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EPSC2015-913, 2015 European Planetary Science Congress 2015 Eeuropeapn Planetarsy Science Ccongress C Author(S) 2015
EPSC Abstracts Vol. 10, EPSC2015-913, 2015 European Planetary Science Congress 2015 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2015 The “Station de Planétologie des Pyrénées” (S2P), a collaborative science program in the course of a long history at Pic du Midi observatory. F. Colas (1), A. Klotz (2), F. Vachier (1), M. Birlan (1), B. Sicardy (3), J. Lecacheux (3), M. Antuna (6), R. Behrend (4), C. Birnbaum (6), G. Blanchard (6), C. Buil (4,5), J. Caquel (6), M. Castets (5), C. Cavadore (4), B. Christophe (6), F. Cochard (4), J.L. Dauvergne (6), F. Deladerriere (6), M. Delcroix (6), V. Denoux (4), J.B. DeVanssay (6), P. Devechere (6), P. Dupouy (5), E. Frappa (6), S. Fauvaud (5), B. Gaillard (6), F. Jabet (6), M. Lavayssiere (6), T. Legault (6), A. Leroy (5), A. Maury (6), M. Meunier (6), C. Pellier (6), C. Rinner (4), E. Rolland (6), O. Stenuit (6), I. Testar (6), P. Thierry (4), O. Thizy (4), B. Tregon (5), F. Vaissiere (4), S. Vauclair (6), C. Viladrich (6), C. Angeli (6), J.E. Arlot (1), M. Assafin (28), D. Bancelin (1), D. Baratoux (29), N. Barrado-Izagirre (8), M.A. Barucci (3), L. Beauvalet (9), P. Bendjoya (13), J. Berthier (1), N. Biver (3), D. Bockelee-Morvan (3), D. Berard (3), S. Bouley (10), S. Bouquillon (9), P. Bourget (11), F. Bragas- Ribas (7), J. Camargo (7), B. Carry (1), S. Chevrel (2), M; Chevreton, (3), P. Colom (3), J. Crovisier (3), J. Demars (1), R. Despiau (2), P. Descamps (1), N. Dolez (2), A. -
Patrimoines Du Sud, 12 | 2020 Comment Évaluer L’Importance Patrimoniale D’Un Lieu Unique Et Complexe Grâce
Patrimoines du Sud 12 | 2020 Patrimoines et numérique : un état de la recherche et des expérimentations Comment évaluer l’importance patrimoniale d’un lieu unique et complexe grâce au numérique ? L’exemple du Pic du Midi How to assess the heritage significance of a unique and complex site using digital tools? The example of the Pic du Midi Loïc Jeanson, Michel Cotte, Florent Laroche et Léa Bland-Dupré Édition électronique URL : http://journals.openedition.org/pds/4837 DOI : 10.4000/pds.4837 ISSN : 2494-2782 Éditeur Conseil régional Occitanie Référence électronique Loïc Jeanson, Michel Cotte, Florent Laroche et Léa Bland-Dupré, « Comment évaluer l’importance patrimoniale d’un lieu unique et complexe grâce au numérique ? L’exemple du Pic du Midi », Patrimoines du Sud [En ligne], 12 | 2020, mis en ligne le 01 septembre 2020, consulté le 02 septembre 2020. URL : http://journals.openedition.org/pds/4837 ; DOI : https://doi.org/10.4000/pds.4837 Ce document a été généré automatiquement le 2 septembre 2020. La revue Patrimoines du Sud est mise à disposition selon les termes de la Licence Creative Commons Attribution - Pas d'Utilisation Commerciale - Pas de Modification 4.0 International. Comment évaluer l’importance patrimoniale d’un lieu unique et complexe grâce ... 1 Comment évaluer l’importance patrimoniale d’un lieu unique et complexe grâce au numérique ? L’exemple du Pic du Midi How to assess the heritage significance of a unique and complex site using digital tools? The example of the Pic du Midi Loïc Jeanson, Michel Cotte, Florent Laroche et Léa Bland-Dupré Introduction 1 Depuis Tarbes, le Pic du Midi semble impossible à éviter. -
Photométrie Et Astrométrie Des Satellites De Jupiter : Application À La Campagne De Phénomènes Mutuels 2015 Eléonore Saquet
