Mar 2 @ 3:15 pm – 4:15 pm BX102
Colloquium Title Gordon MacDonald, NMSU AbstractShare this:TweetPrint
Mar 28 @ 3:15 pm – 4:15 pm Science Hall 109
Seismic Inferences of Gas Giant Planets: Excitation & Interiors Ethan Dederick, NMSU Seismology has been the premier tool of study for understanding the interior structure of the Earth, the Sun, and even other stars. In...
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Sep 28 @ 3:15 pm – 4:15 pm BX102
Spatial Curvature, Dark Energy Dynamics, Neither, or Both? Bharat Ratra, Kansas State University Experiments and observations over the two last decades have persuaded cosmologists that (as yet undetected) dark energy is by far the main...
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Oct 5 @ 3:15 pm – 4:15 pm BX102
Clues to Globular Cluster Formation David Nataf, Johns Hopkins University Globular clusters are now well-established to host “Second-generation” stars, which show anomalous abundances in some or all of He, C, N, O, Na, Al, Mg,...
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Sep 6 @ 3:15 pm – 4:15 pm BX102
Starless clumps and the earliest phases of high-mass star formation in the Milky Way Brian Svoboda, NRAO Jansky Fellow High-mass stars are key to regulating the interstellar medium, star formation activity, and overall evolution of...
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Nov 8 @ 3:15 pm – 4:15 pm BX102
Galaxy Evolution in a Computer Box, or “How to turn a PhD on Theoretical Galaxy Evolution into a Scientific Programming Career with NASA” Jacob Vander Vliet, NASA/SOFIA I graduated from NMSU in 2017 with a...
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Nov 15 @ 3:15 pm – 4:15 pm BX102
Using every photon to learn about the physics of solar plasmas Phil Judge, High Altitude Observatory, Boulder CO. The Sun has traditionally been the Rosetta Stone that can overcome the gap in regimes between laboratory...
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Dec 4 @ 3:00 pm – 4:00 pm BX102
Role of solar Rossby waves in causing space weather on intermediate time-scales Mausumi Dikpati, HAO Forecasting our weather was built on the recognition that global Rossby waves, interacting with mean east-west flow on the Earth’s...
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