International Polar Year 2007–2008 - WMO

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396 IPY 20 07–20 08 including how to incorporate new projects from the NSF, the Russian Academy of science, other agencies (e.g. the National Aeronautics and Space Administration) and other countries. Details about the September 2009 trip to Tiksi, including a list of recently completed and planned installations can be found on the IASOA web site: http://iasoa.org/ iasoa/index.php?option=com_content&task=view &id=282&Itemid=175 (English) and http://iasoa.org/ iasoa/index.php?option=com_content&task=view &id=281&Itemid=174 (Russian) As a result of these intensive collaborations, in spring 2010 the following installations will be completed at the Tiksi Hydrometeorological Observatory: Spring 2010 Installations Measured Parameters Automated meteorological station (AMS) Air temperature, humidity, ground temperature, wind speed and direction, atmospheric pressure Climate Reference Network (CRN) station Temperature, precipitation solar radiation, surface skin temperature, surface winds, soil moisture and soil temperature at 5 depths Vector-M Upper Air Measurements Air temperature, relative humidity, instantaneous and average wind speed and direction, atmospheric pressure Baseline Surface Radiation Network (BSRN) station Direct, downward and upward solar radiation at various spectral intervals Global Atmosphere Watch (GAW) station Primary greenhouse gases (CO , CH , CO, H ); N O, SF ; water vapor concentrations 2 4 2 2 6 These installations mark the beginning of continued observatory upgrades and international collaborations. Summary The International Polar Year 2007–2008 was a fantastic opportunity to harness the immense interest in Arctic meteorology during this time of rapid change. The concepts behind IASOA were articulated in IPY Proposal (http://classic.ipy.org/development/eoi/proposal-details.php?id=196). The goals of the program, as outlined in the proposal, have been addressed during and after IPY with very limited funding. So far, the significant outcomes of the IASOA program are (Darby et al., 2009): • The IASOA web site (www.iasoa.org) • Strong collaborations among SEARCH scientists and engineers at several of the IASOA observatories • Instrument loans to observatories (e.g., NOAA/ESRL loaned a cloud radar to FMI) • The science sessions at AGU where scientists became more acutely aware of scientific investiga- tions and data sets at many of the observatories • The new instrumentation and infrastructure at the Tiksi Hydrometeorological Observatory. There is still much work to do for IASOA to reach its full potential and we look forward to serving the Arctic atmospheric community. References Darby, L.S. et al., 2009. International Arctic Systems for Observing the Atmosphere (IASOA): An Overview of International Polar Year Activities. AMS 10th Conference on Polar Meteorology and Oceanography, 18-21 May 2009, Madison, WI. Paper 10.8. Makshtas, A.P., 2007: Future hydrometeorological observatory in Tiksi. IPY News 2007/08, The International Polar Year 2007/08 in Russian Federation and around the world, Information Bulletin No 3, 8-10
3.5 Meteorological Observing in the Antarctic Lead Author: Jonathan Shanklin Reviewers: Colin Summerhayes and Eduard Sarukhanian The International Geophysical Year of 1957–58 (IGY) provided a big impetus towards setting up continuously operated stations in the Antarctic. Over forty were constructed during and following the IGY years, of which over a dozen are still operating today. This was the peak of manned observation in Antarctica and since then the number of staffed stations has declined (Fig. 3.5-1), though this is offset by an increasing number of automatic stations (Fig. 3.5-2). Some improvement to the observing network took place during International Polar Year of 2007–2008 (IPY), however, the main thrust of IPY initiative was a boost to polar research. Most manned stations are at coastal sites, primarily so that stores can easily be transported ashore. This means that in some ways their weather is not a true representation of the continent as a whole, as they are much milder due to the influence of the sea. Automatic stations are much more widely spread across the continent and give a broader picture of the meteorology. At most manned stations meteorological observations are made regularly throughout the “day” according to WMO standards, however, there is increasing reliance on automatic systems during the “night”. Surface temperature, humidity, sunshine, pressure, wind speed and direction are largely