SVIRCO Observatory - the Rome neutron monitor (5m)¶
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: 5min Average intensity of January-February 1997 = 100%
References¶
Dataset summary¶
internal_name: |
inaf_flux5m_svirco_timeseries |
publisher: |
INAF |
alph_code: |
42B |
id_tmp: |
74 |
short_name: |
flux5m_SVIRCO |
identifier: |
inaf_flux5m_svirco_timeseries |
dynamic: |
Data collection grows in time. |
size: |
80MB |
format: |
CSV |
type: |
timeseries |
records_number: |
2007072 |
time_start: |
1997-05-21 |
time_stop: |
2017-01-01 |
spatial: |
GROUND |
messenger: |
Neutrons |
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 |
inc |
counts |
int |
Counting rates (not pressure corrected) of the cosmic ray secondary nucleonic component measured by the Rome neutron monitor |
3 |
pressure |
hPa |
float |
Pressure measured at the SVIRCO Observatory |
4 |
corr |
counts |
int |
Efficiency and pressure corrected counting rates of the cosmic ray secondary nucleonic component measured by the Rome neutron monitor |