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RF heating in a strong auroral electrojet

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RF heating in a strong auroral electrojet. / Robinson, T. R.; Bond, G.; Eglitis, P. et al.
In: Advances in Space Research, Vol. 21, No. 5, 1998, p. 689-692.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Robinson, TR, Bond, G, Eglitis, P, Honary, F & Rietveld, MT 1998, 'RF heating in a strong auroral electrojet', Advances in Space Research, vol. 21, no. 5, pp. 689-692. https://doi.org/10.1016/S0273-1177(97)01004-1

APA

Robinson, T. R., Bond, G., Eglitis, P., Honary, F., & Rietveld, M. T. (1998). RF heating in a strong auroral electrojet. Advances in Space Research, 21(5), 689-692. https://doi.org/10.1016/S0273-1177(97)01004-1

Vancouver

Robinson TR, Bond G, Eglitis P, Honary F, Rietveld MT. RF heating in a strong auroral electrojet. Advances in Space Research. 1998;21(5):689-692. doi: 10.1016/S0273-1177(97)01004-1

Author

Robinson, T. R. ; Bond, G. ; Eglitis, P. et al. / RF heating in a strong auroral electrojet. In: Advances in Space Research. 1998 ; Vol. 21, No. 5. pp. 689-692.

Bibtex

@article{6ea171f93d5a4c8fb47c3ac02ada6489,
title = "RF heating in a strong auroral electrojet",
abstract = "Results are reported from experiments in which the high power HF facility at Troms{\o}, Norway was employed to modify the Hall current region of the auroral ionosphere during periods when the electrojet became enhanced. During conditions characterised by a weak electrojet and completely underdense heating, observations indicated that RF heating leads to the expected increase in the electron temperature, inferred from EISCAT UHF radar measurements, at all altitudes between 100 and 135 km. However, under conditions characterised by a strong electrojet and slightly underdense heating, observations indicated that RF heating appeared to reduce the electrojet electron temperature, in the altitude range 100–115 km, whilst still enhancing the electron temperatures in the layers above the electrojet, in the altitude range 120–135 km. These, somewhat surprising, results are discussed in terms of a theory of the interaction between high power electromagnetic waves and irregularities excited by the Farley-Buneman instability at electrojet altitudes.",
keywords = "heating DCS-publications-id, art-84, DCS-publications-credits, iono, DCS-publications-personnel-id, 5",
author = "Robinson, {T. R.} and G. Bond and P. Eglitis and F. Honary and Rietveld, {M. T.}",
year = "1998",
doi = "10.1016/S0273-1177(97)01004-1",
language = "English",
volume = "21",
pages = "689--692",
journal = "Advances in Space Research",
publisher = "Elsevier Ltd",
number = "5",

}

RIS

TY - JOUR

T1 - RF heating in a strong auroral electrojet

AU - Robinson, T. R.

AU - Bond, G.

AU - Eglitis, P.

AU - Honary, F.

AU - Rietveld, M. T.

PY - 1998

Y1 - 1998

N2 - Results are reported from experiments in which the high power HF facility at Tromsø, Norway was employed to modify the Hall current region of the auroral ionosphere during periods when the electrojet became enhanced. During conditions characterised by a weak electrojet and completely underdense heating, observations indicated that RF heating leads to the expected increase in the electron temperature, inferred from EISCAT UHF radar measurements, at all altitudes between 100 and 135 km. However, under conditions characterised by a strong electrojet and slightly underdense heating, observations indicated that RF heating appeared to reduce the electrojet electron temperature, in the altitude range 100–115 km, whilst still enhancing the electron temperatures in the layers above the electrojet, in the altitude range 120–135 km. These, somewhat surprising, results are discussed in terms of a theory of the interaction between high power electromagnetic waves and irregularities excited by the Farley-Buneman instability at electrojet altitudes.

AB - Results are reported from experiments in which the high power HF facility at Tromsø, Norway was employed to modify the Hall current region of the auroral ionosphere during periods when the electrojet became enhanced. During conditions characterised by a weak electrojet and completely underdense heating, observations indicated that RF heating leads to the expected increase in the electron temperature, inferred from EISCAT UHF radar measurements, at all altitudes between 100 and 135 km. However, under conditions characterised by a strong electrojet and slightly underdense heating, observations indicated that RF heating appeared to reduce the electrojet electron temperature, in the altitude range 100–115 km, whilst still enhancing the electron temperatures in the layers above the electrojet, in the altitude range 120–135 km. These, somewhat surprising, results are discussed in terms of a theory of the interaction between high power electromagnetic waves and irregularities excited by the Farley-Buneman instability at electrojet altitudes.

KW - heating DCS-publications-id

KW - art-84

KW - DCS-publications-credits

KW - iono

KW - DCS-publications-personnel-id

KW - 5

U2 - 10.1016/S0273-1177(97)01004-1

DO - 10.1016/S0273-1177(97)01004-1

M3 - Journal article

VL - 21

SP - 689

EP - 692

JO - Advances in Space Research

JF - Advances in Space Research

IS - 5

ER -