287 data "https:" "https:" "https:" "https:" "Dr" "Goethe University" positions at Zintellect
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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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climate. Observational work would include data from GRACE, SMAP, GPM or in-situ stations. Model diagnosis and analysis can include CLM, VIC, CLSM, and LIS frameworks including GLDAS and NLDAS. Model
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. Description: The Postdoctoral Fellow will work with a team of world-class collaborators on the JWST Cycle 1 GO Program 2512 (https://www.stsci.edu/jwst/science-execution/program-information.html?id=2512
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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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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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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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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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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