Thematische Bibliographien / Chandrian

Auswahl der wissenschaftlichen Literatur zum Thema „Chandrian“

Autor: Grafiati
Veröffentlicht am 25. Juli 2024
Zuletzt aktualisiert am 31. Juli 2024

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Zeitschriftenartikel zum Thema "Chandrian"

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Nazarudeen, A., G. Rajkumar, Rohith Mathew Mohan und R. Prakashkumar. „Taxonomic notes on the identity of Rungia latior var. anamalayana (Acanthaceae) from Western Ghats, India“. Plant Science Today 7, Nr. 1 (01.01.2020): 23–28. http://dx.doi.org/10.14719/pst.2020.7.1.626.

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Rungia latior Nees var. anamalayana Chandrab. & V. Chandras., examined as part of the revisionary studies on the Acanthaceae of Western Ghats, have shown some taxonomic ambiguity. As the original authors rightly pointed out, the variety ‘does not fit within the circumscription of the typical species’. Based on our recent collections, we also felt that the varietal status is superfluous as the same has got some merits to be recognized as a distinct species. As such the status of the variety has been reassessed; elevated to the specific rank and a new combination has been set, conserving the varietal name as the specific epithet. Accordingly, the species is renamed as Rungia anamalayana (Chandrab. & V. Chandras.) A. Nazarudeen & G. Rajkumar comb. et stat. nov. The distinctive features and alliance of the species is discussed and a full account of the species is presented with illustrations.
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Arisdason, W., und P. Daniel. „Syzygium Chandrasekharanii Chandrab. & V. Chandras., A synonym of Syzygium Fergusonii (Trimen) Gamble (Myrtaceae)“. Indian Journal of Forestry 33, Nr. 2 (01.06.2010): 221–24. http://dx.doi.org/10.54207/bsmps1000-2010-02mmt4.

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Syzygium chandrasekharanii, a new species described from the Anamalais on the Western Ghats, is found to be conspecific with the less known Indo-Srilankan species Syzygium fergusonii (Trimen) Gamble and hence it is synonymized.
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Chandra, Sonaksh. „Comparative Analysis of Gluten Content of Raw and Processed Materials“. Universities' Journal of Phytochemistry and Ayurvedic Heights 2, Nr. 29 (24.12.2020): 47–49. http://dx.doi.org/10.51129/ujpah-2020-29-2(7).

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Abstract-Gluten intolerance /allergies is now a silently rising problem world-wide. Gluten is a protein composite found in cereals, wheat, rice, barley and certain oat varieties. It also causes Celiac disease which is an autoimmune disease (most severe form of gluten intolerance), resulting from glutenintoleranceandisbasedongeneticintolerance. The only therapeutic treatment for the patients with gluten allergies and celiac disease is a strict gluten free diet. Rising demand for gluten free products is a task for the bakers and manufacturers to eliminate gluten completely from their products which is technically not possible. This draws the attention to the fact that mandatory analysis in this field is required. The aim of this work is to find a way to reduce the gluten content in the available materials, and also to find the source of gluten contamination after processing of raw materials. It wasnotedthatgarlicandsugarcontainingcombination were found effective and showed decrease in gluten content and that they were better additivities in the processing process than rest of others.
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Bonde, Suresh D., und Nauneeth K. P. Kumaran. „Taxonomic realignment of the fossil polypodiaceous rhizome Thayeriorhizomoxylon chandrae (“chandraii ”) Patil and Datar from the Deccan Intertrappean beds of India“. TAXON 54, Nr. 1 (Februar 2005): 117–19. http://dx.doi.org/10.2307/25065307.

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Finnigan, John, und James Wilczak. „Jagadish Chandran Kaimal (1930–2021)“. Boundary-Layer Meteorology 180, Nr. 1 (28.04.2021): 1–4. http://dx.doi.org/10.1007/s10546-021-00623-3.

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MAHARAJ, AJESH B., und VINOD CHANDRAN. „Drs. Maharaj and Chandran reply“. Journal of Rheumatology 42, Nr. 6 (Juni 2015): 1062. http://dx.doi.org/10.3899/jrheum.150254.

