International Polar Year 2007–2008 - WMO

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Fig. 3.1-1. Antarctica mosaic image covers the time between 8 December 2007 and 22 January 2008. Yellow square areas show fast glaciers and the location of retreating ice shelves in the Antarctic Peninsula. (Courtesy: JAXA) 362 IPY 20 07–20 08 have worked to develop IPY data ‘portfolios’ that, in total, aim to satisfy a significant number of scientific requirements. The primary objectives of STG meetings have been to review science requirements, to provide agency reports on progress in support of developing the IPY data legacy, and to identify and solicit new members. GIIPSY science requirements were presented at the first STG meeting. STG has met in full session six times. Along with representatives of the space agencies mentioned above, members of GIIPSY (K. Jezek and others), the IPY Joint Committee (T. Mohr and E. Sarukhanian), WCRP (G. Asrar, V. Ryabinin, B. Goodison) and the WMO Secretariat, which provided administrative support, also attended STG meetings. The first meeting was held in January 2007 at the WMO headquarters in Geneva. Since then, the STG has met at EUMETSAT in Darmstadt, Germany in November 2007, at the ESA/ESRIN located in Frascati, Italy in May 2008, WMO Headquarters in Geneva in February and in December 2009 and in Oslo in June 2010. The STG also convened a SAR Working Group chaired by Y. Crevier (Canadian Space Agency). The purpose of the SAR-WG was to address fulfillment, on a best effort basis, of GIIPSY science requirements uniquely related to SAR/InSAR. The SAR-WG first met in March 2008 at the Canadian Space Agency in Montreal. Subsequent meetings were held in October 2008 at the German Aerospace Center in Oberpfaffenhofen and in June 2009 at ESA in Frascati. A full description of GIIPSY science requirements, agency data portfolios and meeting summaries can be found on the GIIPSY web page: http://bprc.osu.edu/rsl/GIIPSY (Drinkwater et al., 2008). Based on GIIPSY recommendations, the STG adopted four primary data acquisition objectives for its contribution to IPY. The fifth objective was added at STG3. These are: • Pole-to-coast multi-frequency InSAR measurements of ice-sheet surface velocity. • Repeat fine-resolution SAR mapping of the entire Southern Ocean sea ice cover for sea ice motion. • One complete high resolution visible and thermal
infrared snapshot of circumpolar permafrost. • Pan-Arctic high and moderate resolution Vis/IR snapshots of freshwater (lake and river) freeze-up and break-up. • Atmospheric dynamics and composition. The STG has made substantial progress towards these acquisition objectives (IPY-STG, 2010). Fig. 3.1-1 shows a JAXA ALOS SAR mosaic image which covers the time between 8 December 2007 and 22 January 2008. Yellow square areas show the location of several fast glaciers and also the location of important ice shelf retreat in the Antarctic Peninsula. Fig. 3.1-2 shows the first measurements of surface velocity along a 250 km long tributary draining into Recovery Glacier, Coates Land, Antarctica (Floricioiu and Jezek, 2009). The tributary was discovered during the Radarsat-1 Antarctic Mapping mission. TerraSAR-X was used to acquire interferometric data along the length of the glacier resulting in the first velocity map of this unusual feature. ASI, CSA, DLR, ESA and JAXA have worked together to acquire the first pole to coast InSAR data sets for measuring surface velocity on both ice sheets. Surface velocity from these campaigns will be used to study the ice flux from the ice sheets into the oceans and to better understand controls on the motion of ice streams and the break-up of ice shelves. Ice shelf studies included an intense, routinemonitoring campaign following the Wilkins Ice Shelf break up, which demonstrated the importance of SAR for satellite daily monitoring of the polar regions (Fig. 3.1-3). COSMO-SkyMed, the Italian X-band SAR constellation, contributed to observations of the Wilkins ice shelf by monitoring the disintegration events and ice movement over large and medium areas (Battazza et. al, 2009a). COSMO-SkyMed data were also used to measure the glacier velocity field of Patagonian glaciers using spotlight high resolution images with time intervals of 8 and 16 days (Fig. 3.1-4), (Battazza et al., 2009b). ESA and CSA have coordinated SAR campaigns to fill gaps in Arctic and Antarctic sea ice cover where either station masks or on-board recorder time have usually precluded routine coverage. Fig. 3.1-2. 2008-09 TerraSAR-X mosaic (left inset) and 1997 RAMP mosaic (right inset) of Recovery Glacier tributary (Antarctica) The main trunk of Recovery Glacier is located in the upper part of the RAMP and TerraSAR-X mosaics. Scenes are centered on 82.5°S 19°W. Central figure shows surface velocity along the entire 250 km length of the tributary measured using TerraSAR-X data. (Image: DLR) 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 363
