Aims and Scope
Geophysical Research Letters (GRL) publishes high-impact, innovative, and timely research on major scientific advances in all the major geoscience disciplines. Papers are communications-length articles and should have broad and immediate implications in their discipline or across the geosciences. GRL maintains the fastest turn-around of all high-impact publications in the geosciences and works closely with authors to ensure broad visibility of top papers.
GRL is a Letters journal; limiting manuscript size expedites the review and publication process. GRL also publishes a limited number of frontier articles, by invitation from Editors. GRL's mission is to disseminate concisely written, high-impact research reports on major scientific advances in AGU disciplines [PDF]. With this goal, the Editorial Board evaluates manuscripts submitted to GRL according to the following criteria:
High impact innovative results with broad geophysical implications at the forefront of one or several AGU disciplines.
Results with immediate impact on the research of others and requiring rapid publication.
Instrument or methods manuscript introducing an innovative technique that makes new science advance possible, with immediate applications to AGU disciplines.
GRL has been in publication since 1974. The Editors are adapting GRL to the evolving needs of the Earth science community. GRL Editors are topical: the subject of the paper determines which Editor handles the review and decision process. For more information, please read this Eos editorial.
Covers (1997–present) are available.
Eos.org: Earth & Space Science News
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Featured Special Collection
Early results from Juno's mission at Jupiter including approach to Jupiter and the first perijove pass (PJ1). Juno's scientific objectives include the study of Jupiter's interior, atmosphere and polar magnetosphere with the goal of understanding Jupiter's origin, formation and evolution. This collection of papers provides early results from Juno's measurements of the gravity and magnetic fields, deep atmospheric microwave sounding, infrared, visible and ultraviolet images/spectra and an array of fields and particles instruments as well as context for the early results with respect to current theory and models of Jupiter's formation and evolution. Topics include both Juno - Jupiter related theoretical models and data analysis as well as collaborative observations made from Earth based assets.