The Martian Anomalies: A Photographic Search for Intelligent Life on Mars

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Sholes, S. F., Montgomery, D. R. & Catling, D. C. Quantitative high‐resolution reexamination of a hypothesized ocean shoreline in Cydonia Mensae on Mars. J. Geophys. Res. Planets 124, 316–336 (2019). Holm, N. G. & Hennet, R. J.-C. in Marine Hydrothermal Systems and the Origin of Life 15–31 (Springer, 1992). Lillis, R. J. et al. An improved crustal magnetic field map of Mars from electron reflectometry: highland volcano magmatic history and the end of the Martian dynamo. Icarus 194, 575–596 (2008). Full details of the RoMAG instrumentation can be found in a previous study 11. The RoMAG is a set of magnetometers with two identical tri-axial fluxgate sensors, one mounted near the top of the mast of the Zhurong rover, and the other fixed on the mast base. The fluxgate magnetometers measure magnetic fields with a dynamic range of ±65,000 nT with a noise level of 0.01 nT −1/2 at 1 Hz, and a normal sample rate of 1 Hz and capacity of 32 Hz in burst mode. The first RoMAG measurements were implemented in the rover static mode on 4 June 2021, which occurred at the first observation point, 5.14 m away from the lander. During the following 90 sols, RoMAG acquired raw data of magnetic vector fields at another 15 observation points over a total distance of 1,089 m. Next, we investigated the diurnal variations at InSight with respect to local true solar time (LTST) and Ls to evaluate the diurnal fluctuations as well as the sol-to-sol variations within Ls from 54° to 95° (Supplementary Fig. 5). It was shown that the median amplitude during the LTST of interest was less than 15 nT (Supplementary Fig. 5a). The peak amplitudes of H component show variations from 10 to 25 nT during Ls from 54° to 95° (Supplementary Fig. 5b). The peak amplitude, to some extent, represented the upper limit of the amplitude of a sol in the LTST of interest. The standard deviation of the peak amplitudes of B H is about 3.5 nT, which can be treated as the sol-to-sol variability in B H. This could be due to the sol-to-sol variations of the ionospheric currents since both the Thermospheric Neutral Wind 38 and/or the electron densities 39, 40 in the Martian ionosphere appear to have sol-to-sol variations. According to the ionospheric current modelling at both Zhurong and InSight, the sol-to-sol variations at Zhurong would also be less than 3.5 nT during the Ls of interest.

Laboratoire de Planétologie et Géodynamique, UMR6112, Université Nantes, Université Angers, CNRS, Nantes, FranceNeumann, G. A. et al. Crustal structure of Mars from gravity and topography. J. Geophys. Res. E Planets 109, https://doi.org/10.1029/2004JE002262 (2004).

Lorenz, R. D. et al. Seismometer detection of dust devil vortices by ground tilt. Bull. Seismol. Soc. Am. 105, 3015–3023 (2015). Neumann, N., Sandiford, M. & Foden, J. Regional geochemistry and continental heat flow: implications for the origin of the South Australian heat flow anomaly. Earth Planet. Sci. Lett. 183, 107–120 (2000).Schumacher, S. & Breuer, D. Influence of a variable thermal conductivity on the thermochemical evolution of Mars. J. Geophys. Res. E Planets https://doi.org/10.1029/2005JE002429 (2006). They also do not allow me to ignore the work (in a separate area) of my friend Dr Judy Wood (who has sued NIST’s contractors for fraud) showing that the WTC was destroyed using some kind of directed energy weapon on 9/11. So, come on, how utterly ridiculous is that for a conclusion?