Rodriguez JV, Onsager TG, Mazur JE (2010) The east-west effect in solar proton flux measurements in geostationary orbit: a new GOES capability. Geo- phys Res Lett 37:L07109. doi:10.1029/2010GL042531Rodriguez, J. V., Onsager, T. G., & Mazur, J. E. (2010). The east-west effect...
The radiative flux terms (inS¯ϕ) are typically separated into short-wave and long-wave fluxes. The short-wave fluxes, also calledsolar fluxes, are separated into direct anddiffuse irradiance. Thedirect irradianceis the nonscattered flux, while the diffuse irradiance is the scattered radiative ...
[1] Electron auroral energy flux is characterized by electron hemispheric power (Hpe) estimated since 1978 from National Oceanic and Atmospheric Administration (NOAA) and Defense Meteorological Satellite Program (DMSP) satellites after the estimates were corrected for instrumental problems and adjusted to ...
(called “dark doldrums”)27. Although with vast enough wind and solar capacity it might still be possible to meet demand in all hours, the required capacity increases exponentially after a point that depends on the renewable resources of that country, and it is this geophysically-dependent poin...
The migration of the open fluxes consists of three parts: open flux areas migrating across the equator, new open flux areas generated in the low latitude and migrating poleward, and new open flux areas locally generated in the polar region. All three components contribute to the reversal of ...
However, the EUV part of the solar spectrum can also increase during a flare, which does drive a response in the ionosphere and thermosphere, although the EUV flux is not always well correlated with the X-ray flux by which the flare is categorized. Several modeling studies have been ...
Krivova NA, Balmaceda L, Solanki SK (2007) Reconstruction of solar total irradiance since 1700 from the surface magnetic flux. Astron Astrophys 467:335–346. doi:10.1051/0004-6361:20066725 Google Scholar Kudela K, Rybak J, Anatalova A, Storini M (2002) Time evolution of low-frequency perio...
The realization of a new method for investigating the geodisturbed region of the solar wind with the help of the ground-based radiotransmitting complex SURA and the Wind spacecraft is reported. We present preliminary results of the experiments on radio occultation in the range of 9 MHz during ...
Because of their speed, their largemagnetic fieldstrength, and their often long-lived and strong southward magnetic field component, many fast CMEs are highly geoeffective; that is, energy is transferred effectively between thesolar windandEarth’smagnetospherethrough the process ofmagnetic reconnection...
Correlation analysis revealed that the O~+/H~+ energy density ratio has the highest correlation coefficient with peak power of the electric field in the ... S Oimatsu,M Nosé,G Le,... - 《Journal of Geophysical Research Space Physics》 被引量: 0发表: 2020年 Ion-Scale Flux Rope Observed...