Search Results - "Dalton III, J. B."

Europa's icy bright plains and dark linea: Exogenic and endogenic contributions to composition and surface properties by Dalton III, J. B., Shirley, J. H., Kamp, L. W.

“…We compare linear spectral modeling solutions yielding surface abundance estimates and water ice grain size information from low‐noise Galileo Near‐Infrared…”
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Low temperature optical constants of some hydrated sulfates relevant to planetary surfaces by Dalton III, J. B., Pitman, K. M.

“…We derive optical constants (n(λ) and k(λ)) from laboratory reflectance spectra acquired at visible to near‐infrared wavelengths for epsomite (MgSO4⋅7H2O),…”
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The spectral variability of kieserite (MgSO4·H2O) with temperature and grain size and its application to the Martian surface by Jamieson, C. S., Noe Dobrea, E. Z., Dalton III, J. B., Pitman, K. M., Abbey, W. J.

“…We spectrally characterize (λ = 0.35–10 µm) the low‐humidity polymorph of kieserite (MgSO4·H2O), which is abundant on Mars and likely present on Europa, at…”
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Magnetospheric ion sputtering and water ice grain size at Europa by Cassidy, T.A., Paranicas, C.P., Shirley, J.H., Dalton III, J.B., Teolis, B.D., Johnson, R.E., Kamp, L., Hendrix, A.R.

“…We present the first calculation of Europa's sputtering (ion erosion) rate as a function of position on Europa's surface. We find a global sputtering rate of…”
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Exogenic controls on sulfuric acid hydrate production at the surface of Europa by Dalton, J.B., Cassidy, T., Paranicas, C., Shirley, J.H., Prockter, L.M., Kamp, L.W.

“…External agents have heavily weathered the visible surface of Europa. Internal and external drivers competing to produce the surface we see include, but are…”
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