measured by automated instruments, but an observer is needed to estimate the visibility and the amount, type and height of clouds, although automatic instruments are being introduced. An observer also needs to keep note of the weather: rain, snow, fog, gale etc., as well as more unusual phenomena, such as diamond dust, halos, mirages and the aurora australis. Traditional weather observing on the polar plateau brings additional problems, with the combination of very low temperature and high altitude. At the Russian Vostok station special suits are worn for outdoor work PA R T T H R E E : I PY OBSERVING SYS T E M S , T H E I R L E G AC Y A N D DATA M A N AG E M E N T under these conditions. The observations are expressed in a numeric code and transmitted to meteorological centres, largely in the northern hemisphere, using the Global Telecommunication System (GTS), the meteorological equivalent of the Internet, where they join thousands of other observations from all over the world. The observations are processed by super-computers, used to forecast the weather and archived for climate studies. The transmission technique has steadily improved since IGY when HF radio was the only medium available to send data from Antarctica in real-time. Satellite relay became widely used in the 1980s, either using Data Collection Platforms (DCPs) transmitting to geostationary satellites at fixed times or random transmissions making use of the ARGOS service on polar orbiting satellites. During IPY, email transmission over permanent Internet links became more common along with short data burst (SDB) transmissions on the Iridium mobile phone system. Automatic stations (Fig. 3.5-3) generally measure a reduced range of parameters, usually pressure, temperature and wind, although some may measure humidity and have housekeeping data such as snow depth. Where there is significant snow accumulation, stations require annual maintenance visits while others may not be revisited after deployment. Most provide real-time access to their data, but others store the data locally for recovery during maintenance visits. Several new stations were set up during IPY. In particular, Russia installed automatic weather stations (AWS) at their formerly manned stations at Leningradskaya, Molodezhnaya and Russkaya, resuming a data series that was interrupted due to closure of these stations in the 1990s. In addition the private operator Adventure Network International, installed an AWS at their Thiel Mountains site and, in a co-operative arrangement with the British Antarctic Survey and U.K. Meteorological o b s e r v I n g s Y s t e m s a n d d a t a m a n a g e m e n t 397
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Understanding Earth’s Polar Chall
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Understanding Earth’s Polar Chall
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iv IPY 20 07-20 08 Table of Content
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vi IPY 20 07-20 08 Preface This sum
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viii IPY 20 07-20 08 Acknowledgemen
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x IPY 20 07-20 08 JC Members, IPO s
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xii IPY 20 07-20 08 Culp, Joseph 3.
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xiv IPY 20 07-20 08 Larsen, Joan Ny
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xvi IPY 20 07-20 08 Virtue, Patti 5
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xviii IPY 20 07-20 08 I N T R O D U
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xx IPY 20 07-20 08 As the polar reg
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xxii IPY 20 07-20 08 from many of t
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xxiv IPY 20 07-20 08
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2 IPY 20 07-20 08 PA R T O N E : PL
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4 IPY 20 07-20 08 References Andree
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Fig. 1.1-1 Carl Weyprecht (1838-188
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8 IPY 20 07-20 08 Box 2 Programme o
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10 IPY 20 07-20 08 Fig. 1.1-4 Globa
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Fig. 1.1-6 First meeting of the Com
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14 IPY 20 07-20 08 at the same Dani
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Fig. 1.1-8 U.S. Navy and constructi
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18 IPY 20 07-20 08 Cooperation.’
