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Journal articleHO CM, TSURUTANI BT, GOLDSTEIN BE, et al., 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 3409-3412, ISSN: 0094-8276
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- Citations: 18
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Journal articleFORSYTH RJ, BALOGH A, SMITH EJ, et al., 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 3321-3324, ISSN: 0094-8276
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- Citations: 39
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Journal articleSMITH EJ, BALOGH A, 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 3317-3320, ISSN: 0094-8276
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- Citations: 163
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Journal articleHORBURY TS, BALOGH A, FORSYTH RJ, et al., 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 3401-3404, ISSN: 0094-8276
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- Citations: 51
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Journal articleBALE SD, KELLOGG PJ, MONSON SJ, et al., 1995, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 100, Pages: 23749-23754, ISSN: 2169-9380
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- Citations: 1
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Journal articleHORBURY TS, BALOGH A, FORSYTH RJ, et al., 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 3405-3408, ISSN: 0094-8276
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- Citations: 39
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Journal articleBOTHMER V, MARSDEN RG, SANDERSON TR, et al., 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 3369-3372, ISSN: 0094-8276
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- Citations: 26
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Journal articleSMITH EJ, BALOGH A, BURTON ME, et al., 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 3325-3328, ISSN: 0094-8276
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- Citations: 49
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Journal articleSMITH EJ, BALOGH A, NEUGEBAUER M, et al., 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 3381-3384, ISSN: 0094-8276
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- Citations: 142
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Journal articlePIERRE F, SOLOMON J, CORNILLEAUWEHRLIN N, et al., 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 3425-3428, ISSN: 0094-8276
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- Citations: 8
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Journal articleTSURUTANI BT, HO CM, ARBALLO JK, et al., 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 3397-3400, ISSN: 0094-8276
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- Citations: 84
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Journal articleLIN NG, KELLOGG PJ, MACDOWALL RJ, et al., 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 3417-3420, ISSN: 0094-8276
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- Citations: 43
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Journal articlePICK M, LANZEROTTI LJ, BUTTIGHOFFER A, et al., 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 3377-3380, ISSN: 0094-8276
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- Citations: 15
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Journal articleSANDERSON TR, BOTHMER V, MARSDEN RG, et al., 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 3357-3360, ISSN: 0094-8276
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- Citations: 40
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Journal articleKIRKWOOD S, NILSSON H, LILENSTEN J, et al., 1995, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 100, Pages: 21343-21355, ISSN: 2169-9380
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- Citations: 10
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Journal articleFARRUGIA CJ, SANDHOLT PE, COWLEY SWH, et al., 1995, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 100, Pages: 21753-21772, ISSN: 2169-9380
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- Citations: 21
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Journal articleMOLDWIN MB, PHILLIPS JL, GOSLING JT, et al., 1995, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 100, Pages: 19903-19910, ISSN: 2169-9380
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- Citations: 95
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Journal articleDEWIT TD, KRASNOSELSKIKH VV, BALE SD, et al., 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 2653-2656, ISSN: 0094-8276
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- Citations: 62
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Journal articleMCCOMAS DJ, BARRACLOUGH BL, GOSLING JT, et al., 1995, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 100, Pages: 19893-19902, ISSN: 2169-9380
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- Citations: 62
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Journal articleYOSHINO K, ESMOND JR, MURRAY JE, et al., 1995, , JOURNAL OF CHEMICAL PHYSICS, Vol: 103, Pages: 1243-1249, ISSN: 0021-9606
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- Citations: 34
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Journal articleFLOWERDEW RJ, HAIGH JD, 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 1693-1696, ISSN: 0094-8276
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- Citations: 67
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Journal articleBalogh A, Southwood DJ, Forsyth RJ, et al., 1995, , 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.
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Journal articleBALOGH A, SMITH EJ, TSURUTANI BT, et al., 1995, , SCIENCE, Vol: 268, Pages: 1007-1010, ISSN: 0036-8075
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- Citations: 261
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Journal articleHAMMOND CM, CRAWFORD GK, GOSLING JT, et al., 1995, , GEOPHYSICAL RESEARCH LETTERS, Vol: 22, Pages: 1169-1172, ISSN: 0094-8276
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- Citations: 20
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Journal articlePICKERING JC, SEMENIUK JI, 1995, , MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 274, Pages: L37-L42, ISSN: 0035-8711
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- Citations: 12
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Journal articleSOUTHWOOD D, 1995, , NATURE, Vol: 375, Pages: 10-10, ISSN: 0028-0836
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Journal articleHAMMOND CM, FELDMAN WC, PHILLIPS JL, et al., 1995, , JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 100, Pages: 7881-7889, ISSN: 2169-9380
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- Citations: 22
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Journal articleBlanco-Cano X, Schwartz SJ, 1995, , Advances in Space 91桃色, Vol: 15, Pages: 97-101-97-101
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Journal articleTHOMPSON P, DOUGHERTY MK, SOUTHWOOD DJ, 1995, , PLANETARY AND SPACE SCIENCE, Vol: 43, Pages: 625-634, ISSN: 0032-0633
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- Citations: 9
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Journal articleReiner MJ, Anderson KA, Roelof E, et al., 1995, , Space Science Reviews, Vol: 72, Pages: 261-266, ISSN: 0038-6308
Both the Ulysses and Galileo spacecraft detected energetic electrons and Langmuir waves that were associated with a type III radio burst on 10 December 1990. At the time of these observations, these spacecraft were in the ecliptic plane and separated by 0.4 AU, with Galileo near the Earth at 1 AU and Ulysses at 1.36 AU. From the measured electron arrival times, the propagation path lengths of the electrons to both Ulysses and Galileo were estimated to be significantly longer than the length of the Parker spiral. These long path lengths are interpreted as due to draping of the interplanetary magnetic field lines around a CME. The onset times of the Langmuir waves at Ulysses and Galileo coincided with the estimated arrival time of the 9 keV and 14 keV electrons, respectively. © 1995 Kluwer Academic Publishers.
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