Commit 34334b5b5e36a0fa9b20ea4d6cde96e69c211ceb

Authored by Elena.Budnik
1 parent 7a303870

PEACE

NumericalData/AMDA/ACE/MFI/ace-mag-real.xml
@@ -51,7 +51,7 @@ @@ -51,7 +51,7 @@
51 <TemporalDescription> 51 <TemporalDescription>
52 <TimeSpan> 52 <TimeSpan>
53 <StartDate>2014-01-06T00:00:00Z</StartDate> 53 <StartDate>2014-01-06T00:00:00Z</StartDate>
54 - <StopDate>2016-11-03T00:59:59Z</StopDate> 54 + <StopDate>2016-11-04T00:59:59Z</StopDate>
55 </TimeSpan> 55 </TimeSpan>
56 <Cadence>PT60S</Cadence> 56 <Cadence>PT60S</Cadence>
57 </TemporalDescription> 57 </TemporalDescription>
NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml
@@ -44,7 +44,7 @@ @@ -44,7 +44,7 @@
44 <TemporalDescription> 44 <TemporalDescription>
45 <TimeSpan> 45 <TimeSpan>
46 <StartDate>2014-01-06T00:00:00Z</StartDate> 46 <StartDate>2014-01-06T00:00:00Z</StartDate>
47 - <StopDate>2016-11-03T00:59:59Z</StopDate> 47 + <StopDate>2016-11-04T00:59:59Z</StopDate>
48 </TimeSpan> 48 </TimeSpan>
49 <Cadence>PT60S</Cadence> 49 <Cadence>PT60S</Cadence>
50 </TemporalDescription> 50 </TemporalDescription>
NumericalData/AMDA/Cluster/Cluster1/PEACE/clust1-pea-mom.xml
@@ -5,46 +5,56 @@ @@ -5,46 +5,56 @@
5 <ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster1/PEACE/clust1-pea-mom</ResourceID> 5 <ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster1/PEACE/clust1-pea-mom</ResourceID>
6 <ResourceHeader> 6 <ResourceHeader>
7 <ResourceName>electron moments</ResourceName> 7 <ResourceName>electron moments</ResourceName>
8 - <AlternateName>Cluster 1 Prime Parameter PEACE Data</AlternateName>  
9 - <ReleaseDate>2015-10-16T16:51:44Z</ReleaseDate>  
10 - <Description>The primary task of this instrument (PEACE: Plasma Electrons and Currents Experiment)  
11 - is to obtain the velocity moments of the distribution function of electrons as frequently and  
12 - as accurately as the spacecraft telemetry will allow. Detector counts are collected in energy,  
13 - polar-angle, and azimuth-angle bins to form a three-dimensional matrix.  
14 - Two sensors are used: LEEA (low-energy electron analyzer) and HEEA (high-energy electron analyzer).  
15 - The energy coverage is from 0.67 eV to 30 KeV in 92 levels. The first 16 levels are equally spaced linearly  
16 - up to 10.7 eV; the remainder are logarithmically spaced. Both sensors can use the full range, but the HEEA  
17 - will normally operate over a higher energy range than the LEEA. The LEEA specializes in coverage of the  
18 - energies from 0.7-10 eV, and has a geometric factor one fifth that of the HEAA. Both sensors consist of  
19 - hemispherical electrostatic analyzers of the top-hat type and a detector in the form of an annular  
20 - micro-channel plate with a position-sensitive readout. Each sensor covers the range 0-180 degrees  
21 - with respect to the spin axis, and they are mounted opposite each other with a view perpendicular  
22 - to the spin axis, thus covering the complete angular range in a half rotation of the spacecraft.  
23 - The field of view perpendicular to the fan is 2 degrees for the LEEA and 5.6 degrees for the HEEA.  
24 - Energy resolution (Delta-E)/E is 0.13 for LEEA and 0.16 for HEEA. There are four sweep modes,  
25 - synchronized to the spin period (4 s), to vary the azimuthal angular resolution.  
