From 4af43a3e6590a562bc66c73e75fed344b02f04ab Mon Sep 17 00:00:00 2001
From: Quentin Brzustowski <quentin.brzustowski@irap.omp.eu>
Date: Wed, 11 Mar 2020 12:16:08 +0100
Subject: [PATCH] added Caveats for PSP
---
Instrument/CDPP-AMDA/PSP/SPC.xml | 7 +++++++
NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-omd.xml | 2 +-
NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-omt.xml | 2 +-
3 files changed, 9 insertions(+), 2 deletions(-)
diff --git a/Instrument/CDPP-AMDA/PSP/SPC.xml b/Instrument/CDPP-AMDA/PSP/SPC.xml
index f0de293..a21decd 100644
--- a/Instrument/CDPP-AMDA/PSP/SPC.xml
+++ b/Instrument/CDPP-AMDA/PSP/SPC.xml
@@ -34,5 +34,12 @@
<InstrumentType>FaradayCup</InstrumentType>
<InvestigationName>Parker Solar Probe SWEAP Investigation</InvestigationName>
<ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/PSP</ObservatoryID>
+ <Caveats>The present SPC dataset contains two types of ion moment calculations, one called "moments" and the other called "fits".
+ The user should be aware that the data in "moments" are derived from straight integration of the SPC ion spectra.
+ It is a basic and generally robust method, albeit with various caveats as provided in the quality flags. The "fits" dataset is by contrast
+ more sensitive to the adjustments and limitations generally associated with the application of multi-component fitting procedures
+ (protons, alphas, and third peak). For those reasons, the unfamiliar user shall use the "moments" data preferentially.
+ If using the "fits" datasets, the user shall carefully check the quality flags and refer to their explanations before using that data.
+ </Caveats>
</Instrument>
</Spase>
diff --git a/NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-omd.xml b/NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-omd.xml
index 292ed15..8b9d68f 100644
--- a/NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-omd.xml
+++ b/NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-omd.xml
@@ -5,7 +5,7 @@
<ResourceID>spase://CNES/NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-omd</ResourceID>
<ResourceHeader>
<ResourceName>omni channel D</ResourceName>
- <AlternateName>Ions composition Group 2</AlternateName>
+ <AlternateName>Ion composition Group 2</AlternateName>
<ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate>
<Description>
Ion composition mode channel D. The available spectras are obtained by summing over all directions.
diff --git a/NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-omt.xml b/NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-omt.xml
index 21ba25c..1005ddc 100644
--- a/NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-omt.xml
+++ b/NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-omt.xml
@@ -5,7 +5,7 @@
<ResourceID>spase://CNES/NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-omt</ResourceID>
<ResourceHeader>
<ResourceName>omni channel T</ResourceName>
- <AlternateName>ION TOF-Only</AlternateName>
+ <AlternateName>Protons TOF only</AlternateName>
<ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate>
<Description>
Ion composition mode channel T. The available spectras are obtained by summing over all directions.
--
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