Statistical Analysis of the Warm Plasma Cloak in the Dayside Magnetosphere: 9 Years of MMS Observations
Metadatos
Mostrar el registro completo del ítemAutor
Montagud-Camps, Víctor; Toledo-Redondo, Sergio; Goldstein, Jerry; Fuselier, Stephen A.; André, Mats; Albert, Inmaculada; Castilla, Aida; Salinas Extremera, Alfonso; Porti Durán, Jorge Andrés; Navarro, Enrique A.Editorial
Wiley
Fecha
2025-07-03Referencia bibliográfica
Montagud‐Camps, V., Toledo‐Redondo, S., Goldstein, J., Fuselier, S. A., André, M., Albert, I. F., et al. (2025). Statistical analysis of the warm plasma cloak in the dayside magnetosphere: 9 years of MMS observations. Geophysical Research Letters, 52, e2025GL116933. https://doi. org/10.1029/2025GL116933
Patrocinador
MCIN/AEI/10.13039/501100011033 - UE (Grant TED2021‐129357A‐I00); Region of Murcia- SENECA (Grant 21910/PI/22); MICIU/AEI/10.13039/501100011033 - FEDER, UE (PID2023‐147331OB‐I00)Resumen
The warm plasma cloak (WPC) is a plasma population located in the outer magnetosphere. It is
composed primarily of electrons and H+ ions with energies of tens to hundreds electronvolts and can contain
significant amounts of O+. We conduct a statistical survey of the WPC using 9 years of observations in the
dayside magnetosphere from the Magnetospheric Multiscale mission. WPC is found in 51% of the observations
and it is 1.6 times more abundant in the dawn than in the dusk sector. O+‐rich WPC is detected in 7.5% of the
observations, being 3 times more probable in the dawn sector. We find that after a peak of strong geomagnetic
activity, it takes approximately 9 hr to detect the WPC in the dayside magnetosphere.





