Al-Biruni: a Great Muslim Scientist, Philosopher and Historian (973 – 1050 Ad)
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Using Crowdsourcing to Prioritize Bicycle Network Improvements
GEORGIA DOT RESEARCH PROJECT 14-39 FINAL REPORT USING CROWDSOURCING TO PRIORITIZE BICYCLE NETWORK IMPROVEMENTS OFFICE OF RESEARCH 15 KENNEDY DRIVE FOREST PARK, GA 30297-2534 This page intentionally left blank. GDOT Research Project RP14-39 Final Report Using Crowdsourcing to Prioritize Bicycle Network Improvements By Dr. Kari E. Watkins Assistant Professor School of Civil and Environmental Engineering Georgia Institute of Technology Dr. Chris LeDantec Assistant Professor School of Literature, Media and Communication Georgia Institute of Technology Contract with Georgia Department of Transportation In cooperation with U.S. Department of Transportation Federal Highway Administration April 2016 The contents of this report reflect the views of the author(s) who is (are) responsible for the facts and the accuracy of the data presented herein. The contents do not necessarily reflect the official views or policies of the Georgia Department of Transportation or the Federal Highway Administration. This report does not constitute a standard, specification, or regulation. i This page intentionally left blank. ii 1.Report No.: 2. Government Accession No.: 3. Recipient's Catalog No.: FHWA-GA-16-1439 4. Title and Subtitle: 5. Report Date: Using Crowdsourcing to Prioritize Bicycle April 2016 Network Improvements 6. Performing Organization Code 7. Author(s): 8. Performing Organ. Report No.: Dr. Kari E. Watkins, PE (P.I.), Dr. Chris LeDantec (co-P.I), Aditi Misra, Mariam Asad, Charlene Mingus, Cary Bearn, Alex Poznanski, Anhong Guo, Rohit Ammanamanchi, Vernon Gentry, Aaron Gooze 9. Performing Organization Name and Address: 10. Work Unit No. Georgia Institute of Technology 11. Contract or Grant No.: School of Civil and Environmental Engineering GDOT Research Project No. -
Ibrāhīm Ibn Sinān Ibn Thābit Ibn Qurra
From: Thomas Hockey et al. (eds.). The Biographical Encyclopedia of Astronomers, Springer Reference. New York: Springer, 2007, p. 574 Courtesy of http://dx.doi.org/10.1007/978-0-387-30400-7_697 Ibrāhīm ibn Sinān ibn Thābit ibn Qurra Glen Van Brummelen Born Baghdad, (Iraq), 908/909 Died Baghdad, (Iraq), 946 Ibrāhīm ibn Sinān was a creative scientist who, despite his short life, made numerous important contributions to both mathematics and astronomy. He was born to an illustrious scientific family. As his name suggests his grandfather was the renowned Thābit ibn Qurra; his father Sinān ibn Thābit was also an important mathematician and physician. Ibn Sinān was productive from an early age; according to his autobiography, he began his research at 15 and had written his first work (on shadow instruments) by 16 or 17. We have his own word that he intended to return to Baghdad to make observations to test his astronomical theories. He did return, but it is unknown whether he made his observations. Ibn Sinān died suffering from a swollen liver. Ibn Sinān's mathematical works contain a number of powerful and novel investigations. These include a treatise on how to draw conic sections, useful for the construction of sundials; an elegant and original proof of the theorem that the area of a parabolic segment is 4/3 the inscribed triangle (Archimedes' work on the parabola was not available to the Arabs); a work on tangent circles; and one of the most important Islamic studies on the meaning and use of the ancient Greek technique of analysis and synthesis. -
In. ^Ifil Fiegree in PNILOSOPNY
ISLAMIC PHILOSOPHY OF SCIENCE: A CRITICAL STUDY O F HOSSAIN NASR Dis««rtation Submitted TO THE Aiigarh Muslim University, Aligarh for the a^ar d of in. ^Ifil fiegree IN PNILOSOPNY BY SHBIKH ARJBD Abl Under the Kind Supervision of PROF. S. WAHEED AKHTAR Cbiimwa, D«ptt. ol PhiloMphy. DEPARTMENT OF PHILOSOPHY ALIGARH IWIUSLIIM UNIVERSITY ALIGARH 1993 nmiH DS2464 gg®g@eg^^@@@g@@€'@@@@gl| " 0 3 9 H ^ ? S f I O ( D .'^ ••• ¥4 H ,. f f 3« K &^: 3 * 9 m H m «< K t c * - ft .1 D i f m e Q > i j 8"' r E > H I > 5 C I- 115m Vi\ ?