Articles | Volume 6, issue 1
https://doi.org/10.5194/gi-6-217-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/gi-6-217-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Wind reconstruction algorithm for Viking Lander 1
Tuomas Kynkäänniemi
CORRESPONDING AUTHOR
School of Science, Aalto University, Espoo, Finland
Osku Kemppinen
Earth Observation, Finnish Meteorological Institute, Helsinki, Finland
currently at: Department of Physics, Kansas State University, Manhattan, Kansas, USA
Ari-Matti Harri
Earth Observation, Finnish Meteorological Institute, Helsinki, Finland
Walter Schmidt
Earth Observation, Finnish Meteorological Institute, Helsinki, Finland
Related authors
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Maria Hieta, Iina Jaakonaho, Jouni Polkko, Andreas Lorek, Stephen Garland, Jean-Pierre de Vera, Maria Genzer, and Ari-Matti Harri
Geosci. Instrum. Method. Data Syst., 13, 337–351, https://doi.org/10.5194/gi-13-337-2024, https://doi.org/10.5194/gi-13-337-2024, 2024
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This paper describes new humidity measurements performed with the humidity instruments of the MSL, Mars 2020 and ExoMars missions. Special facilities are needed to create Martian conditions, and a measurement campaign was performed at the German Aerospace Center (DLR) to obtain datasets for REMS-H, MEDA HS and METEO-H instruments. The results from the campaign improved the humidity data we receive from MEDA HS/Perseverance and can further improve the existing Martian relative humidity data.
Joonas Leino, Ari-Matti Harri, Mark Paton, Jouni Polkko, Maria Hieta, and Hannu Savijärvi
Ann. Geophys., 42, 331–348, https://doi.org/10.5194/angeo-42-331-2024, https://doi.org/10.5194/angeo-42-331-2024, 2024
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The 1-D column model has been used extensively in studying the Martian atmosphere. In this study, we investigated the sensitivity of the column model to its initialization. The results of the model were compared with Curiosity rover measurements. The initial value of airborne dust and surface temperature had the greatest influence on the temperature prediction, while the initial atmospheric moisture content and the shape of the initial moisture profile modified the humidity prediction the most.
Walter Schmidt, Ari-Matti Harri, Timo Nousiainen, Harri Hohti, Lasse Johansson, Olli Ojanperä, Erkki Viitala, Jarkko Niemi, Jani Turpeinen, Erkka Saukko, Topi Rönkkö, and Pekka Lahti
Geosci. Instrum. Method. Data Syst., 9, 397–406, https://doi.org/10.5194/gi-9-397-2020, https://doi.org/10.5194/gi-9-397-2020, 2020
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Combining short-time forecast models, standardized interfaces to a wide range of environment detectors and a flexible user access interface, CITYZER provides decision-making authorities and private citizens with reliable information about the near-future development of critical environmental parameters like air quality and rain. The system can be easily adapted to different areas or different parameters. Alarms for critical situations can be set and used to support authority decisions.
Mark Paton, Ari-Matti Harri, Oliver Vierkens, and Hannu Savijärvi
Geosci. Instrum. Method. Data Syst., 8, 251–263, https://doi.org/10.5194/gi-8-251-2019, https://doi.org/10.5194/gi-8-251-2019, 2019
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A software application for streamlining investigations of the Martian atmosphere is described. The main components are a 1-D model of the Martian atmosphere, observations of the Martian atmosphere and a software wrapper. We verify our model using the application. The model and observations agree except over the winter solstice where mechanical heating of the atmosphere, from downward flowing air, is likely warming the atmosphere. We update our model to include this effect.
