Imperial College London
Alternate

Professor Southwood

Faculty of Natural Sciences, Department of Physics

Senior Research Investigator
 
 
 
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Contact

 

+44 (0)20 7594 7770d.southwood CV

 
 
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Location

 

711AHuxley BuildingSouth Kensington Campus

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Summary

 

Publications

Publication Type
Year
to

243 results found

Southwood DJ, Kivelson MG, 2001, Damping standing Alfven waves in the magnetosphere, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 106, Pages: 10829-10836, ISSN: 2169-9380

Journal article

Southwood DJ, Kivelson MG, 2000, Relationships between phase structure and energy flux in magneto hydro dynamic waves in the magnetosphere, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 105, Pages: 27701-27706, ISSN: 2169-9380

Journal article

Matsuoka A, Southwood DJ, Kokubun S, Mukai Tet al., 2000, Propagation sense of low-frequency MHD waves in the magnetosheath observed by Geotail, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 105, Pages: 18361-18376, ISSN: 2169-9380

Journal article

Woodward TI, Dunlop MW, Southwood DJ, 2000, Separation strategy for co-ordinated measurements, Cluster-II Workshop on Multiscale/Multipoint Plasma Measurements, Publisher: EUROPEAN SPACE AGENCY, Pages: 343-346, ISSN: 0379-6566

Conference paper

Dunlop MW, Dougherty MK, Kellock S, Southwood DJet al., 1999, Operation of the dual magnetometer on Cassini: science performance, Symposium on The Jovian System after Galieo/The Santurnian System before Cassini-Huygens, Publisher: PERGAMON-ELSEVIER SCIENCE LTD, Pages: 1389-1405, ISSN: 0032-0633

Conference paper

Southwood DJ, Kivelson MG, 1997, Frequency doubling in ultralow frequency wave signals, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 102, Pages: 27151-27158

Journal article

Kivelson MG, Khurana KK, Joy S, Russell CT, Southwood DJ, Walker RJ, Polanskey Cet al., 1997, Europa's magnetic signature: Report from Galileo's pass on 19 December 1996, SCIENCE, Vol: 276, Pages: 1239-1241, ISSN: 0036-8075

Journal article

Khurana KK, Kivelson MG, Russell CT, Walker RJ, Southwood DJet al., 1997, Absence of an internal magnetic field at Callisto, NATURE, Vol: 387, Pages: 262-264, ISSN: 0028-0836

Journal article

Southwood 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

Conference paper

Balogh A, Dunlop MW, Cowley SWH, Southwood DJ, Thomlinson JG, Glassmeier KH, Musmann G, Luhr H, Buchert S, Acuna MH, Fairfield DH, Slavin JA, Riedler W, Schwingenschuh K, Kivelson MGet al., 1997, The Cluster magnetic field investigation, SPACE SCIENCE REVIEWS, Vol: 79, Pages: 65-91, ISSN: 0038-6308

Journal article

Southwood 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 paper

Dougherty MK, Southwood DJ, Lachin A, 1997, Ion cyclotron waves in the Jovian magnetosphere, Advances in Space Research, Vol: 20, Pages: 215-219

Journal article

Kivelson MG, Khurana KK, Russell CT, Walker RJ, Coleman PJ, Coroniti FV, Green J, Joy S, McPherron RL, Polanskey C, Southwood DJ, Bennett L, Warnecke J, Huddleston DEet 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

Conference paper

Dunlop MW, Woodward TI, Southwood DJ, Glassmeier KH, Elphic Ret 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

Conference paper

Lofting CFA, Dougherty MK, Southwood DJ, 1997, The Coriolis effect in a rapidly rotating magnetosphere, C3.2 Symposium of COSPAR Scientific Commission C on Planetary Ionospheres and Magnetospheres, at the 31st COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 239-242, ISSN: 0273-1177

Conference paper

Kivelson MG, Khurana KK, Russell CT, Walker RJ, Warnecke J, Coroniti FV, Polanskey C, Southwood DJ, Schubert Get al., 1996, Discovery of Ganymede's magnetic field by the Galileo spacecraft, NATURE, Vol: 384, Pages: 537-541, ISSN: 0028-0836

Journal article

Dougherty MK, Balogh A, Southwood DJ, Smith EJet al., 1996, Ulysses assessment of the Jovian planetary field, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 24929-24941, ISSN: 2169-9380

Journal article

Kivelson MG, Khurana KK, Walker RJ, Warnecke J, Russell CT, Linker JA, Southwood DJ, Polanskey Cet al., 1996, Io's interaction with the plasma torus: Galileo magnetometer report, SCIENCE, Vol: 274, Pages: 396-398, ISSN: 0036-8075

Journal article

Thompson P, Southwood DJ, Goodman S, 1996, Plasma waves radiated by a moving conducting body between successive gyrofrequencies, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 19849-19858, ISSN: 2169-9380

Journal article

Kivelson MG, Southwood DJ, 1996, Mirror instability .2. The mechanism of nonlinear saturation, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 17365-17371, ISSN: 2169-9380

