SVIRCO Observatory - the Rome neutron monitor (1h)¶
Intensity in percent of cosmic ray secondary nucleonic component of Rome neutron monitor. Data corrected for pressure with barometric coefficient variable with solar cycle and corrected for efficiency changes. Resolution: 1h. Average intensity of January-February 1997 = 100%
References¶
Dataset summary¶
internal_name: |
inaf_flux1h_svirco_timeseries |
publisher: |
INAF |
alph_code: |
42C |
id_tmp: |
73 |
short_name: |
flux1h_SVIRCO |
identifier: |
inaf_flux1h_svirco_timeseries |
dynamic: |
Data collection grows in time. |
size: |
13MB |
format: |
CSV |
type: |
timeseries |
records_number: |
479976 |
time_start: |
1966-04-01 |
time_stop: |
2020-12-31 |
spatial: |
GROUND |
messenger: |
Nucleons |
spectral_min: |
6.3 |
spectral_max: |
9999 |
spectral_units: |
GeV |
observable: |
{GLE,GCR} |
latest update: |
2024-03-28 05:08:05 |
Columns specification¶
progr |
column |
units |
type |
description |
|---|---|---|---|---|
1 |
time |
UTC |
datetime |
UTC - Time |
2 |
I |
% |
float |
% - Normalized Intensity of the cosmic ray secondary nucleonic component measured by the Rome neutron monitor. The counting rates have been normalized to the reference value of January-February 1997 (= 100%). |