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Michael L. Stevens

Researcher at Smithsonian Astrophysical Observatory

Publications -  269
Citations -  8338

Michael L. Stevens is an academic researcher from Smithsonian Astrophysical Observatory. The author has contributed to research in topics: Solar wind & Heliosphere. The author has an hindex of 41, co-authored 224 publications receiving 5540 citations. Previous affiliations of Michael L. Stevens include Massachusetts Institute of Technology & Harvard University.

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Solar Wind Electrons Alphas and Protons (SWEAP) Investigation: Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus

Justin C. Kasper, +80 more
TL;DR: The Solar Wind Electrons Alphas and Protons (SWEAP) Investigation on Solar Probe Plus is a four sensor instrument suite that provides complete measurements of the electrons and ionized helium and hydrogen that constitute the bulk of solar wind and coronal plasma.
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Highly structured slow solar wind emerging from an equatorial coronal hole

TL;DR: Measurements from the Parker Solar Probe show that slow solar wind near the Sun’s equator originates in coronal holes, and plasma-wave measurements suggest the existence of electron and ion velocity-space micro-instabilities that are associated with plasma heating and thermalization processes.
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Alfvénic velocity spikes and rotational flows in the near-Sun solar wind

TL;DR: Observations of solar-wind plasma at heliocentric distances of about 35 solar radii reveal an increasing rotational component to the flow velocity of the solar wind around the Sun, peaking at 35 to 50 kilometres per second—considerably above the amplitude of the waves.
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Loss of the Martian atmosphere to space: Present-day loss rates determined from MAVEN observations and integrated loss through time

Bruce M. Jakosky, +131 more
- 15 Nov 2018 - 
TL;DR: In this article, the authors used observations of the Mars upper atmosphere made from the Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft to determine the loss rates of gas from the upper atmosphere to space for a complete Mars year (16 Nov 2014 − 3 Oct 2016).
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MAVEN observations of the response of Mars to an interplanetary coronal mass ejection

Bruce M. Jakosky, +93 more
- 06 Nov 2015 - 
TL;DR: Observations and models both show an enhancement in escape rate of ions to space during the Mars upper atmosphere, ionosphere, and interactions with the Sun and solar wind during an interplanetary coronal mass ejection impact in March 2015.