Table information for 'solar_flux.main'

General

This table is available for ADQL queries and through the TAP endpoint.

Resource Description:

The “Orbita” Radio Polygon at an altitude of 2750 meters conducts solar radio emission observations using state-of-the-art equipment. This includes instruments for monitoring solar radio flux at frequencies of 1 GHz and 2.8 GHz, as well as the Callisto solar radio spectrograph, which is part of the international e-Callisto network. These tools enable the detection of solar radio bursts of types II, III, IV, and V, and provide valuable insights for forecasting the geo-effectiveness of solar flare activity.

The provided dataset consists of daily tables, where each table corresponds to a single observation day. The data includes two columns:

The data is collected and provided by the Institute of Ionosphere (https://ionos.kz/).

For a list of all services and tables belonging to this table's resource, see Information on resource 'Solar Radio Emission Observations at “Orbita” Radio Polygon'

Citing this table

To cite the table as such, we suggest the following BibTeX entry:

@MISC{vo:solar_flux_main,
  year=2024,
  title={Solar Radio Emission Observations at “Orbita” Radio Polygon},
  author={Fesenkov Astrophysical Institute},
  url={https://dachs.fai.kz/tableinfo/solar_flux.main},
  howpublished={{VO} resource provided by the {FAI} archives}
}

Columns

Sorted alphabetically. [Sort by DB column index]

NameTable Head DescriptionUnitUCD
flux Flux Solar radio flux density measured in Solar Flux Units (SFU). SFU phot.flux.density;em.radio
obs_mjd Observed at Universal time of the observation at the detector as MJD. d time.epoch
obs_time Timestamp Universal time of the observation at the detector. N/A time.epoch
source_path Src. File this row was parsed from. N/A meta.id;meta.file

Columns that are parts of indices are marked like this.

Other

The following services may use the data contained in this table:

VOResource

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