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Author |
Antoine, A. |
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Title |
Beneath the Antarctic sea-ice: Fine-scale analysis of Weddell seal (Leptonychotes weddellii, Lesson 1826) behaviour and predator prey interactions, using micro-sonar data and video recordings in Terre Adélie |
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Master 2 |
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Year |
2022 |
Publication ![sorted by Publication field, descending order (down)](img/sort_desc.gif) |
Sorbonne université |
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The sea-ice zone constitutes the breeding and foraging habitat of large populations of ice-based species, pointing at its far-reaching ecological importance. Given its sensitivity to global warming, there is an urgent need for determining how predators use their environment, to understand and predict their response to climate variability. New perspectives are offered by miniature animal-borne sensors: in 2019, 3 sonar tags were deployed on lactating female Weddell seals for 7 days in Terre Adélie to study 3D animal movement and fine-scale predator-prey interactions. Lactating females demonstrated central-place foraging strategy, with restricted foraging area (3-6 km) and mostly benthic dives (97% of dives, visualising the seafloor on echograms). Their foraging effort was constrained by the presence of their pup: females spent most of their time hauling out (77% of overall recordings). The time spent underwater was mostly dedicated to diving (>5m) (1.36 on 7days, 854 dives recorded), as opposed to shallower under ice activities (<5m) (0.3 days). A total of 331 prey capture attempts (PrCA) were recorded, using tri-axial acceleration data, of which 125 prey (4.7 ± 1.5 cm on average) were identified by the sonar on 78 dives (4.24 ± 3.99 PrCA/dive). All PCA occur on the seafloor, at shallower depth than usual Weddell seal records (88 ± 30 m). Lactation is therefore a period of physiological stress, with foraging limited by pup compared with other parts of the life cycle. Using functional principal component analysis and model-based clustering on high resolution dive data, we found that PrCAs occur mostly in 2 of the 5 dive shape clusters. Foraging dives are characterised by W or V shape and high sinuosity, at the scale of the dive (W shapes) or during the ascent phase (V shapes). During the approach phase, seals constantly scan the area by regularly moving their head left to right, suggesting opportunistic behaviour. Shallow phase behaviour was studied using video recordings (2h recorded per seal). Seals spent most of their time interacting with their pup (33%) and hauling-out (42%). Most mother-pup interactions were on sea-ice (71%), as opposed to underwater (29%). The results suggest lactating females’ energy budget changes, with lactation being a period of physiological stress. This period of feeding pressure might put them at higher risk regarding adaptation to environmental variability. |
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8747 |
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Zaroli C, Sambridge M, Lévêque J-J, Debayle E, Nolet G, |
![goto web page (via DOI) doi](img/doi.gif)
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Title |
An objective rationale for the choice of regularisation parameter with application to global multiple-frequency S-wave tomography
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Journal Article |
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2013 |
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Solid Earth |
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4 |
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2 |
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357-371 |
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133, 906 |
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Bachelor's thesis |
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1869-9529 |
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4359 |
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Hanna Silvennoinen, Elena Kozlovskaya, Eduard Kissling |
![find record details (via OpenURL) openurl](img/xref.gif)
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Title |
POLENET/LAPNET teleseismic P wave travel time tomography model of the upper mantle beneath northern Fennoscandia |
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2016 |
Publication ![sorted by Publication field, descending order (down)](img/sort_desc.gif) |
Solid Earth |
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7 |
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2 |
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425-439 |
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Abstract. The Polenet/lapnet (Polar Earth Observing Network) Broadband Seismic Network Was Deployed In Northern Fennoscandia (Finland, Sweden, Norway, And Russia) During The Third International Polar Year 2007–2009. The Array Consisted Of Roughly 60 Seismic Stations. In Our Study, We Estimate The 3-d Architecture Of The Upper Mantle Beneath The Northern Fennoscandian Shield Using High-resolution Teleseismic P Wave Tomography. The P Wave Tomography Method Can Complement Previous Studies In The Area By Efficiently Mapping Lateral Velocity Variations In The Mantle. For This Purpose 111 Clearly Recorded Teleseismic Events Were Selected And The Data From The Stations Hand-picked And Analysed. Our Study Reveals A Highly Heterogeneous Lithospheric Mantle Beneath The Northern Fennoscandian Shield Though Without Any Large High P Wave Velocity Area That May Indicate The Presence Of Thick Depleted Lithospheric “Keel”. The Most Significant Feature Seen In The Velocity Model Is A Large Elongated Negative Velocity Anomaly (Up To −3.5 %) In Depth Range 100–150 Km In The Central Part Of Our Study Area That Can Be Followed Down To A Depth Of 200 Km In Some Local Areas. This Low-velocity Area Separates Three High-velocity Regions Corresponding To The Cratonic Units Forming The Area. |
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1869-9510 |
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8165 |
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Olga Usoltseva, Elena Kozlovskaya |
![find record details (via OpenURL) openurl](img/xref.gif)
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Title |
Studying local earthquakes in the area Baltic-Bothnia Megashear using the data of the POLENET/LAPNET temporary array |
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2016 |
Publication ![sorted by Publication field, descending order (down)](img/sort_desc.gif) |
Solid Earth |
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7 |
Issue |
4 |
Pages |
1095-1108 |
