Differentiating the Acceleration Mechanisms in the Slow and Alfvénic Slow Solar Wind by Yeimy J. Rivera, Samuel T. Badman, J. L. Verniero, Tania Varesano, Michael L. Stevens, Julia E. Stawarz, Katharine K. Reeves, Jim M. Raines, John C. Raymond, Christopher J. Owen, Stefano A. Livi, Susan T. Lepri, Enrico Landi, Jasper. S. Halekas, Tamar Ervin, Ryan M. Dewey, Rossana De Marco, Raffaella D’Amicis, Jean-Baptiste Dakeyo, Stuart D. Bale, B. L. Alterman

Subjects: “…Solar wind…”
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Linear analysis of bump on tail instability with non-Maxwellian distribution function by Noreen, N, Shiekh, A, Habumugisha, I, Zaheer, S, AShah, H

Subjects: “…solar wind, Instability, Growth rate…”
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Exploring the Complex Heliotail Boundary by an Extended Level Set Approach by C. Onubogu, M. Opher, M. Kornbleuth, G. Tóth, V. Florinski

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Propagation of Interplanetary Shocks in the Inner Heliosphere by Munkhjargal Lkhagvadorj, Gábor Facskó, Andrea Opitz, Péter Kovács, David G. Sibeck

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REVIEW OF MONITORING TECHNOLOGIES USED IN HYBRID PHOTOVOLTAIC SYSTEMS by TEODOR POP, RADU-DUMITRU PENTIUC, VISARION-CATALIN IFRIM, CIPRIAN BEJENAR, PAVEL ATANASOAE

Subjects: “…internet of things, monitoring, photovoltaic, hybrid systems, solar, wind, IoT.…”
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Interstellar Pickup Ion Observations to 60 au by D. J. McComas, B. L. Shrestha, G. Livadiotis, J. R. Szalay, E. J. Zirnstein, H. A. Elliott, P. C. Brandt, A. R. Poppe, K. N. Singer, A. Stern, A. Verbiscer, the New Horizons Heliophysics Team

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An Overview of Solar Orbiter Observations of Interplanetary Shocks in Solar Cycle 25 by Domenico Trotta, Andrew Dimmock, Heli Hietala, Xochitl Blanco-Cano, Timothy S. Horbury, Rami Vainio, Nina Dresing, Immanuel Christopher Jebaraj, Francisco Espinosa Lara, Raúl Gómez-Herrero, Javier Rodriguez-Pacheco, Yulia Kartavykh, David Lario, Jan Gieseler, Miho Janvier, Milan Maksimovic, Nasrin Talebpour Sheshvan, Christopher J. Owen, Emilia K. J. Kilpua, Robert F. Wimmer-Schweingruber

“…We characterize energetic particle responses to the passage of IP shocks at different energies, often revealing complex features arising from the interaction between IP shocks and preexisting fluctuations, including solar wind structures being processed upon shock crossing. …”
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