks and soils in Gale crater, Mars. Recent investigations of the Bagnold Dune Field provided the first in situ assessment of an active dune on Mars. The Chemistry and Mineralogy (CheMin) X-ray diffraction instrument on Curiosity performed quantitative mineralogical analyses of the <150m size fraction of the Namib dune at a location called Gobabeb. Gobabeb is dominated by basaltic minerals. Plagioclase, Fo56 olivine, and two Ca-Mg-Fe pyroxenes account for the majority of crystalline phases along with minor magnetite, quartz, hematite, and anhydrite. In addition to the crystalline phases, a minimum similar to 42wt % of the Gobabeb sample is X-ray amorphous. Mineralogical analysis of the Gobabeb data set provides insights into the origin(s) and geologic history of the dune material and offers an important opportunity for ground truth of orbital observations. CheMin's analysis of the mineralogy and phase chemistry of modern and ancient Gale crater dune fields, together with other measurements by Curiosity's science payload, provides new insights into present and past eolian processes on Mars.
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Sara, Michael James. "Dyngjusandur sand sheet, Iceland, as a depositional analog to the Stimson Fm. in Gale Crater, Mars." Thesis, University of Iowa, 2017. https://ir.uiowa.edu/etd/5621.

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Basalts from Askja, Iceland have high MgO (5-18 wt %) and high Fe2O3 (5-18 wt %: Baratoux et al., 2011; Mangold et al., 2013, this study) similar to Martian basalts, which have Fe2O3 from 10-33 wt % McSween et al, 2006; Ming et al., 2008]) and MgO around 11 wt. % (McSween et al., 2009). Askja’s cold desert climate provides a good weathering analogueanalog (Mountney and Russell, 2004). Askja is located in the Northern Volcanic Zone of Iceland and basalts have been weathered to form mafic volcaniclastic deposits in a 40-km long sand sheet to the E-SE of the Askja caldera complex (Fig. 1; (Kuritani et al., 2011). The 2014-2015 Holuhraun eruption was emplaced onto the southeastern part of the sand sheet (Fig. 1) and altered the regional geomorphology and may have impacted the geochemistry of the sand sheet itself by addition of wind-blown ash and crystals, plus weathering of the lava flow (MgO content of ~7.1 wt % Geiger et al., 2016). Mangold et al. (2011) found that Icelandic sands show little chemical variations but that study was limited in the number of samples (12 sand samples and 12 rock seven rock, seven sand; Mangold et al., 2011). Here we expand on that study and we have created a morphological and geochemical database with the goal of identifying relevant trends to past and present Martian environments. The Askja sand sheet, between ~10 cm and ~10 m thick, covers 240 km2 (Mountney and Russell). Mountney and Russell described three distinct sections of the sand sheet. The southwest section is deflationary and defined by very fine to medium grained basaltic sand with cobbles and boulders of lithologies sourced from adjacent to and distal from the sand sheet. The central part is inflating and is dominated by very fine-grained sand, relict lava fields, and small to large sand ripples. The northeast portion is also inflating but that accumulation is limited to topographic depressions. The northeast, characterized by sand mostly composed of pumice from the 1875 Askja eruption and basalt clasts from local lava fields, was not studied in detail here due to the difference in chemistry. Martian basaltic eolian sediments may record a long history of local and global climate change and they may have been potential habitats where water, nutrients and organic carbon mixed below the surface (Blake et al., 2013; Fisk et al., 2013). Basaltic sand fields on Earth have not been characterized as well as felsic sands, but represent a unique analog to deposits such as the Stimson Fm. on Mars (Mangold et al., 2011; Banham et al., 2016; Gupta et al., 2016; Ming et al., 2016; Newsom et al., 2016; Yen et al., 2016) . Eolian dominated weathering prevalent at Askja volcano, Iceland, likely also occurred on Mars and Askja mafic volcaniclastic dunes could be the best morphological and compositional analogueanalog for Martian eolian dunes (Edgett and Lancaster, 1993).
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Rapin, William. "Hydratation de la surface de Mars à partir des données du rover Curiosity." Thesis, Toulouse 3, 2016. http://www.theses.fr/2016TOU30338.

