This data set, created in 2010 by Nand Lal,
contains 30-min resolution fluxes and count rates of
energetic protons, alpha particles, electrons and
X-rays from the E7 experiment (P.I.: J. Trainor, GSFC)
flown on the Helios 1 spacecraft. Accompanying each
flux and count rate is a statistical uncertainty of the
flux or rate. The data are spin-averaged. The data
are in 920-character ASCII records and consist of:
A. Proton fluxes based on pulse height and rate data
in 7 energy windows, 3.40-6.05, 6.05-11.10, 11.10-21.60,
24.52-28.82, 32.00-46.30, 45.30-57.22, 135.2-206.5 MeV.
B. Alpha particle fluxes based on pulse heights and count
rates in 6 energy windows, 3.20-4.98, 4.98-11.50,
11.50-21.60, 24.51-31.12, 31.12-45.53, 45.53-57.53 MeV/n.
C. Combined proton plus alpha particle fluxes based on
LET1 and HET count rates in 6 energy windows, 3-6, 6-11,
11-21, 20-30, 32-45, 45-56 MeV/n.
D. Alpha particle fluxes based on HET count rates in three
energy windows, 20-30, 32-45, 45-57 MeV/n.
E. Two count rates primarily due to electrons at 2-4 and
4-8 MeV.
F. 21 additional count rates corresponding to individual
telescope sensors or sensor combinations. For one sensor,
rates at each of several discrimination levels are given).
These rates are further discussed in the documentation and
in the references provided. A subset of the above
parameters (A, B, E) are available with graphical display
at the OMNIWeb-Plus interface identified below
Version:2.2.9
This data set, created in 2010 by Nand Lal,
contains 30-min resolution fluxes and count rates of
energetic protons, alpha particles, electrons and
X-rays from the E7 experiment (P.I.: J. Trainor, GSFC)
flown on the Helios 1 spacecraft. Accompanying each
flux and count rate is a statistical uncertainty of the
flux or rate. The data are spin-averaged. The data
are in 920-character ASCII records and consist of:
A. Proton fluxes based on pulse height and rate data
in 7 energy windows, 3.40-6.05, 6.05-11.10, 11.10-21.60,
24.52-28.82, 32.00-46.30, 45.30-57.22, 135.2-206.5 MeV.
B. Alpha particle fluxes based on pulse heights and count
rates in 6 energy windows, 3.20-4.98, 4.98-11.50,
11.50-21.60, 24.51-31.12, 31.12-45.53, 45.53-57.53 MeV/n.
C. Combined proton plus alpha particle fluxes based on
LET1 and HET count rates in 6 energy windows, 3-6, 6-11,
11-21, 20-30, 32-45, 45-56 MeV/n.
D. Alpha particle fluxes based on HET count rates in three
energy windows, 20-30, 32-45, 45-57 MeV/n.
E. Two count rates primarily due to electrons at 2-4 and
4-8 MeV.
F. 21 additional count rates corresponding to individual
telescope sensors or sensor combinations. For one sensor,
rates at each of several discrimination levels are given).
These rates are further discussed in the documentation and
in the references provided. A subset of the above
parameters (A, B, E) are available with graphical display
at the OMNIWeb-Plus interface identified below
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | DataProducer | spase://SMWG/Person/Nand.Lal |
Listing of parameters in data records
Primary parameters of data product, with graphical display
Spectral plots and power law fits for arbitrary durations
Proton fluxes and associated statistical
uncertainties for the seven energy ranges 3.40-6.05, 6.05-11.10,
11.10-21.60, 24.52-28.82, 32.00-46.30, 45.30-57.22, 135.2-206.5
MeV. The fluxes are obtained by combining pulse height and count
rate data.
Seven rows of pairs of proton flux and
statistical uncertainty in the flux. The rows correspond
to the seven energy ranges given above.
Alpha particle fluxes and associated statistical
uncertainties for the six energy ranges 3.20-4.98, 4.98-11.50,
11.50-21.60, 24.51-31.12, 31.12-45.53, 45.53-57.53 MeV/n.
The fluxes are obtained by combining pulse height and count
rate data.
Six rows of pairs of alpha particle flux and
statistical uncertainty in the flux. The rows correspond
to the six energy ranges given above.
Fluxes for mixed protons and alpha particles,
and associated statistical uncertainties, for the six energy ranges
3-6, 6-11, 11-21, 20-30, 32-45, 45-56 MeV/n. The fluxes are based
on count rates only, without any pulse height analysis.
Six rows of pairs of proton flux and
statistical uncertainty in the flux. The rows correspond
to the six energy ranges given above.
Fluxes of alpha particles and associated
statistical uncertainties, for the three energy ranges
20-30, 32-45, 45-57 MeV/n. The fluxes are based on count
rates only, without any pulse height analysis.
Three rows of pairs of alpha particle
flux and statistical uncertainty in the flux. The rows correspond
to the three energy ranges given above.
Count rates primarily due to electrons, and
associated statistical uncertainties, for the two energy ranges
2-4 and 4-8 MeV.
Two rows of pairs of electron count rate
and statistical uncertainty in the rate. The rows correspond
to the 2-4 and 4-8 MeV energy ranges.
21 additional count rates corresponding to
individual telescope sensors or sensor combinations. For one
sensor, rates at each of several discrimination levels are
given). These rates are further discussed in the documentation
and in the references provided. They are not likely to be widely
useful
21 rows of pairs of various count rate
and statistical uncertainty in the rate.