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High-latitude artificial aurora using the EISCAT high-gain HF facility

Research output: Contribution to conference - Without ISBN/ISSN › Other

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High-latitude artificial aurora using the EISCAT high-gain HF facility. / Kosch, M. J.; Rietveld, M. T.; Kavanagh, A. J. et al.
2002. 29th General Assembly of the International Union of Radio Science.

Research output: Contribution to conference - Without ISBN/ISSN › Other

Harvard

Kosch, MJ, Rietveld, MT, Kavanagh, AJ, Jussila, J, Isham, B, Kaila, K, McCrea, IW, Senior, A, Holma, H, Honary, F & Hagfors, T 2002, 'High-latitude artificial aurora using the EISCAT high-gain HF facility', 29th General Assembly of the International Union of Radio Science, 1/01/00.

APA

Kosch, M. J., Rietveld, M. T., Kavanagh, A. J., Jussila, J., Isham, B., Kaila, K., McCrea, I. W., Senior, A., Holma, H., Honary, F., & Hagfors, T. (2002). High-latitude artificial aurora using the EISCAT high-gain HF facility. 29th General Assembly of the International Union of Radio Science.

Vancouver

Kosch MJ, Rietveld MT, Kavanagh AJ, Jussila J, Isham B, Kaila K et al.. High-latitude artificial aurora using the EISCAT high-gain HF facility. 2002. 29th General Assembly of the International Union of Radio Science.

Author

Kosch, M. J. ; Rietveld, M. T. ; Kavanagh, A. J. et al. / High-latitude artificial aurora using the EISCAT high-gain HF facility. 29th General Assembly of the International Union of Radio Science.4 p.

Bibtex

@conference{adcd8c7daca54834997240d5efcc331e,
title = "High-latitude artificial aurora using the EISCAT high-gain HF facility",
abstract = "The EISCAT high-frequency (HF) transmitter facility at Ramfjord, Norway, has been used to accelerate F-region electrons sufficiently to excite the oxygen atoms and nitrogen molecules, resulting in optical emissions at 630, 557.7 and 427.8 nm. During O-mode transmissions at 5.423 MHz, using 630 MW effective radiated power, in the hours after sunset on 12 November 2001 several new observations were made, including: (1) The first high-latitude observation of an HF induced optical emission at 427.8 nm and (2) Optical rings being formed at HF on followed by their collapse into a central blob. Both discoveries remain unexplained with current theories.",
keywords = "asc, heating DCS-publications-id, inproc-265, DCS-publications-credits, dasi, iono-fa, scasi, DCS-publications-personnel-id, 7, 9, 51, 5, 56",
author = "Kosch, {M. J.} and Rietveld, {M. T.} and Kavanagh, {A. J.} and J. Jussila and B. Isham and K. Kaila and McCrea, {I. W.} and A. Senior and H. Holma and F. Honary and T. Hagfors",
note = "P1321; 29th General Assembly of the International Union of Radio Science ; Conference date: 01-01-1900",
year = "2002",
month = aug,
language = "English",

}

RIS

TY - CONF

T1 - High-latitude artificial aurora using the EISCAT high-gain HF facility

AU - Kosch, M. J.

AU - Rietveld, M. T.

AU - Kavanagh, A. J.

AU - Jussila, J.

AU - Isham, B.

AU - Kaila, K.

AU - McCrea, I. W.

AU - Senior, A.

AU - Holma, H.

AU - Honary, F.

AU - Hagfors, T.

N1 - P1321

PY - 2002/8

Y1 - 2002/8

N2 - The EISCAT high-frequency (HF) transmitter facility at Ramfjord, Norway, has been used to accelerate F-region electrons sufficiently to excite the oxygen atoms and nitrogen molecules, resulting in optical emissions at 630, 557.7 and 427.8 nm. During O-mode transmissions at 5.423 MHz, using 630 MW effective radiated power, in the hours after sunset on 12 November 2001 several new observations were made, including: (1) The first high-latitude observation of an HF induced optical emission at 427.8 nm and (2) Optical rings being formed at HF on followed by their collapse into a central blob. Both discoveries remain unexplained with current theories.

AB - The EISCAT high-frequency (HF) transmitter facility at Ramfjord, Norway, has been used to accelerate F-region electrons sufficiently to excite the oxygen atoms and nitrogen molecules, resulting in optical emissions at 630, 557.7 and 427.8 nm. During O-mode transmissions at 5.423 MHz, using 630 MW effective radiated power, in the hours after sunset on 12 November 2001 several new observations were made, including: (1) The first high-latitude observation of an HF induced optical emission at 427.8 nm and (2) Optical rings being formed at HF on followed by their collapse into a central blob. Both discoveries remain unexplained with current theories.

KW - asc

KW - heating DCS-publications-id

KW - inproc-265

KW - DCS-publications-credits

KW - dasi

KW - iono-fa

KW - scasi

KW - DCS-publications-personnel-id

KW - 7

KW - 9

KW - 51

KW - 5

KW - 56

M3 - Other

T2 - 29th General Assembly of the International Union of Radio Science

Y2 - 1 January 1900

ER -