![](https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEggjc_bd9GgTzDv1AwHE4-U2FIdiyWZBgpbJwlnEKiGxRXw_DtUlOI01qBxroq1yXXPgyqeF64e3dbWW5cBU6eQ9sLcwPKLocF8-Z21jzJ9No9SIBY3ec8eiDlYwAzyXEHSxRi16Z6JYgQ/s640/kaira_x.png) |
Solar radio Type II and III radio bursts and D-region absorption on 6th of September, seen on the KAIRA realtime display. |
The Sun has been recently quite active. On the 6th, there was an X9-class solar flare, which produced loads of D-region absorption due to increased X-ray flux. There was also solar radio burst activity, including Type III emissions and possibly a Type II emission. The above plot is a screenshot from the KAIRA realtime display, which shows beamlet statistics and D-region absorption measured on one of the RCUs.
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