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Lu, Yin; Pope, Ed; Moernaut, Jasper; Bookman, Revital; Waldmann, Nicolas D; Agnon, Amotz; Marco, Shmuel; Strasser, Michael (2021): Features of sediment density flow deposits in the Dead Sea center (ICDP Core 5017-1) over the last 220 kyr [dataset bundled publication]. PANGAEA, https://doi.org/10.1594/PANGAEA.938454

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Abstract:
The 457 m-long core was drilled from the Dead Sea depocenter during 2010-2011. It covers the past 220 kyr and its age model is built on a combination of 14C and U-Th dating, and δ18O stratigraphy correlation. The recovered sequence comprises seven basic facies which can be classified into four groups, (I) evaporites and related facies: halite, gypsum, and aragonite-detritus laminae (including in situ deformed ones), (II) slump facies, (III) debrite facies and graded turbidite facies, and (IV) homogeneous mud.
The different deposits are identified through their grain size, magnetic susceptibility, and chemical features. The units of homogeneous mud are composed of clay-fine silts without graded bedding. They are showing only relatively small variations in grain size, magnetic susceptibility, Ti and Ca. In contrast, the lower parts of graded turbidites are made up of coarse silts-fine sands and exhibit upward-decreasing particle size, increasing magnetic susceptibility and Ti, and large variations in Ca from bottom to top. Low content of Ti and Ca, and small values in magnetic susceptibility characterize debrites that are composed of coarse sands and are predominantly ungraded.
Homogeneous muds are frequent and thick during interglacials, and less frequent and thinner during glacials. Graded turbidites are frequent but thin during interglacials, and less frequent but thicker during glacials. The fraction of homogeneous mud during interglacials is much higher than during glacials. In addition, the fraction of turbidites and debrites during glacials is much higher than during interglacials. Furthermore, during individual interglacials, the thickness fraction of homogeneous mud is one to ten times higher than turbidites and debrites. In contrast, during individual glacials, the fraction of turbidites and debrites is one to two times as much as homogeneous mud. The dataset reveals (1) overflows are more prominent during interglacials, while underflows are more prominent during glacials; (2) orbital-scale climate changes affected the intensity-frequency of the flows via changing salinity and density of lake brine, lake-level, and source materials.
Keyword(s):
debrite; flash-floods; flood plume; flow processes; Homogeneous mud; Turbidite; turbidity currents
Supplement to:
Lu, Yin; Pope, Ed; Moernaut, Jasper; Bookman, Revital; Waldmann, Nicolas D; Agnon, Amotz; Marco, Shmuel; Strasser, Michael (2022): Stratigraphic record reveals contrasting roles of overflows and underflows over glacial cycles in a hypersaline lake (Dead Sea). Earth and Planetary Science Letters, 594, 117723, https://doi.org/10.1016/j.epsl.2022.117723
Project(s):
International Continental Scientific Drilling Program (ICDP)
Funding:
Austrian Science Fund (FWF), grant/award no. M 2817: In situ and secondary seismogenic sedimentary effects based Dead Sea paleoseismology: Developing a 220 kyr-long continuous earthquake record
Coverage:
Latitude: 31.508056 * Longitude: 35.471111
License:
Creative Commons Attribution 4.0 International (CC-BY-4.0)
Size:
57 datasets

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Datasets listed in this bundled publication

  1. Lu, Y; Pope, E; Moernaut, J et al. (2021): Frequency and average thickness of homogeneous mud, graded turbidite, debrite (with trigger unclear), and seismogenic turbidite through glacial cycles, (Table S2). https://doi.org/10.1594/PANGAEA.938411
  2. Lu, Y; Pope, E; Moernaut, J et al. (2021): Thickness distribution of seven basic facies (regardless of triggers) through glacial cycles in ICDP core 5017-1, (Fig. 4 and Table S2). https://doi.org/10.1594/PANGAEA.938408
