Livrables
Exploitation Dissemination and EPO plan complete plan including all aspects of dissemination papers web site press releases knowledge management etc and EPO activities foreseen within ROADMAP
Report on the prepartion of the climatologiesReport on the prepartion of the climatologies Report on the building of the climatologies Provide atmospheric fields and climatology of basic atmospheric quantities based on model improvements made in Tasks 51 52 and 53
Production of Martian analoguesReport on the production of Martian analogues Size distribution and environmental parametersAnalogue synthesis procedure Description of the milling and centrifugation processes requested for each bulk sample and corresponding size rangeAnalogue characterization 1 Morphological and chemical characterization by combining FESEM and HRTEM microscope analysis with Atomic Force Microscope AFM with confocal Raman probe 2 Size distribution characterization MasterSizer 2000 particles sizer particles 05 micrometer and Dynamic Light Scattering for the smaller particle fractions
Sensitivity study of the aerosol microphysical codeReport on sensitivities in aerosol microphysical code implemented within the GEMMars GCMThere are many assumptions and estimations in the computation of cloud formation and their impact on the atmosphere such as physical and radiative properties of dust and water ice clouds We will explore the sensitivity of the routine to these various parameters with the help of inputs from lab and optical measurements WP2 The optimal number of particle size bins will be tested in preparation for the routine to be included in the global model in WP 5
Impacts of new microphysics on the simulation of temperatures, clouds, circulationReport on impacts of new microphysics on the simulation of temperatures clouds and circulation Simulations in different setups will be performed and the impact on the simulated dust clouds temperatures water vapour and minor species is analysed Different initializations of the dust distribution will be tested Optimal treatment of radiative feedbacks of water ice clouds will be searched for
Initial report on the dust and clouds retrievalReport on the dust and clouds retrievalDust and cloud information will be retrieved from SPICAMUV and NOMAD UVIS and IR channels instruments From solar occultation observations vertical profiles will be obtained while from nadir measurements integrated optical depths will be derived In case of solar occultations vertical profiles of extinction number density loading will be retrieved as well as information on the size of the grains Using the wide spectral interval sounded by NOMAD covering the UVvisible and the IR domains it will be possible to derive more information shape andor composition It will be possible to distinguish dust and ice clouds From nadir observations spatial and seasonal maps of dust and ice cloud OD will be produced from retrievals using the new scattering properties measured in Task 26 and the vertical distribution a priori obtained in Task 54
Sensitivity study of the radiative model into the retrieval codeReport on the implementation of the radiative model into the retrieval code and sensitivity studyASIMUT the radiative transfer code developed at BIRAIASB has been coupled to LIDORT to include the complete treatment of the scattering effects into the radiative transfer calculations The scattering module will be updated with the model developed in Task 33 Validation tests will be run to check the implementation and the improvement in simulating the role of clouds and dust This will be done on a subset of spectra recorded by SPICAMUV and NOMADUVIS both solar occultation and nadir selected to be representative of different dustclouds loading size and shape observed on Mars see Task 42Sensitivity studies will be performed by considering different sizes and shapes solar occultation or scattering properties nadir for the dust and cloud grains use of LIDORT and VLIDORT
Electrification and aerodynamical properties experimentReport on the electrification and aerodynamical properties experimentsIn laboratory experiments particles after interactions with wind and after impacts splash and suspension will be observed microscopically and will be subject to electrical fields Sedimentation will also be observed These observations on high spatial and temporal scale will reveal the morphology and basic parameters of the particles Especially total net charge and aerodynamic cross sections drag coefficients will be givenFurther input parameters considered in this context are atmospheric pressure and particle size
Radiative properties modelReport on the radiative properties model Initial state of the art and Optical properties will be available for different configurations of the Martian dust analogue ie different size and material fractions and aggregation states