- 2 S? 1 i' C £ O H Tl < ACKNOWLEDGEMENT In the name of Allah« the Merciful and the Compassionate. It gives me great pleasure to thanks my kind hearted supervisor Prof. S. Waheed Akhtar, Chairman, Department of Philosophy, who guided me to complete this work. In spite of his multifarious intellectual activities, he gave me valuable time and encouraged me from time to time for this work. Not only he is a philosopher but also a man of literature and sugge'sted me such kind of topic. Without his careful guidance this work could not be completed in proper time. I am indebted to my parents, SK Samser All and Mrs. AJema Khatun and also thankful to my uncle Dr. Sheikh Amjad Ali for encouraging me in research. I am also thankful to my teachers in the department of Philosophy, Dr. M. Rafique, Dr. Tasaduque Hussain, Mr. Naushad, Mr. Muquim and Dr. Sayed. -
The History of Arabic Sciences: a Selected Bibliography
THE HISTORY OF ARABIC SCIENCES: A SELECTED BIBLIOGRAPHY Mohamed ABATTOUY Fez University Max Planck Institut für Wissenschaftsgeschichte, Berlin A first version of this bibliography was presented to the Group Frühe Neuzeit (Max Planck Institute for History of Science, Berlin) in April 1996. I revised and expanded it during a stay of research in MPIWG during the summer 1996 and in Fez (november 1996). During the Workshop Experience and Knowledge Structures in Arabic and Latin Sciences, held in the Max Planck Institute for the History of Science in Berlin on December 16-17, 1996, a limited number of copies of the present Bibliography was already distributed. Finally, I express my gratitude to Paul Weinig (Berlin) for valuable advice and for proofreading. PREFACE The principal sources for the history of Arabic and Islamic sciences are of course original works written mainly in Arabic between the VIIIth and the XVIth centuries, for the most part. A great part of this scientific material is still in original manuscripts, but many texts had been edited since the XIXth century, and in many cases translated to European languages. In the case of sciences as astronomy and mechanics, instruments and mechanical devices still extant and preserved in museums throughout the world bring important informations. A total of several thousands of mathematical, astronomical, physical, alchemical, biologico-medical manuscripts survived. They are written mainly in Arabic, but some are in Persian and Turkish. The main libraries in which they are preserved are those in the Arabic World: Cairo, Damascus, Tunis, Algiers, Rabat ... as well as in private collections. Beside this material in the Arabic countries, the Deutsche Staatsbibliothek in Berlin, the Biblioteca del Escorial near Madrid, the British Museum and the Bodleian Library in England, the Bibliothèque Nationale in Paris, the Süleymaniye and Topkapi Libraries in Istanbul, the National Libraries in Iran, India, Pakistan.. -
The Persian-Toledan Astronomical Connection and the European Renaissance
Academia Europaea 19th Annual Conference in cooperation with: Sociedad Estatal de Conmemoraciones Culturales, Ministerio de Cultura (Spain) “The Dialogue of Three Cultures and our European Heritage” (Toledo Crucible of the Culture and the Dawn of the Renaissance) 2 - 5 September 2007, Toledo, Spain Chair, Organizing Committee: Prof. Manuel G. Velarde The Persian-Toledan Astronomical Connection and the European Renaissance M. Heydari-Malayeri Paris Observatory Summary This paper aims at presenting a brief overview of astronomical exchanges between the Eastern and Western parts of the Islamic world from the 8th to 14th century. These cultural interactions were in fact vaster involving Persian, Indian, Greek, and Chinese traditions. I will particularly focus on some interesting relations between the Persian astronomical heritage and the Andalusian (Spanish) achievements in that period. After a brief introduction dealing mainly with a couple of terminological remarks, I will present a glimpse of the historical context in which Muslim science developed. In Section 3, the origins of Muslim astronomy will be briefly examined. Section 4 will be concerned with Khwârizmi, the Persian astronomer/mathematician who wrote the first major astronomical work in the Muslim world. His influence on later Andalusian astronomy will be looked into in Section 5. Andalusian astronomy flourished in the 11th century, as will be studied in Section 6. Among its major achievements were the Toledan Tables and the Alfonsine Tables, which will be presented in Section 7. The Tables had a major position in European astronomy until the advent of Copernicus in the 16th century. Since Ptolemy’s models were not satisfactory, Muslim astronomers tried to improve them, as we will see in Section 8. -
