Results 41 to 50 of about 178 (93)
Abstract A polar cap patch was observed to exit the polar cap to become a blob as it entered the auroral oval on the nightside of the Earth under moderately quiet geomagnetic conditions (Kp = 3−). Auroral particle precipitation led to an increase in the electron density of the blob.
S. J. Maguire +9 more
wiley +1 more source
SAMI3 data in netCDF format (2019-Apr-15)
SAMI3 (Sami3 is Also a Model of the Ionosphere) is a seamless, three-dimensional, physics-based model of the ionosphere (Huba et al, 2008). It is based on SAMI2, a two-dimensional model of the ionosphere (Huba et al., 2000).
Huba, Joseph +2 more
core +1 more source
This study is based on observations of the atomic oxygen airglow emission at 630 nm obtained with a Fabry—Perot interferometer (FPI) of the National Heliogeophysical Complex.
Budovkina Aleksandra +3 more
doaj +1 more source
On the Seeding of Equatorial Plasma Bubbles by Longitudinal Variations in the Meridional Wind
Abstract We report results from SAMI3/WACCM‐X simulations that small‐scale (∼ ${\sim} $few 100 km) longitudinal variations in the meridional wind provide seeds to initiate equatorial plasma bubbles (EPBs). The meridional wind variations generate variations in the ion density along the magnetic field via ion‐neutral collisions.
J. D. Huba, N. Pedatella, H.‐L. Liu
wiley +1 more source
Quantification of Representation Error in the Neutral Winds and Ion Drifts Using Data Assimilation
In this work we quantify the representation error of the algorithm Estimating Model Parameters from Ionospheric Reverse Engineering (EMPIRE), which estimates global neutral winds and ion drifts given time‐varying plasma densities. SAMI3 (Sami3 is A Model
Jiahui Hu +4 more
doaj +1 more source
This study investigates the low-latitude ionospheric response over the Eastern Hemisphere during two successive geomagnetic storms on 12–13 November 2025.
Shuqiong Liu +2 more
doaj +1 more source
Abstract Two quasi‐orthogonal nighttime medium‐scale traveling ionospheric disturbances (MSTIDs) were observed by conjugate midlatitude all‐sky imagers in Sutherland (32.4° ${}^{\circ}$S, 20.8° ${}^{\circ}$E; magnetic latitude: ∼ ${\sim} $−40.9° ${}^{\circ}$) and Asiago (45.87° ${}^{\circ}$N, 11.53° ${}^{\circ}$E; magnetic latitude: ∼40.3° ${\sim} 40.3{
Zama T. Katamzi‐Joseph +8 more
wiley +1 more source
GRACE-FO radiation pressure modelling for accurate density and crosswind retrieval [PDF]
Uncertainties in radiation pressure modelling play a significant role in the thermospheric density and crosswind observations derived from the GRACE-FO accelerometer, especially during low solar activity.
Hładczuk, Natalia +9 more
core +1 more source
SAMI3 data in netCDF format (2019-Mar-15)
SAMI3 (Sami3 is Also a Model of the Ionosphere) is a seamless, three-dimensional, physics-based model of the ionosphere (Huba et al, 2008). It is based on SAMI2, a two-dimensional model of the ionosphere (Huba et al., 2000).
Huba, Joseph +2 more
core +1 more source
Abstract This study investigates the characteristics of medium scale traveling ionospheric disturbances (MSTIDs) relative amplitudes (δNe/Ne $\delta Ne/Ne$) in the ionospheric E to lower F regions, using the EISCAT VHF radar data measured from 41 daytime runs in years 2008–2024 carried out mostly between 7−13 $7-13$ UT.
Samson T. Moges +5 more
wiley +1 more source