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La recherche des phases hydratées à la surface de Mars est essentielle à la compréhension de son passé habitable et des changements climatiques globaux qu'elle a subis. Le rover MSL/Curiosity apporte de nouveaux moyens pour caractériser l'hydratation de la surface. En particulier, la spectroscopie de plasma induite par laser (LIBS) de l'instrument ChemCam mesure la composition élémentaire à distance. Il permet une détection de l'hydrogène par le pic d'émission H Balmer alpha à 656.6 nm. Cependant la quantification de cet élément n'a été que très peu étudiée. Le modèle de qualification de l'instrument ChemCam a été intégré à un banc LIBS afin d'analyser des séries d'échantillons hydratés au laboratoire. A l'exception de quelques échantillons révélant des phénomènes spécifiques à l'hydrogène, ces tests montrent qu'un étalonnage linéaire est obtenu avec la teneur en eau. Sur Mars, dans le cratère Gale, cette calibration révèle l'hydratation de différentes phases : la bassanite (CaSO4 × 0.5H2O) dans les veines remplissant les fractures des roches, les sulfates de magnésium, les sédiments opalifères et argileux découverts in situ. Les mesures d'abondances en eau effectuées jusqu'à présent étaient restreintes à de rares expériences de pyrolyse ; cette étude montre que ChemCam apporte maintenant un nouveau moyen opérationnel pour la mesure de l'hydrogène à la surface, à l'échelle submillimétrique et couvrant un très grand nombre de roches
The search for hydrated phases lying at the surface of Mars is essential to understand its habitable past and the fate of water on a planet disrupted by global climate changes. The MSL/Curiosity rover provides new tools to characterize surface hydration in situ. Among these, laser induced breakdown spectroscopy (LIBS) performed by the ChemCam instrument enables remote measurement of elementary abundance. However, measuring the LIBS emission peak of hydrogen at 656.6 nm (Balmer alpha) to quantify target water content is poorly documented in the literature. Using the instrument replica, large series of hydrated samples have been analyzed in the laboratory under Martian atmospheric conditions. Except for some samples on which effects specific to the hydrogen signal have been observed, these tests show that a linear calibration can be obtained with target water content. On Mars, at Gale crater, this calibration reveals the hydration of different phases: bassanite (CaSO4 × 0.5H2O) in the veins filling the bedrock fractures, magnesium sulfates, opaline and clay rich sediments discovered in situ. Measurement of water content performed to date have been limited to sparse and bulk pyrolysis experiments; this study shows that ChemCam provides a new technique to measurement hydrogen on the surface, at a submillimeter scale and sampling a very large number of rocks
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Johnson, Jeffrey R., Cherie Achilles, James F. Bell, Steve Bender, Edward Cloutis, Bethany Ehlmann, Abigail Fraeman, et al. "Visible/near-infrared spectral diversity from in situ observations of the Bagnold Dune Field sands in Gale Crater, Mars." AMER GEOPHYSICAL UNION, 2017. http://hdl.handle.net/10150/626566.

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As part of the Bagnold Dune campaign conducted by Mars Science Laboratory rover Curiosity, visible/near-infrared reflectance spectra of dune sands were acquired using Mast Camera (Mastcam) multispectral imaging (445-1013nm) and Chemistry and Camera (ChemCam) passive point spectroscopy (400-840nm). By comparing spectra from pristine and rover-disturbed ripple crests and troughs within the dune field, and through analysis of sieved grain size fractions, constraints on mineral segregation from grain sorting could be determined. In general, the dune areas exhibited low relative reflectance, a weak similar to 530nm absorption band, an absorption band near 620nm, and a spectral downturn after similar to 685nm consistent with olivine-bearing sands. The finest grain size fractions occurred within ripple troughs and in the subsurface and typically exhibited the strongest similar to 530nm bands, highest relative reflectances, and weakest red/near-infrared ratios, consistent with a combination of crystalline and amorphous ferric materials. Coarser-grained samples were the darkest and bluest and exhibited weaker similar to 530nm bands, lower relative reflectances, and stronger downturns in the near-infrared, consistent with greater proportions of mafic minerals such as olivine and pyroxene. These grains were typically segregated along ripple crests and among the upper surfaces of grain flows in disturbed sands. Sieved dune sands exhibited progressive decreases in reflectance with increasing grain size, as observed in laboratory spectra of olivine size separates. The continuum of spectral features observed between the coarse- and fine-grained dune sands suggests that mafic grains, ferric materials, and air fall dust mix in variable proportions depending on aeolian activity and grain sorting.
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Ehlmann, B. L., K. S. Edgett, B. Sutter, C. N. Achilles, M. L. Litvak, M. G. A. Lapotre, R. Sullivan, et al. "Chemistry, mineralogy, and grain properties at Namib and High dunes, Bagnold dune field, Gale crater, Mars: A synthesis of Curiosity rover observations." AMER GEOPHYSICAL UNION, 2017. http://hdl.handle.net/10150/626565.