Photométrie et Astrométrie des Satellites de Jupiter : application à la campagne de phénomènes mutuels 2015 Eléonore Saquet To cite this version: Eléonore Saquet. Photométrie et Astrométrie des Satellites de Jupiter : application à la campagne de phénomènes mutuels 2015. Astrophysique [astro-ph]. Université Paris sciences et lettres, 2017. Français. NNT : 2017PSLEO013. tel-01887821 HAL Id: tel-01887821 https://tel.archives-ouvertes.fr/tel-01887821 Submitted on 4 Oct 2018 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. A` mes parents, qui ont rendu possible le rˆeve d’une petite fille. T´elescope T1M du Pic du Midi. Cr´edit : St´ephane Vetter. Remerciements Ce m´emoire conclue mon travail de th`ese r´ealis´e`al’Institut de M´ecanique C´eleste et de Calculs des Eph´em´erides. Il n’aurait pas ´et´epossible sans l’appui d’un certain nombre de personnes, auxquelles je tiens `aexprimer ma sinc`ere gratitude. Je tiens tout d’abord `aremercier mes deux directeurs de th`ese Vincent Robert et Jean-Eudes Arlot de m’avoir propos´ece sujet puis de m’avoir encadr´ee pendant ces trois ann´ees. -
Observation of Venus and Mercury Transits from the Pic-Du-Midi Observatory
MEETING VENUS C. Sterken, P. P. Aspaas (Eds.) The Journal of Astronomical Data 19, 1, 2013 Observation of Venus and Mercury Transits from the Pic-du-Midi Observatory Guy Ratier 43 rue des Longues All´ees, F-45800 Saint-Jean-de-Braye, France Sylvain Rondi Soci´et´eAstronomique de France, 3 rue Beethoven, F-75016 Paris France Abstract. The Pic-du-Midi, on the French side of the Pyr´en´ees, became a state observatory in the summer of 1882. The first major astronomical event to be observed was the Venus transit of 6 December 1882. Unfortunately this attempt by the well-known Henry brothers was unsuccessful due to bad weather conditions. During the twentieth century, the Pic-du-Midi became famous for the quality of its solar and planetary observations. In the sixties, Jean R¨osch decided to use this experience to monitor the transits of Mercury. The objective was not to measure the parallax, but to determine the diameter of the planet in order to confirm its high density. Observations were made using a photometric method – the Hertzsprung method – during the transits of 1960, 1970 and 1973. The pioneer work of Ch. Boyer on the rotation of the Venus atmosphere as well as some experiments involving Lyot coronographs are also noteworthy. A Venus transit was finally observed on 8 June 2004 with a new CCD camera, providing a significant contribution to the model of the Venus mesosphere. This opened the field for new observations in 2012. 1. Early days of the Pic-du-Midi Observatory The site of the “Pic-du-Midi de Bigorre”, on the forefront of the Pyr´en´ees, has been known since ages as an ideal location to carry out astronomical observations. -
Year of the Dwarves: Ceres and Pluto Take the Stage
Year of the Dwarves: Ceres and Pluto Take the Stage — Paul Schenk, Lunar and Planetary Institute The year 2015 is shaping up to be one of the most interesting in the short history of space exploration. Fresh on the heels of Rosetta’s spectacular and revolutionary ongoing visit to a comet, and after a wait of more than half a century, we finally reach the first of the so-called dwarf planets, the last class of solar system bodies left unexplored. This year the Dawn and New Horizons missions will both reach their primary targets, Ceres and Pluto. Indeed, Dawn is on its final approach to Ceres as this is being written. Both Ceres and Pluto are very planetary in nature. Each is the major representative of its planetary zone. LCeres holds about one-third of the total mass in the asteroid belt, and may be actively venting water vapor into space. Pluto is likely the largest Kuiper belt object (KBO), and even has a significant atmosphere and a family of at least five moons. What will we see at Ceres and Pluto? Scientists and interested laypeople have been speculating quite a lot as we approach these two bodies. In some sense, it is an opportunity to test how well we really understand planetary bodies. Both Ceres P and Pluto (and its large moon Charon) are believed to be rich in water ice. Pluto is known to have other ices on its surface, include methane, nitrogen, and carbon monoxide. We are fortunate that we have already extensively mapped comparably- Our best Earth-based views of Ceres (left) and Pluto (right), sized ice-rich bodies, which serve as both from Hubble Space Telescope images. -
