PAMELA time-profiles of protons during 4 Forbush Decreases

Time-profiles of galactic cosmic-ray protons measured by the PAMELA detector in space during 4 Forbush Decreases from March 2012 to June 2015 in various rigidity intervals. Each profile is scaled for a suitable period of quiet Sun, estimated about 10 days before each Forbush Decrease

References

https://iopscience.iop.org/article/10.3847/1538-4357/aaa0c8

Dataset summary

internal_name:

infn_pamela_flux_timeseries

publisher:

not available in DBF

alph_code:

50B

id_tmp:

90

short_name:

PAMELA-proton

identifier:

aspis://INFN-PAMELA/proton

dynamic:

Data collected starts on March 1, 2012 and is increasing with a daily resolution up until July 17, 2015

size:

200kB

format:

csv

type:

timeseries

records_number:

2394

time_start:

2012-03-01

time_stop:

2015-07-17

spatial:

GEOMAG

messenger:

protons

spectral_min:

0.85

spectral_max:

8.68

spectral_units:

GV

observable:

{GCR}

latest update:

2024-04-04 02:12:29

Columns specification

progr

column

units

type

description

1

time

UTC

datetime

datetime (2012-03-01T12:00:00) - time UTC of the data-taking

2

rig_min

GV

float

GV (0.85) - lower edge of the rigidity interval

3

rig_max

GV

float

GV (1.04) - upper edge of the rigidity interval

4

flux

none

float

none (0.949654) - cosmic-ray flux, normalized for a quiet period before the event generating the decrease

5

error_flux

none

float

none (0.0326884) - error on the proton measurement (stat + syst)

6

num_event

none

int

none (0) - Forbush decrease number