Abstract: An overview of the radio observations during May 2024 is given.
The graphs show both the daily totals (Figure 1) and the hourly numbers (Figure 2) of “all” reflections counted automatically, and of manually counted “overdense” reflections, overdense reflections longer than 10 seconds and longer than 1 minute, as observed here at Kampenhout (BE) on the frequency of our VVS-beacon (49.99 MHz) during the month of May 2024.
The hourly numbers, for echoes shorter than 1 minute, are weighted averages derived from:
The past month has been anything but boring. Local interference and unidentified noise remained quite low for most of the month, but lightning activity was detected on 12 different days. Sometimes it was intense and lasting for hours, as on May 1, 12, 18, 19, and 26, significantly hindering meteor counting.
Also, the Sun was very active, with powerful outbursts almost daily, usually of type III, which sometimes hampered meteor recordings for several minutes (Figures 3 to 5).
On May 10 and 11 exceptionally powerful auroras were also visible from Belgium, the most intense being recorded on the frequency of our beacon (Figures 6 to 8).
During the second half of the month there were temporary problems with the transmission power of our beacon, but these apparently only had a minor impact on the observations.
The meteor activity was also particularly interesting. As expected, the eye-catchers were the eta-Aquariids that reached their maximum on May 4–6. Apparently, the long-lasting reflections (and therefore more massive meteoroids) came earlier than the shorter ones.
The last days of the month were notable for the suddenly increasing number of underdenses and short overdenses. During the entire month 16 reflections longer than 1 minute were recorded. A selection of these, along with some other interesting reflections is included (Figures 9 to 28). More of these are available on request.
In addition to the usual graphs, you will also find the raw counts (subject to strict reservations as previously said) in cvs-format from which the graphs are derived. The table contains the following columns: day of the month, hour of the day, day + decimals, solar longitude (epoch J2000), counts of “all” reflections, overdense reflections, reflections longer than 10 seconds and reflections longer than 1 minute, the numbers being the observed reflections of the past hour.