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Abstract Supplementary Materials References and Notes Information & Authors Metrics & Citations Check Access References Figures Tables Media Share Abstract Theory predicts that a planet with a sufficiently strong magnetic field orbiting close to its host star could induce star-planet magnetic interactions. This is potentially observable as an optical or radio stellar activity signal synchronised with the planet’s orbital period.
Authors and Affiliations Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, Maryland, USA Z. Rustamkulov & D. K. Sing Department of Physics & Astronomy, Johns Hopkins University, Baltimore, MD, USA D. K. Sing, N. H. Allen & L. Ramos-Rosado Department of Astronomy & Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, 95064, USA S. Mukherjee, A. L. Carter, N. M. Batalha, J. J. Fortney & K. Ohno Johns Hopkins APL, Laurel, MD, USA E. M. May, K. B. Stevenson & J.
Abstract The reflectance of the Earth is a fundamental climate parameter that we measured from Big Bear Solar Observatory between 1998 and 2017 by observing the earthshine using modern photometric techniques to precisely determine daily, monthly, seasonal, yearly and decadal changes in terrestrial albedo from earthshine.
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