  3. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Halite (Fig. 2a). https://doi.org/10.1594/PANGAEA.938250
  4. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Gypsum (Fig. 2b). https://doi.org/10.1594/PANGAEA.938271
  5. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Gypsum (Fig. 2c). https://doi.org/10.1594/PANGAEA.938272
  6. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Aragonite-detritus laminae (Fig. 2d). https://doi.org/10.1594/PANGAEA.938273
  7. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Aragonite-detritus laminae (Fig. 2e). https://doi.org/10.1594/PANGAEA.938297
  8. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Aragonite-detritus laminae (Fig. 2f). https://doi.org/10.1594/PANGAEA.938298
  9. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Aragonite-detritus laminae (in situ deformed) (Fig. 2g). https://doi.org/10.1594/PANGAEA.938299
  10. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Aragonite-detritus laminae (in situ deformed) (Fig. 2h). https://doi.org/10.1594/PANGAEA.938301
  11. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Seismogenic turbidite (Fig. 2i). https://doi.org/10.1594/PANGAEA.938371
  12. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Seismogenic turbidite (Fig. 2j). https://doi.org/10.1594/PANGAEA.938372
  13. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Seismogenic turbidite (Fig. 2k). https://doi.org/10.1594/PANGAEA.938373
  14. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Seismogenic turbidite (Fig. 2l). https://doi.org/10.1594/PANGAEA.938374
  15. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) of ICDP core 5017-1, Seismogenic slump (Fig. 2m). https://doi.org/10.1594/PANGAEA.938375
  16. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) of ICDP core 5017-1, Seismogenic debrite (Fig. 2n). https://doi.org/10.1594/PANGAEA.938376
  17. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Homogeneous mud (Fig. 2o). https://doi.org/10.1594/PANGAEA.938377
  18. Lu, Y; Pope, E; Moernaut, J et al. (2021): Mean grain size of ICDP core 5017-1, Homogeneous mud (Fig. 2o). https://doi.org/10.1594/PANGAEA.938378
  19. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Graded turbidite (Fig. 2p). https://doi.org/10.1594/PANGAEA.938385
  20. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Graded turbidite (Fig. 2q). https://doi.org/10.1594/PANGAEA.938386
  21. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Debrite (Fig. 2r). https://doi.org/10.1594/PANGAEA.938387
  22. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Debrite (Fig. 2s). https://doi.org/10.1594/PANGAEA.938388
  23. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Debrite (Fig. 2t). https://doi.org/10.1594/PANGAEA.938389
  24. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Debrite (Fig. 2u). https://doi.org/10.1594/PANGAEA.938390
  25. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Homogeneous mud & graded turbidite (Fig. 2v). https://doi.org/10.1594/PANGAEA.938391
  26. Lu, Y; Pope, E; Moernaut, J et al. (2021): Mean grain size of ICDP core 5017-1, Homogeneous mud & graded turbidite (Fig. 2v). https://doi.org/10.1594/PANGAEA.938392
  27. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ca,Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Homogeneous mud & graded turbidite (Fig. 2w). https://doi.org/10.1594/PANGAEA.938394
  28. Lu, Y; Pope, E; Moernaut, J et al. (2021): Mean grain size of ICDP core 5017-1, Homogeneous mud & graded turbidite (Fig. 2w). https://doi.org/10.1594/PANGAEA.938393
  29. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Homogeneous mud & graded turbidite (Fig. 2x). https://doi.org/10.1594/PANGAEA.938395
  30. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ti, MS (magnetic susceptibility) of ICDP core 5017-1, Graded turbidite (Fig. 2y). https://doi.org/10.1594/PANGAEA.938396
  31. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) of ICDP core 5017-1, Graded turbidite (Fig. 2z). https://doi.org/10.1594/PANGAEA.938397
  32. Lu, Y; Pope, E; Moernaut, J et al. (2021): Cl record of ICDP core 5017-1, (Fig. 3c). https://doi.org/10.1594/PANGAEA.938401
