Scenic Spaces of Isolation1

Total Page:16

File Type:pdf, Size:1020Kb

Scenic Spaces of Isolation1 Scenic spaces of isolation1 Sabine Popp Fine Art Department, Bergen Academy of Arts and Design, Strømgaten 1, 5015 Bergen, Norway. Email: [email protected] Scenic Spaces of Isolation is a body of artistic work grown from two residency periods in the polar night in Ny-Ålesund (2009 – 2010). Focus of the work was the experience of an isolated community in complete darkness, surrounded by a barren landscape under the influence of harsh climate, which isn’t visible but is nevertheless present and palpable. Under investigation was the relationship between physical and mental space on the one hand, and forms of practical solutions for the organisation of daily life on the other. Part of the investigation is complete immersion: Throughout the work, bodily experience and involvement with physical processes is juxtaposed with the examination and application of monitoring systems in the approach to and the understanding of place. 1 This research received funding from The Relief Fund for Visual Artists, Norway Popp A Home for Science, Social Studies of Science 46(6) Ny-Ålesund has the world’s northernmost indoor-climbing wall. One can find it on the same road as the former school, which houses the Indian research station today, beside the old post office. The road leads down to the harbour, and the post office would be in use only in the short summer, when cruise ships arrive in Kongsfjorden and tourists need to stamp a proof of their presence so far to the north on their postcards. In winter, the tiny building’s inside walls and lockers can be covered with a sparkling layer of rime. The settlement is located on a plain at the foot of a mountain range at the southern coastline of the fjord. Buildings are spread along roads as in a normal village, but these roads do not stretch more than 4 km altogether and they end before they can reach the horizon of the settlement. There is no road leading anywhere outside of Ny-Ålesund, apart from the nearby airstrip, former mining areas and the station of a cable-car up Zeppelin Mountain. One can get to Ny-Ålesund only by small plane or boat. It wouldn’t be possible at all to place a village like this so far to the north, without the warm currents of the Gulfstream passing along the west coast of Svalbard, providing the necessary conditions only on this side of the archipelago. In the summer, the sun never sets; between November and the beginning of March it does not rise. From mid-December to mid-January the sun is so far below the horizon that there is no difference between noon and midnight – the period of polar night. Figure 1. Remote Sensing: a play on darkness in four acts, detail, C-print, Titanic Gallery, Turku, Finland, 2011. Popp A Home for Science, Social Studies of Science 46(6) The village came into existence because of coal, which was extracted from 1916 until 1962. In the 1970s, Ny-Ålesund became increasingly interesting for fieldwork in the natural sciences and developed into an International Scientific Research Center, which today has much of its focus on climate change. About twelve nations have their permanent stations there; others would use facilities provided by others to conduct specific research in limited periods. Five stations have personnel on site throughout the whole year. The organization and administration of the overall infrastructure is provided by Kings Bay, the Norwegian state company, which in the early days of the village had responsibility for coal mining. Figure 2(a), (b). Remote Sensing – a play on darkness in four acts, detail, C-prints, Titanic Gallery, Turku, Finland, 2011 The project started as a photographic search for scenic spaces – stage-like artificially lit outdoor areas where actors already had left or not yet entered – to emphasize the unreal feeling of existence on these latitudes (Figure 1). The polar night creates a natural Black Box theatre: objects, bodies and movements seem constructed and staged. Isolated from a larger context, they invite questioning – about their purpose, about their being and acting. In the development of the project, focus shifted from the empty space to actions carried out in space, to the engagement of bodies with their physical surroundings (Figure 2(a), (b), 3). The work responds to and works with the friction between the absurdity of the body’s geographical location and the built-in normality of a village with its domestic infrastructures and daily routines. I approached this continual negotiation from different angles, attending to the work, meals, leisure, infrastructure, power supply, communication systems and emergency exercises that define life in this extraordinary village. To conceptually and physically grasp the place, I extended my physical experience of Ny- Ålesund also to the network of sites that sustain it. In December of 2010 I got on board of the last cargo ship