93030  2300	93031  0900	IR/BzS		8	Simultaneous to mple. bow shock crossings
93153  2000     93155  0300     IR		8       Corrotating IR after a LSS (~330Km/s), 
94148  1400     94149  0600	IR		8	Stream-stream interactive region, press here
94330  0100     94331  1200     IR              W       From LSS to HSS, it includes periods of sharp 
94339  2100     94340  0640     IR              W/8     From LSS to HSS, it includes SBCs, periods of strong
95001  1940     95003  1930     IR              W       From LSS to HSS, starts at a forward IS, with BzN, it includes
95016  0110	95018  0600	BzS/IR/PC/SBC	W	Pressure increases to 18nPa and 20nT near DOY 18
95028  1800     95030  1000     IR              W       From LSS to HSS with ram and magnetic PCs, SBCs.
95041  2300	95044  1300	IR		W	From LSS to HSS with ram and B field PCs
95056  1440     95060  0720     IR              W       From LSS to HSS, starting with BzS, and strong EyCs,
95068  0100     95071  0220     IR              W       From 400 Km/s SW to HSS, including SBCs,
95082  0940     95082  0940     IS              W       Forward shock, start of the IR, ISTP Sun-Earth Connection Event
97173  0300	97175  0000	IR/EyC/PC	W
97178  0100	97178  1300	IR/PC/EyC	W
97188  0200	97189  0000	IR		W
97199  0030	97199  2330	IR/EyC		W
97205  0000	97205  1900	IR/PC/EyC/SBC	W/8
97211  1640	97212  1300	IR		W
97239  2000	97240  1100	IR/EyC/SBC	W	Interval with multiple sharp SBCs
97245  2240	97247  0900	IR/EyC/PC	W	SW low-high speed stream IR
98039  1000	98040  1800	EyC/PC/SBC	W/8	Period with multiple EyC, SBC and PC, a possible stream-stream IR
98069  0030	98070  0000	IR/EyC/BzS/PC	W/8	Period with SW speed changing from under 300 to 550 km/s and
98080  0300	98080  2045	IR/EyC/PC/BzS,N W/8
98107  0100	98108  1520	IR/EyC/PC	W/8
98148  1430	98149  2330	IR/EyC/PC/BSC	W	Interval of time with GEOTAIL in the SW
98154  0320	98154  15	IR/EyC/SBC/PC	W/8	Interval contains a sharp ramPressure pulse 
98156  1100	98158  0045	IR/EyC/PC	W/8
98169  2000	98171  0630   IR/BzS/BzN/PC/EyC	W/8	IR with a possible pressure wave ahead of IR
99138  0015	99138  1910	IR/EyC/PC	W	Possibly CIR interval
99202  0900	99203		IR/EyC/PC	W/ACE   Period with multiple EyCs, 
99227  0941	99229  0140	IR/EyC/PC	ACE	A low-high speed stream-stream SW interaction region
99235  1140	99238  2200	IR		W/ACE
99255  0352	99256  1630	IR/EyC		W/ACE
99269  1850	99270  1600	IR		W/ACE	low-high speed stream-stream interaction region
99282  1500	99283  1100	SBC/PC/EyC 	W/ACE	Possibly part of IR, from low to fast speed stream
99283  0900	99287  2200	PC/EyC/MISC	W/ACE	Possibly extended low-high speed stream-stream IR
99294  0140	99296  		IR		W/ACE
				IR/EyC/PC		and well above historical magnetic field strength in the heliosphere,
99337  0800	99339  0800	IR/EyC/BzS	W/ACE
99364  1600	99364  1600	SBC/EyC/PC/MISC	ACE	Magnetic hole at SBC and possibly IR interface
00027  1356	00027  2322	IR/EyC/PC	W/ACE	Strong corotating compression region between slow and high speed SW streams
00036  1450	00037  0530	IR/EyC/PC	W/ACE
00054  1200     00055  1408	IR/PC/EyC	W/ACE	A near monotonic rise of the solar wind speed from 400 to 800 km/s
00055  1408	00055  1408	IS		ACE	IR related Reverse fast shock, spike in keV shock energized particles
00072  0200	00072  1500	PC/EyC/SBC	W/ACE	Possible slow-fast stream-stream IR
00082  1100	00082  1800	CIR		W/ACE
00108  0400	00108  0940	IR/EyC/PC	W/ACE
00115  0400			IR		W/ACE
00123  0900	00123  1300	IR/SBC/EyC	W/ACE	Low density interval, and in part very fast (solar wind V>900km/s) Ejecta?
00133  1400	00134  0800	IR/PC/EyC	W/ACE
00150  0600	00151  0140	IR		W/ACE
00159		00160  09	IR/MISC		W/ACE	IR possibly associated to more than one polarity HSS interval
00160  0904	00160  1100	PC/EyC/IR	W/ACE
00163  1242	00163  2100	PC/EyC/BzS/BzN	ACE	Possibly IR
00167  0100	00167  1220	IR		W/ACE
00175  1227	00176  0720	EyC/PC/IR	W/ACE
00193  1124	00193  2300	IR/EyC/PC	W/ACE
00218  0000	00218  0800	PC/EyC/BzS	ACE	Possible an IR bw slow and fast SW streams, also IS possible  at ~0400UT
00240  1700	00242  0900	IR		W/ACE
00267  1345	00268  0210	IR/EyC/PC	W/ACE	Interval contains multiple EyCs and PCs (Y-GSE(WI) = -250 RE)
00267  1345	00268  0210	BzS		ACE	A mostly southward IMF (during extended slow-fast stream-stream IR)
00288  1300	00289  0800	IR		W/ACE
00309  0150	00310  0800	IR/PC/SBC/EyC	W/ACE	Possibly LSS-HSS interaction (HSS related to coronal hole)

This server and the information being made available are evolving as the ISTP Pr
oject evolves.
Questions or comments should be sent to the authors at the address below.




Curator:


 Daniel Berdichevsky - Raytheon-ITSS Corporation at ISTP Science Planning and Operations Facility(SPOF) <
b>
(berdi@istp1.gsfc.nasa.gov)


 NASA contact for these pages: Dr. R. Lepping, Code 696, email: rpl@leprpl1.
gsfc.nasa.gov



 Last updated: November 27, 2000