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The Mars Science Laboratory Curiosity rover performed coordinated measurements to examine the textures and compositions of aeolian sands in the active Bagnold dune field. The Bagnold sands are rounded to subrounded, very fine to medium sized (similar to 45-500m) with 6 distinct grain colors. In contrast to sands examined by Curiosity in a dust-covered, inactive bedform called Rocknest and soils at other landing sites, Bagnold sands are darker, less red, better sorted, have fewer silt-sized or smaller grains, and show no evidence for cohesion. Nevertheless, Bagnold mineralogy and Rocknest mineralogy are similar with plagioclase, olivine, and pyroxenes in similar proportions comprising >90% of crystalline phases, along with a substantial amorphous component (35%15%). Yet Bagnold and Rocknest bulk chemistry differ. Bagnold sands are Si enriched relative to other soils at Gale crater, and H2O, S, and Cl are lower relative to all previously measured Martian soils and most Gale crater rocks. Mg, Ni, Fe, and Mn are enriched in the coarse-sieved fraction of Bagnold sands, corroborated by visible/near-infrared spectra that suggest enrichment of olivine. Collectively, patterns in major element chemistry and volatile release data indicate two distinctive volatile reservoirs in Martian soils: (1) amorphous components in the sand-sized fraction (represented by Bagnold) that are Si-enriched, hydroxylated alteration products and/or H2O- or OH-bearing impact or volcanic glasses and (2) amorphous components in the fine fraction (<40m; represented by Rocknest and other bright soils) that are Fe, S, and Cl enriched with low Si and adsorbed and structural H2O. Plain Language Summary The Bagnold dune field is an active sand field with moving dunes and sits between the landing site of the Curiosity rover and rocks of interest higher up on Mount Sharp. When passing through the dune field, we used all of Curiosity's instruments to measure the chemistry, mineralogy, and grain size of sands in the Bagnold dune field in order to figure out where they came from, how the sands are transported, and what volatile materials (like water) lie within Martian soils. We found that the Bagnold sand dunes are very well sorted; no dusty materials are found within them, in stark contrast to soils seen previously with Curiosity and with rovers at other landing sites. We found that the coarser sand grains are enriched in the volcanic minerals olivine and pyroxene, confirming a prediction from orbit that wind-related activity seems to concentrate these phases. We also found that the dunes were much lower in water and other volatile elements like sulfur and chlorine versus all previous Mars soils. Using a combination of the rover's sieving system and chemical measurement tools, we figured out that two types of materials host water. In the first type of material, common in these sands, water is low in abundance (similar to 1%), very tightly bound to the grains, and is not released until temperatures >200 degrees C. In the second type of material, water is higher in abundance (2%) and more easily released by heating. Sieved water-bearing fine materials may be a useful resource for human explorers.
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Tolley, Rebecca. "Frances Kellor, James Braham Phelps and Rose Pastor Stokes, Lenora O'Reilly, Lucy Burns, Margaret Haley, Mary Kenney O'Sullivan, Mary Melinda Kingsbury Simkhovitch, Maud Wood Park, Sue Shelton White, Zona Gale." Digital Commons @ East Tennessee State University, 2005. https://www.amzn.com/0765680513.

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Donahue, Mary [Verfasser], Andreas Akademischer Betreuer] Schober, Hannes [Gutachter] [Töpfer, and Richard [Gutachter] Gale. "Nitric oxide an pH measurement with AlGaN/GaN based ISFETs / Mary Jocelyn Donahue ; Gutachter: Hannes Töpfer, Richard Gale ; Betreuer: Andreas Schober." Ilmenau : TU Ilmenau, 2016. http://d-nb.info/1178174522/34.

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Books on the topic "Mark galer"

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Gallery, William Weston. Masters of printmaking: Fine prints by European and British masters of the 19th and 20th century : a special exhibtion to mark the 25th anniversary of William Weston Galler 1968-1993. London: William Weston Gallery, 1993.

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Ellen, Weiss, and Anne Gayler. Jim Henson Presents Where's the Bear?: Starring The Muppet Babies (TM). Racine, USA: Western Publishing Co., Inc., in conjunction with Hanson Associates, Inc. & adapted from a Parker Bros. book, 1986.

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Day, Walter. Twin Galaxies' Official Video Game & Pinball Book Of World Records; Second Edition, Arcade Volume. Edited by Walter Day and Mr Kelly R. Flewin. Fairfield, IA: 1st World Publishing, 2007.

