Solar Energteic Particle Fluences					
May 2, 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: 	1400 UT on 5/2/98				
End:	2400 UT on 5/5/98				
					
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	0.0399	2.91E+10		5.82E+09	EPAM
1	0.0659	1.05E+10		2.10E+09	
1	0.119	4.46E+09		8.92E+08	
1	0.2073	1.35E+09		2.70E+08	
1	0.3792	4.46E+08		8.92E+07	
1	0.723	1.28E+08		2.56E+07	
1	1.34	3.56E+07		7.12E+06	
1	2.89	7.38E+06		1.48E+06	
					
1	17.32	1.55E+05		3.10E+04	GOES11-Int
1	38.73	3.96E+04		7.92E+03	
1	54.77	1.87E+04		3.74E+03	
1	77.46	7.17E+03		1.43E+03	
					
1	11.6	2.47E+05		4.94E+04	GOES-11-Diff
1	24.5	1.32E+05		2.64E+04	
1	56.6	1.75E+04		3.50E+03	
1	114.9	2.00E+03		4.00E+02	
					PET
					SAMPEX was in
					spin mode at  this
					time and data are 
					more difficult to
					extract