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20 IPY 20 07-20 08 decades (1950-19
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22 IPY 20 07-20 08 References Andre
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24 IPY 20 07-20 08 World Data Cente
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26 IPY 20 07-20 08 Placing the Firs
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28 IPY 20 07-20 08 23 Berkner’s l
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Fig. 1.2-1. Report on the forthcomi
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Fig. 1.2-3.First online publication
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34 IPY 20 07-20 08 Box 1 Neumayer D
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Fig. 1.2-7. Fragment from the minut
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38 Box 2 Proposal to Establish an I
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40 IPY 20 07-20 08 the IPY Planning
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42 Box 3 Extract from the Proceedin
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44 Box 4 IPY 20 07-20 08 Resolution
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46 IPY 20 07-20 08 1-12. Paris. IAG
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48 IPY 20 07-20 08 Notes 1 Andreev
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50 IPY 20 07-20 08 nations needed t
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52 IPY 20 07-20 08 ICSU and WMO Pro
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54 IPY 20 07-20 08 Thiede for SCAR,
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56 IPY 20 07-20 08 PG-3, First Disc
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Fig. 1.3-7 (right). Cover page of t
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60 IPY 20 07-20 08 established by 1
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62 IPY 20 07-20 08 Box 3 The develo
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Fig. 1.3-21 (left). Cover page of t
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Fig. 1.3-24. “A Vision for the In
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68 IPY 20 07-20 08 3 To the nine me
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70 IPY 20 07-20 08 multi-disciplina
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Fig. 1.4-2. SCAR Executive Committe
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74 IPY 20 07-20 08 to understand th
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Fig. 1.4-6. Front page of the AOSB
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78 IPY 20 07-20 08 International Po
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80 IPY 20 07-20 08 experts who atte
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82 IPY 20 07-20 08 and recognized I
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84 IPY 20 07-20 08 References IASC
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86 IPY 20 07-20 08 ATCM References
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88 IPY 20 07-20 08 best expertise f
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90 IPY 20 07-20 08 The EoI database
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92 IPY 20 07-20 08 support from Nor
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94 IPY 20 07-20 08 Box 3 Formal est
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96 IPY 20 07-20 08 Fig. 1.5-7. JC C
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98 IPY 20 07-20 08 Fig. 1.5-9. Fahr
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100 IPY 20 07-20 08 Box 7 Global la
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Fig.1.5-16. JC-8 Meeting in St. Pet
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104 IPY 20 07-20 08 Box 8 “The St
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106 IPY 20 07-20 08 A somewhat cont
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Fig.1.5-20 Jerónimo López-Martín
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Fig.1.5-21 IPY 2007-2008 was offici
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112 IPY 20 07-20 08 References Alli
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114 IPY 20 07-20 08 Portugal, Russi
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116 IPY 20 07-20 08 limited success
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118 IPY 20 07-20 08 Fig. 1.6-1. IPO
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120 Box 1 Meetings and conferences
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122 IPY 20 07-20 08 lished under IP
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Fig.1.6-3. IPO staff members Nicola
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126 IPY 20 07-20 08 References Kais
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128 IPY 20 07-20 08 not sufficient
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130 IPY 20 07-20 08 the IPY Observi
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132 IPY 20 07-20 08 and data manage
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134 IPY 20 07-20 08 PA R T T WO: IP
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136 IPY 20 07-20 08 of which have g
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Fig. 2.1-1. The new building of Tik
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140 IPY 20 07-20 08 instruments on
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Fig. 2.1-4. Time-patterns of the da
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Fig. 2.1-6. Ozone loss rates (parts
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146 IPY 20 07-20 08 fractional sea
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148 IPY 20 07-20 08 Fig. 2.1-9. Sea
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150 IPY 20 07-20 08 vations obtaine
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152 IPY 20 07-20 08 pre-dating the
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154 IPY 20 07-20 08 Sensing, 48(4):
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Table 2.2-1. Estimates of volume, h
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Fig. 2.2-3. Track of the NABOS Crui
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Fig. 2.2-4. Distribution of the oce
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162 IPY 20 07-20 08 quality of the