The Importance of Translation Mathematics Old Script ABSTRACT
Malaysian Journal of Mathematical Sciences 3(1): 55-66 (2009) The Importance of Translation Mathematics Old Script 1Shahrul Nizam Ishak, 2Noor Hayati Marzuki, 3Jamaludin Md. Ali School of Mathematical Sciences, Universiti Sains Malaysia, Pulau Pinang, Malaysia E-mail: [email protected], [email protected], [email protected] ABSTRACT In this paper, a concise discussion of the text study will be carried out by focusing on the significant of Malay mathematics old script translation. We also discuss the importance of the translation work that need to emphasize. Stages of the translation period based on history knowledge also been highlighted. An example of the translation from Rau ḍat al-Ḥuss āb f ī ‘Ilm al-Ḥis āb that was written by Malay ‘Ulama 1 in 1307H/1893M is also shown here. The book was printed in Egypt and has been used in teaching and learning among the student at the Holy Mosque ( Masjid al- Har ām). Therefore, from this work hope that the introduction of the book presented here is sufficient to stimulate interest in readers and researchers to embark and investigate the beauty and the power of script translation in providing more knowledge especially in the mathematics education area. Keywords: Mathematics Translation, Old Script, Rau ḍat al-Ḥuss āb. INTRODUCTION The amount of translation into Arabic from Greek, Syrian, Persian and Sanskrit was at its peak during the ninth and tenth century. ‘Ulama of Islam, Christianity, Judaism and even Zoroastrianism were employed in the translation and writing new scientific masterpieces. In the course of time the works of Euclid, Ptolemy, Aristotle, Apollonius, Archimedes, Heron, Diophantus and the Hindus were accessible in Arabic. -
Bīrūnī's Telescopic-Shape Instrument for Observing the Lunar
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Revistes Catalanes amb Accés Obert Bīrūnī’s Telescopic-Shape Instrument for Observing the Lunar Crescent S. Mohammad Mozaffari and Georg Zotti Abstract:This paper deals with an optical aid named barbakh that Abū al-Ray¬ān al- Bīrūnī (973–1048 AD) proposes for facilitating the observation of the lunar crescent in his al-Qānūn al-Mas‘ūdī VIII.14. The device consists of a long tube mounted on a shaft erected at the centre of the Indian circle, and can rotate around itself and also move in the vertical plane. The main function of this sighting tube is to provide an observer with a darkened environment in order to strengthen his eyesight and give him more focus for finding the narrow crescent near the western horizon about the beginning of a lunar month. We first briefly review the history of altitude-azimuthal observational instruments, and then present a translation of Bīrūnī’s account, visualize the instrument in question by a 3D virtual reconstruction, and comment upon its structure and applicability. Keywords: Astronomical Instrumentation, Medieval Islamic Astronomy, Bīrūnī, Al- Qānūn al-Mas‘ūdī, Barbakh, Indian Circle Introduction: Altitude-Azimuthal Instruments in Islamic Medieval Astronomy. Altitude-azimuthal instruments either are used to measure the horizontal coordinates of a celestial object or to make use of these coordinates to sight a heavenly body. They Suhayl 14 (2015), pp. 167-188 168 S. Mohammad Mozaffari and Georg Zotti belong to the “empirical” type of astronomical instruments.1 None of the classical instruments mentioned in Ptolemy’s Almagest have the simultaneous measurement of both altitude and azimuth of a heavenly object as their main function.2 One of the earliest examples of altitude-azimuthal instruments is described by Abū al-Ray¬ān al- Bīrūnī for the observation of the lunar crescent near the western horizon (the horizontal coordinates are deployed in it to sight the lunar crescent). -
Spherical Trigonometry in the Astronomy of the Medieval Ke Rala School