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Photography Foundations for Art and Design: The creative photography handbook. 4th ed. Focal Press, 2007.

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Notebooks, Marc's. Marc Legendary Gamer: Lined Notebook / Journal Gift, 6 X 9 Inches, Marc Funny Video Games, Boys Legendary Gamer Marc Gift, Personalized Gift Idea for Marc, for Students, Teens, and Kids. Independently Published, 2020.

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Ibsen, Henrik. The Wild Duck: Hedda Gabler. W. W. Norton & Company, 1997.

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(Translator), Michael Leverson Meyer, ed. The Wild Duck: Hedda Gabler. W. W. Norton & Company, 1997.

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Location Photography: Essential Skills, Second Edition (Photography Essential Skills). 2nd ed. Focal Press, 2002.

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Location Photography: Essential Skills. Focal Press, 1999.

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Henning, Meghan. Weeping and Bad Hair. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780190458997.003.0014.

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This chapter draws upon the conceptions of gendered bodily suffering found in the ancient medical corpus (Hippocrates, Galen and inscriptions), martyrdom literature, and the Roman judicial rhetoric of punitive suffering to read apocalyptic depictions of bodily suffering as “effeminizing” punishments, which in turn utilized masculinity and bodily normativity to police behavior, and equated early Christian ethical norms with masculinity and bodily “health.” By highlighting the different types of bodies found in these texts, as well as the ways in which Christian norms interacted with Greek and Roman notions of the body, the chapter shows how masculinity and ancient notions of bodily normativity worked in concert to mark sin in early Christian hell, in turn creating an ancient Christian culture of bodily normativity. These early Christian texts expanded the existing frameworks of bodily suffering as a disciplinary performance and focused on the non-normative body as a punitive spectacle and pedagogical object.
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Book chapters on the topic "Mark galer"

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Anderson, R. C., L. Jandura, A. B. Okon, D. Sunshine, C. Roumeliotis, L. W. Beegle, J. Hurowitz, et al. "Collecting Samples in Gale Crater, Mars; an Overview of the Mars Science Laboratory Sample Acquisition, Sample Processing and Handling System." In Mars Science Laboratory, 57–75. New York, NY: Springer New York, 2012. http://dx.doi.org/10.1007/978-1-4614-6339-9_4.

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Fraeman, Abigail A. "Resolving Martian enigmas, discovering new ones: the case of Curiosity and Gale crater." In Mars Geological Enigmas, 1–10. Elsevier, 2021. http://dx.doi.org/10.1016/b978-0-12-820245-6.00001-x.

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Rizzo, Vincenzo, Richard Armstrong, Hong Hua, Nicola Cantasano, Tommaso Nicolò, and Giorgio Bianciardi. "Life on Mars: Clues, Evidence or Proof?" In Solar Planets and Exoplanets [Working Title]. IntechOpen, 2021. http://dx.doi.org/10.5772/intechopen.95531.

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The search for life on Mars is one of the main objectives of space missions. At “Pahrump Hills Field Site” (Gale Crater, Mojave target), inside the mudstones of the Murray lacustrine sequence, Curiosity rover found organic materials and lozenge shaped laths considered by NASA as pseudomorphic crystals. Besides it detected mineral assemblages suggesting both oxidizing (hematite) and reducing (magnetite) environments, as well as acidic (diagenetic and/or authigenic jarosite) and neutral (apatite) conditions, that might suggest bacterially mediated reactions. Our morphological and morphometrical investigations show that such diagenetic microstructures are unlikely to be lozenge shapes and, in addition to several converging features, they suggest the presence of remnants of complex algal-like biota, similar to terrestrial procaryotes and/or eukaryotes; possible microorganisms that, on the base of absolute dating criteria used by other scholars, lived on Mars about 2.12 +/−0.36 Ga ago.
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Guaita, Cesare. "New Insights into the Search for Life on Mars." In Solar System Planets and Exoplanets [Working Title]. IntechOpen, 2021. http://dx.doi.org/10.5772/intechopen.97176.