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164 IPY 20 07-20 08 much of the ozo
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166 IPY 20 07-20 08 concentration m
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168 IPY 20 07-20 08 Jackson et al.,
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170 IPY 20 07-20 08 developed or pr
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172 IPY 20 07-20 08 decrease in the
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Fig. 2.2-11. The acoustic data from
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176 IPY 20 07-20 08 providing plent
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178 IPY 20 07-20 08 Sampling of the
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Fig. 2.2-15 The position of the ice
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Fig. 2.2-17. Schematic of the scien
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184 IPY 20 07-20 08 48(1): 5-21. Di
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186 IPY 20 07-20 08 doi:10.1029/200
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Table 2.3-1. IPY projects in the So
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Fig. 2.3-1b. Hydrographic sections
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Fig. 2.3-2a. A total of 61,965 prof
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194 IPY 20 07-20 08 period. These p
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Fig.e 2.3-5. The Weddell gyre flow
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Fig. 2.3-7. Dissolved iron, salinit
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200 IPY 20 07-20 08 Fig. 2.3-8. Ver
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Fig. 2.3-9. CAML ship sampling duri
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204 IPY 20 07-20 08 the theory that
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Fig. 2.3-12. Dead krill on the beac
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Fig. 2.3-14. Laser altimeter swath
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210 IPY 20 07-20 08 tions and Infor
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212 IPY 20 07-20 08 solved iron in
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214 IPY 20 07-20 08 Antarctic ice s
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216 IPY 20 07-20 08 so-called Dansg
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218 IPY 20 07-20 08 other Greenland
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Fig. 2.4-3. The newly completed NEE
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222 IPY 20 07-20 08 In July-August
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Fig. 2.4-7. Bed topography map for
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Fig. 2.4-9. The grid over which dat
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228 IPY 20 07-20 08 Fig. 2.4-10. Ta
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Fig. 2.4-12. Airborne lidar and gro
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232 IPY 20 07-20 08 tic and Antarct
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234 IPY 20 07-20 08 Fig. 2.5-1. Sch
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236 IPY 20 07-20 08 our planet: the
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238 IPY 20 07-20 08 base Syowa via
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240 IPY 20 07-20 08 possible to add
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242 IPY 20 07-20 08 sary environmen
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Fig. 2.6-1. An artist’s cross-sec
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246 IPY 20 07-20 08 conditions. The
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Fig. 2.6-3. Russian scientific trav
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250 IPY 20 07-20 08 Fig. 2.6-5a. Co
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252 IPY 20 07-20 08 Emerging Subgla
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254 IPY 20 07-20 08 Masolov V.N., S
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Fig. 2.7-1. Permafrost extent in th
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258 IPY 20 07-20 08 contributed to
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Table 2.7-1. Inventory of Northern
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Table 2.7-2. Inventory of Antarctic
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264 IPY 20 07-20 08 Arctic Circum-P
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266 IPY 20 07-20 08 Northern Circum
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268 IPY 20 07-20 08 Permafrost in t
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270 IPY 20 07-20 08 Engineers Offic
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272 IPY 20 07-20 08 Valcárcel-Día
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Fig. 2.8-1. Antarctica’s Gamburts
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276 IPY 20 07-20 08 sampling at rel
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278 IPY 20 07-20 08 Fig. 2.8-5. PLA
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Fig. 2.8-6. POLENET autonomous, col
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Fig. 2.8-7. Continuouslyrecording G
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284 IPY 20 07-20 08 Seismic imaging
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286 IPY 20 07-20 08 expectations of
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288 IPY 20 07-20 08 Willis, 2009b.
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290 IPY 20 07-20 08 Meet. Suppl., A
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292 IPY 20 07-20 08 mantle beneath
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Table 2.9-1. Terrestrial Projects u
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296 IPY 20 07-20 08 future. For thi
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Fig. 2.9-2. A small moving drill wa
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300 IPY 20 07-20 08 2.9-4. Field si
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302 IPY 20 07-20 08 line zones have
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304 IPY 20 07-20 08 that the Arctic
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Fig. 2.9-7. Olga Bohuslavova, Ph.D.