of the season from Tromsø on the Norwegian coast to Ny-Ålesund. Rather than follow the usual course of a flight, this slower movement allowed me to internalize some of Ny-Ålesund’s relations – its supply chains and data infrastructures – as a corporeal geography, an embodied experience of distance. Popp A Home for Science, Social Studies of Science 46(6) Figure 3. Remote Sensing – a play on darkness in four acts, detail, C-print, Titanic Gallery, Turku, Finland, 2011. Popp A Home for Science, Social Studies of Science 46(6) The gathering of material, conducted with lens-based equipment (photographic and video camera), sound recording devices, notes from dialogues, and the collecting of images and text from archives, led to a public installation in Longyearbyen, the main settlement at Svalbard in 2009 (Figure 4), and a show in a gallery space in Finland in 2011 (Figure 1, 2(a), (b), 3, 5). I regarded my apparatuses as belonging to the same category as the observing technology on site. I questioned their use in the same way as I do regarding Ny- Ålesund’s technology. What can actually be mediated? Figure 4. Future’s Past (Against the Anesthetic of Familiarity), detail, videostills from nine loops for a 72-hours public installation, with videoprojection and sound in former coal mining building, Longyearbyen, 2009. The core of investigation concerns performances of people, objects and matter in the framed space of a locality under specific geographical conditions. As the affective and sensuous dimensions of life in a scientific station resist recording, I carried out a number of physical tasks, including repetitive walks along random lines in the researched area, building of constructions and experimenting with (technical) equipment (Figure 6(a), (b)). These actions don’t need to end in any specific result. The tasks are the goal, with the experience that appears alongside them. These actions have the capacity to create ruptures in the local daily life and to open up for dialogue. Fellow residents would find themselves audience and collaborators alike. The work is driven by the attempt to touch upon issues of the human condition, but without overemphasizing any individual’s narratives. Through a selection of fragments from dialogues, discussions and archival material perspectives blur into each other to open up for a variety of possible meanings. I choose to look at technological devices in two ways: as simple tools extending the body to improve its abilities, or as objects placed between the body and an immediate experience, creating a distancing layer. The more complex the technology, the greater the distance. Maybe. One can see it the other way around: Technology enables the researcher to come much closer to the core of physical conditions than would otherwise be possible, by moving the point of perspective outside the body. But focus of attention thereby shifts from the object of investigation to the tool of observation as the physical reality actually related to – until one gets so used to applying the tool that it’s not seen any longer. As long as it works. In this way function and disfunctionality as such also can provide information on given physical conditions. Popp A Home for Science, Social Studies of Science 46(6) Figure 5. Remote Sensing – a play on darkness in four acts, overview first act, videoloops and sound, Titanic Gallery, Turku, Finland, 2011. Figure 6(a), (b). Wrong Time Wrong Place, on-site installation, videoloops and sound, Ny-Ålesund 2009. Popp A Home for Science, Social Studies of Science 46(6) In contrast to the extreme extension of technology in Ny-Ålesund, the pure bodily experience is an important one, even in scientific research: at the local station of the Norwegian Polar Institute, analog weather observations, called synoptic observation, are performed in addition to the automated monitoring system. This is done three times a day, exactly at the same time (UTC) as on any other station in the world, where these observations are carried out. Observation becomes important where the object of observation can’t be measured: the formations of clouds, their shape, amount, height and accumulation speed, the specific visual quality of fog or precipitation are all recorded (written down) and sent as a codified system to centers collecting meteorological data. The task seems impossible – or at least difficult – in darkness. Conversations on this issue pointed to the importance of heightened awareness of the whole body for surrounding conditions at any time of the day, to develop the ability to make statements about specific conditions at the moment of observation – even without sight. Long term physical engagement with surroundings, based on a structure of everyday routines, and seen as a two-way interaction between body and space, seems obsolete against the backdrop of ever growing mobility of bodies, or the accessibility of places via transferred images or data.
