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Preface The expedition ARK XIX/3 with the German icebreaking RV ...

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pH, resistivity, oxygen and HS - at <strong>the</strong> sediment-water interface were envisaged using <strong>the</strong><br />

ROV to deploy <strong>the</strong> microprofiler at selected spots <strong>with</strong>in <strong>the</strong> above mentioned key<br />

locations.<br />

<strong>The</strong> first working day onboard was dominated by meetings and <strong>the</strong> assignment of<br />

laboratories. <strong>The</strong> working schedules of <strong>the</strong> next days were presented and instruments<br />

were tested. In <strong>the</strong> afternoon we reached our first station where <strong>the</strong> CTD was used to<br />

obtain information about water salinity and temperature at different depths. This data was<br />

necessary for <strong>the</strong> calibration of our sonar systems because among o<strong>the</strong>rs <strong>the</strong> sound<br />

velocity in water is determined by temperature and salinity. Afterwards we worked <strong>the</strong><br />

entire night on a small scale survey grid <strong>with</strong> <strong>the</strong> multi beam sonar system Hydrosweep,<br />

<strong>the</strong> sediment profiling sonar system Parasound and <strong>the</strong> 38 kHz echosounder. With <strong>the</strong><br />

latter we obtained data where spots of high methane release were located. This kind of<br />

information allowed us to collect afterwards samples in <strong>the</strong> water column at high spatial<br />

precision.<br />

On Saturday sediment sampling started by using <strong>the</strong> multicorer while in <strong>the</strong> evening two<br />

free falling lander systems were deployed and soon after <strong>the</strong> first ROV station started. At<br />

1250 m water depth a video survey was carried out during <strong>the</strong> night and <strong>the</strong> information<br />

obtained by doing this was used on Sunday to select some sites of special scientific<br />

interest where sediments covered by white bacterial mats were sampled using plastic<br />

tubes (push corers) operated by <strong>the</strong> manipulator arms of "Victor 6000".<br />

After <strong>the</strong> first succesful mission of "Victor 6000" at <strong>the</strong> Håkon Mosby Mud Volcano which<br />

was finished shortly before midnight on Sunday, we released <strong>the</strong> lander which was<br />

observed before by <strong>the</strong> ROV at more than 1200 m water depth. About thirty minutes later<br />

<strong>the</strong> lander was sighted about 100 m distance in front of "Polarstern". At this moment we<br />

had fog so <strong>the</strong> visibility was below 200 metres. However, <strong>the</strong> lander was equipped <strong>with</strong> a<br />

radio beacon and flash lights providing safety systems for localization under such<br />

conditions. After recovery of <strong>the</strong> lander we worked for about 12 hours on a heat flow<br />

measurement programme. <strong>The</strong>refore, a temperature lance of three metres length was<br />

used <strong>with</strong> one of <strong>the</strong> ship‘s winches. <strong>The</strong> lance becomes rammed into <strong>the</strong> sediment and<br />

measures <strong>the</strong> temperature at different depth strata. This procedure was repeated along a<br />

given waypoint list. At <strong>the</strong> end of this work package we knew that <strong>the</strong> <strong>the</strong> temperature at<br />

about 3 metres below <strong>the</strong> seabed might be much higher (close to 20 °C) than on deck of<br />

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