SPHERICAL TRIGONOMETRY IN THE ASTRONOMY OF THE MEDIEVAL KE RALA SCHOOL KIM PLOFKER Brown University Although the methods of plane trigonometry became the cornerstone of classical Indian math ematical astronomy, the corresponding techniques for exact solution of triangles on the sphere's surface seem never to have been independently developed within this tradition. Numerous rules nevertheless appear in Sanskrit texts for finding the great-circle arcs representing various astro nomical quantities; these were presumably derived not by spherics per se but from plane triangles inside the sphere or from analemmatic projections, and were supplemented by approximate formu las assuming small spherical triangles to be plane. The activity of the school of Madhava (originating in the late fourteenth century in Kerala in South India) in devising, elaborating, and arranging such rules, as well as in refining formulas or interpretations of them that depend upon approximations, has received a good deal of notice. (See, e.g., R.C. Gupta, "Solution of the Astronomical Triangle as Found in the Tantra-Samgraha (A.D. 1500)", Indian Journal of History of Science, vol.9,no.l,1974, 86-99; "Madhava's Rule for Finding Angle between the Ecliptic and the Horizon and Aryabhata's Knowledge of It." in History of Oriental Astronomy, G.Swarup et al., eds., Cambridge: Cambridge University Press, 1985, pp. 197-202.) This paper presents another such rule from the Tantrasangraha (TS; ed. K.V.Sarma, Hoshiarpur: VVBIS&IS, 1977) of Madhava's student's son's student, Nllkantha's Somayajin, and examines it in comparison with a similar rule from Islamic spherical astronomy. -
The Oldest Translation of the Almagest Made for Al-Maʾmūn by Al-Ḥasan Ibn Quraysh: a Text Fragment in Ibn Al-Ṣalāḥ’S Critique on Al-Fārābī’S Commentary
Zurich Open Repository and Archive University of Zurich Main Library Strickhofstrasse 39 CH-8057 Zurich www.zora.uzh.ch Year: 2020 The Oldest Translation of the Almagest Made for al-Maʾmūn by al-Ḥasan ibn Quraysh: A Text Fragment in Ibn al-Ṣalāḥ’s Critique on al-Fārābī’s Commentary Thomann, Johannes DOI: https://doi.org/10.1484/M.PALS-EB.5.120176 Posted at the Zurich Open Repository and Archive, University of Zurich ZORA URL: https://doi.org/10.5167/uzh-190243 Book Section Accepted Version Originally published at: Thomann, Johannes (2020). The Oldest Translation of the Almagest Made for al-Maʾmūn by al-Ḥasan ibn Quraysh: A Text Fragment in Ibn al-Ṣalāḥ’s Critique on al-Fārābī’s Commentary. In: Juste, David; van Dalen, Benno; Hasse, Dag; Burnett, Charles. Ptolemy’s Science of the Stars in the Middle Ages. Turnhout: Brepols Publishers, 117-138. DOI: https://doi.org/10.1484/M.PALS-EB.5.120176 The Oldest Translation of the Almagest Made for al-Maʾmūn by al-Ḥasan ibn Quraysh: A Text Fragment in Ibn al-Ṣalāḥ’s Critique on al-Fārābī’s Commentary Johannes Thomann University of Zurich Institute of Asian and Oriental Research [email protected] 1. Life and times of Ibn al-Ṣalāḥ (d. 1154 ce) The first half of the twelfth century was a pivotal time in Western Europe. In that period translation activities from Arabic into Latin became a common enterprise on a large scale in recently conquered territories, of which the centres were Toledo, Palermo and Antioch. This is a well known part of what was called the Renaissance of the Twelfth Century.1 Less known is the situation in the Islamic World during the same period. -
Thabit Ibn Qurra : History and the Influence to Detemine the Time of Praying Fardhu
PROC. INTERNAT. CONF. SCI. ENGIN. ISSN 1504607797 Volume 4, February 2021 E-ISSN 1505707533 Page 255-258 Thabit Ibn Qurra : History and The Influence to Detemine The Time of Praying Fardhu Muhamad Rizky Febriawan1, Saka Aji Pangestu2 1 Mathematics Department, 2 Mathematics Education Department, Faculty Mathematics and Natural Science, Yogyakarta State University. Jl. Colombo No. 1 Caturtunggal,, Yogyakarta 55281, Indonesia. Tel. (0274)565411 Email: [email protected] Abstract. The application of mathematical history for overcoming with life’s problems are reflection to build more advanced civilizations than previous civilizations, because by studying history a nation can do an evaluation of the past mistakes. In addition, mathematical history gives wide basic understanding against the mathematical consepts for