Journal article

Kivelson MG, Khurana KK, Walker RJ, Russell CT, Linker JA, Southwood DJ, Polanskey Cet al., 1996, A magnetic signature at Io: Initial report from the Galileo magnetometer, SCIENCE, Vol: 273, Pages: 337-340, ISSN: 0036-8075

Journal article

Motschmann U, Woodward TI, Glassmeier KH, Southwood DJ, Pincon JLet al., 1996, Wavelength and direction filtering by magnetic measurements at satellite arrays: Generalized minimum variance analysis, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 101, Pages: 4961-4965, ISSN: 2169-9380

Journal article

Prange R, Rego D, Southwood D, Zarka P, Miller S, Ip Wet al., 1996, Rapid energy dissipation and variability of the Io-Jupiter electrodynamic circuit, Nature, Vol: 379, Pages: 323-325

THE electrodynamic interaction between Jupiter and the closest of its large moons, Io, is unique in the Solar system. Io's volcanoes eject a considerable amount of material into the inner jovian system (>1 tonne per second), much of it in the form of ions(1); the motion of Io through Jupiter's powerful magnetic field in turn generates a million-ampere current(2) between the charged near-Io environment and the planet's ionosphere. This current is presumably carried by Alfven waves(3), the electromagnetic equivalent of sound waves. Here we present far-ultraviolet observations of the atmospheric footprint of this current, which demonstrate that most of the energy is dissipated rapidly when the waves first encounter Jupiter's ionosphere; the position of the footprint varies with time, We see no evidence for the multiple ionospheric interactions that have been proposed to explain the structure of the radio emissions associated with these waves(4).

Journal article

Prange R, Rego D, Southwood D, Zarka P, Miller S, Ip Wet al., 1996, Rapid energy dissipation and variability of the Io-Jupiter electrodynamic circuit., Nature, Vol: 379, Pages: 323-325

Journal article

Kellock S, Austin P, Balogh A, Gerlach B, Marquedant R, Musmann G, Smith E, Southwood D, Szalai Set al., 1996, Cassini dual technique magnetometer instrument (MAG), Cassini/Huygens: A Mission to the Saturnian Systems, Vol: 2803, Pages: 141-152

Journal article

Dunlop MW, Woodward TI, Motschmann U, Southwood DJ, Balogh Aet al., 1996, Analysis of non-planar structures with multipoint measurements, D3 1 Symposium of COSPAR Scientific Commission D on the 3-Dimensional Magnetosphere, at the 30th COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 309-314, ISSN: 0273-1177

Conference paper

Motschmann U, Woodward TI, Glassmeier KH, Southwood DJet al., 1996, Wave field analysis by magnetic measurements at satellite arrays: Generalized minimum variance analysis, D3 1 Symposium of COSPAR Scientific Commission D on the 3-Dimensional Magnetosphere, at the 30th COSPAR Scientific Assembly, Publisher: PERGAMON PRESS LTD, Pages: 315-319, ISSN: 0273-1177

Conference paper

FARRUGIA CJ, SANDHOLT PE, COWLEY SWH, SOUTHWOOD DJ, EGELAND A, STAUNING P, LEPPING RP, LAZARUS AJ, HANSEN T, FRIISCHRISTENSEN Eet al., 1995, RECONNECTION-ASSOCIATED AURORAL ACTIVITY STIMULATED BY 2 TYPES OF UPSTREAM DYNAMIC PRESSURE VARIATIONS - INTERPLANETARY MAGNETIC-FIELD B-Z-SIMILAR-TO-0, B-Y-MUCH-LESS-THAN-0 CASE, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 100, Pages: 21753-21772, ISSN: 2169-9380

Journal article

BALOGH A, SMITH EJ, TSURUTANI BT, SOUTHWOOD DJ, FORSYTH RJ, HORBURY TSet al., 1995, THE HELIOSPHERIC MAGNETIC-FIELD OVER THE SOUTH POLAR-REGION OF THE SUN, SCIENCE, Vol: 268, Pages: 1007-1010, ISSN: 0036-8075

Journal article

Balogh A, Southwood DJ, Forsyth RJ, Horbury TS, Smith EJ, Tsurutani BTet al., 1995, The heliospheric magnetic field over the South polar region of the sun., Science, Vol: 268, Pages: 1007-1010, ISSN: 0036-8075

Magnetic field measurements from the Ulysses space mission overthe south polar regions of the sun showed that the structure and properties of the three-dimensional heliosphere were determined by the fast solar wind flow and magnetic fields from the large coronal holes in the polar regions of the sun. This conclusion applies at the current, minimum phase of the 11-year solar activity cycle. Unexpectedly, the radial component of the magnetic field was independent of latitude. The high-latitude magnetic field deviated significantly from the expected Parker geometry, probably because of large amplitude transverse fluctuations. Low-frequency fluctuations had a high level of variance. The rate of occurrence of discontinuities also increased significantly at high latitudes.

Journal article

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