Tourmalet & Cycling's Greatest Challenges
Tourmalet & Cycling's Greatest Challenges - The Easier Way The peloton of the Tour de France has no time to enjoy the beautiful valleys and mountains of the central Pyrenees, or its authentic villages, great places to stay, and interesting regional cuisine. You will share their cycling challenges with the not insignificant help of e-bikes and travelling at your own pace, then be able to relax each evening in a way they can only dream of. If you love cycling and you love a challenge, but are not superhuman, this is the holiday for you - and one you will remember for all the best reasons. 7 nights - 6 days e-bike cycling Minimum required 1 From point to point With luggage transportation Self-guided Code : FP9PUTF The plus points • The major climbs and cols of the Tour de France • Cycling made easier - and much more enjoyable - thanks to electric bikes • An independent holiday - cycle at your own pace • Good quality, comfortable accommodation - and good meals too FP9PUTF Last update 29/12/2020 1 / 13 Before departure, please check that you have an updated fact sheet. FP9PUTF Last update 29/12/2020 2 / 13 The Tour de France's days in the Pyrenees are the most challenging cycling in the world. Now imagine you breezing up the Col du Tourmalet with a big grin on your face as you reach the summit of the Col d'Aubisque. You can now enjoy the most interesting and famous sections of the Tour de France route with the help of an electric bike - and Purely Pyrenees, the leading walking and cycling tour operator in the Pyrenees. -
Solar Survey at Pic Du Midi: Calibrated Data and Improved Images Laurent Koechlin1, Luc Dettwiller2, Maurice Audejean3, Maël Valais1, and Arturo López Ariste1
A&A 631, A55 (2019) Astronomy https://doi.org/10.1051/0004-6361/201732504 & c L. Koechlin et al. 2019 Astrophysics Solar survey at Pic du Midi: Calibrated data and improved images Laurent Koechlin1, Luc Dettwiller2, Maurice Audejean3, Maël Valais1, and Arturo López Ariste1 1 Institut de recherches en astrophysique et planétologie, Université de Toulouse, CNRS, CNES, UPS, 14 Avenue Edouard Belin, 31400 Toulouse, France e-mail: [email protected] 2 Lycée Blaise Pascal, 36 Avenue Carnot, 63037 Clermont-Ferrand Cedex, France 3 Observateurs associés, Rue de la Cau, 65200 Bagnères de Bigorre, France Received 20 December 2017 / Accepted 5 September 2019 ABSTRACT Context. We carry out a solar survey with images of the photosphere, prominences, and corona at Pic du Midi observatory. This sur- vey, named CLIMSO (for CLIchés Multiples du SOleil), is in the following spectral lines: Fe XIII corona (1.075 µm), Hα (656.3 nm), and He I (1.083 µm) prominences, and Hα and Ca II (393.4 nm) photosphere. All frames cover 1.3 times the diameter of the Sun with an angular resolution approaching one arcsecond. The frame rate is one per minute per channel (weather permitting) for the prominences and chromosphere, and one per hour for the Fe XIII corona. This survey started in 2007 for the disk and prominences and in 2015 for the corona. We have almost completed one solar cycle and hope to cover several more, keeping the same wavelengths or adding others. Aims. We seek to make the CLIMSO images easier to use and more profitable for the scientific community. -
Gresham College