Retrieval of trace gasesReport on the retrieval of trace gases incl datasetsFollowing the results of the sensitivity study the best options will be selected to analyse the full SPICAM and NOMAD data sets This might need further development and optimisation of the code such as implementing an automatic link between the best GCM scenario and the retrieval algorithm or considering fitting parameters associated to the size and shape of the dustclouds see Task 44 to improve the fitting of the trace gases abundancesThe retrieval will focus on ozone and water vapour from spectra recorded by SPICAMUV and NOMAD Ozone will be retrieved by SPICAMUV and the UVIS channel of NOMAD whereas H2O abundances will be deduced from the IR channels of NOMAD Solarstellar occultations and nadir observations will be considered and will provide vertical profiles and integrated columns respectively
New climatologiesProvide final atmospheric fields and climatology of basic atmospheric quantities
Initial report on the dust resuspension experimentReport on the dust resuspension experimentLaboratory experiments of Wind induced resuspension of Mars analogues under Martian atmospheric conditions providing 1 threshold friction velocity shear stress Uth also as a function of deposition depth and structure 2 dust emissivity as a function of U and size distribution
Modifications to dust lifting and settling schemes, quantify the impact on dust spatial distributionReport on the impact of updated radiative properties of dust in the GCM effects on temperature and general circulation patterns WP2 will provide new insights into dust lifting and settling mechanisms such as impact of electrical fields on saltation and deviation of dust sedimentation velocities from the standard formula These mechanisms will be implemented in the GCM and their impacts will be analysed
Definition of Martian analoguesReport on the definition of Martian analogues Definition and production strategy of set of grain sizes geometric and aerodynamical and morphologyThe Martian dust analogues produced by CSIC will be aerosolized within the AU Martian environmental simulator Using Laser Doppler Velocimetry and other specialized laser based sensors measurements will be made of 1 settling velocities and suspension time 2 aerodynamic size distribution and aerodynamic drag coefficients 3 opacity related to dust concentration
Initial report on dust lifting and aggregation modelsInitial report on dust lifting and aggregation modelsDust lifting depends on a number of parameters like grain size shear stress atmospheric pressure and gravity A model for lifting of sand and dust size grains will be worked out starting from an initial state of the art model modified by results of the projects Dust and sand lifted or suspended after the splash of a wind blown particle encounter other particles before the impact again or are resuspended for long time Especially dust grows to larger aggregates by hitandstick collisions The growth process is unknownThis initial report includes the description of the state of the art equations for lifting thresholds and aggregation properties
Dust resuspension experimentReport on the dust resuspension experimentLaboratory experiments of Wind induced resuspension of Mars analogues under Martian atmospheric conditions providing 1 threshold friction velocity shear stress Uth also as a function of deposition depth and structure 2 dust emissivity as a function of U and size distribution
Impact of updated radiative properties of dust in the GCMReport on the impact of updated radiative properties of dust in the GCM effects on temperature and general circulation patterns The GCM requires particles shape through the aspect ratio crosssection refractive index single scattering albedo extinction efficiency and asymmetry factors for dust and water ice particles to compute its radiative effects in the atmosphere These values will be updated for dust using results obtained from Task 26 New simulations will be performed and an evaluation of the impacts will be reported In addition the impact of including polarization in the radiative transfer calculations will be investigated
Dust aggregation state of Martian analoguesReport on the dust aggregation state of Martian analoguesStudies 1 High speed imaging of samples during wind induced resuspension informs about the dust dispersion mechanism and the role of dust aggregates 2 the size distribution of resuspended Mars analogue dust from settling velocity measurements gives quantitative information about both aggregate dispersion and reformation 3 the electrification state of resuspended dust can be determined contributing to understanding the link between aggregation and electrification
Initial report on the dust aggregation state of Martian analoguesInitial report on the dust aggregation state of Martian analoguesStudies 1 High speed imaging of samples during wind induced resuspension informs about the dust dispersion mechanism and the role of dust aggregates 2 the size distribution of resuspended Mars analogue dust from settling velocity measurements gives quantitative information about both aggregate dispersion and reformation 3 the electrification state of resuspended dust can be determined contributing to understanding the link between aggregation and electrification
Initial report on the radiative properties modelInitial report on the radiative properties model This report includes the description of the initial state of the art and the equations and models based on the new laboratory measurements
