diff --git a/doc/CMakeLists.txt b/doc/CMakeLists.txt
index 9806708c4..fcf6b355b 100644
--- a/doc/CMakeLists.txt
+++ b/doc/CMakeLists.txt
@@ -95,7 +95,7 @@ set (UG_IMGS
   images/JT65B.png
   images/keyboard-shortcuts.png
   images/MSK144.png
-  images/QRA64.png
+  images/Q65_6m_ionoscatter.png
   images/WSPR_WideGraphControls.png
   images/WSPR_1a.png
   images/WSPR_2.png
diff --git a/doc/user_guide/en/images/Q65_6m_ionoscatter.png b/doc/user_guide/en/images/Q65_6m_ionoscatter.png
new file mode 100644
index 000000000..3979bf41f
Binary files /dev/null and b/doc/user_guide/en/images/Q65_6m_ionoscatter.png differ
diff --git a/doc/user_guide/en/images/QRA64.png b/doc/user_guide/en/images/QRA64.png
deleted file mode 100644
index 929f5c9fc..000000000
Binary files a/doc/user_guide/en/images/QRA64.png and /dev/null differ
diff --git a/doc/user_guide/en/vhf-features.adoc b/doc/user_guide/en/vhf-features.adoc
index 4d8aa3686..38f5d1609 100644
--- a/doc/user_guide/en/vhf-features.adoc
+++ b/doc/user_guide/en/vhf-features.adoc
@@ -178,8 +178,9 @@ image::JT65B.png[align="center",alt="JT65B"]
 Q65 is designed for propagation paths that produce fast fading
 signals: tropospheric scatter, rain scatter, ionospheric scatter,
 trans-equatorial propagation (TEP), EME, and the like.  The following
-screen shot shows an example with submode Q65-30A on a 6-meter
-ionospheric scatter path of about 1100 km.
+screen shot shows a series of ionospheric scatter QSOs using submode
+Q65-30A on the 6 meter band.  The received signals were barely audible
+most of the time.
 
 image::Q65_6m_ionoscatter.png[align="center",alt="Q65"]
 
diff --git a/samples/CMakeLists.txt b/samples/CMakeLists.txt
index d074bdf30..2489b1922 100644
--- a/samples/CMakeLists.txt
+++ b/samples/CMakeLists.txt
@@ -21,7 +21,6 @@ set (SAMPLE_FILES
   JT9/130418_1742.wav
   MSK144/181211_120500.wav
   MSK144/181211_120800.wav
-  QRA64/QRA64C/161113_0111.wav
   WSPR/150426_0918.wav
   Q65/30A_Ionoscatter_6m/201203_022700.wav
   Q65/30A_Ionoscatter_6m/201203_022800.wav