26 - The spin phasing can be made coincident with that of the CIS instrument, to ensure that the electron  
27 - and ion moments will be measured simultaneously. On-board processing is used to calculate the moments  
28 - of the distribution with an accuracy of 1% and to select suitable parts of the complete distribution  
29 - for transmission. The normal science data format is based on one spin period, and consists of core data  
30 - followed by other optional distributions as can be fit into the available telemetry for that spin.  
31 - The core data (moments, spacecraft potential, and pitch angle distribution) are always transmitted  
32 - (if the spin is nominal). The next distribution is transmitted if, before the end of the spin,  
33 - all the previous data have been sent. Thus the next spin of data will be transmitted slightly late,  
34 - but all of its core data will be transmitted before the following spin of data is started on.  
35 - Eventually the transmission will catch up and be able to transmit the distribution after the core again,  
36 - but only after some time. This applies at all telemetry rates. The instrument can adapt automatically to  
37 - six different telemetry rates: a basic 1.52 Kbps rate (CIS priority); a normal 2.52 Kbps rate;  
38 - an enhanced PEACE priority rate of 3.54 Kbps; and three burst mode rates, with a maximum of 15.98 Kbps.  
39 - For more details of the Cluster mission, the spacecraft, and its instruments,  
40 - see the report Cluster: mission, payload and supporting activities, March 1993, ESA SP-1159,  
41 - and the included article PEACE: a Plasma Electron and Current Experiment, by A. D. Johnstone et al.,  
42 - from which this information was obtained.</Description>  
43 - <Acknowledgement>NASA, Dr. Andrew N. Fazakerley, European Space Agency</Acknowledgement> 8 + <AlternateName>Cluster 1 electron moments</AlternateName>
  9 + <ReleaseDate>2016-10-16T16:51:44Z</ReleaseDate>
  10 + <Description> The CAA Moments data are electron density, velocity vector,
  11 + pressure tensor and heat flux vector. The vectors and tensors are provided in GSE coordinates. Velocity and temperature
  12 + are also provided as components perpendicular and parallel to the magnetic field.
  13 + The magnetic field data is taken from CSDS FGM PP data, at present. In a possible future
  14 + release we would ideally use CAA FGM data, but it is considered unlikely that there will be major differences except in
  15 + very weak field regions. Furthermore :
  16 + * T_perp and T_para are determined by projecting the pressure tensor along the magnetic field and dividing by the density and by Boltzmanns constant. T_perp is the average of the two perpendicular components.
  17 + * v_para = (v.b) b and v_perp = v - (v.b) b. where v is the velocity vector and b is the magnetic field unit vector.
  18 +
  19 + These data are produced on the ground using 3-D data and thus are available at time resolutions which are limited by the
  20 + rate at which 3-D data can be transmitted. The data source used to generate the mome
  21 + nts is always the best available resolution 3-D data; this means mainly 3DR data but in the case 3DX or 3DXP are available these
  22 + are used instead for the MOMENTS production (see Mode_DataOrigin_HEEA/LEEA). Choices on the best way to combine data from the two
  23 + sensors can be made in the moments production software; in the first release the moments are made using LEEA data in the
  24 + energy overlap region.
  25 + In some situations, use of both sensors together may be a better choice, for example in case
  26 + s where the distribution changes
  27 + during a spin as the method can resolve time aliasing errors. If resources allow, the Moments
  28 + product at CAA may be updated to take advantage of this possibility.
  29 + The advantage of these ground - calculated moments is that the best available
  30 + calibration data is used, a correction can be made for the spacecraft potential
  31 + measurements (collected by the EFW experiment), and spacecraft electrons can be
  32 + properly removed. The current release has been generated automatically
  33 + using default values to control the approach to
  34 + potential correction and photoelectron removal, and has not been systematically human
  35 + - validated, so some errors may exist.
  36 + Specifically, the spacecraft potential, Vsc, is set to be 1 V greater than the
  37 + measured probe - spacecraft potential provided by
  38 + the electric field experiment (EFW) and the lower energy cutoff for the moments
  39 + integration is set to reject the energy bin
  40 + containing the EFW potential and the one above that (which in practice
  41 + may also contain counts due to spacecraft electrons).