Aggregation modelReport on aggregation modelDust and sand lifted or suspended after the splash of a wind blown particle encounter other particles before the impact again or are resuspended for long time Especially dust grows to larger aggregates by hitandstick collisions The growht process is unknownThe project will use the experimental results to work out a model that describes the time evolution of particle properties depending on the environment including aggregate size aggregate morphology porosity or fractal dimension and drag coefficients
Dust lifting modelReport on dust liftingDust lifting depends on a number of parameters like grain size shear stress atmospheric pressure and gravity A model for lifting of sand and dust size grains will worked out starting from an initial state of the art model modified by results of the projects This includes equations for lifting thresholds equations for resuspended mass flux and the initial particle properties of resuspended dust These findings will be deduced from experiments where grains are observed und different conditionsEspecially the lifting of dust will be studied in individual collisions with observations at high spatial and temporal resulution
Sensitivity study for the trace gases retrievalReport on the sensitivity study for the trace gases retrieval description of the best options to be consideredSensitivity studies will be performed by considering 1 different sizes and shapes solar occultation or scattering properties nadir for the dust and cloud grains use of LIDORT and VLIDORT2 different a priori knowledge on the vertical distribution of the dust 3 different a priori knowledge on the vertical temperature profiles A priori data will be provided by the GEMMars GCM Task 544 direct retrieval of temperature from the spectra for NOMAD solar occultation and SPICAMUV stellar occultation only Temperature retrieval will be performed using the hydrostatic law on CO2 abundances as was done for SOIR 119 or directly from the absorption features and their dependence on temperature new method which will require development and testing of the retrieval code Retrieved values will be compared to the a priori knowledge and independent data provided by other instrumentsmissions Following the results of the sensitivity study the best options will be selected to analyse the full SPICAM and NOMAD data sets
Dust and clouds retrievalReport on the dust and clouds retrieval including datasetsDust and cloud information will be retrieved from SPICAMUV and NOMAD UVIS and IR channels instruments From solar occultation observations vertical profiles will be obtained while from nadir measurements integrated optical depths will be derived In case of solar occultations vertical profiles of extinction number density loading will be retrieved as well as information on the size of the grains Using the wide spectral interval sounded by NOMAD covering the UVvisible and the IR domains it will be possible to derive more information shape andor composition It will be possible to distinguish dust and ice clouds From nadir observations spatial and seasonal maps of dust and ice cloud OD will be produced from retrievals using the new scattering properties measured in Task 26 and the vertical distribution a priori obtained in Task 54
Exploitation, Dissemination, and Communication activitiesReport on the Exploitation Dissemination and Communication activitiesImplement and coordinate the EPO activities in the Consortium Communications tasks distribution of press releases and announcements production of highquality material for media Production of highquality promotional and educational material about ROADMAP Online material articles images and illustrations visualization of scientific data etc and printed material brochures flyers posters etc to different targets educators general public etc Provide material for exhibitionsOrganize events for general public and students exhibition talks speed dating events handon workshops etc and participate in outreach events like Researchers night Science Day and World Space Week etcEvaluate the implementation of the Dissemination plan quantitative and qualitative evaluation media monitoring etc
Space data sets selectionReports on the selection of the different data setsThree different sets of data will be selected which correspond to 1 UVvisible spectra are highly sensitive to the radiative and microphysical properties of dust and clouds SPICAMUV NOMADUVIS Solarstellar occultation will be the best cases to test the sensitivity towards the size and shape impact because in such observations we can have direct access to the optical depth OD due to only dust and clouds While it is more complicated with nadir observations where the signal is a combination from surface reflection and scattering sometimes multiple by airborne aerosols that have similar spectral behaviour making them difficult to decorrelate Therefore nadir spectra are sensitive to optical depth SSA and phase function of aerosols These data will be further analysed to derive ozone Task 43 and dustclouds Task 44 The selection will be based on different criteria season latitudelongitude local solar time stormno storm conditions etc to build different subsets representative of different dustclouds conditions and characteristics 2 IR spectra of NOMAD are sensitive to water absorption which is very sensitive to temperature From this data set water vapor