Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data

Research output: Contribution to journal › Journal article › Research › peer-review

Standard

Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data. / Lognonné, P.; Banerdt, W. B.; Pike, W. T.; Giardini, D.; Christensen, U.; Garcia, R. F.; Kawamura, T.; Kedar, S.; Knapmeyer-Endrun, B.; Margerin, L.; Nimmo, F.; Panning, M.; Tauzin, B.; Scholz, J. R.; Antonangeli, D.; Barkaoui, S.; Beucler, E.; Bissig, F.; Brinkman, N.; Calvet, M.; Ceylan, S.; Charalambous, C.; Davis, P.; van Driel, M.; Drilleau, M.; Fayon, L.; Joshi, R.; Kenda, B.; Khan, A.; Knapmeyer, M.; Lekic, V.; McClean, J.; Mimoun, D.; Murdoch, N.; Pan, L.; Perrin, C.; Pinot, B.; Pou, L.; Menina, S.; Rodriguez, S.; Schmelzbach, C.; Schmerr, N.; Sollberger, D.; Spiga, A.; Stähler, S.; Stott, A.; Stutzmann, E.; Jacob, A.; Johnson, C. L.; Russell, C. T.

In: Nature Geoscience, Vol. 13, No. 3, 01.03.2020, p. 213-220.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Lognonné, P, Banerdt, WB, Pike, WT, Giardini, D, Christensen, U, Garcia, RF, Kawamura, T, Kedar, S, Knapmeyer-Endrun, B, Margerin, L, Nimmo, F, Panning, M, Tauzin, B, Scholz, JR, Antonangeli, D, Barkaoui, S, Beucler, E, Bissig, F, Brinkman, N, Calvet, M, Ceylan, S, Charalambous, C, Davis, P, van Driel, M, Drilleau, M, Fayon, L, Joshi, R, Kenda, B, Khan, A, Knapmeyer, M, Lekic, V, McClean, J, Mimoun, D, Murdoch, N, Pan, L, Perrin, C, Pinot, B, Pou, L, Menina, S, Rodriguez, S, Schmelzbach, C, Schmerr, N, Sollberger, D, Spiga, A, Stähler, S, Stott, A, Stutzmann, E, Jacob, A, Johnson, CL & Russell, CT 2020, 'Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data', Nature Geoscience, vol. 13, no. 3, pp. 213-220. https://doi.org/10.1038/s41561-020-0536-y

APA

Lognonné, P., Banerdt, W. B., Pike, W. T., Giardini, D., Christensen, U., Garcia, R. F., Kawamura, T., Kedar, S., Knapmeyer-Endrun, B., Margerin, L., Nimmo, F., Panning, M., Tauzin, B., Scholz, J. R., Antonangeli, D., Barkaoui, S., Beucler, E., Bissig, F., Brinkman, N., ... Russell, C. T. (2020). Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data. Nature Geoscience, 13(3), 213-220. https://doi.org/10.1038/s41561-020-0536-y

Vancouver

Lognonné P, Banerdt WB, Pike WT, Giardini D, Christensen U, Garcia RF et al. Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data. Nature Geoscience. 2020 Mar 1;13(3):213-220. https://doi.org/10.1038/s41561-020-0536-y

Author

Lognonné, P. ; Banerdt, W. B. ; Pike, W. T. ; Giardini, D. ; Christensen, U. ; Garcia, R. F. ; Kawamura, T. ; Kedar, S. ; Knapmeyer-Endrun, B. ; Margerin, L. ; Nimmo, F. ; Panning, M. ; Tauzin, B. ; Scholz, J. R. ; Antonangeli, D. ; Barkaoui, S. ; Beucler, E. ; Bissig, F. ; Brinkman, N. ; Calvet, M. ; Ceylan, S. ; Charalambous, C. ; Davis, P. ; van Driel, M. ; Drilleau, M. ; Fayon, L. ; Joshi, R. ; Kenda, B. ; Khan, A. ; Knapmeyer, M. ; Lekic, V. ; McClean, J. ; Mimoun, D. ; Murdoch, N. ; Pan, L. ; Perrin, C. ; Pinot, B. ; Pou, L. ; Menina, S. ; Rodriguez, S. ; Schmelzbach, C. ; Schmerr, N. ; Sollberger, D. ; Spiga, A. ; Stähler, S. ; Stott, A. ; Stutzmann, E. ; Jacob, A. ; Johnson, C. L. ; Russell, C. T. / Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data. In: Nature Geoscience. 2020 ; Vol. 13, No. 3. pp. 213-220.

