The Naval Research Laboratory (NRL) Sami2 is Another Model of the Ionosphere (SAMI2) and Sami3 is Also a Model of the Ionosphere (SAMI3) ionosphere/plasmasphere codes have shown that thermosphere composition and winds significantly affect H+ outflows from the topside ionosphere. In particular, O density inhibits upward diffusion of O+ from the ionosphere F layer, especially during solar maximum conditions. In addition, winds affect the quiet-time latitudinal extent of the F layer, affecting densities at mid-to-high latitudes that are the source of plasmasphere refilling outflows. Evidence for these effects is reviewed and prospects for forecasting these outflows are explored. Open questions for future research are highlighted
The paper discusses how variations in the pattern of convective plasma flows should beincluded in se...
International audienceRecent observations have quantified the auroral wind O+ outflow in response to...
The entire solar system including Earth is enveloped in a region of space where the Sun’s magnetic f...
The Naval Research Laboratory (NRL) Sami3 is Also a Model of the Ionosphere (SAMI3) ionosphere/plasm...
The NRL SAMI3 ionosphere/plasmasphere code[1] has shown that the plasmasphere undergoes diurnal osci...
The Naval Research Laboratory SAMI3 (Sami3 is Also a Model of the Ionosphere) and the RAM‐CPL (Ring ...
Abstraet--A method for quantifying diffusive flows of O + ions in the topside ionosphere from satell...
The thermosphere and ionosphere are two overlapping regions of the atmosphere that are tightly coupl...
High latitude observations of thermal ion outflows, traditionally known as the "polar wind", and hea...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95297/1/jgra19861.pd
The outflow of ions at high latitudes is one mechanism thought to populate the magnetosphere with io...
Since the detection of O^+ ions by satellites in the 1970s it has been known that the ionosphere is ...
Models of ion flow in the topside ionosphere were developed. These models took both H(+) and O(+) in...
Recent studies suggest that the hydrogen (H) density in the exosphere and geocorona might differ fro...
Since the pioneering observation of Shelley et al. shortly before the first Yosemite space physics m...
The paper discusses how variations in the pattern of convective plasma flows should beincluded in se...
International audienceRecent observations have quantified the auroral wind O+ outflow in response to...
The entire solar system including Earth is enveloped in a region of space where the Sun’s magnetic f...
The Naval Research Laboratory (NRL) Sami3 is Also a Model of the Ionosphere (SAMI3) ionosphere/plasm...
The NRL SAMI3 ionosphere/plasmasphere code[1] has shown that the plasmasphere undergoes diurnal osci...
The Naval Research Laboratory SAMI3 (Sami3 is Also a Model of the Ionosphere) and the RAM‐CPL (Ring ...
Abstraet--A method for quantifying diffusive flows of O + ions in the topside ionosphere from satell...
The thermosphere and ionosphere are two overlapping regions of the atmosphere that are tightly coupl...
High latitude observations of thermal ion outflows, traditionally known as the "polar wind", and hea...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95297/1/jgra19861.pd
The outflow of ions at high latitudes is one mechanism thought to populate the magnetosphere with io...
Since the detection of O^+ ions by satellites in the 1970s it has been known that the ionosphere is ...
Models of ion flow in the topside ionosphere were developed. These models took both H(+) and O(+) in...
Recent studies suggest that the hydrogen (H) density in the exosphere and geocorona might differ fro...
Since the pioneering observation of Shelley et al. shortly before the first Yosemite space physics m...
The paper discusses how variations in the pattern of convective plasma flows should beincluded in se...
International audienceRecent observations have quantified the auroral wind O+ outflow in response to...
The entire solar system including Earth is enveloped in a region of space where the Sun’s magnetic f...