Home > Research > Publications & Outputs > Study of the auroral emissions and electron pre...

Electronic data

View graph of relations

Study of the auroral emissions and electron precipitation depending on the solar activity

Research output: Contribution to journalJournal article

Published

Standard

Study of the auroral emissions and electron precipitation depending on the solar activity. / Guineva, V.; Trondsen, E.; Marple, S.; Hall, C.M.; Cannon, P.; Hansen, T.L.

In: Solar-Terrestrial Physics (Russian Academy of Science), Vol. 12, No. 2, 2008, p. 224-228.

Research output: Contribution to journalJournal article

Harvard

Guineva, V, Trondsen, E, Marple, S, Hall, CM, Cannon, P & Hansen, TL 2008, 'Study of the auroral emissions and electron precipitation depending on the solar activity', Solar-Terrestrial Physics (Russian Academy of Science), vol. 12, no. 2, pp. 224-228.

APA

Guineva, V., Trondsen, E., Marple, S., Hall, C. M., Cannon, P., & Hansen, T. L. (2008). Study of the auroral emissions and electron precipitation depending on the solar activity. Solar-Terrestrial Physics (Russian Academy of Science), 12(2), 224-228.

Vancouver

Guineva V, Trondsen E, Marple S, Hall CM, Cannon P, Hansen TL. Study of the auroral emissions and electron precipitation depending on the solar activity. Solar-Terrestrial Physics (Russian Academy of Science). 2008;12(2):224-228.

Author

Guineva, V. ; Trondsen, E. ; Marple, S. ; Hall, C.M. ; Cannon, P. ; Hansen, T.L. / Study of the auroral emissions and electron precipitation depending on the solar activity. In: Solar-Terrestrial Physics (Russian Academy of Science). 2008 ; Vol. 12, No. 2. pp. 224-228.

Bibtex

@article{8521ee31c341400fb9d09f31f9006634,
title = "Study of the auroral emissions and electron precipitation depending on the solar activity",
abstract = "Simultaneous observations of the OI 5577{\AA} and 6300{\AA} emissions, the electron precipitation, the terrestrial magnetic field and the plasma parameters, and the corresponding solar wind, Interplanetary Magnetic Field and geomagnetic activity indices data have been used in order to study the Sun-Earth interactions under various conditions. Images of 5577{\AA} and 6300{\AA} emissions have been obtained from the All-Sky Imager (ASI), positioned at ARR, Andenes (69.3°N, 16.03°E). The Imaging Riometer for Ionospheric Studies (IRIS), at Kilpisj{\"a}rvi, Finland (69.05°N, 20.79°E) gave information about the precipitating electrons with energies in the range 10x100keV and deposition heights centered at about 90 km. The magnetic field components have been measured by the Andenes magnetometer (69.3°N, 16.03°E). The essential ionosphere parameters have been acquired from the measurements of the Digisonde, situated at Troms{\o} (69.6N, 19.2E). A good correlation between the spatial and temporal evolutions of the optical emissions, the precipitating electron fluxes and the terrestrial magnetic field has been observed. The response of the ionosphere to the solar and geomagnetic activity changes has been studied. The study is performed under a project, part from the ALOMAR eARI Project, EU's 6th Framework Programme, Andenes, Norway.",
keywords = "riometer, magnetometer DCS-publications-id, art-951, DCS-publications-credits, iono, iris, DCS-publications-personnel-id, 4",
author = "V. Guineva and E. Trondsen and S. Marple and C.M. Hall and P. Cannon and T.L. Hansen",
note = "In English",
year = "2008",
language = "English",
volume = "12",
pages = "224--228",
journal = "Solar-Terrestrial Physics (Russian Academy of Science)",
number = "2",

}

RIS

TY - JOUR

T1 - Study of the auroral emissions and electron precipitation depending on the solar activity

AU - Guineva, V.

AU - Trondsen, E.

AU - Marple, S.

AU - Hall, C.M.

AU - Cannon, P.

AU - Hansen, T.L.

N1 - In English

PY - 2008

Y1 - 2008

N2 - Simultaneous observations of the OI 5577Å and 6300Å emissions, the electron precipitation, the terrestrial magnetic field and the plasma parameters, and the corresponding solar wind, Interplanetary Magnetic Field and geomagnetic activity indices data have been used in order to study the Sun-Earth interactions under various conditions. Images of 5577Å and 6300Å emissions have been obtained from the All-Sky Imager (ASI), positioned at ARR, Andenes (69.3°N, 16.03°E). The Imaging Riometer for Ionospheric Studies (IRIS), at Kilpisjärvi, Finland (69.05°N, 20.79°E) gave information about the precipitating electrons with energies in the range 10x100keV and deposition heights centered at about 90 km. The magnetic field components have been measured by the Andenes magnetometer (69.3°N, 16.03°E). The essential ionosphere parameters have been acquired from the measurements of the Digisonde, situated at Tromsø (69.6N, 19.2E). A good correlation between the spatial and temporal evolutions of the optical emissions, the precipitating electron fluxes and the terrestrial magnetic field has been observed. The response of the ionosphere to the solar and geomagnetic activity changes has been studied. The study is performed under a project, part from the ALOMAR eARI Project, EU's 6th Framework Programme, Andenes, Norway.

AB - Simultaneous observations of the OI 5577Å and 6300Å emissions, the electron precipitation, the terrestrial magnetic field and the plasma parameters, and the corresponding solar wind, Interplanetary Magnetic Field and geomagnetic activity indices data have been used in order to study the Sun-Earth interactions under various conditions. Images of 5577Å and 6300Å emissions have been obtained from the All-Sky Imager (ASI), positioned at ARR, Andenes (69.3°N, 16.03°E). The Imaging Riometer for Ionospheric Studies (IRIS), at Kilpisjärvi, Finland (69.05°N, 20.79°E) gave information about the precipitating electrons with energies in the range 10x100keV and deposition heights centered at about 90 km. The magnetic field components have been measured by the Andenes magnetometer (69.3°N, 16.03°E). The essential ionosphere parameters have been acquired from the measurements of the Digisonde, situated at Tromsø (69.6N, 19.2E). A good correlation between the spatial and temporal evolutions of the optical emissions, the precipitating electron fluxes and the terrestrial magnetic field has been observed. The response of the ionosphere to the solar and geomagnetic activity changes has been studied. The study is performed under a project, part from the ALOMAR eARI Project, EU's 6th Framework Programme, Andenes, Norway.

KW - riometer

KW - magnetometer DCS-publications-id

KW - art-951

KW - DCS-publications-credits

KW - iono

KW - iris

KW - DCS-publications-personnel-id

KW - 4

M3 - Journal article

VL - 12

SP - 224

EP - 228

JO - Solar-Terrestrial Physics (Russian Academy of Science)

JF - Solar-Terrestrial Physics (Russian Academy of Science)

IS - 2

ER -