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Dr James B. Scoggins (NASA Langley Research Center)15/09/2022, 09:00
I. Introduction
On February 18, 2021, the Mars 2020 Perseverance rover successfully entered the Martian atmosphere and landed safely on the surface. During entry, the Mars 2020 aeroshell was outfitted with a sensor suite, known as Mars Entry, Descent, and Landing Instrumentation 2 (MEDLI2), which measured pressures, in-depth temperatures, and surface heat fluxes at various points on the...
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Eric Won Keun Chang (University of Oxford)15/09/2022, 09:20
Please find the abstract attached.
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Dr Aaron Brandis (NASA Ames Research Center)15/09/2022, 09:45
An overview of the Dragonfly aerothermal environments and simulations performed will be presented. Titan’s atmosphere predominantly consists of nitrogen (~98% by mole) with small amounts of methane (~2% by mole) and other trace gases. CN is a strong radiator and is found in nonequilibrium concentrations for Titan entry, and is of particular importance on the backshell, where radiation...
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116. Experimental VUV Radiation Measurements for 13 and 14 kms Mars Return Re-entry Conditions in X2Samuel Lock (The University of Queensland)15/09/2022, 11:00
This paper presents preliminary stagnation point VUV radiation measurements taken over a 25 mm diameter, 75 mm wide semicylindrical model at 13 and 14 km/s Mars return re-entry conditions using the X2 expansion tube facility at the University of Queensland.
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Brett Cruden (AMA Inc/NASA Ames)15/09/2022, 11:25
In February 2021, the Perseverance rover was brought to the surface of Mars by the Mars 2020 mission. A feature of the Mars 2020 capsule was instrumentation to measure its entry, descent and landing (EDL) with the so-called Mars EDL Instrumentation 2 (MEDLI2) [1]. The MEDLI2 introduced, among other things, backshell instrumentation, including a broadband radiometer. The radiometer was mounted...
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