GRE SHA M . co Reproduction of this tefi, or any efiract from it, must credit Gresham College THE SKY’S THE LIMIT! A Lectire by PROFESSOR HEATHER COUPER BSC DLitt(Hon) FRAS Gresham Professor of Astronomy 16 November 1994 .,, . .. .,,... .,..’.. -. , i GRESH.4.bI COLLEGE Policy & Objectives h independently funded educational institution, Gresham College exists . to continue the free public lectures which have been given for 400 years, and to reinterpret the ‘new lehg’ of Sir ~omas Gresham’s day in contemporary terms; to engage in study, teaching and research, particularly in those disciplines represented by the Gresham Professors; to foster academic consideration of contemporary problems; to challenge those who live or work in the City of London to engage in intellectual debate on those subjects in which the City has a proper concern; and to provide a window on the City for le-ed societies, both national and international. GreshamCollege,Barnard’sInn Hall, Holbom, LondonEClN 2HH Tel: 020783 I 0j75 Fax: 02078315208 e-mail:[email protected] THE SKY’S THE LIMIT! Professor Heather Couper Why do astronomers do astronomy? A lot of people (especially cynical journalists) ask me this question. It’s often assumed that astronomy - at best - is the useless pursuit of measuring the positions of stars in the sky, or - at worst - is something to do with being engaged in a secret follow-up to President Reagan’s Star Was military prograrnme. Whatever, astronomy is believed to be other-worldly, irrelevant, a waste of money, and something that is only studied by old men with long white beards. -
Reviews the History of Astronomy
Reviews The history of astronomy by Heather Couper & Nigel Henbest Cassell Illustrated, 2007. ISBN 978- 1-84403-570-0. Pp 288 (247× 297mm), £30 (hbk). One of the great joys of the history of astronomy is that it can be treated on many different levels. You can delve deep and immerse yourself in four hundred page tomes on the significance of the ob- servations of the comet of 1577, and you can wallow in a huge three volume set of the letters of John Flamsteed, our first Astronomer Royal, or you can flit briefly and joyfully from highlight to highlight. Heather Couper and Nigel Henbest adopt the latter approach. They have travelled widely and interviewed many of the key players in recent astronomical and astrophysical history, as well as those who study the development of as- tronomy over the past few thousand years. The views of the authors and the peo- ing at some of the pictures of famous astro- ple they interviewed have then been skil- nomical scientists, one can often pick up fully knitted together to produce an im- hints of the darker side. I wonder how frus- mensely readable, easily accessible and racy trated Gustav Kirchhoff and Robert Bun- overview of mankind’s stumbling attempts sen felt trying to understand spectral lines to understand the cosmos. From Stonehenge before the electron had been discovered. to SETI (the Search for Extraterrestrial In- Galileo Galilei looks very uncomfortable at telligence), and from black holes to Bethle- his inquisition, moving the Earth from the hem’s star, little has been overlooked. -
Project Periodic Report
PROJECT PERIODIC REPORT Grant Agreement number: 654208 Project acronym: EPN2020-RI Project title: EUROPLANET 2020 Research Infrastructure Call identifier: H2020-INFRAIA-1-2014-2015 Date of latest version of Annex I against which the assessment will be made: 1st March 2016 Periodic report: 1st □ 2nd X 3rd □ 4th □ Period covered: from 1 March 2017 to 31 August 2018 Project website address: http://www.europlanet-2020-ri.eu/ 1 Table of Content List of Figures 7 List of Tables 10 Table of Main Acronyms 11 Project Summary 11 1. Background 11 2. Europlanet 2020 Research Infrastructure - Impact to date 11 3. Collaborations with other EU projects 14 4. Future Plans and Sustainability 15 5. Conclusion 15 1. WP1: Management 16 1.1 Explanation of the work carried out by the beneficiaries and overview of progress 16 Task 1.1 - Management structure and tools 16 Task 1.2 - Regular operations of the management structure 16 Task 1.3 - Reporting 17 Task 1.4 - Call for proposals, evaluation and validation of Transnational Access visits 17 Task 1.5 – Sustainability and Financial Plan 26 Task 1.6 - Data management 27 1.2 Impact 27 2. Deviations from Annex 1 30 2.1 Amendments 30 2.2.2 Additional proposed changes 31 3. Financial reports 31 2. WP2 - TA 1: Planetary Field Analogues (PFA) 34 1.1 Explanation of the work carried out by the beneficiaries and overview of progress 34 Task 2.1-Rio Tinto (INTA) 34 Task 2.2-Ibn Battuta Centre (IRSPS) 35 Task 2.3- The glacial and volcanically active areas of Iceland, Iceland (MATIS) 36 Task 2.4 Lake Tirez (INTA) 37 Task 2.5-Danakil Depression, Ethiopia (IRSPS) 38 1.2 Impact 40 3. -