Ari-Matti Harri, Konstantin Pichkadze, Lev Zeleny, Luis Vazquez, Walter Schmidt, Sergey Alexashkin, Oleg Korablev, Hector Guerrero, Jyri Heilimo, Mikhail Uspensky, Valery Finchenko, Vyacheslav Linkin, Ignacio Arruego, Maria Genzer, Alexander Lipatov, Jouni Polkko, Mark Paton, Hannu Savijärvi, Harri Haukka, Tero Siili, Vladimir Khovanskov, Boris Ostesko, Andrey Poroshin, Marina Diaz-Michelena, Timo Siikonen, Matti Palin, Viktor Vorontsov, Alexander Polyakov, Francisco Valero, Osku Kemppinen, Jussi Leinonen, and Pilar Romero
Geosci. Instrum. Method. Data Syst., 6, 103–124, https://doi.org/10.5194/gi-6-103-2017, https://doi.org/10.5194/gi-6-103-2017, 2017
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Investigations of Mars – its atmosphere, surface and interior – require simultaneous, distributed in situ measurements. We have developed an innovative prototype of the Mars Network Lander (MNL), a small lander/penetrator with a 20 % payload mass fraction. MNL features an innovative Entry, Descent and Landing System to increase reliability and reduce the system mass. It is ideally suited for piggy-backing on spacecraft, for network missions and pathfinders for high-value landed missions.
Gi Young Jeong, Mi Yeon Park, Konrad Kandler, Timo Nousiainen, and Osku Kemppinen
Atmos. Chem. Phys., 16, 12397–12410, https://doi.org/10.5194/acp-16-12397-2016, https://doi.org/10.5194/acp-16-12397-2016, 2016
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Individual Saharan dust particles were investigated by transmission electron microscopy of cross-sectional slices. We classified internal structures, and determined the volume of iron oxide included in the dust particles, the iron content of clay minerals, and the shape of the dust particles. The mineralogical and structural properties of single dust particles provide a basis for the modeling of dust optical properties and the supply of iron as a micronutrient to remote ocean ecosystem.
J. Köhler, R. F. Wimmer-Schweingruber, J. Appel, B. Ehresmann, C. Zeitlin, D. M. Hassler, G. Reitz, D. E. Brinza, S. Böttcher, E. Böhm, S. Burmeister, J. Guo, A.-M. Harri, H. Kahanpää, J. Krauss, H. Lohf, C. Martin, D. Matthiä, A. Posner, and S. Rafkin
Ann. Geophys., 34, 133–141, https://doi.org/10.5194/angeo-34-133-2016, https://doi.org/10.5194/angeo-34-133-2016, 2016
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The Radiation Assessment Detector (RAD), on board the Mars Science Laboratory (MSL) rover Curiosity, measures the energetic charged and neutral particles and the radiation dose rate on the surface of Mars. In this work we compare predicted electron/positron spectra with the signal measured by RAD.
We find that the RAD electron/positron measurements agree well with the spectra predicted by Planetocosmics.
E. Nielsen and W. Schmidt
Hist. Geo Space. Sci., 5, 63–72, https://doi.org/10.5194/hgss-5-63-2014, https://doi.org/10.5194/hgss-5-63-2014, 2014
O. Kemppinen, J. E. Tillman, W. Schmidt, and A.-M. Harri
Geosci. Instrum. Method. Data Syst., 2, 61–69, https://doi.org/10.5194/gi-2-61-2013, https://doi.org/10.5194/gi-2-61-2013, 2013
M. D. Paton, A.-M. Harri, T. Mäkinen, and H. Savijärvi
Geosci. Instrum. Method. Data Syst., 2, 17–27, https://doi.org/10.5194/gi-2-17-2013, https://doi.org/10.5194/gi-2-17-2013, 2013
Related subject area
Space instruments
Laboratory measurements of the performances of the Sweeping Langmuir Probe instrument aboard the PICASSO CubeSat
Creating HiRISE digital elevation models for Mars using the open-source Ames Stereo Pipeline
Multiresolution wavelet analysis applied to GRACE range-rate residuals
Mars submillimeter sensor on microsatellite: sensor feasibility study
TARANIS XGRE and IDEE detection capability of terrestrial gamma-ray flashes and associated electron beams
One-chip analog circuits for a new type of plasma wave receiver on board space missions
The MetNet vehicle: a lander to deploy environmental stations for local and global investigations of Mars
Mass spectrometry of planetary exospheres at high relative velocity: direct comparison of open- and closed-source measurements
Influence of probe geometry on measurement results of non-ideal thermal conductivity sensors
Analysis of COSIMA spectra: Bayesian approach
High-frequency performance of electric field sensors aboard the RESONANCE satellite
COSIMA data analysis using multivariate techniques