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308 IPY 20 07-20 08 Acknowledgement
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310 IPY 20 07-20 08 arctic polar se
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Table 2.10-1. List of active projec
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314 IPY 20 07-20 08 Fig. 2.10-1. IP
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316 IPY 20 07-20 08 Box 1. The ‘f
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318 IPY 20 07-20 08 The field of th
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Table 2.10-2. Recommended ‘Small
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322 IPY 20 07-20 08 as a research a
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Fig. 2.10-7. Participants of the
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Fig. 2.10-9. 6th International Cong
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328 IPY 20 07-20 08 eral models. Th
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330 IPY 20 07-20 08 popularity duri
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332 IPY 20 07-20 08 in an Arctic Re
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334 IPY 20 07-20 08 Vairo, C., R. C
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Fig. 2.11-1. The circumpolar Arctic
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338 IPY 20 07-20 08 and the Danish
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340 IPY 20 07-20 08 Canadian traini
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342 IPY 20 07-20 08 Fig. 2.11-3. Th
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344 IPY 20 07-20 08 logical studies
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Page 388 and 389: Fig. 3.1-1. Antarctica mosaic image
Page 390 and 391: Fig. 3.1-3. Evolution of the Wilkin
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Page 394 and 395: Fig. 3.1-8. Time series of monthly
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Page 426 and 427: Fig. 3.5-3. Servicing the AWS at Bu
Page 428 and 429: Fig. 3.5-6. Sonde launch at Halley
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Page 450 and 451: 424 IPY 20 07-20 08 Fig. 3.9-1. CBM
Page 452 and 453: Fig. 3.9-3. Screenshots of the CBMP
Page 454 and 455: Fig. 3.9-5. (left) Data Coverage by
Page 456 and 457: Table 3.9-2. Current status, trends
Page 458 and 459: Fig. 3.9-9. The components of a com
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Fig. 3.10-10. Group of hunters camp
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Fig. 3.10-12. BSSN Research Assista
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Fig. 3.10-15. The Siku- Inuit-Hila
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Fig. 3.10-17. Meeting with officers
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454 IPY 20 07-20 08 monitoring prod
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456 IPY 20 07-20 08 Edited by I. Kr
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458 IPY 20 07-20 08 the World Ocean
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460 IPY 20 07-20 08 In the period l
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Table 3.11-1. National IPY Data Coo
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464 IPY 20 07-20 08 on basic data m
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466 IPY 20 07-20 08 handling commun
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468 IPY 20 07-20 08 funding agencie
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470 IPY 20 07-20 08 metadata. • M
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472 IPY 20 07-20 08 A major initial
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Table 3.11-2. Summary assessment of
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476 IPY 20 07-20 08 tion and Data.F
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478 IPY 20 07-20 08 PA R T F O U R
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480 IPY 20 07-20 08 Fig. 4.0-2. A w
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482 IPY 20 07-20 08 Historical back
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Fig. 4.1-1. Participants at the Str
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486 IPY 20 07-20 08 students throug
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488 IPY 20 07-20 08 Officers from m
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Fig. 4.1-2. Students in Portugal to
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492 IPY 20 07-20 08 Two internation
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494 IPY 20 07-20 08 the submissions
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Fig. 4.1-4. (left) Teachers partici
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498 IPY 20 07-20 08 conference, ‘
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500 Fig. 4.2-1. IPYPD Basic search
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Table 4.2-2. Distribution of public
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504 IPY 20 07-20 08 Google Groups t
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506 IPY 20 07-20 08 tative/liaison
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508 IPY 20 07-20 08 material had to
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510 IPY 20 07-20 08 References Arct
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512 IPY 20 07-20 08 Highlights from
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514 IPY 20 07-20 08 students throug
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Fig. 4.3-1. Participants of the mee
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Fig. 4.3-3. Early career scientists
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520 IPY 20 07-20 08 management. The
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Fig. 4.3-4. During IPY early career
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524 IPY 20 07-20 08 PA R T FI V E :
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526 IPY 20 07-20 08 ‘legacies’)
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528 IPY 20 07-20 08 sciences_for_ip
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530 IPY 20 07-20 08 of multidiscipl
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Fig. 5.1-2 In situ platforms, inclu
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534 IPY 20 07-20 08 tion documented
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536 IPY 20 07-20 08 warming over th
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538 IPY 20 07-20 08 the Russian Ant
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540 IPY 20 07-20 08 Background with
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542 IPY 20 07-20 08 achievements al