  42 + Sometimes cold electrons are present which can appear in the same energy bin as the spacecraft photoelectrons,
  43 + therefore both the cold electrons and spacecraft photoelectrons are removed resulting in underestimated electron densities.
  44 + Recent work
  45 + by the EFW team suggests a more accurate determination of from would be a term that increases linearly
  46 + above ~10 V (Cully et al., 2007) but this has not yet been
  47 + implemented in our CAA moments generation code.</Description>
  48 + <Acknowledgement>Principal Investigator: Andrew Fazakerley</Acknowledgement>
44 <Contact> 49 <Contact>
45 - <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>  
46 - <Role>TechnicalContact</Role>  
47 - </Contact> 50 + <PersonID>spase://SMWG/Person/Andrew.N.Fazakerley</PersonID>
  51 + <Role>PrincipalInvestigator</Role>
  52 + </Contact>
  53 + <InformationURL>
  54 + <Name>ESA web page</Name>
  55 + <URL>http://www.cosmos.esa.int/web/csa/documentation</URL>
  56 + <Description>This site contains PEACE data documentation</Description>
  57 + </InformationURL>
48 <InformationURL> 58 <InformationURL>
49 <Name>NSSDC Master Catalog listing for Cluster II Rumba Plasma Electron and Current Experiment (PEACE)</Name> 59 <Name>NSSDC Master Catalog listing for Cluster II Rumba Plasma Electron and Current Experiment (PEACE)</Name>
50 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-05</URL> 60 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-05</URL>
@@ -59,12 +69,11 @@ @@ -59,12 +69,11 @@
59 <Name>AMDA at CDPP</Name> 69 <Name>AMDA at CDPP</Name>
60 <URL>http://amda.cdpp.eu</URL> 70 <URL>http://amda.cdpp.eu</URL>
61 </AccessURL> 71 </AccessURL>
62 - <Format>NetCDF</Format>  
63 - <Acknowledgement>NASA, Dr. Andrew N. Fazakerley</Acknowledgement> 72 + <Format>NetCDF</Format>
64 </AccessInformation> 73 </AccessInformation>
65 <ProviderName>CSA</ProviderName> 74 <ProviderName>CSA</ProviderName>
66 <ProcessingLevel>Calibrated</ProcessingLevel> 75 <ProcessingLevel>Calibrated</ProcessingLevel>
67 - <ProviderResourceName>Cluster II Rumba Prime Parameter Plasma Electron and Current Experiment (PEACE) Data</ProviderResourceName> 76 + <ProviderResourceName>C1_CP_PEA_MOMENTS</ProviderResourceName>
68 <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel> 77 <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
69 <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/PEACE</InstrumentID> 78 <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/PEACE</InstrumentID>
70 <MeasurementType>ThermalPlasma</MeasurementType> 79 <MeasurementType>ThermalPlasma</MeasurementType>
@@ -101,7 +110,9 @@ @@ -101,7 +110,9 @@
101 <Parameter> 110 <Parameter>
102 <Name>density</Name> 111 <Name>density</Name>
103 <ParameterKey>c1_pea_dens</ParameterKey> 112 <ParameterKey>c1_pea_dens</ParameterKey>
104 - <Description>Cluster II Rumba Prime Parameter Plasma Electron and Current Experiment electron number density at spin time resolution</Description> 113 + <Description>
  114 + Electron number density at spin time resolution
  115 + </Description>
105 <Ucd>phys.density;phys.electron</Ucd> 116 <Ucd>phys.density;phys.electron</Ucd>
106 <Cadence>PT4S</Cadence> 117 <Cadence>PT4S</Cadence>
107 <Units>cm^-3</Units> 118 <Units>cm^-3</Units>
@@ -124,7 +135,9 @@ @@ -124,7 +135,9 @@
124 <Parameter> 135 <Parameter>
125 <Name>v_gse</Name> 136 <Name>v_gse</Name>
