diff --git a/Instrument/AMDA/Helios1/MAG.xml b/Instrument/AMDA/Helios1/MAG.xml
index c4048de..708b189 100644
--- a/Instrument/AMDA/Helios1/MAG.xml
+++ b/Instrument/AMDA/Helios1/MAG.xml
@@ -7,24 +7,24 @@
       <ResourceName>MAG</ResourceName>
       <AlternateName>Helios Magnetometers : E2, E3</AlternateName>
       <ReleaseDate>2018-10-20T21:10:13Z</ReleaseDate>
-      <Description>E2 : The Förster probe experiment E2 is a three component-vector magnetometer. Its purpose is to
-continuously observe the interplanetary magnetic field in a frequency range up to 4 Hz. Thereby certain
-phenomena are to be analysed as a function of the distance from the sun e.g. the spiral structure and
+      <Description>E2 : The Förster probe experiment E2 is a three component-vector magnetometer. Its purpose is to 
+continuously observe the interplanetary magnetic field in a frequency range up to 4 Hz. Thereby certain 
+phenomena are to be analysed as a function of the distance from the sun e.g. the spiral structure and 
 discontinuities. The measurement ranges are ± 100 nT and ± 400 nT. The resolution is ± 0.2 nT and ±
 0.8 nT respectively.
 
-For accurate measurements of the zero offset of each sensor the component parallel to the spinaxis can
-be flipped by 90°. Depending on telemetry format and bitrate the digital data are fed into a time average
-computer or directly connected to telemetry. A shock identification-computer triggers the S/C core
+For accurate measurements of the zero offset of each sensor the component parallel to the spinaxis can 
+be flipped by 90°. Depending on telemetry format and bitrate the digital data are fed into a time average 
+computer or directly connected to telemetry. A shock identification-computer triggers the S/C core 
 memory in case of discontinuities with variations of the ambient magnetic field magnitude.
 
-The Förster probe experiment E2 is a three-axe vector magnetometer. It is used for the continuous
-observation of the interplanetary magnetic field in a frequency range from 0 to 4 Hz. This will be
-investigated phenomena such as the spiral structure and discontinuities as a function of the distance
-from the Sun. The measuring ranges are ± 100 nT and ± 400 nT with a resolution of ± 0.2 nT or ± 0.8 nT.
-The component that is parallel to the axis of the spin, to perform precise zero point provisions of each
-sensor is rotated 90 degrees. Depending on format and bit rate digital data pass through an average
-computer or directly to the telemetry. A shock wave identification computer triggers the S/C core memory
+The Förster probe experiment E2 is a three-axe vector magnetometer. It is used for the continuous 
+observation of the interplanetary magnetic field in a frequency range from 0 to 4 Hz. This will be 
+investigated phenomena such as the spiral structure and discontinuities as a function of the distance 
+from the Sun. The measuring ranges are ± 100 nT and ± 400 nT with a resolution of ± 0.2 nT or ± 0.8 nT. 
+The component that is parallel to the axis of the spin, to perform precise zero point provisions of each 
+sensor is rotated 90 degrees. Depending on format and bit rate digital data pass through an average 
+computer or directly to the telemetry. A shock wave identification computer triggers the S/C core memory 
 in the presence of discontinuities with magnetic field variations.
 
 E3 :  The Rome‐GSFC magnetic field experiment utilized a triaxial fluxgate (saturable inductor) 
diff --git a/Instrument/AMDA/Helios2/MAG.xml b/Instrument/AMDA/Helios2/MAG.xml
index bfd561e..86eea2f 100644
--- a/Instrument/AMDA/Helios2/MAG.xml
+++ b/Instrument/AMDA/Helios2/MAG.xml
@@ -7,24 +7,24 @@
       <ResourceName>MAG</ResourceName>
       <AlternateName>Helios Magnetometers : E2, E3</AlternateName>
       <ReleaseDate>2018-10-20T21:10:13Z</ReleaseDate>
-      <Description>E2 : The Förster probe experiment E2 is a three component-vector magnetometer. Its purpose is to
-continuously observe the interplanetary magnetic field in a frequency range up to 4 Hz. Thereby certain
-phenomena are to be analysed as a function of the distance from the sun e.g. the spiral structure and
+      <Description>E2 : The Förster probe experiment E2 is a three component-vector magnetometer. Its purpose is to 
+continuously observe the interplanetary magnetic field in a frequency range up to 4 Hz. Thereby certain 
+phenomena are to be analysed as a function of the distance from the sun e.g. the spiral structure and 
 discontinuities. The measurement ranges are ± 100 nT and ± 400 nT. The resolution is ± 0.2 nT and ±
 0.8 nT respectively.
 
-For accurate measurements of the zero offset of each sensor the component parallel to the spinaxis can
-be flipped by 90°. Depending on telemetry format and bitrate the digital data are fed into a time average
-computer or directly connected to telemetry. A shock identification-computer triggers the S/C core
+For accurate measurements of the zero offset of each sensor the component parallel to the spinaxis can 
+be flipped by 90°. Depending on telemetry format and bitrate the digital data are fed into a time average 
+computer or directly connected to telemetry. A shock identification-computer triggers the S/C core 
 memory in case of discontinuities with variations of the ambient magnetic field magnitude.
 
-The Förster probe experiment E2 is a three-axe vector magnetometer. It is used for the continuous
-observation of the interplanetary magnetic field in a frequency range from 0 to 4 Hz. This will be
-investigated phenomena such as the spiral structure and discontinuities as a function of the distance
-from the Sun. The measuring ranges are ± 100 nT and ± 400 nT with a resolution of ± 0.2 nT or ± 0.8 nT.
-The component that is parallel to the axis of the spin, to perform precise zero point provisions of each
-sensor is rotated 90 degrees. Depending on format and bit rate digital data pass through an average
-computer or directly to the telemetry. A shock wave identification computer triggers the S/C core memory
+The Förster probe experiment E2 is a three-axe vector magnetometer. It is used for the continuous 
+observation of the interplanetary magnetic field in a frequency range from 0 to 4 Hz. This will be 
+investigated phenomena such as the spiral structure and discontinuities as a function of the distance 
+from the Sun. The measuring ranges are ± 100 nT and ± 400 nT with a resolution of ± 0.2 nT or ± 0.8 nT. 
+The component that is parallel to the axis of the spin, to perform precise zero point provisions of each 
+sensor is rotated 90 degrees. Depending on format and bit rate digital data pass through an average 
+computer or directly to the telemetry. A shock wave identification computer triggers the S/C core memory 
 in the presence of discontinuities with magnetic field variations.
 
 E3 :  The Rome‐GSFC magnetic field experiment utilized a triaxial fluxgate (saturable inductor) 
--
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