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Mukherjee, Proshanto K. „Chandrika Prasad Srivastava“. WMU Journal of Maritime Affairs 9, Nr. 2 (Oktober 2010): 135–36. http://dx.doi.org/10.1007/bf03195170.

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Chandran, Sunil. „A Conversation with Dr. Sunil Chandran“. Industrial Biotechnology 18, Nr. 6 (01.12.2022): 334–37. http://dx.doi.org/10.1089/ind.2022.29293.sch.

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Baker, Monya. „Chandra Tucker“. Nature Methods 7, Nr. 12 (29.11.2010): 939. http://dx.doi.org/10.1038/nmeth1210-939.

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Tamhane, Swapna. „Mohini Chandra“. Wasafiri 17, Nr. 36 (Juni 2002): 40–42. http://dx.doi.org/10.1080/02690050208589787.

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Dissertationen zum Thema "Chandrian"

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Bhowmik, Shefali. „Bangla Upanyase Prem o Bibaha:Bankim Chandra-Rabindra Nath-Sharat Chandra বাংলা উপন্যাসে প্রেম ও বিবাহ : বঙ্কিমচন্দ্র - রবীন্দ্রনাথ -শরৎচন্দ্র“. Thesis, University of North Bengal, 1998. http://hdl.handle.net/123456789/1652.

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Kakati, Jogesh. „Subhas Chandra Bose and the British Raj“. Thesis, University of North Bengal, 2005. http://hdl.handle.net/123456789/1249.

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Otto, Tobias [Verfasser], Madhukar [Akademischer Betreuer] Chandra, Madhukar [Gutachter] Chandra, Gerd [Gutachter] Wanielik und Martin [Gutachter] Hagen. „Propagation effects influencing polarimetric weather radar measurements / Tobias Otto ; Gutachter: Madhukar Chandra, Gerd Wanielik, Martin Hagen ; Betreuer: Madhukar Chandra“. Chemnitz : Universitätsbibliothek Chemnitz, 2011. http://d-nb.info/1213904889/34.

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Maurya, Devalāla. „Hindī sāhitya kā itihāsa-darśana aura Rāmacandra Śukla /“. Ilāhābāda : Eksīlensa pabliśarsa, 1993. http://catalogue.bnf.fr/ark:/12148/cb36190705w.

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Dalla, Mura Maria Elisabetta. „Ricerca di AGN oscurati nei Chandra Deep Fields“. Master's thesis, Alma Mater Studiorum - Università di Bologna, 2016. http://amslaurea.unibo.it/9893/.

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La forma spettrale dell’X-ray background richiede l’esistenza di un grande numero di AGN mediamente oscurati, oltre alla presenza di AGN fortemente oscurati, la cui densità di colonna supera il limite Compton (Nh>10^24 cm^(-2)). A causa della loro natura, questi oggetti risultano di difficile osservazione, per cui è necessario adottare un approccio multi-banda per riuscire a rivelarli. In questo lavoro di tesi abbiamo studiato 29 sorgenti osservate nel CDF-S e 10 nel CDF-N a 0.0710^23, spettro piatto, riga del ferro): a seguito di questa analisi sono state individuate 9 sorgenti che presentano indicazioni di forte oscuramento. Dallo studio del rapporto tra la luminosità X (2-10 keV) e quella MIR (12.3um) dedotta dal SED-fitting, si è ottenuta una conferma della possibile presenza di forte oscuramento nelle 9 sorgenti selezionate a seguito dell’analisi spettrale. Abbiamo inoltre confrontato il tasso di formazione stellare dedotto dalla banda X (0.5-8 keV) e da quella IR (8-1000um) per identificare le sorgenti nelle quali l’emissione da AGN risulta essere dominante. A seguito di questa analisi abbiamo identificato 9 sorgenti (le stesse di cui sopra) con indicazione di forte oscuramento; di queste, 3 mostrano chiare indicazioni della presenza di un AGN Compton Thick (Nh>10^24 cm^(-2), riga del ferro intensa, basso rapporto LX/MIR).
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Phruksahiran, Narathep [Verfasser], Madhukar [Akademischer Betreuer] Chandra, Madhukar [Gutachter] Chandra und Gerd [Gutachter] Wanielik. „Polarimetrische Streuungseigenschaften und Fokussierungsmethoden zur quantitativen Auswertung der polarimetrischen SAR-Daten / Narathep Phruksahiran ; Gutachter: Madhukar Chandra, Gerd Wanielik ; Betreuer: Madhukar Chandra“. Chemnitz : Universitätsbibliothek Chemnitz, 2013. http://d-nb.info/121424520X/34.

