Table of Contents

ath9k spectral scan

Atheros 802.11n chipsets include a built-in spectral analysis feature. AR92xx and AR93xx have the ability to report FFT data from the baseband under software controlled conditions, including:

These information can be used to create an open source spectrum analyzer or interference classifier. To try it out, you must first have a kernel compiled with config option ATH9K_COMMON_SPECTRAL and one or both of ATH9K_DEBUGFS and ATH9K_HTC_DEBUGFS. Then you can use the following commands to acquire samples for all channels which can be scanned:

echo chanscan > /sys/kernel/debug/ieee80211/phy0/ath9k/spectral_scan_ctl
iw dev wlan0 scan
cat /sys/kernel/debug/ieee80211/phy0/ath9k/spectral_scan0 > samples
echo disable > /sys/kernel/debug/ieee80211/phy0/ath9k/spectral_scan_ctl

Spectral scan configuration parameters can be read and changed /sys/kernel/debug/ieee80211/phy0/ath9k/:

Spectral scan parameters

Frame format

HT20:

      0       1       2       3       4       5       6       7       8
      +---------------------------------------------------------------+
 0    |       [7:0]: bin -28 magnitude (|i| + |q|) >> max_exp         |
      +---------------------------------------------------------------+
 1    |       [7:0]: bin -27 magnitude (|i| + |q|) >> max_exp         |
      +---------------------------------------------------------------+
 2-54 |                                                               |
      +---------------------------------------------------------------+
 55   |       [7:0]: bin 27 magnitude (|i| + |q|) >> max_exp          |
      +---------------------------------------------------------------+
 56   |       [7:0]: all_bins {max_magnite[1:0], bitmap_weight[5:0]}  |
      +---------------------------------------------------------------+
 57   |               [7:0]: all_bins {max_magnite[9:2]}              |
      +---------------------------------------------------------------+
 58   |       [7:0]: all_bins {max_index[5:0], max_magnite[11:10]}    |
      +---------------------------------------------------------------+
 59   |                       [3:0] max_exp                           |
      +---------------------------------------------------------------+

HT40:

      0       1       2       3       4       5       6       7       8
      +---------------------------------------------------------------+
0     |       [7:0]: bin -64 magnitude (|i| + |q|) >> max_exp         |
      +---------------------------------------------------------------+
1     |       [7:0]: bin -63 magnitude (|i| + |q|) >> max_exp         |
      +---------------------------------------------------------------+
2-125 |                                                               |
      +---------------------------------------------------------------+
127   |       [7:0]: bin 63 magnitude (|i| + |q|) >> max_exp          |
      +---------------------------------------------------------------+
128   |    [7:0]: lower_bins {max_magnite[1:0], bitmap_weight[5:0]}   |
      +---------------------------------------------------------------+
129   |               [7:0]: lower_bins {max_magnite[9:2]}            |
      +---------------------------------------------------------------+
130   |       [7:0]: lower_bins {max_index[5:0], max_magnite[11:10]}  |
      +---------------------------------------------------------------+
131   |    [7:0]: upper_bins {max_magnite[1:0], bitmap_weight[5:0]}   |
      +---------------------------------------------------------------+
132   |               [7:0]: upper_bins {max_magnite[9:2]}            |
      +---------------------------------------------------------------+
133   |       [7:0]: upper_bins {max_index[5:0], max_magnite[11:10]}  |
      +---------------------------------------------------------------+
134   |                       [3:0] max_exp                           |
      +---------------------------------------------------------------+

Received power computation

Assuming the noise floor is equal to -96dbm(*) and the magnitude of each sample in a 20MHz bin equals the RSSI, the received signal strength of each FFT bin on HT20 channel can be computed as follow:

power(i) = nf + RSSI + 10*log(b(i)^2) - bin_sum

where:

For 40MHz channel, previous formula should be used for 64 bins of control and extension channels, keeping in mind for HT40+ mode the extension channel is above the primary one (lower=ctl, upper=ext) and for HT40- the extension channel is below the primary one (lower=ext, upper=ctl).

(*) nf can differ from -96dbm due to noise and spikes leading to a reduced reported RSSI.

Userspace programs

FFT samples gathered from Atheros NICs could be drawn using userspace programs:

(based on Adrian Chadd's documentation https://wiki.freebsd.org/dev/ath_hal%284%29/SpectralScan)