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PAMELA time-profiles of protons during 4 Forbush Decreases
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.. contents:: The tiny table of contents

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

Data description
~~~~~~~~~~~~~~~~

**internal_name:** infn_pamela_flux_timeseries

**publisher:** not available in DBF

**alphanumeric_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
~~~~~~~~~~~~~~~~~~~~~

.. list-table:: 
   :widths: 7 20 15 10 48
   :align: right 
   :header-rows: 1

   * - 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
