Index: /trunk/BNC/bnchelp.html
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--- /trunk/BNC/bnchelp.html	(revision 1870)
+++ /trunk/BNC/bnchelp.html	(revision 1871)
@@ -410,5 +410,5 @@
 </p>
 <p>
-When using clocks from Broadcast Ephemeris (with or without applied corrections) or clocks from SP3 files, it is important to understand that they are not corrected for the 2nd-order relativistic effect. The 2nd-order relativistic effect is a priodic time correction defined as -2 (R * V) / c^2 and includes the scalar product of satallite position and velocity divided by the speed of light raised to the second power.
+When using clocks from Broadcast Ephemeris (with or without applied corrections) or clocks from SP3 files, it may beimportant to understand that they are not corrected for the 2nd-order relativistic effect. The 2nd-order relativistic effect is a priodic time correction defined as -2 (R * V) / c^2 and includes the scalar product of satallite position and velocity divided by the speed of light raised to the second power.
 </p>
 
@@ -482,5 +482,5 @@
 </pre>
 <p>
-In case of RTCM message types 1058 or 1064 the first four parameters are followed by
+In case of RTCM message types 1058 or 1064 the first five parameters are followed by
 </p>
 <ul>
@@ -505,5 +505,5 @@
 </p>
 <p>
-In case of RTCM message types 1060 or 1066 the first four parameters are followed by
+In case of RTCM message types 1060 or 1066 the first five parameters are followed by
 <p>
 <ul>
@@ -537,5 +537,5 @@
 </p>
 <p>
-In case of RTCM message types 1059 or 1065 the first four parameters are followed by
+In case of RTCM message types 1059 or 1065 the first five parameters are followed by
 <ul>
 <li>Number of Code Biases</li>
Index: /trunk/BNS/bnshelp.html
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--- /trunk/BNS/bnshelp.html	(revision 1870)
+++ /trunk/BNS/bnshelp.html	(revision 1871)
@@ -316,5 +316,5 @@
 
 <p>
-When using clocks from Broadcast Ephemeris (with or without corrections) and clocks from SP3 files in the same application, it is important to understand that Broadcast Ephemeris clocks - according to the Interface Control Documents (ICD) - are corrected for the 2nd-order relativistic effect whereas clocks from SP3 files are not. The 2nd-order relativistic effect is a priodic time correction defined as -2 (R * V) / c^2 and includes the scalar product of satallite position and velocity divided by the speed of light raised to the second power. 
+When using clocks from Broadcast Ephemeris (with or without applied corrections) or clocks from SP3 files, it may be important to understand that they are not corrected for the 2nd-order relativistic effect. The 2nd-order relativistic effect is a priodic time correction defined as -2 (R * V) / c^2 and includes the scalar product of satallite position and velocity divided by the speed of light raised to the second power. 
 </p>