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Journal articleCargill PJ, Spicer DS, Zalesak ST, 1997, , ASTROPHYSICAL JOURNAL, Vol: 488, Pages: 854-866, ISSN: 0004-637X
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- Citations: 38
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Journal articleLucek EA, Balogh A, 1997, , GEOPHYSICAL RESEARCH LETTERS, Vol: 24, Pages: 2387-2390, ISSN: 0094-8276
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- Citations: 14
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Journal articleGaland M, Lilensten J, Kofman W, et al., 1997, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 102, Pages: 22261-22272
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- Citations: 51
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Journal articleGiacalone J, Burgess D, Schwartz SJ, et al., 1997, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 102, Pages: 19789-19804
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- Citations: 46
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Journal articleBale SD, 1997, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 102, Pages: 19773-19778
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- Citations: 12
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Journal articleLaxton NF, Balogh A, Cowley SWH, et al., 1997, , PLANETARY AND SPACE SCIENCE, Vol: 45, Pages: 1143-1170, ISSN: 0032-0633
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- Citations: 25
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Journal articleBale SD, Chisham G, Burgess D, et al., 1997, , Advances in Space 91桃色, Vol: 20, Pages: 695-698-695-698
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Journal articleBlanco-Cano X, Schwartz SJ, 1997, , Advances in Space 91桃色, Vol: 20, Pages: 707-711-707-711
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Journal articleFlowerdew RJ, Haigh JD, 1997, , JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, Vol: 102, Pages: 17163-17171, ISSN: 2169-897X
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- Citations: 5
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Journal articleKellogg PJ, Goetz K, Monson SJ, et al., 1997, , ASTROPHYSICAL JOURNAL, Vol: 484, Pages: 432-438, ISSN: 0004-637X
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Journal articleBale SD, Burgess D, Kellogg PJ, et al., 1997, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 102, Pages: 11281-11286
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- Citations: 44
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Journal articleBale SD, Owen CJ, Bougeret JL, et al., 1997, , GEOPHYSICAL RESEARCH LETTERS, Vol: 24, Pages: 1427-1430, ISSN: 0094-8276
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- Citations: 38
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Journal articleKivelson MG, Khurana KK, Joy S, et al., 1997, , SCIENCE, Vol: 276, Pages: 1239-1241, ISSN: 0036-8075
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- Citations: 83
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Journal articleKhurana KK, Kivelson MG, Russell CT, et al., 1997, , NATURE, Vol: 387, Pages: 262-264, ISSN: 0028-0836
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- Citations: 42
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Journal articleDesai MI, Marsden RG, Sanderson TR, et al., 1997, , GEOPHYSICAL RESEARCH LETTERS, Vol: 24, Pages: 1155-1158, ISSN: 0094-8276
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- Citations: 11
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Journal articleChisham G, Bale SD, Burgess D, et al., 1997, , Advances in Space 91桃色, Vol: 19, Pages: 869-872-869-872
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Conference paperPierre F, Solomon J, CornilleauWehrlin N, et al., 1997, , Meeting on Solar and Heliospheric Plasma Physics, Publisher: KLUWER ACADEMIC PUBL, Pages: 327-334, ISSN: 0038-0938
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Journal articleBalogh A, 1997,
Will Cluster ride again?
, NEW SCIENTIST, Vol: 154, Pages: 53-53, ISSN: 0262-4079 -
Journal articleCargill PJ, Klimchuk JA, 1997, , ASTROPHYSICAL JOURNAL, Vol: 478, Pages: 799-806, ISSN: 0004-637X
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- Citations: 152
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Journal articleRezeau L, CornilleauWehrlin N, Belmont G, et al., 1997, , PLANETARY AND SPACE SCIENCE, Vol: 45, Pages: 483-&, ISSN: 0032-0633
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- Citations: 8
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Journal articleTsurutani BT, Arballo JK, Goldstein BE, et al., 1997, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 102, Pages: 4751-4764
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- Citations: 16
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Journal articleBlanco-Cano X, Schwartz SJ, 1997, , Annales Geophysicae, Vol: 15, Pages: 273-288-273-288
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Journal articleBaring MG, Ogilvie KW, Ellison DC, et al., 1997, , ASTROPHYSICAL JOURNAL, Vol: 476, Pages: 889-902, ISSN: 0004-637X
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- Citations: 63
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Journal articleNilsson H, Kirkwood S, Lilensten J, et al., 1997, , Annales Geophysicae, Vol: 14, Pages: 1462-1472, ISSN: 0992-7689
Detailed model calculations of auroral secondary and photoelectron distributions for varying conditions have been used to calculate the theoretical enhancement of incoherent scatter plasma lines. These calculations are compared with EISCAT UHF radar measurements of enhanced plasma lines from both the E and F regions, and published EISCAT VHF radar measurements. The agreement between the calculated and observed plasma line enhancements is good. The enhancement from the superthermal distribution can explain even the very strong enhancements observed in the auroral E region during aurora, as previously shown by Kirkwood et al. The model calculations are used to predict the range of conditions when enhanced plasma lines will be seen with the existing high-latitude incoherent scatter radars, including the new EISCAT Svalbard radar. It is found that the detailed structure, i.e. the gradients in the suprathermal distribution, are most important for the plasma line enhancement. The level of superthermal flux affects the enhancement only in the region of low phase energy where the number of thermal electrons is comparable to the number of suprathermal electrons and in the region of high phase energy where the suprathermal fluxes fall to such low levels that their effect becomes small compared to the collision term. To facilitate the use of the predictions for the different radars, the expected signal-to-noise ratios (SNRs) for typical plasma line enhancements have been calculated. It is found that the high-frequency radars (Søndre Strømfjord, EISCAT UHF) should observe the highest SNR. but only for rather high plasma frequencies. The VHF radars (EISCAT VHF and Svalbard) will detect enhanced plasma lines over a wider range of frequencies, but with lower SNR.
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Journal articleMoncuquet M, MeyerVernet N, Hoang S, et al., 1997, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 102, Pages: 2373-2379
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- Citations: 26
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Journal articleGuo LJ, Moore JM, Haigh JD, 1997, , INTERNATIONAL JOURNAL OF REMOTE SENSING, Vol: 18, Pages: 243-254, ISSN: 0143-1161
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- Citations: 3
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Journal articleCarpenter DL, Galand M, Bell TF, et al., 1997, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 102, Pages: 347-361
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- Citations: 4
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Journal articleBalogh A, Dunlop MW, Cowley SWH, et al., 1997, , SPACE SCIENCE REVIEWS, Vol: 79, Pages: 65-91, ISSN: 0038-6308
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- Citations: 442
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Journal articleSchmidt R, Escoubet CP, Schwartz SJ, 1997, , ßr, Vol: 79, Pages: 557-582-557-582
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Journal articleBalogh A, 1997, , PLANETARY AND SPACE SCIENCE, Vol: 45, Pages: 1-2, ISSN: 0032-0633
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- Citations: 6
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