Commit 964c4231d905d20cf468d78dab53e54c1b414ca9
1 parent
70938250
Exists in
master
and in
12 other branches
MESS spec param def
Showing
1 changed file
with
9 additions
and
6 deletions
Show diff stats
NumericalData/AMDA/MESSENGER/EPS/mess-eps-spec.xml
| @@ -32,12 +32,7 @@ | @@ -32,12 +32,7 @@ | ||
| 32 | <ProviderName>PDS</ProviderName> | 32 | <ProviderName>PDS</ProviderName> |
| 33 | <ProviderResourceName>MESS-E_V_H_SW-EPPS-3-EPS-DDR-V1.0/EPS_PA_DAILY_SPECTROGRAM</ProviderResourceName> | 33 | <ProviderResourceName>MESS-E_V_H_SW-EPPS-3-EPS-DDR-V1.0/EPS_PA_DAILY_SPECTROGRAM</ProviderResourceName> |
| 34 | <InstrumentID>spase://CDPP/Instrument/AMDA/MESSENGER/EPS</InstrumentID> | 34 | <InstrumentID>spase://CDPP/Instrument/AMDA/MESSENGER/EPS</InstrumentID> |
| 35 | - <MeasurementType>EnergeticParticles</MeasurementType> | ||
| 36 | - <Caveats>EPS PDS data products are derivate from the “Shaped” channel on EPS which is an integrated (hardware) channel. | ||
| 37 | - The hardware channel responded to all particles (ion and electron) that are above the threshold (~30 keV). | ||
| 38 | - Our experience at Mercury’s magnetosphere is that the primary particles are mostly energetic electrons. | ||
| 39 | - Please note that the D03 detector on the EPS has a very high background and is not useable for any of these science data products. | ||
| 40 | - </Caveats> | 35 | + <MeasurementType>EnergeticParticles</MeasurementType> |
| 41 | <TemporalDescription> | 36 | <TemporalDescription> |
| 42 | <TimeSpan> | 37 | <TimeSpan> |
| 43 | <StartDate>2008-08-20T16:03:35Z</StartDate> | 38 | <StartDate>2008-08-20T16:03:35Z</StartDate> |
| @@ -46,12 +41,20 @@ | @@ -46,12 +41,20 @@ | ||
| 46 | <Cadence>PT120S</Cadence> | 41 | <Cadence>PT120S</Cadence> |
| 47 | </TemporalDescription> | 42 | </TemporalDescription> |
| 48 | <ObservedRegion>Mercury</ObservedRegion> | 43 | <ObservedRegion>Mercury</ObservedRegion> |
| 44 | + <Caveats>EPS PDS data products are derivate from the “Shaped” channel on EPS which is an integrated (hardware) channel. | ||
| 45 | + The hardware channel responded to all particles (ion and electron) that are above the threshold (~30 keV). | ||
| 46 | + Our experience at Mercury’s magnetosphere is that the primary particles are mostly energetic electrons. | ||
| 47 | + Please note that the D03 detector on the EPS has a very high background and is not useable for any of these science data products. | ||
| 48 | + </Caveats> | ||
| 49 | <Parameter> | 49 | <Parameter> |
| 50 | <Name>countrate</Name> | 50 | <Name>countrate</Name> |
| 51 | <ParameterKey>mes_eps_pad</ParameterKey> | 51 | <ParameterKey>mes_eps_pad</ParameterKey> |
| 52 | <Description></Description> | 52 | <Description></Description> |
| 53 | <Ucd/> | 53 | <Ucd/> |
| 54 | <Units>cnts/s</Units> | 54 | <Units>cnts/s</Units> |
| 55 | + <RenderingHints> | ||
| 56 | + <DisplayType>Spectrogram</DisplayType> | ||
| 57 | + </RenderingHints> | ||
| 55 | <Structure> | 58 | <Structure> |
| 56 | <Size>16</Size> | 59 | <Size>16</Size> |
| 57 | </Structure> | 60 | </Structure> |