Solar Energteic Particle Fluences					
May 6, 1998  Event					
Based on Data from ACE/EPAM; GOES-8,11,&12; and SAMPEX/PET					
					
Note: Statistical Uncertainties on GOES andEPAM data are negligible.					
To account for systematic uncertainties in combining data from different					
   sensors we add 20% in quadrature with the statistical uncertainties					
					
Fluence Spectra					
Start: 	0800 UT on 5/6/98				
End:	2400 UT on 5/8/98				
					
Compiled by R. A. Mewaldt (RMewaldt@srl.caltech.edu)					
	with help from Mark Looper, Christina Cohen, and Dennis Haggerty				
					
			    Statistical		
Z	E	Fluence		Sigma	20% sigma	Instrument
1	0.122	4.24E+08		8.48E+07	EPAM
1	0.211	1.60E+08		3.20E+07	
1	0.384	9.23E+07		1.85E+07	
1	0.729	5.66E+07		1.13E+07	
1	1.348	2.73E+07		5.46E+06	
1	2.903	7.53E+06		1.51E+06	
					
1	17.32	1.18E+05		2.36E+04	GOES11-Int
1	38.73	1.95E+04		3.90E+03	
1	54.77	7.54E+03		1.51E+03	
1	77.46	2.63E+03		5.26E+02	
					
1	11.6	2.45E+05		4.90E+04	GOES-11-Diff
1	24.5	9.06E+04		1.81E+04	
1	56.6	7.03E+03		1.41E+03	
1	114.9	6.44E+02		1.29E+02	
					PET
					SAMPEX was in
					spin mode at  this
					time and data are 
					more difficult to
					extract