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| Format: | Recurso digital |
| Langue: | anglais |
| Publié: |
Zenodo
2025
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| Accès en ligne: | https://doi.org/10.5281/zenodo.17016513 |
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| _version_ | 1866902017209794560 |
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| author | Martens, Janna |
| author_facet | Martens, Janna |
| contents | <p>This Python 3 script reads and corrects RSTN 1 second data (available from <a href="https://www.ngdc.noaa.gov/stp/space-weather/solar-data/solar-features/solar-radio/rstn-1-second/">https://www.ngdc.noaa.gov/stp/space-weather/solar-data/solar-features/solar-radio/rstn-1-second/</a>) from one of the four stations (Learmonth, Palehua, Sagamore Hill and San Vito) for a defined time period. It stores the downloaded raw data in a subfolder. After reading the data into a pandas DataFrame, the data is corrected using the corresponding daily fluxes from Nobeyama Radio Polarimeters (<a href="https://solar.nro.nao.ac.jp/norp/data/daily/">https://solar.nro.nao.ac.jp/norp/data/daily/</a>), to ensure reliable flux values during bursts. Additionally, the background (calculated at a fixed timestamp, defined in 'config.json') is subtracted. The script returns a pandas DataFrame of the raw and corrected fluxes and plots a simple time series with both.</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_17016513 |
| institution | Zenodo |
| language | eng |
| publishDate | 2025 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | RSTN reader with correction and background subtraction Martens, Janna <p>This Python 3 script reads and corrects RSTN 1 second data (available from <a href="https://www.ngdc.noaa.gov/stp/space-weather/solar-data/solar-features/solar-radio/rstn-1-second/">https://www.ngdc.noaa.gov/stp/space-weather/solar-data/solar-features/solar-radio/rstn-1-second/</a>) from one of the four stations (Learmonth, Palehua, Sagamore Hill and San Vito) for a defined time period. It stores the downloaded raw data in a subfolder. After reading the data into a pandas DataFrame, the data is corrected using the corresponding daily fluxes from Nobeyama Radio Polarimeters (<a href="https://solar.nro.nao.ac.jp/norp/data/daily/">https://solar.nro.nao.ac.jp/norp/data/daily/</a>), to ensure reliable flux values during bursts. Additionally, the background (calculated at a fixed timestamp, defined in 'config.json') is subtracted. The script returns a pandas DataFrame of the raw and corrected fluxes and plots a simple time series with both.</p> |
| title | RSTN reader with correction and background subtraction |
| url | https://doi.org/10.5281/zenodo.17016513 |