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Research in the Adams lab concentrated on the fundamentals of gas-phase ionic reaction processes and their application to natural plasmas, with relevance to the interstellar medium and to planetary atmospheres. To measure pertinent reactions in the laboratory, he was co-inventor of the powerful Selected Ion Flow Tube (SIFT) method for studying ion molecule reactions under conditions that simulate the low temperature, low pressure plasmas of the ISM. Adams also developed and refined the Flowing Afterglow Langmuir Probe (FALP) apparatus, which is used to examine electron-ion recombination, a key process in the formation of many species of interest in Space Physics. His work was groundbreaking in the identification and quantification of the neutral products of ion-electron recombination reactions. During his career he published over 200 scientific papers, edited several books, and was an invited speaker at numerous conferences and symposia. Adams retired on July 31, 2014 after almost 25 years in the Department of Chemistry at the University of Georgia. He is survived by his loving family: his wife Lucia; his children Liz, Robin, Ian, and Lydia; his sisters Beryl and Zena; and his grandson Jamie; as well as many nieces and nephews.
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Springer Handbook of Atomic, Molecular, and Optical PhysicsSpringer Handbookspp.597-607, (2023)
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ASTROPHYSICAL JOURNAL SUPPLEMENT SERIESno. 1 (2012): 21
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