Recommended publications
  • DTA Scoring Form
    Daytime Astronomy SHADOWS Score Form Date ____/____/____ Student _______________________________________ Rater _________________ Problem I. (Page 3) Accuracy of results Draw a dot on this map to show where you think Tower C is. Tower C is in Eastern US Tower C is in North Eastern US Tower C is somewhere in between Pennsylvania and Maine Modeling/reasoning/observation How did you figure out where Tower C is? Matched shadow lengths of towers A and B/ pointed flashlight to Equator Tried different locations for tower C/ inferred location of tower C Matched length of shadow C/considered Latitude (distance from Equator) Matched angle of shadow C/ considered Longitude (East-West direction) Problem II. (Page 4) Accuracy of results How does the shadow of Tower A look at 10 AM and 3 PM?... Which direction is the shadow moving? 10 AM shadow points to NNW 10 AM shadow is shorter than noon shadow 3 PM shadow points to NE 3 PM shadow is longer than noon shadow Clockwise motion of shadows Modeling/reasoning/observation How did you figure out what the shadow of Tower A looks like at 10 AM and 3 PM? Earth rotation/ "Sun motion" Sunlight coming from East projects a shadow oriented to West Sunlight coming from West projects a shadow oriented to East Sunlight coming from above us projects a shadow oriented to North Sun shadows are longer in the morning than at noon Morning Sun shadows become shorter and shorter until its noon The shortest Sun shadow is at noon Sun shadows are longer in the afternoon than at noon Afternoon Sun shadows become longer and longer until it gets dark (Over, please) - 1 - 6/95 Problem III.
    [Show full text]
  • Ny-Ålesund Research Station
    Ny-Ålesund Research Station Research Strategy Applicable from 2019 DEL XX / SEKSJONSTITTEL Preface Svalbard research is characterised by a high degree of interna- tional collaboration. In Ny-Ålesund more than 20 research About the Research Council of Norway institutes have long-term research and monitoring activities. The station is one of four research localities in Svalbard (Ny-Ålesund, Longyearbyen, Barentsburg and Hornsund). The Research Council of Norway is a national strategic and research community, trade and industry and the public Close cooperation between these communities is essential funding agency for research activities. The Council serves as administration. It is the task of the Research Council to identify for the further development of Ny-Ålesund. the key advisor on research policy issues to the Norwegian Norway’s research needs and recommend national priorities Photo: John-Arne Røttingen Government, the government ministries, and other central and to use different funding schemes to help to translate In 2016, the Norwegian Government announced (Meld.St.32 institutions and groups involved in research and development national research policy goals into action. The Research Council (2015-2016)) the development of a research strategy for the (R&D). The Research Council also works to increase financial provides a central meeting place for those who fund, carry out Ny-Ålesund research station. Guidelines and principles for investment in, and raise the quality of, Norwegian R&D and and utilise research and works actively to promote the research activity were established by the government in 2018 to promote innovation in a collaborative effort between the internationalisation of Norwegian research.
    [Show full text]
  • Limits of Acceptable Change Caused by Local Activities in Ny-Ålesund
    Limits of acceptable change caused by local activities in Ny-Ålesund Report from a pre-project, containing a proposal for a main project Gunnar Sander, Norwegian Polar Institute 1 Preface Ny-Ålesund has been established as a research town on the assumption that this is an ideal area to study an environment shaped only by natural forces. Consequently the need to keep the environ- mental impacts resulting from local human activities at a low level has been emphasized in many policy statements from the Norwegian government and the actors in Ny-Ålesund. Following up on such policy objectives and recommendations from earlier Environmental Impact Assessments (EIAs) prepared for Ny-Ålesund, Kings Bay initiated a project to operationalize the environmental limits of the operations. During the work, it was clear that it would not be possible to do this without better information about environmental conditions in Ny-Ålesund. New fieldwork would be required to collect data and conduct detailed assessment as to which degree observed changes can be attributed to local activities. The steering group therefore decided to prepare a pre- project, planning a main project that will allow for better definitions of environmental limits. It decided to focus on three areas that according to the EIAs are likely to be most negatively affected by station activities: air quality, vegetation and birds. This report consists of a general part containing an update on the EIAs from Ny-Ålesund with recom- mendations on the general environmental work, and a framework for a main project. Detailed project descriptions of sub-projects on air quality, vegetation and birds are found in annexes.