giving a solution against the problems. Not only about the ideal world held by the Platonist. As example, in the golden age of islam, the scientist at that moment developed knowledge especially mathematics with the principal to solve the problems with in daily life. The one of them is Thabit ibn qurra. Thabit ibn qurra used the principal of geometry to decide motion of the sun. The method used was by means of a shadow that produced by sunlight. So, the muslim can pray fardhu on time. This research is meant to reconstruct the method was used by Thabit ibn qurrah, so that the mathematics especially, the topic of geometry is no longer a matter that cannot be expressed in real or real terms. So that, the young generations, especially muslim will realize that learn the mathematics is invaluable in this life. -
By Sean Jenkins
Web-Based Homework versus Paper-Based Homework in United Arab Emirates Secondary Mathematics By Sean Jenkins A Dissertation Submitted in Fulfilment Of the Requirements for the Degree of Master of Philosophy (Mathematics Education) Of University College London Institute of Education Department of Curriculum, Pedagogy and Assessment University College London March 05, 2021 Abstract This study investigated whether Web-based homework (WBH) in mathematics is a method of homework delivery more suitable than traditional paper-based homework (PBH) for United Arab Emirates (UAE) secondary students in Abu Dhabi. Few studies have addressed delivery methods for mathematics homework outside of a context where homework is considered usual practice. The study centres in the UAE because of its culturally distinctive attitudes towards homework completion and reportedly low levels of self-efficacy among Emirate students. If homework completion and performance were to increase, WBH could offer opportunities to enrich student learning and engagement in mathematics. This study used the WBH tools Myimaths and GeoGebra in selected school years. The research questions for this study were as follows: (1) Do students interact more with WBH than with PBH? (2) What are student perceptions of their learning with WBH and PBH? The sample consisted of approximately 2,000 students. The data for this two-group, pre-and post-test control group design was collected over three years, covering school years 2012 to 2015. As a measure of interaction, a Pearson Chi-square test suggested that student homework completion was significantly higher in the WBH group. The result led to the rejection of the null hypothesis for the first research question, suggesting that students do interact more with WBH than with PBH. -
Homework #3 Solutions Astronomy 10, Section 2 Due: Monday, September 20, 2011
Homework #3 Solutions Astronomy 10, Section 2 due: Monday, September 20, 2011 Chapter 3; Review Questions 5) If a lunar eclipse occurred at midnight, where in the sky would you look to see it? During a lunar eclipse, the Moon, Earth, and Sun must lie along a line. There are only two possible positions in the Moonʼs orbit where this can happen: at the full moon (lunar eclipse) and at the new moon (solar eclipse). If it is midnight and the moon is in its full phase, it will be at its highest possible position in the sky (depends on latitude). If you are in the northern hemisphere, this will be slightly south of your zenith position. 6) Why do solar eclipses happen only at new moon Why not every new moon? Solar eclipses happen when the moon is directly between the Earth and the Sun. This corresponds to the New Moon phase. Solar eclipses do not occur every New Moon because of the small tilt of the Moonʼs orbital plane relative to the ecliptic. Solar eclipses occur when the Earth/Sun/Moon all lie along the line that is the intersection between the ecliptic plane and the Moonʼs orbital plane. Chapter 4; Review Questions 5) When Tycho observed the new star of 1572, he could detect no parallax. Why did that result sustain belief in the Ptolemaic system? If the Earth is orbiting the Sun (and not vice-versa as in the geocentric model), we would be observing the Universe from two different vantage points. This would give us “depth perception” in that weʼd be able to distinguish nearby stars from distant stars via the angular shift in position that is parallax.