abundances will be retrieved Task 43 These spectra also allow the retrieval of CO2 In case of solar occultation temperature can be retrieved either from CO2 densities or directly from the spectra These quantities CO2 and temperature will help the comparison with model fields Task 54 The selection will be driven mostly by the spectral range sounded by the instrument which should contain features of H2O Another criterion which will be considered for both 1 and 2 data at least for NOMAD data is the simultaneity of the observations ie when both IR and UVIS channels are operating together This will allow us to derive a data set of ozone water dustclouds CO2 temperature obtained at the same time and same location probing the same portion of atmosphere 3 Data from other space missions will be also considered in this study They will first serve as validation for the new retrieval performed in Tasks 43 and 44 but also to increase the spacetime coverage needed to build representative climatologies Task 54 For nadir measurements recorded above Martian Rovers could be of particular interest as the aerosol optical depth could be constrained Spirit Opportunity and Curiosity Rovers perform direct measurements of the OD4 Data from groundbased observatories will be considered Members of BIRAIASB are involved in such observations through allocated time at ALMA SOFIA IRAM SUBARU for example Data obtained during previous and concurrent observation campaigns will be collected
Initial report on the database of experimental scattering matricesDatabase of experimental scattering matrices at 488nm 514nm and 640 nm spanning the scattering angle range from 3 to 177 degreesObtaining experimental scattering matrices for a complete set of well characterized Martian dust analogue samples By covering a broad range of sizes shapes and compositions we will be able to disentangle the effect of the physical properties of the particles in their scattering patternHere we will report on measurements performed at three different wavelengths 488 nm 514 nm and 627 nm spanning the scattering angle range from 3 to 177 degrees
ROADMAP Webpage and Open Access portal creationCreation of the website foreseeing the following aspectsCreation and maintenance of the ROADMAP webpage and Open Access portal Regular updates of the web portal by promoting conferences events high impact publications by adding new data generated or used within ROADMAPDesign and maintain the web site and its up to date contents for different audiences media educators general public etc and manage the social media presence of ROADMAP Disseminate scientific papers and general papers about the project results in relevant open access journals The peerreviewed publications will address the major science topics methods and tools including analysis of data obtained by European space missions to Mars atmospheric modelling Mars dust analogue laboratory and modellingDisseminate project results at major planetary science conferences as well as relevant laboratory remote sensing and computer conferences and workshopsCreate links to highlevel data products through PSA ESA and other public data archives like VESPA or CODULABCreate and preserve a reference archive of the Consortium publications reports deliveries and data by ensuring the followup preservation of the ROADMAP Open Access portal
Data Management Plan describing the different types of data collected and created by the project
Database of experimental scattering matrices at 488nm, 514nm, and 640 nm spanning the scattering angle range from 3 to 177 degreesObtaining experimental scattering matrices for a complete set of well characterized Martian dust analogue samples. By covering a broad range of sizes, shapes, and compositions, we will be able to disentangle the effect of the physical properties of the particles in their scattering pattern.Here we will report on measurements performed at three different wavelengths, 488 nm, 514 nm, and 627 nm spanning the scattering angle range from 3 to 177 degrees.
Publications
Auteurs:
M. R. Patel, G. Sellers, J. P. Mason, J. A. Holmes, M. A. J. Brown, S. R. Lewis, K. Rajendran, P. M. Streeter, C. Marriner, B. G. Hathi, D. J. Slade, M. R. Leese, M. J. Wolff, A. S. J. Khayat, M. D. Smith, S. Aoki, A. Piccialli, A. C. Vandaele, S. Robert, F. Daerden, I. R. Thomas, B. Ristic, Y. Willame, C. Depiesse, G. Bellucci, J.‐J. Lopez‐Moreno
Publié dans:
Journal of Geophysical Research: Planets, Numéro 126/11, 2021, Page(s) e2021JE006837, ISSN 2169-9097
Éditeur:
American Geophysical Union
DOI:
10.1029/2021je006837
Auteurs:
S. Aoki, K. Shiobara, N. Yoshida, L. Trompet, T. Yoshida, N. Terada, H. Nakagawa, G. Liuzzi, A. C. Vandaele, I. R. Thomas, G. L. Villanueva, M. A. Lopez-Valverde, A. Brines, M. R. Patel, S. Faggi, F. Daerden, J. T. Erwin, B. Ristic, G. Bellucci, J. J. Lopez-Moreno, H. Kurokawa and Y. Ueno
Publié dans:
The Planetary Science Journal, Numéro 4(5), 2023, Page(s) 97, ISSN 2632-3338
Éditeur:
American Astronomical Society
DOI:
10.3847/psj/acd32f
Auteurs:
Tim Becker, Jens Teiser, Teresa Jardiel, Marco Peiteado, Olga Munoz, Julia Martikainen, Juan Carlos Gomez Martin, Gerhard Wurm
Publié dans:
The Planetary Science Journal, Numéro 00358711, 2022, Page(s) 195, ISSN 0035-8711
Éditeur:
Blackwell Publishing Inc.
