UPC-PreciseNetwork: EUV solar flux rate
Last modified on Dec 5th, 2023
In This Page
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 (1)
- Name
- Extreme Ultra-Violet solar flux rate
- Observed Property
- Dimensionality Instance
- Dimensionality Timeline
- Units
- Qualifiers
Further Resources and Information
Resources
Go to Metadata FileQuality Assessment
- Data Quality Flags
Data Levels
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 |