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Aqbi, Sadiq [Verfasser], Madhukar [Akademischer Betreuer] Chandra, Madhukar [Gutachter] Chandra und Ian Andrew [Gutachter] Glover. „Improving the Performance of Dual Linear Polarization Antennas with Metamaterial Structures / Sadiq Aqbi ; Gutachter: Madhukar Chandra, Ian Andrew Glover ; Betreuer: Madhukar Chandra“. Chemnitz : Universitätsbibliothek Chemnitz, 2018. http://d-nb.info/121464984X/34.

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Ibba, Tiziana. „Chandra investigation of 3CRR radio sources at high redshift“. Master's thesis, Alma Mater Studiorum - Università di Bologna, 2020. http://amslaurea.unibo.it/20023/.

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In this thesis the main goal is to investigate the nuclear regions of high-redshift AGN, in order to characterize their X-ray properties and make a comparison with sources at lower redshifts. In the local Universe, a correlation between accretion estimated with the X-ray luminosity between 2-10keV and with the [OIII] IR emission, has been inferred. It is intriguing to observe if this is still valid for the AGN at high redshifts, even if the observation for this sources are more challenging. For this purpose, I proceeded reducing and analysing the X-ray data available in the Chandra public archive for all the sources at z>1 in the 3CRR catalog. This catalog is well observed in all the spectral range, but the X-ray band permits the investigation of the nuclear energetic processes at scales ranging from the kpc to (less than)pc. In addition, a systematic qualitative imaging has been used has a guiding tool during the analysis. In two sources a clear sign of rich environment was visible. Almost all the objects were well represented by a simple absorbed power law model, with the exception of three objects which showed other features (i.e., the Fe line and a thermal component). The luminosity obtained were compared to the [OIII] and they showed a discrepancy. Being aware of the observational limits in the X-ray band and suspecting an observational bias, an investigation based on the IR absorption was carried on. From this scrutiny emerged that most of the radio galaxies, due to their complexity, are more absorbed than the X-ray analysis managed to find. Assuming the existence of this bias and removing the biased objects from the sample, the X-ray and O[III] luminosity are in agreement. Doing a comparison with the radio galaxies at lower redshift studied by Macconi et al. (2020), the objects in my sample successfully reproduce the same correlation, shifted at higher accretion values.
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Rutherford, John (John Morton). „Imaging X-ray spectroscopy with micro-X and Chandra“. Thesis, Massachusetts Institute of Technology, 2013. http://hdl.handle.net/1721.1/84183.

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Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2013.
This electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections.
Cataloged from student-submitted PDF version of thesis.
Includes bibliographical references (pages 245-258).
High spectral resolution observations of X-ray phenomena have the potential to uncover new physics. Currently, only point sources can be probed with high resolution spectra, using gratings. Extended objects like supernova remnants cannot be dispersed, leaving the dense forest of emission lines blended by the moderate resolution of modern instruments. In the first half of this thesis, I undertake two investigations of the supernova remnant Cassiopeia A using the flagship X-ray observatory, Chandra. The first study combines the spatial resolution of the ACIS instrument with the spectral resolution of the dispersive HETG to investigate the evolution of ejecta knots. The second improves on statistical limits of radioactive ejecta, and simulates what higher resolution instruments may observe. Micro-X, a new high resolution X-ray telescope, is the focus of the second half. I detail the commissioning of this novel sounding rocket payload, which uses a focal plane of micro-calorimeters to achieve high spectral resolution in each pixel. The flight hardware is in a final state of testing and integration before the launch, which is anticipated in 2014.
by John Rutherford.
Ph.D.
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Rosignoli, Luca. „Analisi dettagliata di nuove osservazioni Chandra di Abell 2495“. Master's thesis, Alma Mater Studiorum - Università di Bologna, 2022. http://amslaurea.unibo.it/25297/.

