Cosmic ray neutron count data was collected from a neutron monitor at the Jang Bogo Station in Antarctica. The dataset documents variations in neutron flux at a southern high-latitude location. It was produced by the AMD_KOPRI organization and last updated in September 2021.
Use Cases
- Analyzing temporal variations in neutron count to correlate with solar activity cycles.
- Studying the relationship between neutron flux intensity and geomagnetic conditions at high southern latitudes.
- Validating and calibrating models for cosmic ray propagation and modulation in the heliosphere using ground-based Antarctic measurements.
Strengths
- Data originates from a dedicated neutron monitor at a unique Antarctic research station.
- Focuses on cosmic ray measurements from the southern high-latitude region, a key location for space weather studies.
Limitations
- The specific temporal coverage within 2021 is unknown, limiting longitudinal analysis.
- The dataset size, row count, and available features are unspecified, hindering assessment of scope.
Provenance
- Source
- AMD_KOPRI via NASA Earthdata.
- Collection Method
- Measured from a neutron monitor.
- Time Range
- 2021
- Freshness
- Data is from 2021, with no stated update frequency.
- Geography
- Jang Bogo Station, Antarctica (southern high latitude).