Utah State University
Center for Atmospheric and Space Science
Bear Lake Observatory
25.5 MHz Riometer
for studies of the ionospheric D Region
Riometers receive radio frequency energy, and then produce a voltage relative
to the amount of energy received. The BLO (Bear Lake Observatory) Riometer
specifically measures frequencies between 25.2 and 25.8 MHz. The BLO Riometer
can produce anywhere from zero volts, meaning no energy is being received, to
its maximum of 7.2 volts. Its antennae allow for coverage of the majority of
the sky. For the most part, the energy received comes from astronomical radio
sources like the star Cassiopeia A, Jupiter, the Milky Way center, and the
sun, but there are also some terrestrial sources occasionally picked up by
the riometer.
The objective of the riometer is to allow us to analyze absorption of radio
waves in the upper atmosphere (particularly the ionosphere). This subject is
of interest because the level of absorption affects communications here on
earth. If the absorption is low, communications will not be affected greatly
but if absorption is high communication with radio waves can be virtually
useless. While we know some of the reasons for fluctuations in absorption
there are still many unknowns. Hopefully we can discover some of these
unknowns by cross-referencing our riometer data with phenomena that may be
affecting absorption in the ionosphere and thus discover reasons for the
fluctuations.
Daily plots in the summaries include the minimum, maximum, and median
values for 30 second acquisition intervals. Solar x-ray flares of M-
and X-class are indicated on the plot, as are Type II and Type IV solar
radio bursts in the HF range. Due to frequent power outages, the hourly
calibration pulses in the riometer data are not time-synchronized.