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Questo lavoro di tesi consiste in uno studio in banda X dell'ammasso di galassie Abell 2495 (z~0.079), basato sull'analisi dettagliata di nuove osservazioni del telescopio spaziale Chandra della durata di ~130 ks. Sono stati confermati alcuni dei risultati trovati in precedenza da uno studio basato su una singola esposizione di ~8 ks. In particolare, la presenza di due offset spaziali: il primo tra il picco di emissione X e la radio galassia centrale (~6 kpc), mentre il secondo tra il picco di emissione Hα e quello X (~4 kpc). Inoltre, sono state osservate due coppie di depressioni in brillanza, simili a quelle trovate in precedenza e supposte essere cavità scavate dai getti radio dell'AGN centrale. In particolare, una coppia risulta vicina all'AGN, con un raggio di r~3 kpc, mentre la seconda si trova più esternamente, in contrapposizione rispetto al picco di emissione X e con un raggio di ~5 kpc. Infine, dall'analisi morfologica è emersa una possibile discontinuità nel profilo di brillanza, successivamente identificata come cold front dovuta all'oscillazione del gas. L'analisi spettrale ha permesso di creare i profili delle quantità termodinamiche del gas con una risoluzione e una statistica molto maggiori rispetto al lavoro precedente. Eseguendo un bilancio energetico tra la potenza delle cavità e la luminosità entro il raggio di cooling è emerso che l'energia immessa dall'AGN è capace di controbilanciare il raffreddamento del gas, sebbene la presenza di offset tra il picco di emissione X e l'AGN centrale possa compromettere il ciclo di AGN feedback. In questo contesto l'interpretazione preferita risulta essere quella basata sul fenomeno di oscillazione del gas (sloshing) la cui periodicità potrebbe attivare l'AGN, mantenendo così il ciclo di feedback. Questo scenario, che è in grado di spiegare la presenza degli offset osservati, è supportato dal fatto che la stima del tempo di oscillazione risulta consistente con la differenza di età delle due coppie di cavità.
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Bücher zum Thema "Chandrian"

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Academy, Kalpatharu Research, Hrsg. Lalitārchana-chandrikā. Bangalore: Kalpatharu Research Academy, 2004.

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Coulter, Catherine. Chandra. Moskva: AST, 2000.

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Kelegama, Keerthi. Good-bye Chandrika. Colombo: K. Kelegama, 1999.

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Rāmavarmā. Chandrikā kalā pidam. Herausgegeben von Seshadri S und Kācinātan̲ Naṭan̲a. Madras: Government Oriental Manuscripts Library, 1995.

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Shashi, Pravin C. Patel. Amasno chandra. Ahmedabad: Navbharat Sahitya, 1998.

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Chandra, Avinash. Avinash Chandra. London: the gallery, 1987.

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S, Chandrasekhar, und Manas Pratim Das. Remembering Chandra. Kolkata: Ganadarpan, 2010.

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1460-1539, Vyāsatīrtha, und Pandurangi Krishnacharya Tamanacharya 1918-, Hrsg. Essentials of Tātparya chandrikā and Śloka Tātparya chandrikā of Śrī Vyāsatīrtha. Novi Michigan: World Forum of Sri Vyasaraja Devotees, 2006.

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Debo, Sarat Chandra. Sarat Chandra Debo. Bhubaneswar: Working Artists' Association of Orissa, 1987.

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author, Nandi Subrata, Hrsg. Bidhan Chandra Roy. Kolkata: Readers Service, 2013.

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Buchteile zum Thema "Chandrian"

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Langlois, Anthony J. „Kukathas, Chandran“. In Encyclopedia of Global Justice, 618–20. Dordrecht: Springer Netherlands, 2011. http://dx.doi.org/10.1007/978-1-4020-9160-5_14.

