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S. Schreiner

Researcher at Massachusetts Institute of Technology

Publications -  31
Citations -  521

S. Schreiner is an academic researcher from Massachusetts Institute of Technology. The author has contributed to research in topics: In situ resource utilization & Regolith. The author has an hindex of 12, co-authored 27 publications receiving 429 citations. Previous affiliations of S. Schreiner include University of Minnesota & California Institute of Technology.

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An Independent Assessment of the Technical Feasibility of the Mars One Mission Plan

TL;DR: In this article, the authors present an independent assessment of the technical feasibility of the Mars One mission architecture, using a Mars settlement analysis tool that integrates a habitat simulation with an ISRU sizing model and a sparing analysis to predict the required number of launchers and provide a preliminary estimate of a portion of the program cost.
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Observations of large-amplitude, narrowband whistlers at stream interaction regions

TL;DR: In this paper, the first solar wind observations of large-amplitude, narrowband waveforms in the frequency range 10-100 Hz consistent with the whistler mode were presented.
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An independent assessment of the technical feasibility of the Mars One mission plan – Updated analysis☆

TL;DR: In this paper, the authors performed an independent analysis of the technical feasibility of the Mars One mission plan, focusing on the architecture of the life support and in-situ resource utilization (ISRU) systems, and their impact on sparing and space logistics.
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Thermophysical property models for lunar regolith

TL;DR: In this paper, a set of thermophysical property models for lunar regolith are presented, which are based on data from Apollo samples and high-temperature molten regolith simulants, extending significantly beyond existing models in the literature.
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STEREO and Wind observations of intense cyclotron harmonic waves at the Earth's bow shock and inside the magnetosheath

TL;DR: In this article, the first observations of electron cyclotron harmonic waves at the Earth's bow shock from STEREO and Wind burst waveform captures were presented. But the results were limited to a few tens to more than 500 millivolts/meter peak-peak.