Results 151 to 160 of about 74,585 (251)

Power Density Dissipated by Field‐Aligned Currents in the Topside Ionosphere Derived From Swarm‐A Observations

Journal of Geophysical Research: Space Physics, Volume 130, Issue 11, November 2025.
Abstract Magnetosphere‐ionosphere (MI) coupling is mainly achieved by field‐aligned currents (FACs) that inject energy and momentum into the high‐latitude ionosphere. A fraction of this energy is locally dissipated and converted into kinetic energy of the ionospheric plasma.
F. Giannattasio, S. Mestici, A. Pignalberi, P. De Michelis, R. Tozzi, T. Alberti, M. Pezzopane, I. Coco, G. Consolini   +8 more
wiley   +1 more source

Gamma ray astronomy with IceCube [PDF]

, 2003
F. Halzen, Dan Hooper
openalex   +1 more source

Correlation Patterns of Muon Flux With Vertical Atmospheric Profiles: Insights From Monte Carlo Simulations

Journal of Geophysical Research: Space Physics, Volume 130, Issue 11, November 2025.
Abstract The production, attenuation, and absorption of secondary cosmic rays (SCR) are influenced by atmospheric parameters such as air pressure and temperature. To reliably correlate SCR flux measurements with atmospheric ionization driven by energetic particle precipitation, these dependencies must be quantified.
A. Al‐Qaaod, V. Pierrard, A. Winant, U. Stolzenberg, I. Ambrozova, M. Sommer, J. Slegl, J. Solc, A. Gkikoudi, A. G. Georgakilas, A. Papayannis, F. S. Krasniqi   +11 more
wiley   +1 more source

Multi‐Platform Observations of the Radial Penetration of Substorm Injected Electrons and Subsequent Slot‐Filling Event

Journal of Geophysical Research: Space Physics, Volume 130, Issue 11, November 2025.
Abstract On 15 February 2018 a co‐rotating interaction region (CIR) from an equatorial coronal hole reached the Earth. The CIR initiated a moderate and slowly intensifying geomagnetic storm, which began with a large and strong substorm injection.
Geoffrey D. Reeves, Jean‐Francois Ripoll, Lauren W. Blum, Christopher M. Cully, Christopher A. Colpitts, Mélanie Cosmides, Sadie S. Elliot, Reihaneh Ghaffari, Ashley D. Greeley, Richard B. Horne, Keisuke Hosokawa, Allison N. Jaynes, Yoshi Kasahara, Satoshi Kasahara, Kunihiro Keika, Satoshi Kurita, David M. Malaspina, Adam T. Michael, Robyn M. Millan, Takefumi Mitani, Yoshizumi Miyoshi, Viviane Pierrard, Drew L. Turner, Hilde N. Nesse, Aleksandr Y. Ukhorskiy, Maria E. Usanova, Maria Voskresenskaya, Shoichiro Yokota   +27 more
wiley   +1 more source

The Impact of a Long‐Lived Basal Magma Ocean on the Thermochemical Evolution of Mars

Journal of Geophysical Research: Planets, Volume 130, Issue 11, November 2025.
Abstract A basal magma ocean (BMO) has been suggested to form as a consequence of cumulate overturn following crystallization of an initial global magma ocean. As a consequence of enrichment in iron and heat‐producing elements (HPE), the BMO stabilizes gravitationally at the base of the planetary mantle, affecting the efficiency of mantle convection ...
Kar Wai Cheng, Maxim D. Ballmer, Paul J. Tackley, Amir Khan   +3 more
wiley   +1 more source

Measurement of correlated charge noise in superconducting qubits at an underground facility. [PDF]

Nat Commun
Bratrud G, Lewis S, Anyang K, Colón Cesaní A, Dyson T, Magoon H, Sabhari D, Spahn G, Wagner G, Gualtieri R, Kurinsky NA, Linehan R, McDermott R, Sussman S, Temples DJ, Uemura S, Bathurst C, Cancelo G, Chen R, Chou A, Hernandez I, Hollister M, Hsu L, James C, Kennard K, Khatiwada R, Lukens P, Novati V, Raha N, Ray S, Ren R, Rodriguez A, Schmidt B, Stifter K, Yu J, Baxter D, Figueroa-Feliciano E, Bowring D.   +37 more
europepmc   +1 more source

On the Origins of Mercury's Sodium Exospheric Cold Poles Enhancement: A Multiscale Exosphere Global Model

Journal of Geophysical Research: Planets, Volume 130, Issue 11, November 2025.
Abstract Mercury's exosphere is sustained by the continuous ejection of atoms from its surface, driven by solar wind, micro‐meteoroid impacts, and surface heating. Due to its 3:2 spin‐orbit resonance, some longitudes experience greater solar exposure, creating temperature variations from ∼90 to 700 K.
S. Verkercke, L. Morrissey, J. Y. Chaufray, A. Georgiou, A. Ricketts, F. Leblanc   +5 more
wiley   +1 more source

Exploring the extremes: The cosmic laboratory. [PDF]

Innovation (Camb)
Yang H, Shunxuan H, Liang G, Zhengyang L, Yongna M, Jifeng L.   +5 more
europepmc   +1 more source

R Aquarii and Gamma Ray Astronomy [PDF]

, 2018
Kenji Tanabe, Yuko Motizuki
openalex   +1 more source

Solar Radio Wide‐Band Spectroscopy and Imaging Facilities of the Chinese Meridian Project Phase II

Space Weather, Volume 23, Issue 11, November 2025.
Abstract Solar eruptions, including flares and coronal mass ejections, are the most energetic phenomena in the solar system. These explosive events accelerate high‐energy particles and generate electromagnetic radiation from radio to gamma‐ray wavelengths, producing heliospheric disturbances and acting as primary drivers of space weather hazards.
Yihua Yan, Wei Wang, Linjie Chen, Jin Fan, Yao Chen, Shuwang Chang, Fabao Yan, Lihong Geng, Sha Li, Cang Su, Zhijun Chen, Chengming Tan, Bing Wang, Guang Lu, Chuanyang Li, Zhichao Zhou, Fei Liu, Suli Ma, Jun Cheng, Jing Du   +19 more
wiley   +1 more source