    [Show full text]
  • Svalbard (Norway)
    Svalbard (Norway) Cross border travel - People - Depending on your citizenship, you may need a visa to enter Svalbard. - The Norwegian authorities do not require a special visa for entering Svalbard, but you may need a permit for entering mainland Norway /the Schengen Area, if you travel via Norway/the Schengen Area on your way to or from Svalbard. - It´s important to ensure that you get a double-entry visa to Norway so you can return to the Schengen Area (mainland Norway) after your stay in Svalbard! - More information can be found on the Norwegian directorate of immigration´s website: https://www.udi.no/en/ - Find more information about entering Svalbard on the website of the Governor of Svalbard: https://www.sysselmannen.no/en/visas-and-immigration/ - Note that a fee needs to be paid for all visa applications. Covid-19 You can find general information and links to relevant COVID-19 related information here: https://www.sysselmannen.no/en/corona-and-svalbard/ Note that any mandatory quarantine must be taken in mainland Norway, not on Svalbard! Find more information and quarantine (hotels) here: https://www.regjeringen.no/en/topics/koronavirus-covid- 19/the-corona-situation-more-information-about-quarantine- hotels/id2784377/?fbclid=IwAR0CA4Rm7edxNhpaksTgxqrAHVXyJcsDBEZrtbaB- t51JTss5wBVz_NUzoQ You can find further information regarding the temporary travel restrictions here: https://nyalesundresearch.no/covid-info/ - Instrumentation (import/export) - In general, it is recommended to use a shipping/transport agency. - Note that due to limited air cargo capacity to and from Ny-Ålesund, cargo related to research activity should preferably be sent by cargo ship.
    [Show full text]
  • Final Report Venus Exploration Targets Workshop May 19–21
    Final Report Venus Exploration Targets Workshop May 19–21, 2014, Lunar and Planetary Institute, Houston, TX Conveners: Virgil (Buck) Sharpton, Larry Esposito, Christophe Sotin Breakout Group Leads Science from the Surface Larry Esposito, Univ. Colorado Science from the Atmosphere Kevin McGouldrick, Univ. Colorado Science from Orbit Lori Glaze, GSFC Science Organizing Committee: Ben Bussey, Martha Gilmore, Lori Glaze, Robert Herrick, Stephanie Johnston, Christopher Lee, Kevin McGouldrick Vision: The intent of this “living” document is to identify scientifically important Venus targets, as the knowledge base for this planet progresses, and to develop a target database (i.e., scientific significance, priority, description, coordinates, etc.) that could serve as reference for future missions to Venus. This document will be posted in the VEXAG website (http://www.lpi.usra.edu/vexag/), and it will be revised after the completion of each Venus Exploration Targets Workshop. The point of contact for this document is the current VEXAG Chair listed at ABOUT US on the VEXAG website. Venus Exploration Targets Workshop Report 1 Contents Overview ....................................................................................................................................................... 2 1. Science on the Surface .............................................................................................................................. 3 2. Science within the Atmosphere ...............................................................................................................