DOI:
10.3847/psj/ac8477
Auteurs:
Felix Jungmann, Maximilian Kruss, Jens Teiser, Gerhard Wurm
Publié dans:
Icarus, Numéro 373, 2022, Page(s) 114766, ISSN 0019-1035
Éditeur:
Academic Press
DOI:
10.1016/j.icarus.2021.114766
Auteurs:
Alain S. J. Khayat, Michael D. Smith, Michael Wolff, Frank Daerden, Lori Neary, Manish R. Patel, Arianna Piccialli, Ann C. Vandaele, Ian Thomas, Bojan Ristic, Jon Mason, Yannick Willame, Cedric Depiesse, Giancarlo Bellucci, José Juan López‐Moreno
Publié dans:
Journal of Geophysical Research: Planets, Numéro 126/11, 2021, Page(s) e2021JE006834, ISSN 2169-9097
Éditeur:
American Geophysical Union
DOI:
10.1029/2021je006834
Auteurs:
J. Martikainen, O. Muñoz, T. Jardiel, J. C. Gómez Martín, M. Peiteado, Y. Willame, A. Penttilä, K. Muinonen, G. Wurm, and T. Becker
Publié dans:
Astrophysical Journal Supplement Series, Numéro 268:47, 2023, Page(s) 1-13, ISSN 1538-4357
Éditeur:
American Astronomical Society
DOI:
10.3847/1538-4365/acf0be
Auteurs:
L. Trompet, A.C. Vandaele, I. Thomas, S. Aoki, F. Daerden, J. Erwin, Z. Flimon, A. Mahieux, L. Neary, S. Robert, G. Villanueva, G. Liuzzi, Lopez Valverde, A. Brines, G. Bellucci, J. J. Lopez-Moreno, M. R. Patel
Publié dans:
J. Geophys. Res. Planets, Numéro 128(3), 2023, ISSN 2169-9097
Éditeur:
Wiley-Blackwell Publishing Ltd.
DOI:
10.1029/2022je007279
Auteurs:
M. M. J. Crismani, G. L. Villanueva, G. Liuzzi, M. D. Smith, E. W. Knutsen, F. Daerden, L. Neary, M. J. Mumma, S. Aoki, L. Trompet, I. R. Thomas, B. Ristic, G. Bellucci, A. Piccialli, S. Robert, A. Mahieux, J.‐J. Lopez Moreno, G. Sindoni, M. Giuranna, M. R. Patel, A. C. Vandaele
Publié dans:
Journal of Geophysical Research: Planets, Numéro 126/11, 2021, Page(s) e2021JE006878, ISSN 2169-9097
Éditeur:
American Geophysical Union
DOI:
10.1029/2021je006878
Auteurs:
Miguel Angel López-Valverde, Bernd Funke, Adrian Brines, Aurèlien Stolzenbach, Ashimananda Modak, Brittany Hill, Francisco González-Galindo, Ian Thomas, Loic Trompet, Shohei Aoki, Gerónimo Villanueva, Giuliano Liuzzi, Justin Erwin, Udo Grabowski, Francois Forget, José Juan López-Moreno, Julio Rodriguez-Gómez, Bojan Ristic, Frank Daerden, Giancarlo Bellucci, Manish Patel, Ann-Carine Vandaele
Publié dans:
J. Geophys. Res. Planets, Numéro Volume128, Numéro2, 2023, ISSN 2169-9100
Éditeur:
Wiley-Blackwell Publishing Ltd.