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Earthquakes in areas within continental plates are still not completely understood, and progress on understanding intraplate seismicity is slow due to a short history of instrumental seismology and sparse regional seismic networks in seismically non-active areas. However, knowledge about position and depth of seismogenic structures in such areas is necessary in order to estimate seismic hazard for such critical facilities such as nuclear power plants and nuclear waste deposits. In the present paper we address the problem of seismicity in the intraplate area of northern Fennoscandia using the information on local events recorded by the POLENET/LAPNET (Polar Earth Observing Network) temporary seismic array during the International Polar Year 2007–2009. We relocate the seismic events using the program HYPOELLIPS (a computer program for determining local earthquake hypocentral parameters) and grid search method. We use the first arrivals of P waves of local events in order to calculate a 3-D tomographic P wave velocity model of the uppermost crust (down to 20 km) for a selected region inside the study area and show that the velocity heterogeneities in the upper crust correlate well with known tectonic units. We compare the position of the velocity heterogeneities with the seismogenic structures delineated by epicentres of relocated events and demonstrate that these structures generally do not correlate with the crustal units formed as a result of crustal evolution in the Archaean and Palaeoproterozoic. On the contrary, they correlate well with the postglacial faults located in the area of the Baltic-Bothnia Megashear (BBMS). Hypocentres of local events have depths down to 30 km. We also obtain the focal mechanism of a selected event with good data quality. The focal mechanism is of oblique type with strike-slip prevailing. Our results demonstrate that the Baltic-Bothnia Megashear is an important large-scale, reactivated tectonic structure that has to be taken into account when estimating seismic hazard in northern Fennoscandia. |
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1021 |
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1869-9510 |
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yes |
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8168 |
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J. Plomerová, L. Vecsey, V. Babuška, LAPNET Working Group |
![find record details (via OpenURL) openurl](img/xref.gif)
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Title |
Domains of Archean mantle lithosphere deciphered by seismic anisotropy – inferences from the LAPNET array in northern Fennoscandia |
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2011 |
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Solid Earth |
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2 |
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2 |
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303-313 |
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An international LAPNET array (2007–2009, http://www.oulu.fi/sgo-oty/lapnet) of the POLENET/LAPNET sub-project of the POLENET-IPY consortium, related to seismic and geodetic studies in the Arctic regions, consisted of about 60 broadband seismic stations located on the territory of northern Finland and adjacent parts of Sweden, Norway and Russia. We analyze relative P-wave travel-time deviations evaluated for a subset of 90 teleseismic events recorded by the LAPNET array and show examples of lateral variations of shear-wave splitting to demonstrate variability of fabrics of the Archean mantle lithosphere. The initial results clearly demonstrate the Archean mantle lithosphere consists of domains with consistent fabrics reflecting fossil anisotropic structures. 3-D self-consistent anisotropic models with inclined symmetry axes accommodate two independent sets of body-wave anisotropic observations. Individual domains are delimited by boundaries (sutures), where the anisotropic parameters change. The results obtained from the LAPNET array fill a gap in structural studies of the upper mantle beneath northern Fennoscandia. |
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1021 |
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1869-9510 |
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yes |
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8170 |
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Author |
Duprat J. |
![find record details (via OpenURL) openurl](img/xref.gif)
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Title |
On the Origin of Interplanetary organics at the surface of icy bodies |
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Conference - International - Communication |
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2017 |
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Solar System symposium,13-15 February 2017, Sapporo, Japan |
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1120 |
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Bachelor's thesis |
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7918 |
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Fily M., Leroux C., Lenoble J. & Sergent C. |
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Terrestrial snow studies from remote sensing in the solar spectrum and the thermal infrared. |
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1998 |
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Solar System Ices |
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421-441 |
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254 |
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410 |
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Démoulin, P.; Klein, K.-L.; Goff, C.; van Driel-Gesztelyi, L.; Culhane, J.; Mandrini, C.; Matthews, S.; Harra, L. |
![find record details (via OpenURL) openurl](img/xref.gif)
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Title |
Decametric N Burst: A Consequence of the Interaction of Two Coronal Mass Ejections |
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Journal Article |
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2007 |
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Solar physics |
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240 |
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2 |
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301-313 |