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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
Page 338 and 339: Table 2.10-1. List of active projec
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Page 350 and 351: Fig. 2.10-7. Participants of the
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Page 362 and 363: Fig. 2.11-1. The circumpolar Arctic
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Page 390 and 391: Fig. 3.1-3. Evolution of the Wilkin
Page 392 and 393: Fig. 3.1-5. Threedimensional mappin
Page 394 and 395: Fig. 3.1-8. Time series of monthly
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Page 398 and 399: Fig. 3.2-1. Potential temperature/
Page 400 and 401: Fig. 3.2-3. A Distributed Biologica
Page 402 and 403: Fig. 3.2-4. Fresh water content (FW
Page 404 and 405: Fig. 3.2-6. Composite changes in th
Page 406 and 407: Fig. 3.2-7. Mooring components (lef
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Page 416 and 417: Fig. 3.3-5. Map showing the locatio
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Page 424 and 425: Fig. 3.5-1. Antarctic stations at t
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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Fig. 3.7-1. Examples of the cryosph
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414 IPY 20 07-20 08 Global Cryosphe
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416 IPY 20 07-20 08 and build on ex
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Fig. 3.8-1. SAON website - www. arc
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420 IPY 20 07-20 08 be necessary to
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422 IPY 20 07-20 08 on data sharing
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424 IPY 20 07-20 08 Fig. 3.9-1. CBM
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Fig. 3.9-3. Screenshots of the CBMP
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Fig. 3.9-5. (left) Data Coverage by
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Table 3.9-2. Current status, trends
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Fig. 3.9-9. The components of a com
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434 IPY 20 07-20 08 CAFF CBMP Repor
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436 IPY 20 07-20 08 polar communiti
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438 IPY 20 07-20 08 Fig. 3.10-3. Mo
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Fig. 3.10-5. Combining data on trad
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Fig. 3.10-6. NOMAD Expedition camp
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444 IPY 20 07-20 08 and visual form
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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
Page 652 and 653:
626 IPY 20 07-20 08 emissions of me
Page 654 and 655:
628 IPY 20 07-20 08 Epilogue Lead A
Page 656 and 657:
Table E-1: What Does It Take to Com
Page 658 and 659:
632 IPY 20 07-20 08 both ICSU and W
Page 660 and 661:
634 IPY 20 07-20 08
Page 662 and 663:
636 IPY 20 07-20 08 Robin Bell is a
Page 664 and 665:
638 IPY 20 07-20 08 Tillmann Mohr i
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640 IPY 20 07-20 08 Volker Rachold
Page 668 and 669:
642 IPY 20 07-20 08 A PPENDIX 2 IPY
Page 670 and 671:
644 IPY 20 07-20 08 Activity ID Tit
Page 672 and 673:
Page 674 and 675:
Page 676 and 677:
650 IPY 20 07-20 08 A PPENDIX 3 Joi
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652 IPY 20 07-20 08 Third Meeting o
Page 680 and 681:
654 IPY 20 07-20 08 Fifth Meeting o
Page 682 and 683:
656 IPY 20 07-20 08 Seventh Meeting
Page 684 and 685:
658 IPY 20 07-20 08 Ninth Meeting o
Page 686 and 687:
660 IPY 20 07-20 08 A PPENDIX 5 Sub
Page 688 and 689:
662 A PPENDIX 6 IPY Project Charts,
Page 690 and 691:
Appendix 6 Fig.3. Version 3.4, Apri
Page 692 and 693:
Appendix 6 Fig.5. Version 6.4, May
Page 694 and 695:
668 A PPENDIX 7 List of the Nationa
Page 696 and 697:
670 IPY 20 07-20 08 Poland IPY Nati
Page 698 and 699:
672 IPY 20 07-20 08 A PPENDIX 9 IPY
Page 700 and 701:
674 IPY 20 07-20 08 2002 February.
Page 702 and 703:
676 IPY 20 07-20 08 January 22. Int
Page 704 and 705:
678 IPY 20 07-20 08 November 24. Ar
Page 706 and 707:
680 IPY 20 07-20 08 March 2. IPY Da
Page 708 and 709:
682 IPY 20 07-20 08 February 16. Sc
Page 710 and 711:
684 IPY 20 07-20 08 2008 January 20
Page 712 and 713:
686 IPY 20 07-20 08 February 26. Th
Page 714 and 715:
688 IPY 20 07-20 08 A PPENDIX 10 Se
Page 716 and 717:
690 IPY 20 07-20 08 A PPENDIX 11 Li
Page 718 and 719:
692 IPY 20 07-20 08 FWC Freshwater
Page 720 and 721:
694 IPY 20 07-20 08 OCH Oscillating
Page 724:
698 The International Polar Year (I
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International Polar Year 2007–2008 - WMO

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