ICARUS Signal Processing With HEPnOS
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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Neutrinos are hard to study. Cosmic Rays are easier, so they can be used to understand the detector. The ratio of the Monte Carlo simulations and the experimental data gives insights into uncertainties stemming from the detector.
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Presentation given by academic subcontractor for work performed under LDRD contract
Italian Summer Student Program @ FNAL – Final reviews 2022
Summer Students at Fermilab program 2022
Italian Summer Students Final Presentation - day2
Italian Summer Students Program Final presentation 2023
Italian Summer Students Final Presentations 2023
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Neutrino Joint Theory-Experiment Seminar, Summer Reports
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The dataset encompasses QA/QC TBS data, including TBS altitude, atmospheric pressure, dew point, POPs number concentrations and mean aerosol size, relative humidity, temperature, equivalent potential temperature, equivalent temperature, and date and time. These data are provided per day for at least one TBS flight. Supporting data from the AMF3 aligned with the timestamps of the TBS data include cloud base distance from TBS, if the time corresponds to cloud base transit of the TBS, surface-based pressure, surface-based precipitation rate, surface-based UHSAS data, ceilometer cloud base height, KAZR cloud top height, and MWR liquid water content. Both POPS and UHSAS aerosol number concentrations are provided as: (1) absolute (i.e. concentrations for each instrument's total size range) and (2) the overlapping size range (i.e. the same size bins for both instruments).