63 sec pulse, ripples, dropouts polb
02feb22
Intro
Callisto data from 02feb22 was used to examine
the callisto output.
We saw:
- a 63 second periodic pulse around 27 MHz
- 2.4 MHz ripple across the band that turned on suddenly.
- dropouts in pol B
The data:
The first plots shows the total power
(20 to 80 MHz) vs time for then entire day (.ps) (.pdf)
- Black is polA, red is pol B
- The points are sampled every .25 seconds.
- The green lines show the data used to look at the 63 second
period pulses.
- The blue line has the start of the ripples
- Both polA and B increase when the ripples start (polA more
than pol B).
- The negative going spikes in pol B are the pol B dropouts.
- the blowup plots show that they are not resolved in the .25
sec spectra.
- Looking at the dynamic spectra, the dropouts are across the
entire band.
- They are not seen in polA.
The second set of plots have blowups around the 2 regions
(.ps) (.pdf)
- Page 1: 63 second pulses total and pol B dropouts
- Top: 45 minutes of total power vs time using 25 to 30 MHz.
- the positive going spikes are the 63 sec pulse.
- The large negative going pulses (pol B) are the pol B
dropouts. they are about 2 counts.
- Middle: total power spectrum (magnitude).
- 45 minutes of data (at .25 sec sampling) was transformed
to get the frequency of the pulses.
- There is a comb present.
- the 29th harmonic is .47528 hz , so the fundamental is
(.47528/30)= .01584 Hz or 63.1 seconds.
- bottom: fold the total power vs time data at 63.1 seconds
- Black is polA, red is pol B.
- blue is a single period before folding.
- The power goes down (below the mean value) for about
3 seconds and then goes up (above the mean value) for 2
seconds.
- The image shows the
dynamic spectra for these 45 minutes (.gif)
- The pulses are occurring around 27 MHz.
- the lower frame is pol B. The vertical black strips are
the pol B dropouts.
- The power dropout before the pulse would normally be caused
by out of band compression.
- If the signal was compressed for 3 seconds, we should also
see a dark line across the entire band (which we don't see).
- This may be an instrumental affect.
- Page 2: spectral ripples.
- Top: total power vs time when ripples start
- black is polA, red is pol B
- the ripples turn on around 13.587. Both polA and pol B
power increase at the turn on.
- the negative red going spikes are the pol B dropouts.
- 2nd: total power vs time blowup at ripple turnon.
- the +'s are the .25 second samples
- the polA spike comes 1 sample before the pol B spike.
- 3rd: spectral density plots at the ripple turn on.
- black is before the start
- red is at the start
- green is after the start.
- bottom: average acf of the spectra
- The acf was computed for each spectra (starting after the
turn on) and then averaged
- The plot shows the acf vs the lag delay (in usecs).
- There is a spike at .405 microseconds. This would be a
1/.405 2.47 MHz ripple.
- We saw a similar lag delay in the 27jan22 data.
The following images show the dynamic spectra and acf vs lag delay
at the ripple turnon
SUMMARY:
- A 63.1 second periodic pulse around 27.5 MHz is seen in the
data
- there is a 3 second total power decrease followed by a 2
second increase
- Since the decrease is not seen across the entire freq band,
it is probably not out of band compression.
- Dropouts were seen in pol B
- they cover the entire frequency band
- they are not resolved in the .25 second samples.
- they do not occur in polA
- 2.4 MHz ripples
- Turn on fast (1 sample)
- At turn on there is a large oscillation (at the 2.4 MHz
ripple period) across a portion of the band.
- The large oscillation occurs 1 time sample (.25 sec) later
in pol B.
- this has been seen in multiple days.
processing: x101/220202/callisto_ripple_dropouts.pro
callisto page