  33. Lu, Y; Pope, E; Moernaut, J et al. (2021): Homogeneous mud record of ICDP core 5017-1, (Fig. 3d-e). https://doi.org/10.1594/PANGAEA.938402
  34. Lu, Y; Pope, E; Moernaut, J et al. (2021): Graded turbidite record of ICDP core 5017-1, (Fig. 3f-g). https://doi.org/10.1594/PANGAEA.938403
  35. Lu, Y; Pope, E; Moernaut, J et al. (2021): Return time and thickness of homogeneous mud during interglacials of ICDP core 5017-1, (Fig. 3h). https://doi.org/10.1594/PANGAEA.938404
  36. Lu, Y; Pope, E; Moernaut, J et al. (2021): Return time and thickness of homogeneous mud during glacials of ICDP core 5017-1, (Fig. 3i). https://doi.org/10.1594/PANGAEA.938405
  37. Lu, Y; Pope, E; Moernaut, J et al. (2021): Return time and thickness of graded turbidite during interglacials of ICDP core 5017-1, (Fig. 3j). https://doi.org/10.1594/PANGAEA.938406
  38. Lu, Y; Pope, E; Moernaut, J et al. (2021): Return time and thickness of graded turbidite during glacials of ICDP core 5017-1, (Fig. 3k). https://doi.org/10.1594/PANGAEA.938407
  39. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) and Ti features of homogeneous mud in ICDP core 5017-1, (Fig. S1a). https://doi.org/10.1594/PANGAEA.938428
  40. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) and Ti features of homogeneous mud in ICDP core 5017-1, (Fig. S1b). https://doi.org/10.1594/PANGAEA.938431
  41. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) and Ti features of homogeneous mud in ICDP core 5017-1, (Fig. S1c). https://doi.org/10.1594/PANGAEA.938432
  42. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) of homogeneous mud in ICDP core 5017-1, (Fig. S1d). https://doi.org/10.1594/PANGAEA.938436
  43. Lu, Y; Pope, E; Moernaut, J et al. (2021): Ti features of homogeneous mud in ICDP core 5017-1, (Fig. S1d). https://doi.org/10.1594/PANGAEA.938437
  44. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) and Ti features of homogeneous mud in ICDP core 5017-1, (Fig. S1e). https://doi.org/10.1594/PANGAEA.938439
  45. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) and Ti features of homogeneous mud in ICDP core 5017-1, (Fig. S1f). https://doi.org/10.1594/PANGAEA.938440
  46. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) and Ti features of homogeneous mud in ICDP core 5017-1, (Fig. S1g). https://doi.org/10.1594/PANGAEA.938441
  47. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) and Ti features of homogeneous mud in ICDP core 5017-1, (Fig. S1h). https://doi.org/10.1594/PANGAEA.938442
  48. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) and Ti features of homogeneous mud in ICDP core 5017-1, (Fig. S1i). https://doi.org/10.1594/PANGAEA.938443
  49. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) of debrite in ICDP core 5017-1, (Fig. S2a). https://doi.org/10.1594/PANGAEA.938444
  50. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) and Ti features of debrite in ICDP core 5017-1, (Fig. S2c). https://doi.org/10.1594/PANGAEA.938445
  51. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) and Ti features of debrite in ICDP core 5017-1, (Fig. S2d). https://doi.org/10.1594/PANGAEA.938446
  52. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) and Ti features of debrite in ICDP core 5017-1, (Fig. S2e). https://doi.org/10.1594/PANGAEA.938447
  53. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) and Ti features of debrite in ICDP core 5017-1, (Fig. S2f). https://doi.org/10.1594/PANGAEA.938448
  54. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) and Ti features of debrite in ICDP core 5017-1, (Fig. S2g). https://doi.org/10.1594/PANGAEA.938449
  55. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) and Ti features of debrite in ICDP core 5017-1, (Fig. S2i). https://doi.org/10.1594/PANGAEA.938450
  56. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) and Ti features of debrite in ICDP core 5017-1, (Fig. S2j). https://doi.org/10.1594/PANGAEA.938451
  57. Lu, Y; Pope, E; Moernaut, J et al. (2021): MS (magnetic susceptibility) and Ti features of debrite in ICDP core 5017-1, (Fig. S2l). https://doi.org/10.1594/PANGAEA.938452