CDPP / CNES

Commit 41b9ddefcfe1f52dd1a08581f2b5b15bc4429506

Authored by Elena.Budnik
1 parent 7ad64f7a
Exists in master and in 12 other branches amdadev, aschulz, autocommit, bepi_master, bepi_update, branch_q, cleanup_registry, cleanup_registry_master, cleanup_registry_merged, juice_jdc, juno_jade, soar

lap final

Showing 6 changed files with 18 additions and 4 deletions   Show diff stats
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NumericalData/AMDA/Rosetta/LAP/ros-lap-asw.xml
  Diff comments   View file @41b9dde
... ... @@ -7,7 +7,8 @@
7 7 <ResourceName>parameters from sweeps (ASW)</ResourceName>
8 8 <AlternateName>Analyzed sweeps (ASW). Miscellaneous physical high-level quantities derived from individual sweeps.</AlternateName>
9 9 <ReleaseDate>2016-10-15T14:08:29Z</ReleaseDate>
10   - <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>
  10 + <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.
  11 + This is a preliminary data set which will be replaced by another in a few months.</Description>
11 12 <Contact>
12 13 <PersonID>spase://CDPP/Person/Anders.Eriksson</PersonID>
13 14 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/AMDA/Rosetta/LAP/ros-lap-efl.xml
  Diff comments   View file @41b9dde
... ... @@ -34,6 +34,8 @@ measurements. The data themselves look very clean and well behaved [Karlsson et
34 34 André et al, 2017], with very little of common mode signal remaining, despite the s/c poten tial
35 35 being both high and highly variable. The technique with floating probes is proven on numerous
36 36 sounding rockets in the terrestrial ionosphere [Maynard, 1998].
  37 +
  38 +This is a preliminary data set which will be replaced by another in a few months.
37 39 </Description>
38 40 <Contact>
39 41 <PersonID>spase://CDPP/Person/Anders.Eriksson</PersonID>
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NumericalData/AMDA/Rosetta/LAP/ros-lap-ned.xml
  Diff comments   View file @41b9dde
... ... @@ -19,6 +19,8 @@ sweep parameter N_E from ASW dataset was used for the calibration of U_SC to N_E
19 19 This is a good calibration source precisely when MIP data are scarce, as low plasma density
20 20 means low s/c potential, meaning that the otherwise very negative spacecraft potential here
21 21 does not prevent plasma electrons from reaching the Langmuir probes.
  22 +
  23 +This is a preliminary data set which will be replaced by another in a few months.
22 24 </Description>
23 25 <Contact>
24 26 <PersonID>spase://CDPP/Person/Anders.Eriksson</PersonID>
... ...
NumericalData/AMDA/Rosetta/LAP/ros-lap-nel.xml
  Diff comments   View file @41b9dde
... ... @@ -10,7 +10,10 @@ when RPC-MIP is not delivering cross-calibrated density products&lt;/AlternateName&gt;
10 10 <ReleaseDate>2016-10-15T14:08:29Z</ReleaseDate>
11 11 <Description>This data set is based on LAP data with use of a long-term LAP-MIP cross calibration for some time intervals
12 12 when MIP-LAP density is not available. Plasma density derived from individual current
13   -measurements or floating potential measurements on one probe.</Description>
  13 +measurements or floating potential measurements on one probe.
  14 +
  15 +This is a preliminary data set which will be replaced by another in a few months.
  16 + </Description>
14 17 <Contact>
15 18 <PersonID>spase://CDPP/Person/Anders.Eriksson</PersonID>
16 19 <Role>PrincipalInvestigator</Role>
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NumericalData/AMDA/Rosetta/LAP/ros-lap-pho.xml
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... ... @@ -27,7 +27,10 @@ However, around perihelion all methods returned about 50% less photoemission tha
27 27 expected from the Earth and Mars EUV fluxes. This may be a real effect, for example because
28 28 of attenuation of solar EUV radiation by large numbers of small dust grains at large distance
29 29 from the nucleus. It is also possible that this somehow relates to probe surface contamination,
30   -though no other such effects have been noted on LAP1</Description>
  30 +though no other such effects have been noted on LAP1.
  31 +
  32 +This is a preliminary data set which will be replaced by another in a few months.
  33 + </Description>
31 34 <Contact>
32 35 <PersonID>spase://CDPP/Person/Anders.Eriksson</PersonID>
33 36 <Role>PrincipalInvestigator</Role>
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NumericalData/AMDA/Rosetta/LAP/ros-lap-usc.xml
  Diff comments   View file @41b9dde
... ... @@ -21,7 +21,10 @@
21 21 probe position.
22 22  
23 23 A parameter DATA_SOURCE indicates which of these methods have been
24   - used for every single sweep.</Description>
  24 + used for every single sweep.
  25 +
  26 +This is a preliminary data set which will be replaced by another in a few months.
  27 + </Description>
25 28 <Contact>
26 29 <PersonID>spase://CDPP/Person/Anders.Eriksson</PersonID>
27 30 <Role>PrincipalInvestigator</Role>
... ...