diff --git a/NumericalData/AMDA/Rosetta/LAP/ros-lap-asw.xml b/NumericalData/AMDA/Rosetta/LAP/ros-lap-asw.xml
index d97de69..b79bfcc 100644
--- a/NumericalData/AMDA/Rosetta/LAP/ros-lap-asw.xml
+++ b/NumericalData/AMDA/Rosetta/LAP/ros-lap-asw.xml
@@ -7,7 +7,8 @@
<ResourceName>parameters from sweeps (ASW)</ResourceName>
<AlternateName>Analyzed sweeps (ASW). Miscellaneous physical high-level quantities derived from individual sweeps.</AlternateName>
<ReleaseDate>2016-10-15T14:08:29Z</ReleaseDate>
- <Description>Time series of sweep-based estimates of electron density, ion bulk speed, electron temperature, and photoelectron knee potential. Timestamps represent the middle of the corresponding sweeps.</Description>
+ <Description>Time series of sweep-based estimates of electron density, ion bulk speed, electron temperature, and photoelectron knee potential. Timestamps represent the middle of the corresponding sweeps.
+ This is a preliminary data set which will be replaced by another in a few months.</Description>
<Contact>
<PersonID>spase://CDPP/Person/Anders.Eriksson</PersonID>
<Role>PrincipalInvestigator</Role>
diff --git a/NumericalData/AMDA/Rosetta/LAP/ros-lap-efl.xml b/NumericalData/AMDA/Rosetta/LAP/ros-lap-efl.xml
index 4767346..82c6973 100644
--- a/NumericalData/AMDA/Rosetta/LAP/ros-lap-efl.xml
+++ b/NumericalData/AMDA/Rosetta/LAP/ros-lap-efl.xml
@@ -34,6 +34,8 @@ measurements. The data themselves look very clean and well behaved [Karlsson et
André et al, 2017], with very little of common mode signal remaining, despite the s/c poten tial
being both high and highly variable. The technique with floating probes is proven on numerous
sounding rockets in the terrestrial ionosphere [Maynard, 1998].
+
+This is a preliminary data set which will be replaced by another in a few months.
</Description>
<Contact>
<PersonID>spase://CDPP/Person/Anders.Eriksson</PersonID>
diff --git a/NumericalData/AMDA/Rosetta/LAP/ros-lap-ned.xml b/NumericalData/AMDA/Rosetta/LAP/ros-lap-ned.xml
index 819b150..b4a40e4 100644
--- a/NumericalData/AMDA/Rosetta/LAP/ros-lap-ned.xml
+++ b/NumericalData/AMDA/Rosetta/LAP/ros-lap-ned.xml
@@ -19,6 +19,8 @@ sweep parameter N_E from ASW dataset was used for the calibration of U_SC to N_E
This is a good calibration source precisely when MIP data are scarce, as low plasma density
means low s/c potential, meaning that the otherwise very negative spacecraft potential here
does not prevent plasma electrons from reaching the Langmuir probes.
+
+This is a preliminary data set which will be replaced by another in a few months.
</Description>
<Contact>
<PersonID>spase://CDPP/Person/Anders.Eriksson</PersonID>
diff --git a/NumericalData/AMDA/Rosetta/LAP/ros-lap-nel.xml b/NumericalData/AMDA/Rosetta/LAP/ros-lap-nel.xml
index 5f21eec..ada883d 100644
--- a/NumericalData/AMDA/Rosetta/LAP/ros-lap-nel.xml
+++ b/NumericalData/AMDA/Rosetta/LAP/ros-lap-nel.xml
@@ -10,7 +10,10 @@ when RPC-MIP is not delivering cross-calibrated density products</AlternateName>
<ReleaseDate>2016-10-15T14:08:29Z</ReleaseDate>
<Description>This data set is based on LAP data with use of a long-term LAP-MIP cross calibration for some time intervals
when MIP-LAP density is not available. Plasma density derived from individual current
-measurements or floating potential measurements on one probe.</Description>
+measurements or floating potential measurements on one probe.
+
+This is a preliminary data set which will be replaced by another in a few months.
+ </Description>
<Contact>
<PersonID>spase://CDPP/Person/Anders.Eriksson</PersonID>
<Role>PrincipalInvestigator</Role>
diff --git a/NumericalData/AMDA/Rosetta/LAP/ros-lap-pho.xml b/NumericalData/AMDA/Rosetta/LAP/ros-lap-pho.xml
index 14ab86a..fb7a25c 100644
--- a/NumericalData/AMDA/Rosetta/LAP/ros-lap-pho.xml
+++ b/NumericalData/AMDA/Rosetta/LAP/ros-lap-pho.xml
@@ -27,7 +27,10 @@ However, around perihelion all methods returned about 50% less photoemission tha
expected from the Earth and Mars EUV fluxes. This may be a real effect, for example because
of attenuation of solar EUV radiation by large numbers of small dust grains at large distance
from the nucleus. It is also possible that this somehow relates to probe surface contamination,
-though no other such effects have been noted on LAP1</Description>
+though no other such effects have been noted on LAP1.
+
+This is a preliminary data set which will be replaced by another in a few months.
+ </Description>
<Contact>
<PersonID>spase://CDPP/Person/Anders.Eriksson</PersonID>
<Role>PrincipalInvestigator</Role>
diff --git a/NumericalData/AMDA/Rosetta/LAP/ros-lap-usc.xml b/NumericalData/AMDA/Rosetta/LAP/ros-lap-usc.xml
index bde0c48..486aa2d 100644
--- a/NumericalData/AMDA/Rosetta/LAP/ros-lap-usc.xml
+++ b/NumericalData/AMDA/Rosetta/LAP/ros-lap-usc.xml
@@ -21,7 +21,10 @@
probe position.
A parameter DATA_SOURCE indicates which of these methods have been
- used for every single sweep.</Description>
+ used for every single sweep.
+
+This is a preliminary data set which will be replaced by another in a few months.
+ </Description>
<Contact>
<PersonID>spase://CDPP/Person/Anders.Eriksson</PersonID>
<Role>PrincipalInvestigator</Role>
--
libgit2 0.21.2