Results
- Showing results for:
- Reset all filters
Search results
-
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
- Cite
- Citations: 152
-
Journal articleRezeau L, CornilleauWehrlin N, Belmont G, et al., 1997, , PLANETARY AND SPACE SCIENCE, Vol: 45, Pages: 483-&, ISSN: 0032-0633
- Cite
- Citations: 8
-
Journal articleTsurutani BT, Arballo JK, Goldstein BE, et al., 1997, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 102, Pages: 4751-4764
- Cite
- Citations: 16
-
Journal articleBlanco-Cano X, Schwartz SJ, 1997, , Annales Geophysicae, Vol: 15, Pages: 273-288-273-288
-
Journal articleBaring MG, Ogilvie KW, Ellison DC, et al., 1997, , ASTROPHYSICAL JOURNAL, Vol: 476, Pages: 889-902, ISSN: 0004-637X
- Cite
- Citations: 63
-
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.
-
Journal articleMoncuquet M, MeyerVernet N, Hoang S, et al., 1997, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 102, Pages: 2373-2379
- Cite
- Citations: 26
-
Journal articleGuo LJ, Moore JM, Haigh JD, 1997, , INTERNATIONAL JOURNAL OF REMOTE SENSING, Vol: 18, Pages: 243-254, ISSN: 0143-1161
- Cite
- Citations: 3
-
Journal articleCarpenter DL, Galand M, Bell TF, et al., 1997, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 102, Pages: 347-361
- Cite
- Citations: 4
-
Journal articleBalogh A, Dunlop MW, Cowley SWH, et al., 1997, , SPACE SCIENCE REVIEWS, Vol: 79, Pages: 65-91, ISSN: 0038-6308
- Cite
- Citations: 442
-
Journal articleSchmidt R, Escoubet CP, Schwartz SJ, 1997, , ßr, Vol: 79, Pages: 557-582-557-582
-
Journal articleBalogh A, 1997, , PLANETARY AND SPACE SCIENCE, Vol: 45, Pages: 1-2, ISSN: 0032-0633
- Cite
- Citations: 6
-
Conference paperSouthwood DJ, 1997, , Workshop on Mercury - The Planet and Its Magnetosphere, Publisher: PERGAMON-ELSEVIER SCIENCE LTD, Pages: 113-117, ISSN: 0032-0633
- Cite
- Citations: 17
-
Conference paperLin NG, Kellogg PJ, MacDowall RJ, et al., 1997, , DO-2 Symposium of COSPAR Scientific Commission D on the Heliosphere at Solar Minimum and Beyond, at the 31st COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 877-881, ISSN: 0273-1177
- Cite
- Citations: 2
-
Journal articleChen J, Cargill PJ, Palmadesso P, 1997,
Predicting Geoeffective Solar Wind Structures
, Journal of Geophysical Research-Atmospheres, Vol: 102, Pages: 14701-14720 -
Conference paperLand PE, Haigh JD, 1997, , Conference on Ocean Optics XIII, Publisher: SPIE - INT SOC OPTICAL ENGINEERING, Pages: 609-613
- Cite
- Citations: 1
-
Conference paperErdos G, Balogh A, Kota J, 1997, , DO-2 Symposium of COSPAR Scientific Commission D on the Heliosphere at Solar Minimum and Beyond, at the 31st COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 843-846, ISSN: 0273-1177
- Cite
- Citations: 4
-
Journal articleHorbury TS, Balogh A, 1997,
Structure function measurements of the intermittent turbulent cascade
, Nonlinear Processes in Geophysics, Vol: 4, Pages: 185-199 -
Conference paperKivelson MG, Khurana KK, Russell CT, et al., 1997, , C3.2 Symposium of COSPAR Scientific Commission C on Planetary Ionospheres and Magnetospheres, at the 31st COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 193-204, ISSN: 0273-1177
- Cite
- Citations: 26
-
Conference paperHorbury TS, Balogh A, Forsyth RJ, et al., 1997, , DO-2 Symposium of COSPAR Scientific Commission D on the Heliosphere at Solar Minimum and Beyond, at the 31st COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 847-850, ISSN: 0273-1177
- Cite
- Citations: 52
-
Journal articleDougherty MK, Southwood DJ, Lachin A, 1997,
Ion cyclotron waves in the Jovian magnetosphere
, Advances in Space Research, Vol: 20, Pages: 215-219 -
Conference paperSouthwood DJ, Kivelson MG, 1997,
The magnetic fields of the Galilean moons of Jupiter: The Galileo spacecraft magnetometer results
, Dordrecht, conference on the 3 galileos: the man, the spacecraft, the telescope JAN 07-10, 1997 PADUA, ITALY, Publisher: Kluwer Academic Publ, Pages: 299-310 -
Conference paperSmith EJ, Balogh A, Burton ME, et al., 1997, , E2.2 Symposium of COSPAR Scientific Commission E on the Sun and Its Role in the Heliosphere, at the 31st COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 47-53, ISSN: 0273-1177
- Cite
- Citations: 23
-
Conference paperForsyth FJ, Balogh A, Horbury TS, et al., 1997, , DO-2 Symposium of COSPAR Scientific Commission D on the Heliosphere at Solar Minimum and Beyond, at the 31st COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 839-842, ISSN: 0273-1177
- Cite
- Citations: 5
-
Conference paperBrindley HE, Harries JE, 1997,
The impact of far infra-red absorption on greenhouse forcing: sensitivity studies at high spectral resolution
, International Radiation Symposium, Publisher: A. Deepak -
Conference paperKrupp N, Keppler E, Seidel R, et al., 1997, , C3.2 Symposium of COSPAR Scientific Commission C on Planetary Ionospheres and Magnetospheres, at the 31st COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 225-228, ISSN: 0273-1177
- Cite
- Citations: 11
-
Journal articleLand PE, Haigh JD, 1997,
Atmospheric correction over case 2 waters with an iterative fitting algorithm: relative humidity effects
, Applied Optics, Vol: 36, Pages: 9448-9455, ISSN: 0003-6935 -
Conference paperSmith EJ, Neugebauer M, Tsurutani BT, et al., 1997, , E2.2 Symposium of COSPAR Scientific Commission E on the Sun and Its Role in the Heliosphere, at the 31st COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 55-63, ISSN: 0273-1177
- Cite
- Citations: 14
-
Conference paperDunlop MW, Woodward TI, Southwood DJ, et al., 1997, , D0.1 Symposium of COSPAR Scientific Commission D on Results of the IASTP Program at the 31st COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 1101-1106, ISSN: 0273-1177
- Cite
- Citations: 20
This data is extracted from the Web of Science and reproduced under a licence from Thomson Reuters. You may not copy or re-distribute this data in whole or in part without the written consent of the Science business of Thomson Reuters.