TY - JOUR
T1 - Ground-based instruments of the PWING project to investigate dynamics of the inner magnetosphere at subauroral latitudes as a part of the ERG-ground coordinated observation network
AU - Shiokawa, Kazuo
AU - Katoh, Yasuo
AU - Hamaguchi, Yoshiyuki
AU - Yamamoto, Yuka
AU - Adachi, Takumi
AU - Ozaki, Mitsunori
AU - Oyama, Shin Ichiro
AU - Nosé, Masahito
AU - Nagatsuma, Tsutomu
AU - Tanaka, Yoshimasa
AU - Otsuka, Yuichi
AU - Miyoshi, Yoshizumi
AU - Kataoka, Ryuho
AU - Takagi, Yuki
AU - Takeshita, Yuhei
AU - Shinbori, Atsuki
AU - Kurita, Satoshi
AU - Hori, Tomoaki
AU - Nishitani, Nozomu
AU - Shinohara, Iku
AU - Tsuchiya, Fuminori
AU - Obana, Yuki
AU - Suzuki, Shin
AU - Takahashi, Naoko
AU - Seki, Kanako
AU - Kadokura, Akira
AU - Hosokawa, Keisuke
AU - Ogawa, Yasunobu
AU - Connors, Martin
AU - Michael Ruohoniemi, J.
AU - Engebretson, Mark
AU - Turunen, Esa
AU - Ulich, Thomas
AU - Manninen, Jyrki
AU - Raita, Tero
AU - Kero, Antti
AU - O'Ksanen, Arto
AU - Back, Marko
AU - Kauristie, Kirsti
AU - Mattanen, Jyrki
AU - Baishev, Dmitry
AU - Kurkin, Vladimir
AU - Oinats, Alexey
AU - Pashinin, Alexander
AU - Vasilyev, Roman
AU - Rakhmatulin, Ravil
AU - Bristow, William
AU - Karjala, Marty
N1 - Publisher Copyright:
© 2017 The Author(s).
PY - 2017/12/1
Y1 - 2017/12/1
N2 - The plasmas (electrons and ions) in the inner magnetosphere have wide energy ranges from electron volts to mega-electron volts (MeV). These plasmas rotate around the Earth longitudinally due to the gradient and curvature of the geomagnetic field and by the co-rotation motion with timescales from several tens of hours to less than 10 min. They interact with plasma waves at frequencies of mHz to kHz mainly in the equatorial plane of the magnetosphere, obtain energies up to MeV, and are lost into the ionosphere. In order to provide the global distribution and quantitative evaluation of the dynamical variation of these plasmas and waves in the inner magnetosphere, the PWING project (study of dynamical variation of particles and waves in the inner magnetosphere using ground-based network observations, http://www.isee.Nagoya-u.ac.jp/dimr/PWING/) has been carried out since April 2016. This paper describes the stations and instrumentation of the PWING project. We operate all-sky airglow/aurora imagers, 64-Hz sampling induction magnetometers, 40-kHz sampling loop antennas, and 64-Hz sampling riometers at eight stations at subauroral latitudes (~ 60° geomagnetic latitude) in the northern hemisphere, as well as 100-Hz sampling EMCCD cameras at three stations. These stations are distributed longitudinally in Canada, Iceland, Finland, Russia, and Alaska to obtain the longitudinal distribution of plasmas and waves in the inner magnetosphere. This PWING longitudinal network has been developed as a part of the ERG (Arase)-ground coordinated observation network. The ERG (Arase) satellite was launched on December 20, 2016, and has been in full operation since March 2017. We will combine these ground network observations with the ERG (Arase) satellite and global modeling studies. These comprehensive datasets will contribute to the investigation of dynamical variation of particles and waves in the inner magnetosphere, which is one of the most important research topics in recent space physics, and the outcome of our research will improve safe and secure use of geospace around the Earth.[Figure not available: see fulltext.]
AB - The plasmas (electrons and ions) in the inner magnetosphere have wide energy ranges from electron volts to mega-electron volts (MeV). These plasmas rotate around the Earth longitudinally due to the gradient and curvature of the geomagnetic field and by the co-rotation motion with timescales from several tens of hours to less than 10 min. They interact with plasma waves at frequencies of mHz to kHz mainly in the equatorial plane of the magnetosphere, obtain energies up to MeV, and are lost into the ionosphere. In order to provide the global distribution and quantitative evaluation of the dynamical variation of these plasmas and waves in the inner magnetosphere, the PWING project (study of dynamical variation of particles and waves in the inner magnetosphere using ground-based network observations, http://www.isee.Nagoya-u.ac.jp/dimr/PWING/) has been carried out since April 2016. This paper describes the stations and instrumentation of the PWING project. We operate all-sky airglow/aurora imagers, 64-Hz sampling induction magnetometers, 40-kHz sampling loop antennas, and 64-Hz sampling riometers at eight stations at subauroral latitudes (~ 60° geomagnetic latitude) in the northern hemisphere, as well as 100-Hz sampling EMCCD cameras at three stations. These stations are distributed longitudinally in Canada, Iceland, Finland, Russia, and Alaska to obtain the longitudinal distribution of plasmas and waves in the inner magnetosphere. This PWING longitudinal network has been developed as a part of the ERG (Arase)-ground coordinated observation network. The ERG (Arase) satellite was launched on December 20, 2016, and has been in full operation since March 2017. We will combine these ground network observations with the ERG (Arase) satellite and global modeling studies. These comprehensive datasets will contribute to the investigation of dynamical variation of particles and waves in the inner magnetosphere, which is one of the most important research topics in recent space physics, and the outcome of our research will improve safe and secure use of geospace around the Earth.[Figure not available: see fulltext.]
KW - All-sky airglow/aurora imager
KW - EMCCD camera
KW - EMIC wave
KW - Induction magnetometer
KW - Inner magnetosphere
KW - Loop antenna
KW - Magnetospheric ELF/VLF wave
KW - Radiation belts
KW - Riometer
KW - SAR arc
UR - http://www.scopus.com/inward/record.url?scp=85037062876&partnerID=8YFLogxK
U2 - 10.1186/s40623-017-0745-9
DO - 10.1186/s40623-017-0745-9
M3 - Journal Article
AN - SCOPUS:85037062876
SN - 1343-8832
VL - 69
JO - Earth, Planets and Space
JF - Earth, Planets and Space
IS - 1
M1 - 160
ER -