    [Show full text]
  • Exploring Solar Cycle Influences on Polar Plasma Convection
    Comparison of Terrestrial and Martian TEC at Dawn and Dusk during Solstices Angeline G. Burrell1 Beatriz Sanchez-Cano2, Mark Lester2, Russell Stoneback1, Olivier Witasse3, Marco Cartacci4 1Center for Space Sciences, University of Texas at Dallas 2Radio and Space Plasma Physics, University of Leicester 3European Space Agency, ESTEC – Scientific Support Office 4Istituto Nazionale di Astrofisica, Istituto di Astrofisica e Planetologia Spaziali 52nd ESLAB Symposium Outline • Motivation • Data and analysis – TEC sources – Data selection – Linear fitting • Results – Martian variations – Terrestrial variations – Similarities and differences • Conclusions Motivation • The Earth and Mars are arguably the most similar of the solar planets - They are both inner, rocky planets - They have similar axial tilts - They both have ionospheres that are formed primarily through EUV and X- ray radiation • Planetary differences can provide physical insights Total Electron Content (TEC) • The Global Positioning System • The Mars Advanced Radar for (GPS) measures TEC globally Subsurface and Ionosphere using a network of satellites and Sounding (MARSIS) measures ground receivers the TEC between the Martian • MIT Haystack provides calibrated surface and Mars Express TEC measurements • Mars Express has an inclination - Available from 1999 onward of 86.9˚ and a period of 7h, - Includes all open ground and allowing observations of all space-based sources locations and times - Specified with a 1˚ latitude by 1˚ • TEC is available for solar zenith longitude resolution with error estimates angles (SZA) greater than 75˚ Picardi and Sorge (2000), In: Proc. SPIE. Eighth International Rideout and Coster (2006) doi:10.1007/s10291-006-0029-5, 2006. Conference on Ground Penetrating Radar, vol. 4084, pp. 624–629.
    [Show full text]
  • The Ny-Ålesund Charter
    THE NY-ÅLESUND CHARTER April 2013 THE NY-ÅLESUND SCIENCE MANAGERS COMMITTEE CONTENTS Preface 3 Introduction 3 Ny-Ålesund Charter Charter Contents 4 1. Mission Statement for Ny-Ålesund 5 2. Visitors to Ny-Ålesund - approval process 6 3. Research project approval 6 4. Safety policy agreed by NySMAC 2003 7 5. Ny-Ålesund accident and incident plan 8 6. Weapon training 8 APPENDIX 1. NySMAC founding articles 9 2. Ny-Ålesund stations/infrastructures 11 3. NySMAC meetings and Ny-Ålesund seminars 12 4. Kings Bay AS 13 5. Svalbard Science Forum (SSF) 13 6. Ny-Ålesund environment impact assessment (EIA) 14 7. Waste management 16 8. Ny-Ålesund Science Plan 17 1. Overall vision for the plan period 18 2. Science focus 18 3. Educational focus 21 4. Coordination activities within KIRB 21 5. Implementation of the Science Plan 23 9. Ny-Ålesund Flagship Programmes 24 10. EU funding initiatives 24 11. SIOS – Svalbard Integrated Earth Observing System 25 12. Fishery protection in Kongsfjorden 26 13. Gold prospecting at Svansen 27 14. UNINETT Internet Infrastructure 27 2 PREFACE Charter: “A written contract between individuals” This charter document endeavors to record policies agreed by the Ny-Ålesund Science Managers Committee (NySMAC) since its creation in 1994. The document also includes milestones in the evolution of the International Research Community at Ny-Ålesund since its beginning in 1991. Nick Cox April 2013 INTRODUCTION The Kings Bay Kull Company mined coal at Ny-Ålesund from 1916 to 1962 with brief interludes when it was a supply station for the fishing industry and a period with no activity during the Second World War.
