UPC-PreciseNetwork: EUV solar flux rate
Last modified on Dec 5th, 2023, 08:00 UTC
Type
Description
Estimating with Least Mean Squares, and independently every 30 seconds, the EUV solar flux rate proxy as the slope in the solar-zenith angle cosine dependence of the solar flare ionospheric footprint (equation 2 in Hernández-Pajares et al. 2012, figures 1, 3 and 5).
Capabilities
Extreme Ultra-Violet solar flux rate
Extreme Ultra-Violet solar flux rate
- Observed Property
- Dimensionality Instance
- Dimensionality Timeline
- Units
- Qualifiers
Data Levels
Quality Assessment
Data Quality Flags
Resources and Further Information
Resources
Metadata File (XML)More Properties
| Property | Value |
|---|---|
| Algorithm | Not used |
| Software Reference | Not used |
Metadata Information
| Editor | Polytechnic University of Catalonia |
| Version | 1 |
| Created | Tuesday 5th Dec. 2023, 08:00 |
| Last Modified | Tuesday 5th Dec. 2023, 08:00 |