The Alma-Ata Cosmic Ray Station operates the 18NM-64 neutron supermonitor
at an altitude of 3340 meters above sea level with a geomagnetic cutoff
rigidity of 6.7 GeV. The station provides real-time minute-level measurements of
cosmic ray intensity and atmospheric pressure, contributing data to the
international NMDB network (http://www.nmdb.eu).
This service publishes daily tables containing two columns:
- **timestamp**: Actual measurement times, ensuring accurate tracking.
- **counts/sec**: Cosmic ray intensity in counts per second.
The timestamps reflect actual measurement times, ensuring accurate
tracking even when delayed data from previous days is incorporated into
current files due to communication delays with space stations.
The data is collected and provided by the Institute of Ionosphere (https://ionos.kz/).
Solar Radio Emission Observations at “Orbita” Radio Polygon
Short Name:
solar_flux data
Date:
12 Dec 2024 19:58:36
Publisher:
Fesenkov Astrophysical Institute
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:
- **timestamp**: The time of observation at the detector.
- **SFU**: The solar flux unit measurement, representing the intensity of solar radio emission in SFU (Solar Flux Units).
The data is collected and provided by the Institute of Ionosphere (https://ionos.kz/).