Bibtex

@article{0f97fb5269054a0698da86cad4855286,
title = "Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data",
abstract = "Mars{\textquoteright}s seismic activity and noise have been monitored since January 2019 by the seismometer of the InSight (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) lander. At night, Mars is extremely quiet; seismic noise is about 500 times lower than Earth{\textquoteright}s microseismic noise at periods between 4 s and 30 s. The recorded seismic noise increases during the day due to ground deformations induced by convective atmospheric vortices and ground-transferred wind-generated lander noise. Here we constrain properties of the crust beneath InSight, using signals from atmospheric vortices and from the hammering of InSight{\textquoteright}s Heat Flow and Physical Properties (HP3) instrument, as well as the three largest Marsquakes detected as of September 2019. From receiver function analysis, we infer that the uppermost 8–11 km of the crust is highly altered and/or fractured. We measure the crustal diffusivity and intrinsic attenuation using multiscattering analysis and find that seismic attenuation is about three times larger than on the Moon, which suggests that the crust contains small amounts of volatiles.",
author = "P. Lognonn{\'e} and Banerdt, {W. B.} and Pike, {W. T.} and D. Giardini and U. Christensen and Garcia, {R. F.} and T. Kawamura and S. Kedar and B. Knapmeyer-Endrun and L. Margerin and F. Nimmo and M. Panning and B. Tauzin and Scholz, {J. R.} and D. Antonangeli and S. Barkaoui and E. Beucler and F. Bissig and N. Brinkman and M. Calvet and S. Ceylan and C. Charalambous and P. Davis and {van Driel}, M. and M. Drilleau and L. Fayon and R. Joshi and B. Kenda and A. Khan and M. Knapmeyer and V. Lekic and J. McClean and D. Mimoun and N. Murdoch and L. Pan and C. Perrin and B. Pinot and L. Pou and S. Menina and S. Rodriguez and C. Schmelzbach and N. Schmerr and D. Sollberger and A. Spiga and S. St{\"a}hler and A. Stott and E. Stutzmann and A. Jacob and Johnson, {C. L.} and Russell, {C. T.}",
year = "2020",
month = mar,
day = "1",
doi = "10.1038/s41561-020-0536-y",
language = "English",
volume = "13",
pages = "213--220",
journal = "Nature Geoscience",
issn = "1752-0894",
publisher = "nature publishing group",
number = "3",

}

RIS

TY - JOUR

T1 - Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data

AU - Lognonné, P.

AU - Banerdt, W. B.

AU - Pike, W. T.

AU - Giardini, D.

AU - Christensen, U.

AU - Garcia, R. F.

AU - Kawamura, T.

AU - Kedar, S.

AU - Knapmeyer-Endrun, B.

AU - Margerin, L.

AU - Nimmo, F.

AU - Panning, M.

AU - Tauzin, B.

AU - Scholz, J. R.

AU - Antonangeli, D.

AU - Barkaoui, S.

AU - Beucler, E.

AU - Bissig, F.

AU - Brinkman, N.

AU - Calvet, M.

AU - Ceylan, S.

AU - Charalambous, C.

AU - Davis, P.

AU - van Driel, M.

AU - Drilleau, M.

AU - Fayon, L.

AU - Joshi, R.

AU - Kenda, B.

AU - Khan, A.

AU - Knapmeyer, M.

AU - Lekic, V.

AU - McClean, J.

AU - Mimoun, D.

AU - Murdoch, N.

AU - Pan, L.

AU - Perrin, C.

AU - Pinot, B.

AU - Pou, L.

AU - Menina, S.

AU - Rodriguez, S.

AU - Schmelzbach, C.

AU - Schmerr, N.

AU - Sollberger, D.

AU - Spiga, A.

AU - Stähler, S.

AU - Stott, A.

AU - Stutzmann, E.

AU - Jacob, A.

AU - Johnson, C. L.

AU - Russell, C. T.

PY - 2020/3/1

Y1 - 2020/3/1

N2 - Mars’s seismic activity and noise have been monitored since January 2019 by the seismometer of the InSight (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) lander. At night, Mars is extremely quiet; seismic noise is about 500 times lower than Earth’s microseismic noise at periods between 4 s and 30 s. The recorded seismic noise increases during the day due to ground deformations induced by convective atmospheric vortices and ground-transferred wind-generated lander noise. Here we constrain properties of the crust beneath InSight, using signals from atmospheric vortices and from the hammering of InSight’s Heat Flow and Physical Properties (HP3) instrument, as well as the three largest Marsquakes detected as of September 2019. From receiver function analysis, we infer that the uppermost 8–11 km of the crust is highly altered and/or fractured. We measure the crustal diffusivity and intrinsic attenuation using multiscattering analysis and find that seismic attenuation is about three times larger than on the Moon, which suggests that the crust contains small amounts of volatiles.

AB - Mars’s seismic activity and noise have been monitored since January 2019 by the seismometer of the InSight (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) lander. At night, Mars is extremely quiet; seismic noise is about 500 times lower than Earth’s microseismic noise at periods between 4 s and 30 s. The recorded seismic noise increases during the day due to ground deformations induced by convective atmospheric vortices and ground-transferred wind-generated lander noise. Here we constrain properties of the crust beneath InSight, using signals from atmospheric vortices and from the hammering of InSight’s Heat Flow and Physical Properties (HP3) instrument, as well as the three largest Marsquakes detected as of September 2019. From receiver function analysis, we infer that the uppermost 8–11 km of the crust is highly altered and/or fractured. We measure the crustal diffusivity and intrinsic attenuation using multiscattering analysis and find that seismic attenuation is about three times larger than on the Moon, which suggests that the crust contains small amounts of volatiles.

U2 - 10.1038/s41561-020-0536-y

DO - 10.1038/s41561-020-0536-y

M3 - Journal article

AN - SCOPUS:85079827100

VL - 13

SP - 213

EP - 220

JO - Nature Geoscience

JF - Nature Geoscience

SN - 1752-0894

IS - 3

ER -

ID: 251602512