Spectral plots of energetic particle Fluxes, all observed species

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Multi-Source Spectral Plots (MSSP-2) of energetic particle fluxes, all observed species

About the data
About using this interface
Heliocentric locations of spacecraft
Spectra of H and He from many sources

Please enter your selections and time span, then click on the Submit button below.

Data source	Time span	Time Res.	Species
Data source	Time span	Time Res.	H	He	C	N	O	Ne	Na	Mg	Al	Si	S	Ar	Ca	Fe	Ni
ACE EPAM	1997-08-30 - 2015-05-30	1day
ACE SIS	1997-08-29 - 2020-05-20	1-hr
ACE ULEIS	1998-02-19 - 2020-05-20	1-hr
ACE CRIS	1997-08-27 - 2020-05-20	1-day
ACE SEPICA	1997-10-07 - 2005-02-05	1-hr
NEW HORIZONS	2007-09-19 - 2015-01-15	1-hr
STEREO-A LET, Caltech	2006-11-14 - 2020-04-30	1-hr
STEREO-A SIT, Caltech	2007-01-01 - 2020-05-23	1-hr
STEREO-A SIT Berkeley	2007-03-15 - 2020-02-29	1-hr
STEREO-B LET, Caltech	2006-11-14 - 2014-09-27	1-hr
STEREO-B SIT, Caltech	2007-01-27 - 2014-09-27	1-hr
STEREO-B SIT, Berkeley	2007-03-15 - 2014-09-27	1-hr
Ulysses HISCALE	1990-11-14 - 2009-06-08	1day
Wind EPACT/LEMT	1994-11-03 - 2019-12-31	1-hr
Wind EPACT/STEP	1995-01-01 - 2019-06-16	1-hr

Enter start and stop times over which to make average fluxes for first spectral plot
(Use YYYYMMDD format)
Start Stop

Optional specifications

Enter energy range(MeV/n) for plot and power law fit: Start Stop

Y scale range: Bottom (e.g., 1.0e-5) Top (e.g., 1.0e+1)

Character size(0.5-2.0): Connect Type:

Symbol Size(0.1-4.0): Image size (pixels): X: Y:

This interface was built for the Virtual Energetic Particle Observatory, whose Principal Investigator is John F. Cooper

If you have any questions/comments about this service contact: Dr. Natalia Papitashvili, SPDF, Code 672, NASA/Goddard Space Flight Center, Greenbelt, MD 20771

Character size(0.5-2.0):	Connect Type:
Symbol Size(0.1-4.0):	Image size (pixels): X: Y:

NASA Official: Robert Candey (Robert.M.Candey@nasa.gov), Head of the Space Physics Data Facility