DOI:
10.1029/2022je007278
Auteurs:
L. Trompet, A.C. Vandaele, I. Thomas, S. Aoki, F. Daerden, J. Erwin, Z. Flimon, A. Mahieux, L. Neary, S. Robert, G. Villanueva, G. Liuzzi, Lopez-Valverde, A. Brines, G. Bellucci, J. J. Lopez-Moreno, M. R. Patel
Publié dans:
J. Geophys. Res. Planets, Numéro 128(3), 2023, Page(s) JGR Planets, ISSN 2169-9097
Éditeur:
Wiley-Blackwell Publishing Ltd.
DOI:
10.1029/2022je007277
Auteurs:
T. Becker, J. Teiser, T. Jardiel, M. Peiteado, O. Munoz, J. Martikainen, J. C. Gomez Martin, J. Merrison, and G. Wurm
Publié dans:
Planetary Science Journal, Numéro 4:180, 2023, Page(s) 1-8, ISSN 2632-3338
Éditeur:
American Astronomical Society
DOI:
10.3847/psj/acf318
Auteurs:
Villanueva, G., G. Liuzzi, S. Aoki, S. W. Stone, A. Brines, I. R. Thomas, M. A. Lopez-Valverde, L. Trompet, J. Erwin, F. Daerden, B. Ristic, M. D. Smith, M. Mumma, S. Faggi, V. Kofman, S. Robert, L. Neary, M. Patel , G. Bellucci, J. J. Lopez-Moreno and A. C. Vandaele
Publié dans:
Geophys. Res. Lett., Numéro 00948276, 2022, Page(s) e2022GL098161, ISSN 0094-8276
Éditeur:
American Geophysical Union
DOI:
10.1029/2022gl098161
Auteurs:
Daerden, F., L. Neary, G. Villanueva, G. Liuzzi, S. Aoki, R. T. Clancy, J. A. Whiteway, B. J. Sandor, M. D. Smith, M. J. Wolff, A. Pankine, A. Khayat, R. Novak, B. Cantor, M. Crismani, M. J. Mumma, S. Viscardy, J. Erwin, C. Depiesse, A. Mahieux, A. Piccialli, S. Robert, L. Trompet, Y. Willame, E. Neefs, I. Thomas, B. Ristic and A. C. Vandaele
Publié dans:
J. Geophys. Research Planets, Numéro 127 (2), 2022, Page(s) e2021JE007079, ISSN 2169-9097
Éditeur:
American Geophysical Union
DOI:
10.1029/2021je007079
Auteurs:
A. Piccialli, A. C. Vandaele, Y. Willame, A. Määttänen, L. Trompet, J. T. Erwin, F. Daerden, L. Neary, S. Aoki, S. Viscardy, I. R. Thomas, C. Depiesse, B. Ristic, J. P. Mason, M. R. Patel, M. J. Wolff, A. S. J. Khayat, G. Bellucci, J.-J. Lopez-Moreno
Publié dans:
Earth and Space Science, Numéro 10(2), 2023, ISSN 2333-5084
Éditeur:
Wiley Periodicals LLC
DOI:
10.1029/2022ea002429
Auteurs:
Streeter, P., G. Sellers, M.J. Wolff, J.P. Mason, M.R. Patel, S. Lewis, J. Holmes, F. Daerden, I.R. Thomas, B. Ristic, Y. Willame, C. Depiesse; A.C. Vandaele, G. Bellucci, J.J. Lopez-Moreno
Publié dans:
J. Geophys. Research Planets, Numéro 127(5), 2021, Page(s) e2021JE007065, ISSN 2169-9097
Éditeur:
American Geophysical Union
DOI:
10.1029/2021je007065
Auteurs:
Giuliano Liuzzi, Geronimo L. Villanueva, Loïc Trompet, Matteo M. J. Crismani, Arianna Piccialli, Shohei Aoki, Miguel Angel Lopez‐Valverde, Aurélien Stolzenbach, Frank Daerden, Lori Neary, Michael D. Smith, Manish R. Patel, Stephen R. Lewis, R. Todd Clancy, Ian R. Thomas, Bojan Ristic, Giancarlo Bellucci, Jose‐Juan Lopez‐Moreno, Ann Carine Vandaele
Publié dans:
