A Long‐Lived Planetesimal Dynamo Powered by Core Crystallization by Clara Maurel, James F. J. Bryson, Jay Shah, Rajesh V. Chopdekar, Linda T. Elkins‐Tanton, Carol A. Raymond, Benjamin P. Weiss

“…We find that the core of the IIE parent body generated a dynamo, likely powered by core crystallization, starting before 78 ± 13 Ma after solar system formation and lasting at least 80 Ma. …”
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Algorithm for designing load-bearing structures of a multi-storey building using the visual programming environment DYNAMO STUDIO by T. A. Yurosheva, A. V. Kalinichenko, V. G. Makiev

“…The article is devoted to the actual problem of minimizing the designer's work time using Dynamo Studio as a powerful tool for automating design tasks.Method. …”
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Dynamic regimes in planetary cores: $\tau $–$\ell $ diagrams by Nataf, Henri-Claude, Schaeffer, Nathanaël

“…We highlight the role of the available convective power in controlling this dynamics, together with the relevant force balance, for which we derive a very telling $\tau $–$\ell $ translation. …”
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The Internal Structure and Dynamics of Jupiter Unveiled by a High‐Resolution Magnetic Field and Secular Variation Model by S. Sharan, B. Langlais, H. Amit, E. Thébault, M. Pinceloup, O. Verhoeven

“…We use properties of the power spectrum of the static field to infer the upper boundary of the dynamo convective region at 0.830 ± 0.022 Jupiter radius. …”
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Linear perturbations of the Bloch type of space-periodic magnetohydrodynamic steady states. III. Asymptotics of branching by Chertovskih R, Zheligovsky V

Subjects: “…Power series expansion…”
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Synthesizing auroral substorm processes based on magnetosphere-ionosphere electric currents by Syun-Ichi Akasofu, A. T. Y. Lui, Lou-Chuang Lee

“…When the solar wind-magnetosphere dynamo power starts to increase above 1011 W, the current cannot flow in a quiet (low conductive) ionosphere, so that the current is initially blocked, causing energy accumulation of about 1016 J and inflation of the inner magnetosphere during the growth phase. …”
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Electrical Conductivity of Dense MgSiO3 Melt Under Static Compression by Yoshiyuki Okuda, Kei Hirose, Kenji Ohta, Saori Kawaguchi‐Imada, Kenta Oka

“…Nevertheless, the strong temperature dependence of the ionic conductivity found in this study suggests that super‐Earths’ hotter magma ocean with larger‐scale convection could power a dynamo that drives magnetic fields, which plays key roles in sustaining planetary surface environments.…”
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A user-friendly NoSQL framework for managing agricultural field trial data by Steven H. Wu, Tristan A. Mueller

“…The backend database for DynamoField is powered by Amazon Web Services DynamoDB, a NoSQL database, and DynamoField also provides a front-end interactive web interface. …”
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A 22 yr Cycle of the Network Topology of Solar Active Regions by Eduardo Flández, Alejandro Zamorano, Víctor Muñoz

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A Multi-Input Single-Ended Primary Inductor Converter (SEPIC): Performance Analysis for Hybrid Sources of Renewable Energy by Nayeem Ahmed, Afrid U. Araf, Sheikh M. A. Rakeen

“…The renewable energy sources (RES) that are used to build the prototype are Photovoltaic Panel and Bi-Cycle Dynamo. Due to the limitations of the PV Panels to generate power during the night and gloomy weather, the Bi-Cycle dynamo works as the backup power source. …”
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Magnetic Reconnection: An Alternative Explanation of Radio Emission in Galaxy Clusters by Subham Ghosh, Pallavi Bhat

“…We show that the resulting electron energy spectra have power-law indices that are consistent with those inferred from observations. …”
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The Cross‐Over From Viscous to Inertial Lengthscales in Rapidly‐Rotating Convection by C. Guervilly, E. Dormy

“…Abstract Convection is the main heat transport mechanism in the Earth's liquid core and is thought to power the dynamo that generates the geomagnetic field. …”
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Revisiting the Activity–Rotation Relation for Evolved Stars by Henggeng Han, Song Wang, Xue Li, Chuanjie Zheng, Jifeng Liu

“…Our results show that evolved stars and dwarfs obey a similar power law in the unsaturated region of the activity–rotation relation, indicating a common dynamo mechanism in both giants and dwarfs. …”
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A short period and compressional Pc3 magnetic pulsation possibly caused by a lamb wave and plasmaspheric cavity resonance by T. Iyemori, Y. Yokoyama, T. Aoyama

“…The difference between this and other usual compressional Pc3 pulsations observed in low- or mid-latitudes is its spectral structure. The power spectral density (PSD) usually peaks at the periods between 20 and 30 s, but in this event observed on the dayside orbit around the time when the Lamb wave passed under the Swarm orbit, the PSD peaks below 20 s and is small in the periods longer than 20 s. …”
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Ionospheric Response to the Extreme 2024 Mother's Day Geomagnetic Storm Over the Latin American Sector by C. S. Carmo, L. Dai, C. M. Wrasse, D. Barros, H. Takahashi, C. A. O. B. Figueiredo, C. Wang, H. Li, Z. Liu

“…Abstract Geomagnetic storms affect Earth in various severe ways, including damaging satellites, disrupting power grids, and inducing prompt penetration electric fields (PPEF) through Joule heating in the auroral region. …”
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Observations of 1/f Noise at Mercury’s Solar Wind Using MESSENGER Data by Rayta A. Pradata, Sohom Roy, William H. Matthaeus, Jiaming Wang, Rohit Chhiber, Francesco Pecora, Yan Yang

“…Low-frequency signals having a band-limited scale-invariant power, or “1/ f ” noise, have been detected in the interplanetary medium and inferred from coronal and photospheric observations. …”
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Searching for Stellar Activity Cycles Using Flares: The Short- and Long-timescale Activity Variations of TIC-272272592 by Tobin M. Wainer, James R. A. Davenport, Guadalupe Tovar Mendoza, Adina D. Feinstein, Tom Wagg

“…This quantifiable approach to describing flare-rate variation is a powerful new method for measuring the months-to-years changes in surface magnetic activity, and provides important constraints on activity cycles and dynamo models for low-mass stars.…”
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GraphVelo allows for accurate inference of multimodal velocities and molecular mechanisms for single cells by Yuhao Chen, Yan Zhang, Jiaqi Gan, Ke Ni, Ming Chen, Ivet Bahar, Jianhua Xing

“…Abstract RNA velocities and generalizations emerge as powerful approaches for extracting time-resolved information from high-throughput snapshot single-cell data. …”
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Ab Initio Study of the Conductivities of B2 FeSi Under Core‐Mantle Boundary Conditions by Yonghui Huang, Yunguo Li, Dario Alfè, Monica Pozzo, Huaiwei Ni

“…The exceptionally high conductivities of B2 FeSi would enhance heat transfer and elevate temperatures within ULVZs, if B2 FeSi is present, thereby promoting the core dynamo and powering hotspots, consistent with seismic observations of ULVZs.…”
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A Long-duration Superflare on the K Giant HD 251108 by Hans Moritz Günther, Dheeraj Pasham, Alexander Binks, Stefan Czesla, Teruaki Enoto, Michael Fausnaugh, Franz-Josef Hambsch, Shun Inoue, Hiroyuki Maehara, Yuta Notsu, Jan Robrade, J. H. M. M. Schmitt, P. C. Schneider

“…Large outbursts in these emission features can set limits on the magnetic field strength and thus constrain the mechanism of the underlying dynamo. HD 251108 is a Li-rich active K-type giant. …”
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