Cosmic noise measurements at 38.2 MHz were recorded by a solid-state riometer and dual dipole antenna at the Italian Antarctic Base in Terra Nova Bay. The data are intended for studying ionospheric absorption in the lower ionosphere and the physical-chemical mechanisms in the D region. The dataset was last updated in February 1994 and originates from the SCIOPS organization.
Use Cases
- Modeling ionospheric absorption based on cosmic noise measurements.
- Investigating physical-chemical mechanisms in the D ionospheric region.
- Developing multivariate indices for monitoring the ionosphere-magnetosphere system.
- Analyzing long-term cosmic noise time series for space weather studies.
Strengths
- Data is sourced from a specific, documented location: Terra Nova Bay, Italian Antarctic Base.
- Measurements are from a defined instrument: a solid-state riometer and dual dipole antenna at 38.2 MHz.
Limitations
- Last updated 1994-02-03 23:59:59.999000; freshness should be verified.
- Column-level documentation is absent; field semantics must be inferred after download.
- Row count and file formats are unknown, which may limit suitability assessment.
Provenance
- Source
- SCIOPS
- Collection Method
- Cosmic noise received at 38.2 MHz by a solid-state riometer and dual dipole antenna.
- Time Range
- null
- Freshness
- Last updated 1994-02-03 23:59:59.999000.
- Geography
- Terra Nova Bay, Italian Antarctic Base, Antarctica.