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1“...Galaxy spins can be predicted from the initial conditions in the early Universe through the tidal...”
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2by Manucharyan, Georgy E., Lopez-Acosta, Rosalinda, Wilhelmus, Monica M.“... of isolated spinning sea ice floes in marginal ice zones. Using over two decades of satellite observations...”
Published in Scientific Reports (2022)
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3by Keswani, N., Lopes, R., Nakajima, Y., Singh, R., Chauhan, N., Som, T., Kumar, S., Pereira, A. R., Das, P.“... pyrochlore solids, a classical analogue of monopole was observed as a result of excitation of spin ice...”
Published in Scientific Reports (2020)
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4by Keswani, Neeti, Lopes, Ricardo J. C., Nakajima, Yoshikata, Singh, Ranveer, Chauhan, Neha, Som, Tapobrata, Kumar, D. Sakthi, Pereira, Afranio R., Das, Pintu“... pyrochlore solids, a classical analogue of monopole was observed as a result of excitation of spin ice...”
Published in Scientific Reports (2021)
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5“...We propose a two-spin quantum-mechanical model with applied magnetic fields acting on the Poincar...”
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6“..., according to the size and spin of the respective polar cyclone. Moreover, the analysis successfully predicts...”
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7by Huguenin, Maurice F., Holmes, Ryan M., England, Matthew H.“..., using a spin-up that improves on earlier approaches, to investigate recent OHU trends basin-by-basin...”
Published in Nature Communications (2022)
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8“... spin-up of the cyclonic Weddell Gyre played a crucial role in generating the 2017 Maud Rise Polynya...”
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9“...), tibia I length 8–10.38 (8.99), femur/carapace ratio 1.84–2.11 (1.99). Females ( N = 5): total length...”
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10“...), tibia I length 8–10.38 (8.99), femur/carapace ratio 1.84–2.11 (1.99). Females ( N = 5): total length...”
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