Results
- Showing results for:
- Reset all filters
Search results
-
Journal articleKivelson MG, Khurana KK, Joy S, et al., 1997,
Europa's magnetic signature: Report from Galileo's pass on 19 December 1996
, SCIENCE, Vol: 276, Pages: 1239-1241, ISSN: 0036-8075- Author Web Link
- Cite
- Citations: 74
-
Journal articleKhurana KK, Kivelson MG, Russell CT, et al., 1997,
Absence of an internal magnetic field at Callisto
, NATURE, Vol: 387, Pages: 262-264, ISSN: 0028-0836- Author Web Link
- Cite
- Citations: 38
-
Journal articleDesai MI, Marsden RG, Sanderson TR, et al., 1997,
Particle acceleration at corotating reverse shocks in the southern hemisphere: Ulysses results
, GEOPHYSICAL RESEARCH LETTERS, Vol: 24, Pages: 1155-1158, ISSN: 0094-8276- Author Web Link
- Cite
- Citations: 10
-
Journal articleChisham G, Bale SD, Burgess D, et al., 1997,
A large magnetic depression observed in the solar wind close to the earth’s bow shock
, Advances in Space Research, Vol: 19, Pages: 869-872-869-872 -
Conference paperPierre F, Solomon J, CornilleauWehrlin N, et al., 1997,
Oblique emission of whistler-mode waves around interplanetary shocks
, Meeting on Solar and Heliospheric Plasma Physics, Publisher: KLUWER ACADEMIC PUBL, Pages: 327-334, ISSN: 0038-0938 -
Journal articleBalogh A, 1997,
Will Cluster ride again?
, NEW SCIENTIST, Vol: 154, Pages: 53-53, ISSN: 0262-4079 -
Journal articleCargill PJ, Klimchuk JA, 1997,
A nanoflare explanation for the heating of coronal loops observed by Yohkoh
, ASTROPHYSICAL JOURNAL, Vol: 478, Pages: 799-806, ISSN: 0004-637X- Author Web Link
- Cite
- Citations: 147
-
Journal articleRezeau L, CornilleauWehrlin N, Belmont G, et al., 1997,
Possible role of electromagnetic low frequency waves in the Io torus in the production of Jovian aurorae
, PLANETARY AND SPACE SCIENCE, Vol: 45, Pages: 483-&, ISSN: 0032-0633- Author Web Link
- Cite
- Citations: 8
-
Journal articleTsurutani BT, Arballo JK, Goldstein BE, et al., 1997,
Plasma wave characteristics of the Jovian magnetopause boundary layer: Relationship to the Jovian aurora?
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 102, Pages: 4751-4764- Author Web Link
- Cite
- Citations: 16
-
Journal articleBlanco-Cano X, Schwartz SJ, 1997,
Identification of low-frequency kinetic wave modes in the Earth’s ion foreshock
, Annales Geophysicae, Vol: 15, Pages: 273-288-273-288 -
Journal articleBaring MG, Ogilvie KW, Ellison DC, et al., 1997,
Acceleration of solar wind ions by nearby interplanetary shocks: Comparison of Monte Carlo simulations with Ulysses observations
, ASTROPHYSICAL JOURNAL, Vol: 476, Pages: 889-902, ISSN: 0004-637X- Author Web Link
- Cite
- Citations: 62
-
Journal articleMoncuquet M, MeyerVernet N, Hoang S, et al., 1997,
Detection of Bernstein wave forbidden bands in the Jovian magnetosphere: A new way to measure the electron density
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 102, Pages: 2373-2379- Author Web Link
- Cite
- Citations: 24
-
Journal articleNilsson H, Kirkwood S, Lilensten J, et al., 1997,
Enhanced incoherent scatter plasma lines
, Annales Geophysicae, Vol: 14, Pages: 1462-1472, ISSN: 0992-7689Detailed 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 articleGuo LJ, Moore JM, Haigh JD, 1997,
Simulated reflectance technique for ATM image enhancement
, INTERNATIONAL JOURNAL OF REMOTE SENSING, Vol: 18, Pages: 243-254, ISSN: 0143-1161- Author Web Link
- Cite
- Citations: 2
-
Journal articleCarpenter DL, Galand M, Bell TF, et al., 1997,
Quasiperiodic similar to 5-60 s fluctuations of VLF signals propagating in the Earth-ionosphere waveguide: A result of pulsating auroral particle precipitation?
, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 102, Pages: 347-361- Author Web Link
- Cite
- Citations: 3
-
Conference paperSouthwood DJ, 1997,
The magnetic field of Mercury
, Workshop on Mercury - The Planet and Its Magnetosphere, Publisher: PERGAMON-ELSEVIER SCIENCE LTD, Pages: 113-117, ISSN: 0032-0633- Author Web Link
- Cite
- Citations: 16
-
Journal articleSchmidt R, Escoubet CP, Schwartz SJ, 1997,
The Cluster Science Data System (csds) - a New Approach to the Distribution of Scientific Data
, ßr, Vol: 79, Pages: 557-582-557-582 -
Journal articleBalogh A, 1997,
Mercury: The planet and its magnetosphere - Introduction
, PLANETARY AND SPACE SCIENCE, Vol: 45, Pages: 1-2, ISSN: 0032-0633- Author Web Link
- Cite
- Citations: 6
-
Journal articleBalogh A, Dunlop MW, Cowley SWH, et al., 1997,
The Cluster magnetic field investigation
, SPACE SCIENCE REVIEWS, Vol: 79, Pages: 65-91, ISSN: 0038-6308- Author Web Link
- Cite
- Citations: 418
-
Conference paperLin NG, Kellogg PJ, MacDowall RJ, et al., 1997,
Low frequency plasma waves in the solar wind: From ecliptic plane to the solar polar regions
, 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- Author Web Link
- Cite
- Citations: 2
-
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 paperHorbury TS, Balogh A, Forsyth RJ, et al., 1997,
Ulysses observations of intermittent heliospheric turbulence
, 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- Author Web Link
- Cite
- Citations: 51
-
Conference paperKivelson MG, Khurana KK, Russell CT, et al., 1997,
Galileo at Jupiter: Changing states of the magnetosphere and first looks at Io and Ganymede
, 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- Author Web Link
- Cite
- Citations: 24
-
Conference paperLaxton NF, Balogh A, Cowley SWH, et al., 1997,
Gradients and flows in Jupiter's magnetosphere determined from the anisotropies of similar to 1 MeV protons
, C3.2 Symposium of COSPAR Scientific Commission C on Planetary Ionospheres and Magnetospheres, at the 31st COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 221-224, ISSN: 0273-1177 -
Journal articleHorbury TS, Balogh A, 1997,
Structure function measurements of the intermittent turbulent cascade
, Nonlinear Processes in Geophysics, Vol: 4, Pages: 185-199 -
Conference paperErdos G, Balogh A, Kota J, 1997,
Separation rate of the magnetic field lines observed by Ulysses at high latitude
, 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- Author Web Link
- Cite
- Citations: 4
-
Conference paperLand PE, Haigh JD, 1997,
Atmospheric correction over case 2 waters using an iterative fitting algorithm including relative humidity
, Conference on Ocean Optics XIII, Publisher: SPIE - INT SOC OPTICAL ENGINEERING, Pages: 609-613- Author Web Link
- Cite
- Citations: 1
-
Journal articleChen J, Cargill PJ, Palmadesso P, 1997,
Predicting Geoeffective Solar Wind Structures
, Journal of Geophysical Research-Atmospheres, Vol: 102, Pages: 14701-14720 -
Conference paperSmith EJ, Balogh A, Burton ME, et al., 1997,
Radial and azimuthal components of the heliospheric magnetic field: Ulysses observations
, 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- Author Web Link
- Cite
- Citations: 23
-
Conference paperDunlop MW, Woodward TI, Southwood DJ, et al., 1997,
Merging 4 spacecraft data: Concepts used for analysing discontinuities
, 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- Author Web Link
- 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.