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The discovery by the Lander Phoenix (summer 2008) that the Mars polar soil is rich of perchloric acid salts (Na, Mg, Ca perchlorate) strongly could change the interpretation of the Martian experiment of 14CO2 release (LR, Labeled release experiment), performed in 70’s by both Viking Landers. The LR experiment gave substantially positive results but, at that time, possibility of Martian bacteria was ruled out because the CGMS instruments on board of both Vikings didn’t detect any trace of complex organic molecules. But Martian organics exist and were found in fair quantities by Curiosity, landed inside the Gale crater on 2012. So it is likely that Viking CGMS, working at about 500°C, could not see any organic substances (natural or bacterial) because, at that temperature, perchlorates decompose, releasing Oxygen that destroyed organics BEFORE their detection. In any case, the discovery of keragenic compounds by Curiosity, could also be indication of a presence of archea bacteria in the distant past of Mars, when the atmosphere of the Red Planet was wetter and denser than now.
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"The roles of speech and language therapists working in community clinics, child development centres and hospitals: Sue Roulstone, Mary Gale and Helen Marks." In Speech and Language Therapy, 56–65. Routledge, 2013. http://dx.doi.org/10.4324/9780203125595-14.

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Barker, Graeme, and David Mattingly. "Cores and Peripheries Revisited: The Mining Landscapes of Wadi Faynan (Southern Jordan) 5000 BC–AD 700." In Communities and Connections. Oxford University Press, 2007. http://dx.doi.org/10.1093/oso/9780199230341.003.0015.

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One of Barry Cunliffe’s major areas of research interest has been societies in transition, especially in the context of core/periphery relationships between expanding states and societies on their margins. Much of this work has been on the relationships between Rome and the Iron Age societies of southern Britain on the northwestern margins of the empire, and the subsequent pathways of resistance, interaction, and transformation. In this chapter we focus on events and processes on the opposite margins of the Roman empire in the Levant, where the Nabataean state was formally incorporated into the Roman imperial system some sixty years after the Claudian invasion of Britain. We draw on the results of the Wadi Faynan Landscape Survey (1996–2000), an interdisciplinary and diachronic investigation of evidence of environmental and climatic change, settlement pattern, and human activity in the Wadi Faynan in southern Jordan (figure 7.1). Situated about 40 kilometres from the Nabataean capital of Petra, the Wadi Faynan lies in the hot and hyper-arid Jordanian Desert, at a distinctive and spectacular mountain front that reaches 1500m above the desert floor. This landform marks the eastern margin of the desert lowlands of the great Jordanian rift valley, with the trough of the Wadi ‘Arabah to the south and west, and the highlands of the Mountains of Edom and the Jordanian tablelands to the east and north (Bienkowski and Galor 2006). The mean summer temperature on the Jordanian tablelands is in the order of 178c, compared with winter temperatures of about 12ºc (Bruins 2006; Rabb’a 1994). Winter temperatures on the desert floor in the Wadi Faynan are much the same as on the plateau, but in summer temperatures frequently reach 40ºc. Seasonality is strong, with most rain falling between December and March and virtually no precipitation occurring between June and September. Annual rainfall in the lower Wadi Faynan is around 63mm and even less in theWadi ‘Arabah (‘Aqaba receives 30mm for example), whereas the Jordanian Tablelands have an average precipitation exceeding 200mm per year.
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Conference papers on the topic "Mark galer"

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Heydari, Ezat, Fred J. Calef, Jeffrey F. Schroeder, Jason Van Beek, Scott K. Rowland, Alberto G. Fairén, and Timothy Parker. "RAPID INUNDATION OF GALE CRATER, MARS." In GSA Annual Meeting in Phoenix, Arizona, USA - 2019. Geological Society of America, 2019. http://dx.doi.org/10.1130/abs/2019am-335837.

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Burt, Donald M., and L. Paul Knauth. "THE MYSTERY WATER OF MARS (GALE CRATER)." In GSA Annual Meeting in Denver, Colorado, USA - 2016. Geological Society of America, 2016. http://dx.doi.org/10.1130/abs/2016am-284011.

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Heydari, Ezat, Jeffrey F. Schroeder, Jason Van Beek, Fred J. Calef, Scott K. Rowland, Timothy Parker, and Alberto G. Fairén. "FLOOD-DEPOSITED RHYTHMITES IN GALE CRATER, MARS." In GSA Annual Meeting in Phoenix, Arizona, USA - 2019. Geological Society of America, 2019. http://dx.doi.org/10.1130/abs/2019am-336066.

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Kah, Linda C., Rachel Kronyak, and Stephanie C. TerMaath. "UNDERSTANDING FRACTURE FORMATION CONDITIONS IN GALE CRATER, MARS." In GSA Annual Meeting in Indianapolis, Indiana, USA - 2018. Geological Society of America, 2018. http://dx.doi.org/10.1130/abs/2018am-318281.

