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Electron auroral imager (EAI) at Syowa Station, Antarctica.

ResourceID
spase://IUGONET/Instrument/NIPR/Aurora/SYO/EAI

Description

The electron auroral imager (EAI) is an all-sky imager designed to observe the electron aurora, which is emitted from atmospheric atoms/molecules excited by precipitating auroral electrons. At Syowa Station, two EAIs (EAI-1 and EAI-2) were installed during JARE52 (the 52nd Japanese Antarctic Research Expedition) and JARE53. The hardwares of EAI-1 and EAI-2 are respectively from CAI used until JARE50 and ASI-2 used until JARE52. EAI-1 and EAI-2 are equipped with interference filters with different transparent wavelengths (427.8 nm for N2+1NG and 557.7 nm for OI). Comparison between EAI-1 and EAI-2 data provides information about energy characteristics of precipitating electrons. EAI consists of an optical system, a CCD controller and a control PC. The optical system contains a fish eye lens (Fisheye-Nikkor 16mm, F2.8), a dedicated reduced-size optical system manufactured by Nikon, and a digital CCD camera (Hamamatsu C4880-21-26A). The HiPic8.4.0 software (Hamamatsu) is used for data acquisition. The exposure time and acquisition interval are respectively 7 sec and 15 sec. The acquisition time is set according to the PC's internal clock, which is adjusted to the NTP server placed at Syowa Station.

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Details

Version:2.5.0

Instrument

ResourceID
spase://IUGONET/Instrument/NIPR/Aurora/SYO/EAI
ResourceHeader
ResourceName
Electron auroral imager (EAI) at Syowa Station, Antarctica.
ReleaseDate
2013-05-14 12:00:00
Description

The electron auroral imager (EAI) is an all-sky imager designed to observe the electron aurora, which is emitted from atmospheric atoms/molecules excited by precipitating auroral electrons. At Syowa Station, two EAIs (EAI-1 and EAI-2) were installed during JARE52 (the 52nd Japanese Antarctic Research Expedition) and JARE53. The hardwares of EAI-1 and EAI-2 are respectively from CAI used until JARE50 and ASI-2 used until JARE52. EAI-1 and EAI-2 are equipped with interference filters with different transparent wavelengths (427.8 nm for N2+1NG and 557.7 nm for OI). Comparison between EAI-1 and EAI-2 data provides information about energy characteristics of precipitating electrons. EAI consists of an optical system, a CCD controller and a control PC. The optical system contains a fish eye lens (Fisheye-Nikkor 16mm, F2.8), a dedicated reduced-size optical system manufactured by Nikon, and a digital CCD camera (Hamamatsu C4880-21-26A). The HiPic8.4.0 software (Hamamatsu) is used for data acquisition. The exposure time and acquisition interval are respectively 7 sec and 15 sec. The acquisition time is set according to the PC's internal clock, which is adjusted to the NTP server placed at Syowa Station.

Contacts
RolePersonStartDateStopDateNote
1.PrincipalInvestigatorspase://IUGONET/Person/Akira.Kadokura
2.MetadataContactspase://IUGONET/Person/Yuka.Sato
InstrumentType
Imager
InvestigationName
Auroral Observation at Syowa Station
ObservatoryID