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on SAR and optical images, GPS, seismometer waveforms, and gravity measurements. Time series analysis of the SAR interferometry and other data is a key part of the research. We then infer the structure and
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capability of CMEs, as derived from the interplanetary radio emission associated with these solar eruptions. Spacecraft data obtained by white-light coronagraphs and radio instruments are used
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plasmas. This work provides some of the atomic physics data needed for modelling celestial spectra and also valuable operational and calibration experience with these very sensitive spectrometers. Location
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the galaxy from their sources to the Earth. A developed Monte Carlo computer code is used to study the acceleration process by plasma shocks, while mathematical models have been designed to describe how
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transiting exoplanets with data from space-based facilities like TESS, HST, JWST, and/or ground-based facilities, or with data simulations in preparation for Roman. Potential areas of research include: (1
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-band ISRO‘s OceanSat-2. There is concurrently a large set of passive microwave radiometric windspeed data from sensors such as AMSR-E, WindSat, TRMM, GPM and recently L-band (~1 GHz) from Aquarius. In
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Imaging System (E-THEMIS) will measure global, regional and local surface temperatures at three thermal infrared wavelengths under various conditions of local time and emission angles. These data will
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troposphere and stratosphere (UT/S) - and its role in climate. We use a combination of satellite data, high-altitude aircraft measurements, and models to investigate variations in and processes that impact
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, high precision spectroscopic data of bright, active stars to determine how best to identify and separate these signals from the true Keplerian reflex motion induced by orbiting planets. We aim to paint a
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individuals and as communities comprising larger ecosystems. Traits are also often used as parameters in computer models of terrestrial ecosystems and even the entire Earth System (such as climate models used