diff --git a/NumericalData/AMDA/Rosetta/IES/ros-elc-az.xml b/NumericalData/AMDA/Rosetta/IES/ros-elc-az.xml index e8546fc..7dacdee 100644 --- a/NumericalData/AMDA/Rosetta/IES/ros-elc-az.xml +++ b/NumericalData/AMDA/Rosetta/IES/ros-elc-az.xml @@ -12,7 +12,7 @@ * Azimuth 225.0-247.5 - Anode #2 * Azimuth 247.5-270.0 - Anode #3 * Azimuth 270.0-292.5 - Anode #4 - I * Azimuth 292.5-315.0 - Anode #5 + * Azimuth 292.5-315.0 - Anode #5 * Azimuth 315.0-337.5 - Anode #6 * Azimuth 337.5-360.0 - Anode #7 * Azimuth 00.0 - 22.5 - Anode #8 @@ -77,11 +77,11 @@ It was discovered after launch, apparently as a result of a light leak, that whe elevation steps 6 and 7 a high count rate may be seen in anodes 8 - 10. - counts + ion counts ros_elc_az - counts + cnts Spectrogram diff --git a/NumericalData/AMDA/Rosetta/IES/ros-ion-az.xml b/NumericalData/AMDA/Rosetta/IES/ros-ion-az.xml index 842018c..cd37170 100644 --- a/NumericalData/AMDA/Rosetta/IES/ros-ion-az.xml +++ b/NumericalData/AMDA/Rosetta/IES/ros-ion-az.xml @@ -12,7 +12,7 @@ * Azimuth 315-360 - Anode #2 * Azimuth 310-315 - Anode #3 * Azimuth 305-310 - Anode #4 - I * Azimuth 300-305 - Anode #5 + * Azimuth 300-305 - Anode #5 * Azimuth 295-300 - Anode #6 * Azimuth 290-295 - Anode #7 * Azimuth 285-290 - Anode #8 @@ -78,11 +78,11 @@ It was discovered after launch, apparently as a result of a light leak, that whe anodes 2 and 3, a high count rate is seen in anode 12. It is also seen in anode 13 when counts in 12 and 13 are combined. - counts + ion counts ros_ion_az - counts + cnts Spectrogram -- libgit2 0.21.2