Geophysical Research Letters, Numéro 48/22, 2021, Page(s) e2021GL095895, ISSN 0094-8276
Éditeur:
American Geophysical Union
DOI:
10.1029/2021gl095895
Auteurs:
F. C. Onyeagusi, C. Meyer, J. Teiser, T. Becker, and G. Wurm
Publié dans:
Atmosphere, Numéro 14:1065, 2023, Page(s) 1-10, ISSN 2073-4433
Éditeur:
Rotoweb Cantelli
DOI:
10.3390/atmos14071065
Auteurs:
F. Daerden,L. Neary,M. J. Wolff,R. T. Clancy,F. Lefèvre,J. A. Whiteway,S. Viscardy,A. Piccialli,Y. Willame,C. Depiesse,S. Aoki,I. R. Thomas,B. Ristic,J. Erwin,J.-C. Gérard,B. J. Sandor,A. Khayat,M. D. Smith,J. P. Mason,M. R. Patel,G. L. Villanueva,G. Liuzzi,G. Bellucci,J.-J. Lopez-Moreno,A. C. Vandaele
Publié dans:
Geophys. Res. Letters, Numéro 00948276, 2022, Page(s) e2022GL098821, ISSN 0094-8276
Éditeur:
American Geophysical Union
DOI:
10.1029/2022gl098821
Auteurs:
T. Becker, T. Steinpilz, J. Teiser, G. Wurm
Publié dans:
Monthly Notices of the Royal Astronomical Society, Numéro 00358711, 2022, Page(s) 5814-5817, ISSN 0035-8711
Éditeur:
Blackwell Publishing Inc.
DOI:
10.1093/mnras/stac1320
Auteurs:
A. Brines, M. A. López-Valverde, A. Stolzenbach, A. Modak, B. Funke, F. G. Galindo, S. Aoki, G. L. Villanueva, G. Liuzzi, I. R. Thomas, J. T. Erwin, U. Grabowski, F. Forget, J. J. Lopez-Moreno, J. Rodriguez-Gomez, F. Daerden, L. Trompet, B. Ristic, M. R. Patel, G. Bellucci, A. C. Vandaele
Publié dans:
J. Geophys. Res. Planets (in press), e2022JE007273,, Numéro Volume128, Numéro11, 2023, ISSN 2169-9100
Éditeur:
Wiley-Blackwell Publishing Ltd.
DOI:
10.1029/2022je007273
Auteurs:
A. Waza, J. Kjer, M. Peiteado, T. Jardiel, J. Iversen, K. Rasmussen, J. Merrison
Publié dans:
Planetary and Space Science, Numéro 227, 2023, Page(s) 1-9, ISSN 1873-5088
Éditeur:
Elsevier Ltd
DOI:
10.1016/j.pss.2023.105638
Auteurs:
Aoki S., A.C. Vandaele, F. Daerden, G. Villanueva, G. Liuzzi, R.T. Clancy, M.A. Lopez-Valverde, A. Brines, I.R. Thomas, L. Trompet, J.T. Erwin, L. Neary, S. Robert, A. Piccialli, J. Holmes, M. Patel, N. Yoshida, J. Whiteway, M.D. Smith, B. Ristic, G. Bellucci, J.J. Lopez-Moreno, A. Fedorov
Publié dans:
J. Geophys. Research Planets, Numéro 00948276, 2022, Page(s) e2022JE007231, ISSN 0094-8276
Éditeur:
American Geophysical Union
DOI:
10.1029/2022je007231
Auteurs:
M. Kruss, T. Salzmann, E. Parteli, F. Jungmann, J. Teiser, L. Schönau, G. Wurm
Publié dans:
Planetary Science Journal, Numéro 2, 2021, Page(s) 238, ISSN 2632-3338
Éditeur:
AAS Publishing
DOI:
10.3847/psj/ac38a4
Auteurs:
Vandaele A.C.
Publié dans:
Europlanet Magazine, Numéro 1, 2021, Page(s) 24-25
Éditeur:
Europlanet
Auteurs:
Vandaele A.C.
Publié dans:
The Innovation Platform, Numéro 7, 2021, Page(s) 82-83, ISSN 2634-0208
Éditeur:
Innovation News Network
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