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Heydari, Ezat, Jeffrey F. Schroeder, Jason Van Beek, Fred J. Calef, Scott K. Rowland, Alberto Fairén, Timothy Parker, and Samantha R. Jacob. "SIGNIFICANCE OF FLOOD DEPOSITS IN GALE CRATER, MARS." In GSA Annual Meeting in Indianapolis, Indiana, USA - 2018. Geological Society of America, 2018. http://dx.doi.org/10.1130/abs/2018am-319960.

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Ming, D. W., A. S. Yen, E. B. Rampe, J. P. Grotzinger, D. F. Blake, T. F. Bristow, S. J. Chipera, et al. "DIAGENESIS ALONG FRACTURES IN AN EOLIAN SANDSTONE, GALE CRATER, MARS." In GSA Annual Meeting in Denver, Colorado, USA - 2016. Geological Society of America, 2016. http://dx.doi.org/10.1130/abs/2016am-279126.

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Miklusicak, N. B., R. E. Kronyak, and L. C. Kah. "MINERALIZED FRACTURES IN THE SICCAR POINT GROUP, GALE CRATER, MARS." In 67th Annual Southeastern GSA Section Meeting - 2018. Geological Society of America, 2018. http://dx.doi.org/10.1130/abs/2018se-311733.

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Heydari, Ezat, Jeffrey F. Schroeder, Jason Van Beek, Fred John Calef, Scott K. Rowland, Timothy Parker, Alberto G. Fairén, and Lucy M. Thompson. "SPECTACULAR OUTCROPS OF THE CLAY-BEARING UNIT, GALE CRATER, MARS." In GSA Annual Meeting in Phoenix, Arizona, USA - 2019. Geological Society of America, 2019. http://dx.doi.org/10.1130/abs/2019am-338081.

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Jackson, Ryan S., Roger C. Wiens, Jens Frydenvang, Luther W. Beegle, Agnes Cousin, D. T. Vaniman, Olivier Forni, and Horton E. Newsom. "CHEMCAM INVESTIGATION OF THE STIMSON DRILL SITES, GALE CRATER, MARS." In 113th Annual GSA Cordilleran Section Meeting - 2017. Geological Society of America, 2017. http://dx.doi.org/10.1130/abs/2017cd-292902.

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Czarnecki, Sean M., Craig J. Hardgrove, Craig J. Hardgrove, Patrick J. Gasda, and Patrick J. Gasda. "BULK HYDRATION OF A CLAY-RICH UNIT IN GALE CRATER, MARS." In GSA Annual Meeting in Phoenix, Arizona, USA - 2019. Geological Society of America, 2019. http://dx.doi.org/10.1130/abs/2019am-337731.

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Reports on the topic "Mark galer"

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Joseph, Rhawn. Mars: Algae, Lichens, Fossils, Minerals, Microbial Mats, and Stromatolites in Gale Crater. Journal of Astrobiology and Space Science, March 2020. http://dx.doi.org/10.37720/jassr.03082020.

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Berger, B., D. Blaney, J. Bridges, A. Cousin, O. Forni, O. Gasnault, J. Lasue, et al. POSSIBLE ALTERATION OF ROCKS OBSERVED BY CHEMCAM ALONG THE TRAVERSE TO GLENELG IN GALE CRATER ON MARS. Office of Scientific and Technical Information (OSTI), April 2013. http://dx.doi.org/10.2172/1077020.

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DeJaeghere, Joan, Vu Dao, Bich-Hang Duong, and Phuong Luong. Inequalities in Learning in Vietnam: Teachers’ Beliefs About and Classroom Practices for Ethnic Minorities. Research on Improving Systems of Education (RISE), February 2021. http://dx.doi.org/10.35489/bsg-rise-wp_2021/061.

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Global and national education agendas are concerned with improving quality and equality of learning outcomes. This paper provides an analysis of the case of Vietnam, which is regarded as having high learning outcomes and less inequality in learning. But national data and international test outcomes may mask the hidden inequalities that exist between minoritized groups and majority (Kinh) students. Drawing on data from qualitative videos and interviews of secondary teachers across 10 provinces, we examine the role of teachers’ beliefs, curricular design and actions in the classroom (Gale et al., 2017). We show that teachers hold different beliefs and engage in curricular design – or the use of hegemonic curriculum and instructional practices that produce different learning outcomes for minoritized students compared to Kinh students. It suggests that policies need to focus on the social-cultural aspects of teaching in addition to the material and technical aspects.
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