Abstract This study investigates the contribution of energetic (E >30 keV) particle precipitation during a pulsating aurora event over Kilpisjärvi (L = 6.2) on 26 February 2014. It is based on the comparison of auroral blue-line emission (427.8 nm) data from an all-sky camera and cosmic noise absorption (CNA) data obtained from a multibeam experiment of the Kilpisjärvi Atmospheric Imaging Receiver Array (KAIRA) riometer. The data sets are compared for three KAIRA beams close to magnetic zenith. Results show a clear correlation between the measured CNA and the auroral blue-line emission during the event, for each beam. In addition, individual pulsations are observed for the first time in the cosmic noise absorption data measured by KAIRA ...
We study here energetic-electron (E > 30 keV) precipitation using cosmic noise absorption (CNA) duri...
Abstract Pulsating auroras (PsAs) are low‐intensity diffuse aurora, which switch on and off with a ...
In this study, we report observations made by filtered (557.7 and 630.0 nm) All-Sky Imagers located ...
This study investigates the contribution of energetic (E > 30 keV) particle precipitation during ...
Pulsating aurora (PsA) is a diffuse type of aurora with different structures switching on and off wi...
Abstract This study focused on a pulsating aurora event associated with aurora morphological change...
18th EISCAT symposiumSession E4: Aurora and airglowMay 30 (Tue), National Institute for Japanese Lan...
The Tenth Symposium on Polar Science/Ordinary sessions: [OS] Space and upper atmospheric sciences, W...
Pulsating aurora (PsA) is a diffuse type of aurora with different structures switching on and off wi...
Abstract During disturbed geomagnetic conditions, the energetic particles in the inner magnetospher...
Motivated by recent event studies and modeling efforts on pulsating aurora, which conclude that the ...
Abstract Motivated by recent event studies and modeling efforts on pulsating aurora, which conclude...
Pulsating auroras (PsAs) are low‐intensity diffuse aurora, which switch on and off with a quasiperio...
Pulsating aurora (PsA) is a diffuse type of aurora with different structures switching on and off ...
Pulsating auroras (PsAs) are low‐intensity diffuse aurora, which switch on and off with a quasiperio...
We study here energetic-electron (E > 30 keV) precipitation using cosmic noise absorption (CNA) duri...
Abstract Pulsating auroras (PsAs) are low‐intensity diffuse aurora, which switch on and off with a ...
In this study, we report observations made by filtered (557.7 and 630.0 nm) All-Sky Imagers located ...
This study investigates the contribution of energetic (E > 30 keV) particle precipitation during ...
Pulsating aurora (PsA) is a diffuse type of aurora with different structures switching on and off wi...
Abstract This study focused on a pulsating aurora event associated with aurora morphological change...
18th EISCAT symposiumSession E4: Aurora and airglowMay 30 (Tue), National Institute for Japanese Lan...
The Tenth Symposium on Polar Science/Ordinary sessions: [OS] Space and upper atmospheric sciences, W...
Pulsating aurora (PsA) is a diffuse type of aurora with different structures switching on and off wi...
Abstract During disturbed geomagnetic conditions, the energetic particles in the inner magnetospher...
Motivated by recent event studies and modeling efforts on pulsating aurora, which conclude that the ...
Abstract Motivated by recent event studies and modeling efforts on pulsating aurora, which conclude...
Pulsating auroras (PsAs) are low‐intensity diffuse aurora, which switch on and off with a quasiperio...
Pulsating aurora (PsA) is a diffuse type of aurora with different structures switching on and off ...
Pulsating auroras (PsAs) are low‐intensity diffuse aurora, which switch on and off with a quasiperio...
We study here energetic-electron (E > 30 keV) precipitation using cosmic noise absorption (CNA) duri...
Abstract Pulsating auroras (PsAs) are low‐intensity diffuse aurora, which switch on and off with a ...
In this study, we report observations made by filtered (557.7 and 630.0 nm) All-Sky Imagers located ...