Search Results - "Gruesbeck, J. R"
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The Drivers of the Martian Bow Shock Location: A Statistical Analysis of Mars Atmosphere and Volatile EvolutioN and Mars Express Observations
Published in Journal of geophysical research. Space physics (01-05-2022)“…The Martian interaction with the solar wind leads to the formation of a bow shock upstream of the planet. The shock dynamics appear complex, due to the…”
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First results of the MAVEN magnetic field investigation
Published in Geophysical research letters (16-11-2015)“…Two Mars Atmosphere and Volatile EvolutioN magnetic field sensors sample the ambient magnetic field at the outer edge of each solar array. We characterized…”
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Autocorrelation Study of Solar Wind Plasma and IMF Properties as Measured by the MAVEN Spacecraft
Published in Journal of geophysical research. Space physics (01-04-2018)“…It has long been a goal of the heliophysics community to understand solar wind variability at heliocentric distances other than 1 AU, especially at ∼1.5 AU due…”
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Transient Foreshock Structures Upstream of Mars: Implications of the Small Martian Bow Shock
Published in Geophysical research letters (28-04-2023)“…The typical subsolar stand‐off distance of Mars' bow shock is of the order of a solar wind ion convective gyroradius, making it highly non‐planar to incident…”
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Martian magnetic storms
Published in Journal of geophysical research. Space physics (01-06-2017)“…The response of Mars to the major space weather events called interplanetary coronal mass ejections (ICMEs) is of interest for both general planetary solar…”
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CHARGE STATE EVOLUTION IN THE SOLAR WIND. II. PLASMA CHARGE STATE COMPOSITION IN THE INNER CORONA AND ACCELERATING FAST SOLAR WIND
Published in The Astrophysical journal (10-12-2012)“…In the present work, we calculate the evolution of the charge state distribution within the fast solar wind. We use the temperature, density, and velocity…”
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A Global Two-temperature Corona and Inner Heliosphere Model: A Comprehensive Validation Study
Published in The Astrophysical journal (20-01-2012)“…The recent solar minimum with very low activity provides us a unique opportunity for validating solar wind models. During CR2077, the number of sunspots was…”
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Solar cycle–dependent helicity transport by magnetic clouds
Published in Journal of Geophysical Research - Space Physics (01-08-2005)“…Magnetic clouds observed with the Wind and ACE spacecraft are fit with the static, linear force‐free cylinder model to obtain estimates of the chirality,…”
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A Generalized Magnetospheric Disturbance Index: Initial Application to Mars Using MAVEN Observations
Published in Journal of geophysical research. Space physics (01-12-2021)“…Since MAVEN's arrival at Mars in 2014, in situ observations of the magnetic field have been made continually. During this time, the Martian magnetosphere has…”
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Variability of Upstream Proton Cyclotron Wave Properties and Occurrence at Mars Observed by MAVEN
Published in Journal of geophysical research. Space physics (01-02-2021)“…The presence of plasma waves upstream from the Martian bow shock, with frequencies near the local proton cyclotron frequency in the spacecraft frame,…”
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The Influence of Crustal Magnetic Fields on the Martian Bow Shock Location: A Statistical Analysis of MAVEN and Mars Express Observations
Published in Journal of geophysical research. Space physics (01-05-2022)“…Previous missions underlined the complex influence of the crustal magnetic fields on the Martian environment, including the plasma boundaries. Their influence…”
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Switchback Boundary Dissipation and Relative Age
Published in The Astrophysical journal (01-07-2021)“…We examine Parker Solar Probe (PSP) magnetic field and plasma observations during its first encounter with the Sun in early 2018 November. During this…”
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The Modulation of Solar Wind Hydrogen Deposition in the Martian Atmosphere by Foreshock Phenomena
Published in Journal of geophysical research. Space physics (01-08-2019)“…The neutral exosphere of Mars extends far upstream beyond the bow shock, and as a result, solar wind protons can charge exchange with this neutral exosphere to…”
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CARBON IONIZATION STAGES AS A DIAGNOSTIC OF THE SOLAR WIND
Published in The Astrophysical journal (10-01-2012)“…Oxygen charge states measured by in situ instrumentation have long been used as a powerful diagnostic of the solar corona and to discriminate between different…”
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The Martian Ionospheric Response to the Co-Rotating Interaction Region That Caused the Disappearing Solar Wind Event at Mars
Published in Journal of geophysical research. Space physics (01-03-2024)“…An unusually low density solar wind event was observed in December 2022 moving past both Earth and Mars. The source was traced back to a coronal hole and…”
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NEW SOLAR WIND DIAGNOSTIC USING BOTH IN SITU AND SPECTROSCOPIC MEASUREMENTS
Published in The Astrophysical journal (10-05-2012)“…We develop a new diagnostic technique that utilizes, at the same time, two completely different types of observations-in situ determinations of solar wind…”
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NEW SOLAR WIND DIAGNOSTIC USING BOTH IN SITU AND SPECTROSCOPIC MEASUREMENTS
Published in The Astrophysical journal (10-05-2012)Get full text
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18
Will we find Martian lightning via Schumann resonances?
Published in Frontiers in astronomy and space sciences (13-09-2023)“…Schumann resonances are electromagnetic resonances generally associated with lightning. If they exist on Mars, Schumann resonances are expected to resonate…”
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Transient Foreshock Structures Upstream of Mars: Implications of the Small Martian Bow Shock
Published 26-01-2023“…Geophysical Research Letters Volume 50, Issue8 28 April 2023 e2022GL101734 We characterize the nature of magnetic structures in the foreshock region of Mars…”
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The dependence of Martian ion escape on solar EUV irradiance as observed by MAVEN
Published in Icarus (New York, N.Y. 1962) (15-03-2023)“…We analyze the planetary ion, solar wind, interplanetary magnetic field (IMF), and solar extreme ultraviolet (EUV) irradiance data from the NASA Mars…”
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