Magnetic Influences on Coronal Heating and the Solar Wind Lauren Woolsey, Harvard University Abstract The physical mechanism(s) that generate and accelerate the solar wind have not been conclusively determined after decades of study, though not...
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The Chemical History and Evolution of Titan’s Atmosphere as Revealed by ALMA Alexander Thelen, NMSU Saturn’s largest moon, Titan, possesses a substantial atmosphere containing significant minorities of nitrile and hydrocarbon species, predominantly due to the...
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Utilizing Planetary Oscillations to Constrain the Interior Structure of the Jovian Planets Ethan Dederick Seismology has been the premier tool of study for understanding the interior structure of the Earth, the Sun, and even other stars....
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Outer Planets Update Dr. Amy Simon, NASA The Hubble Outer Planet Atmospheres Legacy (OPAL) program is a yearly program for observing each of the outer planets over two full rotations. Observations began with Uranus in...
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JIVE/JOVIAL, a network for Jupiter’s seismology and atmosphere dynamics F.X. Schmider, Observatoire de la Cote d’AzurShare this:TweetPrint
The AAS: What Has it Done for You Lately?Share this:TweetPrint
Characterizing the oscillatory response of the chromosphere during solar flares Laurel Farris; NMSU Astronomy Department Quasi-periodic pulsations (QPPs) are observed in the emission of solar flares over a wide range of wavelengths, particularly in the radio...
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