A magnetic cloud is a transient ejection in the solar wind defined by relatively strong magnetic fields, a large and smooth rotation of the magnetic field direction over approximately 0.25AU at 1AU, and a low proton temperature [Burlaga et al., 1981]. Magnetic clouds are ideal objects for solar-terrestrial studies because of their simplicity and their extended intervals of southward and northward magnetic fields [Burlaga et al., 1990].
Interval #1 of the First Inter Agency Consultative Group Science Campaign was October 18-21, 1995, which foruitously encompasses this October 1995 magnetic cloud and related events observed by WIND. Many space science teams are working on various aspects of this magnetic cloud, its possible solar origin, and its effects on the Earth's magnetosphere, e.g., see Lepping et al., 1997.
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YR | MON Day(DOY) HR | MON Day(DOY) HR | DT* PHI THETA V** Dia | B H |CHI| asf% [QUAL+] CA%& F# Figures Ref
| | | (deg)(deg) (km/s) (AU) | (nT)
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95 | Feb 8 (039) 03 | Feb 8 (039) 22 | 20 92 6 410 0.224 | 14.2 L .0167 25.0 [1] 34 5.5 f1 f2
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95 | Mar 4 (063) 11 | Mar 5 (064) 04 | 18 205 -82 443 0.190 | 14.4 L .0296 12.2 [2] 52 3.9 f1 f2
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95 | Apr 6 (096) 07 | Apr 6 (096) 18 | 12 147 65 334 0.096 | 14.7 L .0194 11.7 [2] 76 1.0 f1 f2
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95 | May 13 (133) 10.1 | May 13 (133) 15.8 | 5.7 107 -3 331 0.165 | 20.5 L .0088 3.2 [3] 98 4.3 f1 f2
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95 | Aug 22 (234) 22 | Aug 23 (235) 19 | 22 268 4 360 0.233 | 11.8 R .0137 14.5 [1] 35 4.9 f1 f2
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95 | Oct 18 (291) 19 | Oct 20 (293) 00 | 30 289 -10 404 0.249 | 25.6 R .0141 3.3 [1] 8 12.7 f1 f2