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, ionopause current layers, ionospheric fluxropes, nightside ionospheric holes, cometary type-I ion tails, induced magnetic tails, and plasma wake effects. Extensive data sets relevant to these phenomena from
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. Description: Context: Laboratory Astrophysics is a core capability at NASA Ames Research Center. Laboratory experiments and quantum-chemical computations simulating astrophysical conditions generate data
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feedbacks and the uncertainty in the NASA GISS Earth System model and provide information about future changes particularly with respect to the evolution of the marine and terrestrial sinks. Research
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timescales (daily to yearly). The data to be analyzed will be from a combination of facilities, including the the Keck Planet Finder (KPF), PARVI, and NEID instruments, each of which has (or will soon have) a
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. Description: This opportunity encompasses any atmospheric dynamics or structure research using imaging data from the Hubble Space Telescope Outer Planet Atmospheres Legacy (OPAL) program. The dataset consists
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. Sterczewski, Mathieu Fradet, Clifford Frez, Siamak Forouhar, Mahmood Bagheri First published: 15 September 2022 https://doi.org/10.1002/lpor.202200224 Field of Science: Technology Development Advisors: Siamak
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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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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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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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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