A change in directed proton flux is noted, and study of the available spectrometer data shows a c/pi scale length for proton scattering, where the Ogo 5 JPL plasma probe density measurements have been used. This scale length is based upon the time required for scattering the protons into ...
Other articles where near-Earth object is discussed: Earth impact hazard: Objects that pose a threat: …comets in short-period orbits—together called near-Earth objects (NEOs)—and those long-period comets that make their closest approach to the Sun ins
Solar wind control of plasma number density in the near-Earth plasma sheet: three-dimensional structure [1] The plasma number density in the plasma sheet depends on the solar wind number density and the north-south component of interplanetary magnetic field (... D Nagata,S Machida,S Ohtani,....
Earth’s magnetic field was in a highly unusual state when macroscopic animals of the Ediacara Fauna diversified and thrived. Any connection between these events is tantalizing but unclear. Here, we present single crystal paleointensity data from 2054 an
density:2.34protons/cm3 more data:ACE,DSCOVR Updated: Today at 0522 UT X-ray Solar Flares 6-hr max:C12324 UT Jan10 24-hr:C92246 UTJan10 explanation|more data Updated: Today at: 0525 UT Daily Sun: 10 Jan 25 Expand:labels|no labels|Carrington ...
The prediction of a supersonic solar wind1 was first confirmed by spacecraft near Earth2,3 and later by spacecraft at heliocentric distances as small as 62 solar radii4. These missions showed that plasma accelerates as it emerges from the corona, aided b
Fig. 4. Plasma and magnetic field along the orbit of the Moon on the j × B hybrid model (red lines, from top to bottom): the density of protons (n), the total bulk speed of protons (U), the thermal pressure of protons (p = n kB T), the temperature of protons (T)...
Distribution of charged particles in near-earth space 来自 ResearchGate 喜欢 0 阅读量: 15 作者: SI Nikolskii 摘要: Topics discussed include the planetary distribution of cosmic ray intensities based on stratospheric measurements, temporal variations in cosmic ray intensity, and the vertical ...
nuclear densitynuclear forcesnuclear shapenuclear sizenuclei with mass number 150 to 189protons/ neutron drip lineneutron-rich isotopesThe properties of neutron-rich Zr isotopes up to the neutron drip line and beyond it have been investigated on the basis of the Hartree-Fock method with the Skyrme...
Within about 200 light-years of Sol the density is around 7×10-2 atoms/cm3, because Sol in inside a bubble. Elsewhere it varies from 10-4 to 106 atoms/cm3 depending upon what sort of space you are in. Remember, this was one of the problems a Bussard Ramjet was designed to solve....