CLUSTER–STAFF search coil magnetometer calibration – comparisons with FGM
In-flight calibration of double-probe electric field measurements on Cluster
In-flight calibration of the Cluster PEACE sensors
In-flight calibration of the Hot Ion Analyser on board Cluster
Background subtraction for the Cluster/CODIF plasma ion mass spectrometer
Interpretation of Cluster WBD frequency conversion mode data
Enhanced timing accuracy for Cluster data
In-flight calibration of the Cluster/CODIF sensor
Calibration of non-ideal thermal conductivity sensors
Investigating thermal properties of gas-filled planetary regoliths using a thermal probe
Sylvain Ranvier and Jean-Pierre Lebreton
Geosci. Instrum. Method. Data Syst., 12, 1–13, https://doi.org/10.5194/gi-12-1-2023, https://doi.org/10.5194/gi-12-1-2023, 2023
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The Sweeping Langmuir Probe on board the PICASSO CubeSat was designed to measure plasma parameters. Before launch, the instrument was tested in a plasma chamber. It is shown that the traditional method to interpret the data cannot be applied directly for this type of probe, and an adaptation is proposed. It is reported how, with a reduced number of data points, the plasma parameters can still be retrieved. Finally, the effects of the contamination of the probe surface are discussed.
Adam J. Hepburn, Tom Holt, Bryn Hubbard, and Felix Ng
Geosci. Instrum. Method. Data Syst., 8, 293–313, https://doi.org/10.5194/gi-8-293-2019, https://doi.org/10.5194/gi-8-293-2019, 2019
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Currently, there exist thousands of unprocessed stereo pairs of satellite imagery which can be used to create models of the surface of Mars. This paper sets out a new open–source and free to use pipeline for creating these models. Our pipeline produces models of comparable quality to the limited number released to date but remains free to use and easily implemented by researchers, who may not necessarily have prior experience of DEM creation.
Saniya Behzadpour, Torsten Mayer-Gürr, Jakob Flury, Beate Klinger, and Sujata Goswami
Geosci. Instrum. Method. Data Syst., 8, 197–207, https://doi.org/10.5194/gi-8-197-2019, https://doi.org/10.5194/gi-8-197-2019, 2019
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In this paper, we present an approach to represent underlying errors in measurements and physical models in the temporal gravity field determination using GRACE observations. This study provides an opportunity to improve the error model and the accuracy of the GRACE parameter estimation, as well as its successor GRACE Follow-On.
Richard Larsson, Yasuko Kasai, Takeshi Kuroda, Shigeru Sato, Takayoshi Yamada, Hiroyuki Maezawa, Yutaka Hasegawa, Toshiyuki Nishibori, Shinichi Nakasuka, and Paul Hartogh
Geosci. Instrum. Method. Data Syst., 7, 331–341, https://doi.org/10.5194/gi-7-331-2018, https://doi.org/10.5194/gi-7-331-2018, 2018
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We are planning a Mars mission. The mission will carry an instrument capable of measuring and mapping molecular oxygen and water in the Martian atmosphere, as well as the temperature, wind, and magnetic field. Water and oxygen are vital parts of the Martian atmospheric chemistry and must be better understood. Using computer simulation results, the paper gives a description of how the measurements will work, some problems we expect to encounter, and the sensitivity of the measurements.
David Sarria, Francois Lebrun, Pierre-Louis Blelly, Remi Chipaux, Philippe Laurent, Jean-Andre Sauvaud, Lubomir Prech, Pierre Devoto, Damien Pailot, Jean-Pierre Baronick, and Miles Lindsey-Clark
Geosci. Instrum. Method. Data Syst., 6, 239–256, https://doi.org/10.5194/gi-6-239-2017, https://doi.org/10.5194/gi-6-239-2017, 2017
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The TARANIS spacecraft will be launched at the end of 2018. It is one of the first dedicated to the study of terrestrial gamma-ray flashes (TGF) and associated electrons (TEB), produced by thunderstorms. We present two of the six instruments on board the TARANIS spacecraft: a gamma-ray and energetic electron detector (XGRE) and an electron detector (IDEE). We compare them to other instruments that have already detected TGF and TEB, and use them to estimate the detection rate of TARANIS.