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544 IPY 20 07-20 08 with a Sunyaev-
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546 IPY 20 07-20 08 doing will cont
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548 IPY 20 07-20 08 IPY 2007-2008 (
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Fig.5.2-4. Proposed structure of th
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552 IPY 20 07-20 08 from April 2010
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554 IPY 20 07-20 08 References ACIA
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556 IPY 20 07-20 08 and China agree
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Fig.5.3-1. Routine CTD profiling du
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560 IPY 20 07-20 08 Svalbard, Norwa
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Fig.5.3-7. Comparison of geostrophi
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Fig.5.3-9. Participants of the IPY
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Fig.5.3-11. Japanese- Swedish Antar
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Fig.5.3-13. Memorial photo after th
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570 IPY 20 07-20 08 Fig.5.3-15. New
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Fig.5.3-17. Malaysian biologist Che
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Fig.5.3-19. Malaysian Arctic sampli
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576 IPY 20 07-20 08 their role via
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578 IPY 20 07-20 08 IPY 2007-2008 g
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Fig. 5.4-3. Community meeting organ
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582 IPY 20 07-20 08 Krupnik and Jol
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584 IPY 20 07-20 08 training may be
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586 IPY 20 07-20 08 of the universi
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Table 5.4-1: UArctic Members and St
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Fig. 5.4-11. Inaugural IAI meeting
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592 IPY 20 07-20 08 References Refe
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594 IPY 20 07-20 08 Council (AC) in
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596 IPY 20 07-20 08 established in
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598 IPY 20 07-20 08 cal cycle, perm
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600 IPY 20 07-20 08 Fig.5.5-3. In t
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602 IPY 20 07-20 08 New Role of the
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604 IPY 20 07-20 08 Fig. 5.5-6. Ice
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Fig.5.5-8. Paul Berkman, Chair of t
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608 IPY 20 07-20 08 speakers and pa
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610 IPY 20 07-20 08 Approach for Br
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612 IPY 20 07-20 08 promoted since
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614 IPY 20 07-20 08 states in polar
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Fig.5.6-2. The IPY Oslo Science Con
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618 Box 1 Oslo Science Conference P
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Fig. 5.6-6 The inclusion of early c
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622 IPY 20 07-20 08 2008 implementa
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624 IPY 20 07-20 08 capacity buildi
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626 IPY 20 07-20 08 emissions of me
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628 IPY 20 07-20 08 Epilogue Lead A
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Table E-1: What Does It Take to Com
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632 IPY 20 07-20 08 both ICSU and W
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634 IPY 20 07-20 08
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636 IPY 20 07-20 08 Robin Bell is a
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638 IPY 20 07-20 08 Tillmann Mohr i
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640 IPY 20 07-20 08 Volker Rachold
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642 IPY 20 07-20 08 A PPENDIX 2 IPY
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644 IPY 20 07-20 08 Activity ID Tit
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650 IPY 20 07-20 08 A PPENDIX 3 Joi
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652 IPY 20 07-20 08 Third Meeting o
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654 IPY 20 07-20 08 Fifth Meeting o
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656 IPY 20 07-20 08 Seventh Meeting
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658 IPY 20 07-20 08 Ninth Meeting o
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660 IPY 20 07-20 08 A PPENDIX 5 Sub
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662 A PPENDIX 6 IPY Project Charts,
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Appendix 6 Fig.3. Version 3.4, Apri
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Appendix 6 Fig.5. Version 6.4, May
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668 A PPENDIX 7 List of the Nationa
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670 IPY 20 07-20 08 Poland IPY Nati
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672 IPY 20 07-20 08 A PPENDIX 9 IPY
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674 IPY 20 07-20 08 2002 February.
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676 IPY 20 07-20 08 January 22. Int
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678 IPY 20 07-20 08 November 24. Ar
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680 IPY 20 07-20 08 March 2. IPY Da
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682 IPY 20 07-20 08 February 16. Sc
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684 IPY 20 07-20 08 2008 January 20
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686 IPY 20 07-20 08 February 26. Th
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688 IPY 20 07-20 08 A PPENDIX 10 Se
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690 IPY 20 07-20 08 A PPENDIX 11 Li
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692 IPY 20 07-20 08 FWC Freshwater
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694 IPY 20 07-20 08 OCH Oscillating
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698 The International Polar Year (I
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International Polar Year 2007–2008 - WMO

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