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Kreutzer, Eberhard. „Chandra, Vikram“. In Kindlers Literatur Lexikon (KLL), 1. Stuttgart: J.B. Metzler, 2020. http://dx.doi.org/10.1007/978-3-476-05728-0_9167-1.

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Bainbridge, Susan, und Norine Wark. „Gunawardena, Chandra“. In The Encyclopedia of Female Pioneers in Online Learning, 124–36. New York: Routledge, 2022. http://dx.doi.org/10.4324/9781003275329-13.

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Ghosh, J. K. „Prasanta Chandra Mahalanobis“. In Statisticians of the Centuries, 434–38. New York, NY: Springer New York, 2001. http://dx.doi.org/10.1007/978-1-4613-0179-0_93.

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Bonnafé, Cédric. „Harish-Chandra Induction“. In Representations of SL2(Fq), 29–35. London: Springer London, 2011. http://dx.doi.org/10.1007/978-0-85729-157-8_3.

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Dixmier, Jacques. „Harish-Chandra modules“. In Graduate Studies in Mathematics, 295–324. Providence, Rhode Island: American Mathematical Society, 1996. http://dx.doi.org/10.1090/gsm/011/09.

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Sil, Narasingha. „Chatterjee, Bankim Chandra“. In Hinduism and Tribal Religions, 1–4. Dordrecht: Springer Netherlands, 2018. http://dx.doi.org/10.1007/978-94-024-1036-5_570-1.

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Sil, Narasingha. „Chatterjee, Bankim Chandra“. In Hinduism and Tribal Religions, 1–4. Dordrecht: Springer Netherlands, 2019. http://dx.doi.org/10.1007/978-94-024-1036-5_570-2.

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Naskar, Sourav. „Bankim Chandra Chattopadhyay“. In Reappraising Modern Indian Thought, 215–36. Singapore: Springer Nature Singapore, 2022. http://dx.doi.org/10.1007/978-981-19-1415-7_10.

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Ashu J. „Bipin Chandra Pal“. In Reappraising Modern Indian Thought, 169–202. Singapore: Springer Nature Singapore, 2022. http://dx.doi.org/10.1007/978-981-19-1415-7_8.

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Konferenzberichte zum Thema "Chandrian"

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Yeom, Inhwa, und Seogsung Jang. „Chandra X“. In SA '22: SIGGRAPH Asia 2022 Art Gallery. New York, NY, USA: ACM, 2022. http://dx.doi.org/10.1145/3550470.3558419.

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„The use of human-in-the-loop and constructive simulation to support operations research into MH-60R tactics development“. In 21st International Congress on Modelling and Simulation (MODSIM2015). Modelling and Simulation Society of Australia and New Zealand, 2015. http://dx.doi.org/10.36334/modsim.2015.d2.chandran.

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Tjahjono, Eka Budi, Fahmi Umasangadji und Oktavia Fatmawati. „Analisis Sistem Prosedur Penggunaan Peralatan Keselamatan Kerja Untuk Menghindari Kecelakaan Kerja Di Atas Kapal MT. Surya“. In Peran Penelitian Di Era 4.0 Dalam Menciptakan Sumber Daya Manusia Yang Link And Match Di Industri Maritim. Sekolah Tinggi Ilmu Pelayaran Jakarta, 2021. http://dx.doi.org/10.36101/pcsa.v3i1.167.