    [Show full text]
  • Morphology and Dynamics of the Venus Atmosphere at the Cloud Top Level As Observed by the Venus Monitoring Camera
    Morphology and dynamics of the Venus atmosphere at the cloud top level as observed by the Venus Monitoring Camera Von der Fakultät für Elektrotechnik, Informationstechnik, Physik der Technischen Universität Carolo-Wilhelmina zu Braunschweig zur Erlangung des Grades eines Doktors der Naturwissenschaften (Dr.rer.nat.) genehmigte Dissertation von Richard Moissl aus Grünstadt Bibliografische Information Der Deutschen Bibliothek Die Deutsche Bibliothek verzeichnet diese Publikation in der Deutschen Nationalbibliografie; detaillierte bibliografische Daten sind im Internet über http://dnb.ddb.de abrufbar. 1. Referentin oder Referent: Prof. Dr. Jürgen Blum 2. Referentin oder Referent: Dr. Horst-Uwe Keller eingereicht am: 24. April 2008 mündliche Prüfung (Disputation) am: 9. Juli 2008 ISBN 978-3-936586-86-2 Copernicus Publications, Katlenburg-Lindau Druck: Schaltungsdienst Lange, Berlin Printed in Germany Contents Summary 7 1 Introduction 9 1.1 Historical observations of Venus . .9 1.2 The atmosphere and climate of Venus . .9 1.2.1 Basic composition and structure of the Venus atmosphere . .9 1.2.2 The clouds of Venus . 11 1.2.3 Atmospheric dynamics at the cloud level . 12 1.3 Venus Express . 16 1.4 Goals and structure of the thesis . 19 2 The Venus Monitoring Camera experiment 21 2.1 Scientific objectives of the VMC in the context of this thesis . 21 2.1.1 UV Channel . 21 2.1.1.1 Morphology of the unknown UV absorber . 21 2.1.1.2 Atmospheric dynamics of the cloud tops . 21 2.1.2 The two IR channels . 22 2.1.2.1 Water vapor abundance and cloud opacity . 22 2.1.2.2 Surface and lower atmosphere .
    [Show full text]
  • Solar Wind Fluence to the Lunar Surface
    44th Lunar and Planetary Science Conference (2013) 2015.pdf SOLAR WIND FLUENCE TO THE LUNAR SURFACE. D. M. Hurley1,3, W. M. Farrell2,3, 1JHU Applied Phys- ics Laboratory ([email protected]), 2NASA Goddard Space Flight Center, 3NASA Lunar Science Institute. Monolayers delivered in one lunation Introduction: The unperturbed solar wind bom- 90 bards the dayside of the Moon with electrons, protons, 60 and heavier ions throughout most of a lunation. Ex- cept when the Moon is in the Earth’s magnetotail for a 30 few days each lunation, the solar wind (shocked solar 0 N. Latitude wind in the magnetosheath, and unshocked solar wind -30 beyond Earth’s bow shock) has access to the dayside -60 surface of the Moon. Investigations of how the solar -90 wind could contribute to the composition and optical 0 90 180 270 360 properties of the lunar surface have a long history (e.g. E. Longitude [1-7]. Yet, it is instructive to revisit this issue and ex- Figure 2. The solar wind proton fluence as a function of amine the solar wind interaction piece by piece. selenographic position is shown in terms of fractions of Delivered Flux: The upper limit on the solar wind an equivalent monolayer of OH. The solid lines neglect thermal effects while the dashed lines include thermal as a potential source of OH can be established by as- effects. suming all of the incident solar wind protons are re- tained in the lunar regolith. The quiescent solar wind is implanted 3He as a resource guide. Fig. 2 shows the variable, but has density, n, of ~5 p+cm-3 and velocity, calculated fluence for one lunation assuming a spheri- v, of ~350 km s-1.
    [Show full text]
  • The Observational Analemma
    On times and shadows: the observational analemma Alejandro Gangui IAFE/Conicet and Universidad de Buenos Aires, Argentina Cecilia Lastra Instituto de Investigaciones CEFIEC, Universidad de Buenos Aires, Argentina Fernando Karaseur Instituto de Investigaciones CEFIEC, Universidad de Buenos Aires, Argentina The observation that the shadows of objects change during the course of the day and also for a fixed time during a year led curious minds to realize that the Sun could be used as a timekeeper. However, the daily motion of the Sun has some subtleties, for example, with regards to the precise time at which it crosses the meridian near noon. When the Sun is on the meridian, a clock is used to ascertain this time and a vertical stick determines the angle the Sun is above the horizon. These two measurements lead to the construction of a diagram (called an analemma) as an extremely useful resource for the teaching of astronomy. In this paper we report on the construction of this diagram from roughly weekly observations during more than a year. PACS: 01.40.-d, 01.40.ek, 95.10.-a Introduction Since early times, astronomers and makers of sundials have had the concept of a "mean Sun". They imagined a fictitious Sun that would always cross the celestial meridian (which is the arc joining both celestial poles through the observer's zenith) at intervals of exactly 24 hours. This may seem odd to many of us today, as we are all acquainted with the fact that one day -namely, the time it takes the Sun to cross the meridian twice- is in fact 24 hours and there is no need to invent any new Sun.
