Cosmic ray origin neutron count measured from a neutron monitor at Jang Bogo Station, Antarctica. AMD_KOPRI collected this data for studying neutron count variation in the southern high latitude. The dataset was last updated in April 2016.
Use Cases
- Analyze temporal variation in neutron count to study solar modulation of cosmic rays.
- Correlate neutron count data with other solar activity indices from the same period.
- Use neutron count measurements for calibrating atmospheric radiation models in Antarctica.
Strengths
- Data originates from a neutron monitor at a dedicated Antarctic research station.
- Focuses on neutron count variation in the southern high latitude, a unique geographic region.
Limitations
- The dataset appears to be a single snapshot from 2016, lacking a clear temporal range.
- No sample data or column information is available, limiting understanding of data structure.
Provenance
- Source
- AMD_KOPRI
- Collection Method
- Measured from neutron monitor at Jang Bogo Station, Antarctica.
- Time Range
- 2016
- Geography
- Jang Bogo Station, Antarctica