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Previously unreported optical emissions generated during ionospheric heating

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Previously unreported optical emissions generated during ionospheric heating. / Mutiso, C.K.; Hughes, J.M.; Sivjee, G.G.; Pedersen, T.; Gustavsson, B.; Kosch, M.J.

In: Geophysical Research Letters, Vol. 35, No. L14103, 19.07.2008, p. 1-6.

Research output: Contribution to journalJournal articlepeer-review

Harvard

Mutiso, CK, Hughes, JM, Sivjee, GG, Pedersen, T, Gustavsson, B & Kosch, MJ 2008, 'Previously unreported optical emissions generated during ionospheric heating', Geophysical Research Letters, vol. 35, no. L14103, pp. 1-6. https://doi.org/10.1029/2008GL034563

APA

Mutiso, C. K., Hughes, J. M., Sivjee, G. G., Pedersen, T., Gustavsson, B., & Kosch, M. J. (2008). Previously unreported optical emissions generated during ionospheric heating. Geophysical Research Letters, 35(L14103), 1-6. https://doi.org/10.1029/2008GL034563

Vancouver

Mutiso CK, Hughes JM, Sivjee GG, Pedersen T, Gustavsson B, Kosch MJ. Previously unreported optical emissions generated during ionospheric heating. Geophysical Research Letters. 2008 Jul 19;35(L14103):1-6. https://doi.org/10.1029/2008GL034563

Author

Mutiso, C.K. ; Hughes, J.M. ; Sivjee, G.G. ; Pedersen, T. ; Gustavsson, B. ; Kosch, M.J. / Previously unreported optical emissions generated during ionospheric heating. In: Geophysical Research Letters. 2008 ; Vol. 35, No. L14103. pp. 1-6.

Bibtex

@article{e628e07db9f345199900a311f5838cdf,
title = "Previously unreported optical emissions generated during ionospheric heating",
abstract = "Several radio-induced optical emissions were generated during an ionospheric heating experiment performed at the High Power Auroral Stimulation (HIPAS) facility near Two Rivers, Alaska. The O+ 732–733 nm and O(3 D o) 799.0 nm emissions, previously unreported from ionospheric heating experiments, were detected, in addition to the already documented O(3 P) 844.6 nm and O(5 P) 777.4 nm emissions. Maximum emission intensity was observed in the magnetic zenith, when the heater was transmitting continuous wave O-mode, at a frequency of 2.85 MHz. A modified Czerny-Turner grating spectrometer was used to acquire high resolution optical spectra of the induced emissions, which were synchronized to the heater duty cycle. Candidate mechanisms for the production of the radio-induced emissions, which occurred before the “double resonance” condition, are presented.",
keywords = "heating DCS-publications-id, art-1028, DCS-publications-credits, iono, DCS-publications-personnel-id, 193, 7",
author = "C.K. Mutiso and J.M. Hughes and G.G. Sivjee and T. Pedersen and B. Gustavsson and M.J. Kosch",
note = "Copyright (2008) American Geophysical Union. Further reproduction or electronic distribution is not permitted.",
year = "2008",
month = jul,
day = "19",
doi = "10.1029/2008GL034563",
language = "English",
volume = "35",
pages = "1--6",
journal = "Geophysical Research Letters",
issn = "0094-8276",
publisher = "John Wiley & Sons, Ltd",
number = "L14103",

}

RIS

TY - JOUR

T1 - Previously unreported optical emissions generated during ionospheric heating

AU - Mutiso, C.K.

AU - Hughes, J.M.

AU - Sivjee, G.G.

AU - Pedersen, T.

AU - Gustavsson, B.

AU - Kosch, M.J.

N1 - Copyright (2008) American Geophysical Union. Further reproduction or electronic distribution is not permitted.

PY - 2008/7/19

Y1 - 2008/7/19

N2 - Several radio-induced optical emissions were generated during an ionospheric heating experiment performed at the High Power Auroral Stimulation (HIPAS) facility near Two Rivers, Alaska. The O+ 732–733 nm and O(3 D o) 799.0 nm emissions, previously unreported from ionospheric heating experiments, were detected, in addition to the already documented O(3 P) 844.6 nm and O(5 P) 777.4 nm emissions. Maximum emission intensity was observed in the magnetic zenith, when the heater was transmitting continuous wave O-mode, at a frequency of 2.85 MHz. A modified Czerny-Turner grating spectrometer was used to acquire high resolution optical spectra of the induced emissions, which were synchronized to the heater duty cycle. Candidate mechanisms for the production of the radio-induced emissions, which occurred before the “double resonance” condition, are presented.

AB - Several radio-induced optical emissions were generated during an ionospheric heating experiment performed at the High Power Auroral Stimulation (HIPAS) facility near Two Rivers, Alaska. The O+ 732–733 nm and O(3 D o) 799.0 nm emissions, previously unreported from ionospheric heating experiments, were detected, in addition to the already documented O(3 P) 844.6 nm and O(5 P) 777.4 nm emissions. Maximum emission intensity was observed in the magnetic zenith, when the heater was transmitting continuous wave O-mode, at a frequency of 2.85 MHz. A modified Czerny-Turner grating spectrometer was used to acquire high resolution optical spectra of the induced emissions, which were synchronized to the heater duty cycle. Candidate mechanisms for the production of the radio-induced emissions, which occurred before the “double resonance” condition, are presented.

KW - heating DCS-publications-id

KW - art-1028

KW - DCS-publications-credits

KW - iono

KW - DCS-publications-personnel-id

KW - 193

KW - 7

U2 - 10.1029/2008GL034563

DO - 10.1029/2008GL034563

M3 - Journal article

VL - 35

SP - 1

EP - 6

JO - Geophysical Research Letters

JF - Geophysical Research Letters

SN - 0094-8276

IS - L14103

ER -