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Abstract Radio emissions of electron beams in the solar corona and interplanetary space are tracers of the underlying magnetic configuration and of its evolution. We analyse radio observations from the Culgoora and WIND/WAVES spectrographs, in combination with SOHO/LASCO and SOHO/MDI data, to understand the origin of a type N burst originating from NOAA AR 10540 on January 20, 2004, and its relationship with type II and type III emissions. All bursts are related to the flares and the CME analysed in a previous paper (Goff et al., 2007). A very unusual feature of this event was a decametric type N burst, where a type III-like burst, drifting towards low frequencies (negative drift), changes drift first to positive, then again to negative. At metre wavelengths, i.e., heliocentric distances ?1.5R ?, these bursts are ascribed to electron beams bouncing in a closed loop. Neither U nor N bursts are expected at decametric wavelengths because closed quasi-static loops are not thought to extend to distances ?1.5R ?. We take the opportunity of the good multi-instrument coverage of this event to analyse the origin of type N bursts in the high corona. Reconnection of the expanding ejecta with the magnetic structure of a previous CME, launched about 8 hours earlier, injects electrons in the same manner as with type III bursts but into open field lines having a local dip and apex. The latter shape was created by magnetic reconnection between the expanding CME and neighbouring (open) streamer field lines. This particular flux tube shape in the high corona, between 5R ? and 10R ?, explains the observed type N burst. Since the required magnetic configuration is only a transient phenomenon formed by reconnection, severe timing and topological constraints are present to form the observed decametric N burst. They are therefore expected to be rare features. |
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0038-0938 |
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IPEV @ Thierry.Lemaire @ |
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5581 |
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Masson, S., Klein, K.-L., Buetikofer, R., Flueckiger, E., Kurt, V., Yushkov B. & Krucker, S. |
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Acceleration of Relativistic Protons during the 20 January 2005 Flare and CME |
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2009 |
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SOLAR PHYSICS |
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257 |
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305 |
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The origin of relativistic solar protons during large flare/CME events has not been uniquely identified so far. We perform a detailed comparative analysis of the time profiles of relativistic protons detected by the worldwide network of neutron monitors at Earth with electromagnetic signatures of particle acceleration in the solar corona during the large particle event of 20 January 2005. The intensity – time profile of the relativistic protons derived from the neutron monitor data indicates two successive peaks. We show that microwave, hard X-ray, and ! -ray emissions display several episodes of particle acceleration within the impulsive flare phase. The first relativistic protons detected at Earth are accelerated together with relativistic electrons and with protons that produce pion-decay ! rays during the second episode. The second peak in the relativistic proton profile at Earth is accompanied by new signatures of particle acceleration in the corona within !1R" above the photosphere, revealed by hard X-ray and microwave emissions of low intensity and by the renewed radio emission of electron beams and of a coronal shock wave. We discuss the observations in terms of different scenarios of particle acceleration in the corona. |
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0038-0938 |
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5862 |
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Klein K-L, Trottet G, Samwel S, Malandraki O, |
![find record details (via OpenURL) openurl](img/xref.gif)
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Title |
Particle Acceleration and Propagation in Strong Flares without Major Solar Energetic Particle Events
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Journal Article |
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2011 |
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Solar Physics |
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269 |
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2 |
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309-333 |
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Physics and Astronomy, |
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Solar energetic particles (SEPs) detected in space are statistically associated with flares and coronal mass ejections (CMEs). But it is not clear how these processes actually contribute to the acceleration and transport of the particles. The present work addresses the question why flares accompanied by intense soft X-ray bursts may not produce SEPs detected by observations with the GOES spacecraft. We consider all X-class X-ray bursts between 1996 and 2006 from the western solar hemisphere. 21 out of 69 have no signature in GOES proton intensities above 10 MeV, despite being significant accelerators of electrons, as shown by their radio emission at cm wavelengths. The majority (11/20) has no type III radio bursts from electron beams escaping towards interplanetary space during the impulsive flare phase. Together with other radio properties, this indicates that the electrons accelerated during the impulsive flare phase remain confined in the low corona. This occurs in flares with and without a CME. Although GOES saw no protons above 10 MeV at geosynchronous orbit, energetic particles were detected in some (4/11) confined events at Lagrangian point L1 aboard ACE or SoHO. These events have, besides the confined microwave emission, dm-m wave type II and type IV bursts indicating an independent accelerator in the corona. Three of them are accompanied by CMEs. We conclude that the principal reason why major solar flares in the western hemisphere are not associated with SEPs is the confinement of particles accelerated in the impulsive phase. A coronal shock wave or the restructuring of the magnetically stressed corona, indicated by the type II and IV bursts, can explain the detection of SEPs when flare-accelerated particles do not reach open magnetic field lines. But the mere presence of these radio signatures, especially of a metric type II burst, is not a sufficient condition for a major SEP event. |
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227 |
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Bachelor's thesis |
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Springer Netherlands |
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0038-0938 |
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yes |
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3577 |
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