Takahiro Zushi, Hirotsugu Kojima, and Hiroshi Yamakawa
Geosci. Instrum. Method. Data Syst., 6, 159–167, https://doi.org/10.5194/gi-6-159-2017, https://doi.org/10.5194/gi-6-159-2017, 2017
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Plasma waves are important observational targets for scientific missions investigating space plasma phenomena. Conventional plasma wave receivers have the disadvantages of a large size and a narrow dynamic range. We proposes a new receiver that overcomes the disadvantages of conventional receivers. The analog section of the new receiver was realized using application-specific integrated circuit (ASIC) technology in order to reduce the size, and an ASIC chip was successfully developed.
Ari-Matti Harri, Konstantin Pichkadze, Lev Zeleny, Luis Vazquez, Walter Schmidt, Sergey Alexashkin, Oleg Korablev, Hector Guerrero, Jyri Heilimo, Mikhail Uspensky, Valery Finchenko, Vyacheslav Linkin, Ignacio Arruego, Maria Genzer, Alexander Lipatov, Jouni Polkko, Mark Paton, Hannu Savijärvi, Harri Haukka, Tero Siili, Vladimir Khovanskov, Boris Ostesko, Andrey Poroshin, Marina Diaz-Michelena, Timo Siikonen, Matti Palin, Viktor Vorontsov, Alexander Polyakov, Francisco Valero, Osku Kemppinen, Jussi Leinonen, and Pilar Romero
Geosci. Instrum. Method. Data Syst., 6, 103–124, https://doi.org/10.5194/gi-6-103-2017, https://doi.org/10.5194/gi-6-103-2017, 2017
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Investigations of Mars – its atmosphere, surface and interior – require simultaneous, distributed in situ measurements. We have developed an innovative prototype of the Mars Network Lander (MNL), a small lander/penetrator with a 20 % payload mass fraction. MNL features an innovative Entry, Descent and Landing System to increase reliability and reduce the system mass. It is ideally suited for piggy-backing on spacecraft, for network missions and pathfinders for high-value landed missions.
Stefan Meyer, Marek Tulej, and Peter Wurz
Geosci. Instrum. Method. Data Syst., 6, 1–8, https://doi.org/10.5194/gi-6-1-2017, https://doi.org/10.5194/gi-6-1-2017, 2017
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We developed a prototype of the Neutral Gas and Ion Mass spectrometer (NIM) of the Particle Environment Package (PEP) for the JUICE mission of ESA. NIM will be used to measure the chemical composition of the exospheres of the icy Jovian moons. The NIM prototype was successfully tested under realistic conditions and we find that the closed source behaves as expected within the JUICE mission phase velocities. No additional fragmentation of the species recorded with the closed source is observed.
Patrick Tiefenbacher, Norbert I. Kömle, Wolfgang Macher, and Günter Kargl
Geosci. Instrum. Method. Data Syst., 5, 383–401, https://doi.org/10.5194/gi-5-383-2016, https://doi.org/10.5194/gi-5-383-2016, 2016
H. J. Lehto, B. Zaprudin, K. M. Lehto, T. Lönnberg, J. Silén, J. Rynö, H. Krüger, M. Hilchenbach, and J. Kissel
Geosci. Instrum. Method. Data Syst., 4, 139–148, https://doi.org/10.5194/gi-4-139-2015, https://doi.org/10.5194/gi-4-139-2015, 2015
M. Sampl, W. Macher, C. Gruber, T. Oswald, M. Kapper, H. O. Rucker, and M. Mogilevsky
Geosci. Instrum. Method. Data Syst., 4, 81–88, https://doi.org/10.5194/gi-4-81-2015, https://doi.org/10.5194/gi-4-81-2015, 2015
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We present the high-frequency properties of the eight electric field sensors as proposed to be launched on the spacecraft “RESONANCE” in the near future. Due to the close proximity of the conducting spacecraft body, the sensors (antennas) have complex receiving features and need to be well understood for an optimal mission and spacecraft design. In particular techniques like wave polarization analysis and incident direction finding depend crucially on the presented antenna characteristics.
