![(A) Non-local turbulence as a function of Local True Solar Time (LTST) for spring 835 (Sol 200) and autumn (Sol 591) on Mars [reproduced from Figure 2 of Chatain et al. 2021]. (B) 836 Recreated analysis showing non-local turbulence (Pa) as a function of LTST for Sol 200 (blue) 837 and Sol 591 (orange). The turbulence peaks during the daytime, around 12–13 hours LTST, with 838 minimal activity at night. (C) Scatter plots of horizontal wind speed (m/s) as a function of non839 local turbulence (Pa) for Sol 200 (blue) and Sol 591 (orange). Higher wind speeds are associated 840 with increased turbulence, with Sol 591 exhibiting stronger winds overall. [Figure and caption 841 generated by the Mars IDEA.] -- Journal of Geophysical Research: Machine Learning and Computation](https://astrobiology.newspackstaging.com/wp-content/uploads/2025/08/Tricorder-Tech-IDEA.png)
A new artificial intelligence tool developed by researchers at the University of Hawai‘i (UH) at Mānoa is making it easier for scientists to explore complex geoscience data—from tracking sea levels on Earth to analyzing atmospheric conditions on Mars. Called the Intelligent Data Exploring Assistant (IDEA), the software framework combines the power of large language models, […]
Category: Apps – Games
Posted inApps - Games, Arctic / Antarctic / Alpine, Astrogeology, Atmospheres, Climate, Weather, Biogeochemical Cycles & Geobiology, Cryobiology, Extremeophiles and Extreme Environments, Gaia - Planetary Perspectives, Habitable Zones, Icy Worlds, Reports, Roadmaps, & Plans, Terraforming & Geoengineering, Water/Hycean Worlds & Oceanography
Ice Planet Update: State of the Cryosphere Report 2024 – Lost Ice, Global Damage
![Continuum noise power and FX complex correlator measurements, observed on MJD 60586, are presented together with the statistical power of 3.7 Hz bandwidth, 0.27 s duration polarized pulse pairs, recorded during the 123.8 day experiment. The high correlator response at 5.5 hr RA is due to the Orion A emission nebula at -5.4º DEC. [10][11]. Instrument delay difference of -82 ns between interferometer elements was compensated by choosing to display the -5 x 16 ns correlator tap. The bandwidth of the continuum and correlator measurements is approximately 50 MHz, at 0.27 s integration. The timedependent geometric space delay was not compensated, resulting in the approximate sawtooth phase response across RA, indicating a period of 0.117 hr RA. The prior pointing direction of interest indicates greater than 6 standard deviations Cohen’s d in the 5.1675 ± 0.00375 hr RA bin, within the prior range, 5.25 ± 0.15 hr RA. A second apparent response is indicated in two adjacent bins centered at 8.8425 hr RA, with apparent RA aliasing at ±0.12 hr RA. Figs. 2 and 3 show detail. -- eess.SP](https://astrobiology.newspackstaging.com/wp-content/uploads/2024/12/A-Signal-Discovery-Step-In-Interstellar.png)
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