107 V Ariations on the Unexpected
107 Variations on the Unexpected SURPRISE 107 Variations on the Unexpected Dedication and Prelude To Raine Daston In his essay “Of Travel,” Francis Bacon recommends that diaries be used to register the things “to be seen and observed.” Upon returning home, the traveler should not entirely leave the visited countries, but maintain a correspondence with those she met, and let her experi- ence appear in discourse rather than in “apparel or gesture.” Your itineraries through a vast expanse of the globe of knowledge seem to illustrate Bacon’s recommendations, and have inspired many to em- bark on the exploration of other regions—some adjacent, some dis- tant from the ones you began to clear. Yet not all have journeyed as well equipped as you with notebooks, nor assembled them into a trove apt to become, as Bacon put it, “a good key” to inquiry. As you begin new travels, you may add the present collection to yours, and adopt the individual booklets as amicable companions on the plane or the U-Bahn. Upon wishing you, on behalf of all its contributors, Gute Reise! and Bon voyage!, let us tell you something about its gen- esis and intention. Science depends on the unexpected. Yet surprise and its role in the process of scientific knowledge-making has hitherto received lit- tle attention, let alone systematic investigation. If such a study ex- isted, it would no doubt have been produced in your Department at the Max Planck Institute for the History of Science. The topic is a seamless match with your interest in examining ideals and practices of scientific and cultural rationality—ideals and practices often so fundamental that they appear to transcend history or are overlooked altogether. -
The Pre-Embryonic State of the AAVSO
154 Saladyga, JAAVSO Volume 27, 1999 THE “PRE-EMBRYONIC” STATE OF THE AAVSO: AMATEUR OBSERVERS OF VARIABLE STARS IN THE UNITED STATES FROM 1875 TO 1911 Michael Saladyga AAVSO Headquarters 25 Birch Street Cambridge, MA 02138 Presented at the 87th Annual Meeting of the AAVSO, October 31, 1998 Abstract For 35 years before the formation of the AAVSO, independent amateur variable star astronomers in the United States were making significant contributions to the field. Skilled, dedicated individuals like S. C. Chandler, E. F. Sawyer, and P. S. Yendell laid the foundation in variable star work that was expanded upon by Harvard College Observatory Director E. C. Pickering, under whose direction a new generation of enthusiastic amateur and professional astronomers continued to further the cause of variable star research. This paper is a survey of the contributions made by several independent amateur variable star astronomers, and it is also a chronology of the growth of a broader, more popularized, amateur involvement in variable star astronomy which led to the organization of the AAVSO in 1911. 1. Introduction The German astronomer Friedrich Argelander is well-known in variable star histories as the “father of variable star observing.” The professional astronomer Argelander in 1844 first brought to the attention of the astronomical community the phenomena of variable stars and the need for observations of them. His Uranometria Nova catalogue of the magnitudes of over 3,500 northern stars was a great boost to the involvement of amateur observers of variable stars in Europe. This catalogue was not widely available in America, hence the late start here in amateur variable star work.