J. Silén, H. Cottin, M. Hilchenbach, J. Kissel, H. Lehto, S. Siljeström, and K. Varmuza
Geosci. Instrum. Method. Data Syst., 4, 45–56, https://doi.org/10.5194/gi-4-45-2015, https://doi.org/10.5194/gi-4-45-2015, 2015
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COSIMA, an advanced TOF-SIMS instrument measuring the mass spectrum of dust grains collected at comet P67 by the ROSETTA spacecraft, is predicted to encounter complex mixtures of minerals and organic compounds. To extract information from this data set, we have developed a multivariate technique tested on laboratory measurements made by an identical instrument under controlled conditions. We have shown that minerals can be identified and separated with high level of confidence.
P. Robert, N. Cornilleau-Wehrlin, R. Piberne, Y. de Conchy, C. Lacombe, V. Bouzid, B. Grison, D. Alison, and P. Canu
Geosci. Instrum. Method. Data Syst., 3, 153–177, https://doi.org/10.5194/gi-3-153-2014, https://doi.org/10.5194/gi-3-153-2014, 2014
Y. V. Khotyaintsev, P.-A. Lindqvist, C. M. Cully, A. I. Eriksson, and M. André
Geosci. Instrum. Method. Data Syst., 3, 143–151, https://doi.org/10.5194/gi-3-143-2014, https://doi.org/10.5194/gi-3-143-2014, 2014
N. Doss, A. N. Fazakerley, B. Mihaljčić, A. D. Lahiff, R. J. Wilson, D. Kataria, I. Rozum, G. Watson, and Y. Bogdanova
Geosci. Instrum. Method. Data Syst., 3, 59–70, https://doi.org/10.5194/gi-3-59-2014, https://doi.org/10.5194/gi-3-59-2014, 2014
A. Blagau, I. Dandouras, A. Barthe, S. Brunato, G. Facskó, and V. Constantinescu
Geosci. Instrum. Method. Data Syst., 3, 49–58, https://doi.org/10.5194/gi-3-49-2014, https://doi.org/10.5194/gi-3-49-2014, 2014
C. G. Mouikis, L. M. Kistler, G. Wang, and Y. Liu
Geosci. Instrum. Method. Data Syst., 3, 41–48, https://doi.org/10.5194/gi-3-41-2014, https://doi.org/10.5194/gi-3-41-2014, 2014
J. S. Pickett, I. W. Christopher, and D. L. Kirchner
Geosci. Instrum. Method. Data Syst., 3, 21–27, https://doi.org/10.5194/gi-3-21-2014, https://doi.org/10.5194/gi-3-21-2014, 2014
K. H. Yearby, S. N. Walker, and M. A. Balikhin
Geosci. Instrum. Method. Data Syst., 2, 323–328, https://doi.org/10.5194/gi-2-323-2013, https://doi.org/10.5194/gi-2-323-2013, 2013
L. M. Kistler, C. G. Mouikis, and K. J. Genestreti
Geosci. Instrum. Method. Data Syst., 2, 225–235, https://doi.org/10.5194/gi-2-225-2013, https://doi.org/10.5194/gi-2-225-2013, 2013
N. I. Kömle, W. Macher, G. Kargl, and M. S. Bentley
Geosci. Instrum. Method. Data Syst., 2, 151–156, https://doi.org/10.5194/gi-2-151-2013, https://doi.org/10.5194/gi-2-151-2013, 2013
M. D. Paton, A.-M. Harri, T. Mäkinen, and S. F. Green
Geosci. Instrum. Method. Data Syst., 1, 7–21, https://doi.org/10.5194/gi-1-7-2012, https://doi.org/10.5194/gi-1-7-2012, 2012
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Short summary
The new wind reconstruction algorithm developed in this article extends the amount of available sols from the Viking Lander 1 (VL1) mission from 350 to 2245. The reconstruction of wind measurement data enables the study of both short-term phenomena, such as daily variations in wind conditions or dust devils, and long-term phenomena, such as the seasonal variations in Martian tides.
The new wind reconstruction algorithm developed in this article extends the amount of available...