    [Show full text]
  • Svalbard 2015–2016 Meld
    Norwegian Ministry of Justice and Public Security Published by: Norwegian Ministry of Justice and Public Security Public institutions may order additional copies from: Norwegian Government Security and Service Organisation E-mail: [email protected] Internet: www.publikasjoner.dep.no KET T Meld. St. 32 (2015–2016) Report to the Storting (white paper) Telephone: + 47 222 40 000 ER RY M K Ø K J E L R I I Photo: Longyearbyen, Tommy Dahl Markussen M 0 Print: 07 PrintMedia AS 7 9 7 P 3 R 0 I 1 08/2017 – Impression 1000 N 4 TM 0 EDIA – 2 Svalbard 2015–2016 Meld. St. 32 (2015–2016) Report to the Storting (white paper) 1 Svalbard Meld. St. 32 (2015–2016) Report to the Storting (white paper) Svalbard Translation from Norwegian. For information only. Table of Contents 1 Summary ........................................ 5 6Longyearbyen .............................. 39 1.1 A predictable Svalbard policy ........ 5 6.1 Introduction .................................... 39 1.2 Contents of each chapter ............... 6 6.2 Areas for further development ..... 40 1.3 Full overview of measures ............. 8 6.2.1 Tourism: Longyearbyen and surrounding areas .......................... 41 2Background .................................. 11 6.2.2 Relocation of public-sector jobs .... 43 2.1 Introduction .................................... 11 6.2.3 Port development ........................... 44 2.2 Main policy objectives for Svalbard 11 6.2.4 Svalbard Science Centre ............... 45 2.3 Svalbard in general ........................ 12 6.2.5 Land development in Longyearbyen ................................ 46 3 Framework under international 6.2.6 Energy supply ................................ 46 law .................................................... 17 6.2.7 Water supply .................................. 47 3.1 Norwegian sovereignty .................. 17 6.3 Provision of services .....................
    [Show full text]
  • Your Cruise Cruising Arctic Norway: Glaciers, Ice Floes, And
    Cruising Arctic Norway: Glaciers, Ice Floes, and Polar Bears – with Smithsonian Journeys From 6/15/2022 From Longyearbyen, Spitsbergen Ship: LE BOREAL to 6/22/2022 to Longyearbyen, Spitsbergen In alliance with Smithsonian Journeys. This cruise is part of a collection of PONANT voyages that are specially-tailored for English-speaking travelers who want to engage with the world. In addition to the usual elements of the PONANT experience, the listed price for these voyages includes transfers to and from the ship, talks and discussions aboard ship by world class experts, and a shore excursion or activity in each port of call that encourages guests to embrace the sights, sounds, tastes, and smells of the local environment and culture. PONANT invites you to experience something exceptional by discovering the Far North and the immense open spaces of the polar Arctic and its ice floes that extend to the North Pole. You will board the ship at Longyearbyen in Norway for an 8-day expedition Overnight in Paris + roundtrip flights cruise to the heart of Spitsbergen, the largest island in the Svalbard Paris/Longyearbyen/Paris + Overnight in Paris + transfers archipelago. During this expedition at sea aboard Le Boreal, in the company of our team of naturalists, you will discover the exceptional flora and fauna that lives in these extreme conditions, where temperatures reach -30°C in winter. First, you will set sail south. There, you will discover Hornsund, one of the island’s most beautiful fjords, boasting an impressive glacier front, as well as Bellsund, whose lush valleys are sure to win you over.
    [Show full text]