First estimates of volume distribution of HF-pump enhanced emissions at 6300 and 5577 angstrom: a comparison between observations and theory

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First estimates of volume distribution of HF-pump enhanced emissions at 6300 and 5577 angstrom: a comparison between observations and theory. / Gustavsson, B.; Kosch, M.; Wong, A. et al.
In: Annales Geophysicae, Vol. 26, No. 12, 2008, p. 3999-4012.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Gustavsson, B, Kosch, M, Wong, A, Pedersen, T, Heinselman, C, Mutiso, C, Bristow, B, Hughes, J & Wang, W 2008, 'First estimates of volume distribution of HF-pump enhanced emissions at 6300 and 5577 angstrom: a comparison between observations and theory', Annales Geophysicae, vol. 26, no. 12, pp. 3999-4012. https://doi.org/10.5194/angeo-26-3999-2008

APA

Gustavsson, B., Kosch, M., Wong, A., Pedersen, T., Heinselman, C., Mutiso, C., Bristow, B., Hughes, J., & Wang, W. (2008). First estimates of volume distribution of HF-pump enhanced emissions at 6300 and 5577 angstrom: a comparison between observations and theory. Annales Geophysicae, 26(12), 3999-4012. https://doi.org/10.5194/angeo-26-3999-2008

Vancouver

Gustavsson B, Kosch M, Wong A, Pedersen T, Heinselman C, Mutiso C et al. First estimates of volume distribution of HF-pump enhanced emissions at 6300 and 5577 angstrom: a comparison between observations and theory. Annales Geophysicae. 2008;26(12):3999-4012. doi: 10.5194/angeo-26-3999-2008

Author

Gustavsson, B. ; Kosch, M. ; Wong, A. et al. / First estimates of volume distribution of HF-pump enhanced emissions at 6300 and 5577 angstrom: a comparison between observations and theory. In: Annales Geophysicae. 2008 ; Vol. 26, No. 12. pp. 3999-4012.

Bibtex

@article{f62359a187e54e4a821895ba512bbffd,

title = "First estimates of volume distribution of HF-pump enhanced emissions at 6300 and 5577 angstrom: a comparison between observations and theory",

abstract = "We present bi-static observations of radio-wave induced optical emissions at 6300 and 5577 angstrom from a night-time radio-induced optical emission ionospheric pumping experiment at the HIPAS (Fairbanks) facility in Alaska. The optical observations were made at HIPAS and from HAARP located 285 km south-east. From these observations the altitude distribution of the emissions is estimated with tomography-like methods. These estimates are compared with theoretical models. Other diagnostics used to support the theoretical calculations include the new Poker Flat AMISR UHF radar near HIPAS. We find that the altitude distribution of the emissions agree with electron transport modeling with a source of accelerated electrons located 20 km below the upper-hybrid altitude.",

keywords = "HAARP, IONOSPHERE, DYNAMICS, AIRGLOW, Active experiments, MODEL, HEATING EXPERIMENTS, FLUXES, Ionosphere-atmosphere interactions, Ionosphere, Ionospheric physics, Radio science, THERMOSPHERE, EISCAT",

author = "B. Gustavsson and M. Kosch and A. Wong and T. Pedersen and C. Heinselman and C. Mutiso and B. Bristow and J. Hughes and W. Wang",

year = "2008",

doi = "10.5194/angeo-26-3999-2008",

language = "English",

volume = "26",

pages = "3999--4012",

journal = "Annales Geophysicae",

issn = "0992-7689",

publisher = "European Geosciences Union",

number = "12",

}

RIS

TY - JOUR

T1 - First estimates of volume distribution of HF-pump enhanced emissions at 6300 and 5577 angstrom: a comparison between observations and theory

AU - Gustavsson, B.

AU - Kosch, M.

AU - Wong, A.

AU - Pedersen, T.

AU - Heinselman, C.

AU - Mutiso, C.

AU - Bristow, B.

AU - Hughes, J.

AU - Wang, W.

PY - 2008

Y1 - 2008

N2 - We present bi-static observations of radio-wave induced optical emissions at 6300 and 5577 angstrom from a night-time radio-induced optical emission ionospheric pumping experiment at the HIPAS (Fairbanks) facility in Alaska. The optical observations were made at HIPAS and from HAARP located 285 km south-east. From these observations the altitude distribution of the emissions is estimated with tomography-like methods. These estimates are compared with theoretical models. Other diagnostics used to support the theoretical calculations include the new Poker Flat AMISR UHF radar near HIPAS. We find that the altitude distribution of the emissions agree with electron transport modeling with a source of accelerated electrons located 20 km below the upper-hybrid altitude.

AB - We present bi-static observations of radio-wave induced optical emissions at 6300 and 5577 angstrom from a night-time radio-induced optical emission ionospheric pumping experiment at the HIPAS (Fairbanks) facility in Alaska. The optical observations were made at HIPAS and from HAARP located 285 km south-east. From these observations the altitude distribution of the emissions is estimated with tomography-like methods. These estimates are compared with theoretical models. Other diagnostics used to support the theoretical calculations include the new Poker Flat AMISR UHF radar near HIPAS. We find that the altitude distribution of the emissions agree with electron transport modeling with a source of accelerated electrons located 20 km below the upper-hybrid altitude.

KW - HAARP

KW - IONOSPHERE

KW - DYNAMICS

KW - AIRGLOW

KW - Active experiments

KW - MODEL

KW - HEATING EXPERIMENTS

KW - FLUXES

KW - Ionosphere-atmosphere interactions

KW - Ionosphere

KW - Ionospheric physics

KW - Radio science

KW - THERMOSPHERE

KW - EISCAT

U2 - 10.5194/angeo-26-3999-2008

DO - 10.5194/angeo-26-3999-2008

M3 - Journal article

VL - 26

SP - 3999

EP - 4012

JO - Annales Geophysicae

JF - Annales Geophysicae

SN - 0992-7689

IS - 12

ER -

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