11 research outputs found

    Recent Progress in Physics-Based Models of the Plasmasphere

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    Meteoroids as One of the Sources for Exosphere Formation on Airless Bodies in the Inner Solar System

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    AbstractThis manuscript represents a review on progress made over the past decade concerning our understanding of meteoroid bombardment on airless solar system bodies as one of the sources of the formation of their exospheres. Specifically, observations at Mercury by MESSENGER and at the Moon by LADEE, together with progress made in dynamical models of the meteoroid environment in the inner solar system, offer new tools to explore in detail the physical phenomena involved in this complex relationship. This progress is timely given the expected results during the next decade that will be provided by new missions such as DESTINY+, BepiColombo, the Artemis program or the Lunar Gateway

    Augmented Empirical Models of Plasmaspheric Density and Electric Field Using IMAGE and CLUSTER Data

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    The Mars Atmosphere and Volatile Evolution (MAVEN) Mission

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    The MAVEN spacecraft launched in November 2013, arrived at Mars in September 2014, and completed commissioning and began its one-Earth-year primary science mission in November 2014. The orbiter’s science objectives are to explore the interactions of the Sun and the solar wind with the Mars magnetosphere and upper atmosphere, to determine the structure of the upper atmosphere and ionosphere and the processes controlling it, to determine the escape rates from the upper atmosphere to space at the present epoch, and to measure properties that allow us to extrapolate these escape rates into the past to determine the total loss of atmospheric gas to space through time. These results will allow us to determine the importance of loss to space in changing the Mars climate and atmosphere through time, thereby providing important boundary conditions on the history of the habitability of Mars. The MAVEN spacecraft contains eight science instruments (with nine sensors) that measure the energy and particle input from the Sun into the Mars upper atmosphere, the response of the upper atmosphere to that input, and the resulting escape of gas to space. In addition, it contains an Electra relay that will allow it to relay commands and data between spacecraft on the surface and Earth

    Augmented Empirical Models of Plasmaspheric Density and Electric Field Using IMAGE and CLUSTER Data

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    The Mars Atmosphere and Volatile Evolution (MAVEN) Mission

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    Plasmaspheric Density Structures and Dynamics: Properties Observed by the CLUSTER and IMAGE Missions

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    Aeronomy of the Venus Upper Atmosphere

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