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Dalam pengoperasian kapal ditemukan banyak pekerjaan berat yang beresiko terhadap keselamatan awak kapal. Dalam skripsi ini penulis mengamati aspek keselamatan kerja awak kapal di atas kapal MT. Surya Chandra. Selama penulis melaksanakan praktek laut di atas kapal MT. Surya Chandra, penulis seringkali menemukan pelanggaran pelanggaran yang dilakukan oleh beberapa awak kapal yang tidak mematuhi perturan tentang prosedur diatas kapal. Beberapa kali pun sering terjadi kecelakaan kecelakaan yang diakibatkan kelalaian dan ketidaktaatan awak kapal dalam menjalankan prosedur keselamatan kerja Dengan dasar seperti itu penulis akan memaparkan pengalaman dan ilmu yang diperoleh selama di kapal pada saat praktek laut dan dalam skripsi ini secara penulis melaksanakan penelitian dengan sifat penelitian yaitu secara metodologi penelitian kualitatif , yakni penulis lebih menggunakan teknik analisis, mengkaji masalah secara khusus dengan cara menuliskan kendala-kendala dalam penerapan penggunaan alat keselamatan kerja guna menghindari kecelakaan di atas kapal pada saat melaksanakan praktek laut di atas kapal MT. SURYA CHANDRAPeraturan-peraturan ini secara global bertujuan untuk mencegah dan atau mengurangi kecelakaan dan akibatnya serta menjamin keselamatan kerja bagi kru di atas kapal. Manfaat dari penelitian ini untuk mendapatkan model yang paling tepat dalam menerapkan sistem prosedur keselamatan kerja diatas MT. Surya Chandra.
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Rots, Arnold H., Sherry L. Winkelman, Stephane Paltani und Edward E. DeLuca. „Chandra data archive operations“. In Astronomical Telescopes and Instrumentation, herausgegeben von Peter J. Quinn. SPIE, 2002. http://dx.doi.org/10.1117/12.460662.

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McKendrick, Leon. „Chandra Operations Lessons Learned“. In Space 2004 Conference and Exhibit. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2004. http://dx.doi.org/10.2514/6.2004-6040.

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Blackwell, Jr., William C., Joseph I. Minow, Stephen L. O'Dell, Robert M. Suggs, Douglas A. Swartz, Allyn F. Tennant, Shanil N. Virani und Kevin M. Warren. „Modeling the Chandra space environment“. In International Symposium on Optical Science and Technology, herausgegeben von Kathryn A. Flanagan und Oswald H. W. Siegmund. SPIE, 2000. http://dx.doi.org/10.1117/12.409105.

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Spitzbart, Brad D., Scott J. Wolk und Takashi Isobe. „Chandra monitoring, trends, and response“. In Astronomical Telescopes and Instrumentation, herausgegeben von Peter J. Quinn. SPIE, 2002. http://dx.doi.org/10.1117/12.460657.

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8

Brickhouse, Nancy S. „The chandra emission line project“. In The 12th topical conference on atomic processes in plasmas. AIP, 2000. http://dx.doi.org/10.1063/1.1361796.

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9

Kashyap, Vinay L., Jeremy J. Drake und Sun Mi Chung. „Chandra HRC-S degapping corrections“. In SPIE Astronomical Telescopes + Instrumentation, herausgegeben von Guenther Hasinger und Martin J. L. Turner. SPIE, 2004. http://dx.doi.org/10.1117/12.551790.

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10

Spitzbart, Bradley D., und Scott J. Wolk. „Chandra automated point source processing“. In SPIE Astronomical Telescopes + Instrumentation. SPIE, 2004. http://dx.doi.org/10.1117/12.552138.

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Berichte der Organisationen zum Thema "Chandrian"

1

Fabian, A. C. A Deep Chandra Observation of the Centaurus Cluster:Bubbles, Filaments and Edges. Office of Scientific and Technical Information (OSTI), März 2005. http://dx.doi.org/10.2172/839898.

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2

Kouveliotou, C. Chandra Observations of the X-Ray Environs of SN 1998BW / GRB 980425. Office of Scientific and Technical Information (OSTI), Juli 2004. http://dx.doi.org/10.2172/827302.

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3

Madejski, Grzegorz. Simultaneous Chandra and RXTE Observations of the nearby bright Seyfert 2 galaxy NGC 4945. Office of Scientific and Technical Information (OSTI), Januar 2003. http://dx.doi.org/10.2172/812617.

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4

Kaastra, J. S., N. Werner, J. W. A. den Herder, F. B. S. Paerels, J. de Plaa, A. P. Rasmussen und C. P. de Vries. The O VII X-Ray Forest Toward Markarian 421: Consistency between XMM-Newton and Chandra. Office of Scientific and Technical Information (OSTI), April 2006. http://dx.doi.org/10.2172/881780.

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