Physics of the Earth and Planetary InteriorsAnderson, O. L., and D. G. Isaak (2002), Another look at the core density deficit of Earth's outer core, Phys. Earth Planet. Inter., 131, 19-27, doi:10.1016/S0031-9201
yielded no further signals. However, due to the shallow transit depth,Kepler’s pixel scale of 4”, and the size of the photometric aperture, contamination from a nearby star at 13.6” (EPIC 201595004) had not been sufficiently ruled out, leaving room for doubt as to the true origin and ...
The warm plasma cloak is a source of magnetospheric plasma that contain significant O +. When the O + density in the magnetosphere near the magnetopause is >0.2 cm-3 and the H + density is 20% due to mass-loading only about 2% to 4% of the time. However, during geomagnetic storms,...
outer radiation beltwave-particle interactionsaccelerationlosstransport[1] We report on internal, magnetospheric processes related to markedly different storm-time responses of phase space density (PSD) in invariant coordinates corresponding to equatorially mirroring, relativistic electrons in Earth's outer ...
and neutral densities are crucial to extract ion distributions through inversion of the acquired images. This work develops a technique to estimate the Earth's outer exospheric density distributions using far-ultraviolet wide-field data acquired by the Lyman-Alpha Imaging Camera (LAICA) onboard the ...
An ultra-short-period super-Earth with an extremely high density and an outer companiondoi:10.1038/s41598-024-76490-yWe present the discovery and characterization of a new multi-planetary system around the Sun-like star K2-360 (EPIC201595106). K2-360 was first identified inK2photometry as the...
The surface of this solid layer, where the pressure is lowest, is composed of an extremely dense form of iron. Another important characteristic of neutron stars is the presence of very strong magnetic fields, upward of 1012 gauss (Earth’s magnetic field is 0.5 gauss), which causes the ...
Earth's outer magnetosphereits effectThe warm plasma cloak is a source of magnetospheric plasma that contain significant O~+. When the O~+ density in the magnetosphere near the magnetopause is >0.2 cm~(‐3) and the H+ density is<1.5 cm~(‐3), then O~+ dominates the magnetospheric ion...
Journal of Geophysical Research Space PhysicsTurner, D. L., X. Li, G. D. Reeves, and H. J. Singer (2010), On phase space density radial gradients of Earth's outer-belt electrons prior to sudden solar wind pressure enhancements: Results from distinctive events and a superposed epoch ...
Journal of Geophysical Research Space PhysicsTurner, D. L., X. Li, G. D. Reeves, and H. J. Singer (2010), On phase space density radial gradients of Earth's outer-belt electrons prior to sudden solar wind pressure enhancements: Results from distinctive events and a superposed epoch ...