126 <ParameterKey>c1_pea_vgse</ParameterKey> 137 <ParameterKey>c1_pea_vgse</ParameterKey>
127 - <Description>Cluster II Rumba Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 138 + <Description>
  139 + Electron velocity at spin time resolution
  140 + </Description>
128 <Ucd>phys.veloc;phys.electron</Ucd> 141 <Ucd>phys.veloc;phys.electron</Ucd>
129 <Cadence>PT4S</Cadence> 142 <Cadence>PT4S</Cadence>
130 <Units>km/s</Units> 143 <Units>km/s</Units>
@@ -171,7 +184,9 @@ @@ -171,7 +184,9 @@
171 <Parameter> 184 <Parameter>
172 <Name>v_gsm</Name> 185 <Name>v_gsm</Name>
173 <ParameterKey>c1_pea_vgsm</ParameterKey> 186 <ParameterKey>c1_pea_vgsm</ParameterKey>
174 - <Description>Cluster II Rumba Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 187 + <Description>
  188 + Electron velocity at spin time resolution, in GSM
  189 + </Description>
175 <Ucd>phys.veloc;phys.electron</Ucd> 190 <Ucd>phys.veloc;phys.electron</Ucd>
176 <Cadence>PT4S</Cadence> 191 <Cadence>PT4S</Cadence>
177 <Units>km/s</Units> 192 <Units>km/s</Units>
@@ -218,7 +233,9 @@ @@ -218,7 +233,9 @@
218 <Parameter> 233 <Parameter>
219 <Name>v_para_gse</Name> 234 <Name>v_para_gse</Name>
220 <ParameterKey>c1_pea_vpar</ParameterKey> 235 <ParameterKey>c1_pea_vpar</ParameterKey>
221 - <Description>Cluster II Rumba Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 236 + <Description>
  237 + Electron parallel velocity at spin time resolution, in GSE
  238 + </Description>
222 <Ucd>phys.veloc;phys.electron</Ucd> 239 <Ucd>phys.veloc;phys.electron</Ucd>
223 <Cadence>PT4S</Cadence> 240 <Cadence>PT4S</Cadence>
224 <Units>km/s</Units> 241 <Units>km/s</Units>
@@ -265,7 +282,9 @@ @@ -265,7 +282,9 @@
265 <Parameter> 282 <Parameter>
266 <Name>v_para_gsm</Name> 283 <Name>v_para_gsm</Name>
267 <ParameterKey>c1_pea_vpar_gsm</ParameterKey> 284 <ParameterKey>c1_pea_vpar_gsm</ParameterKey>
268 - <Description>Cluster II Rumba Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 285 + <Description>
  286 + Electron parallel velocity at spin time resolution, in GSM
  287 + </Description>
269 <Ucd>phys.veloc;phys.electron</Ucd> 288 <Ucd>phys.veloc;phys.electron</Ucd>
270 <Cadence>PT4S</Cadence> 289 <Cadence>PT4S</Cadence>
271 <Units>km/s</Units> 290 <Units>km/s</Units>
@@ -312,7 +331,9 @@ @@ -312,7 +331,9 @@
312 <Parameter> 331 <Parameter>
313 <Name>v_perp_gse</Name> 332 <Name>v_perp_gse</Name>
314 <ParameterKey>c1_pea_vperp</ParameterKey> 333 <ParameterKey>c1_pea_vperp</ParameterKey>
315 - <Description>Cluster II Rumba Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 334 + <Description>
  335 + Electron perpendicular velocity at spin time resolution, in GSE
  336 + </Description>
316 <Ucd>phys.veloc;phys.electron</Ucd> 337 <Ucd>phys.veloc;phys.electron</Ucd>
317 <Cadence>PT4S</Cadence> 338 <Cadence>PT4S</Cadence>
318 <Units>km/s</Units> 339 <Units>km/s</Units>
@@ -359,7 +380,9 @@ @@ -359,7 +380,9 @@
359 <Parameter> 380 <Parameter>
360 <Name>v_perp_gsm</Name> 381 <Name>v_perp_gsm</Name>
361 <ParameterKey>c1_pea_vperp_gsm</ParameterKey> 382 <ParameterKey>c1_pea_vperp_gsm</ParameterKey>
362 - <Description>Cluster II Rumba Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 383 + <Description>
  384 + Electron perpendicular velocity at spin time resolution, in GSM
  385 + </Description>
363 <Ucd>phys.veloc;phys.electron</Ucd> 386 <Ucd>phys.veloc;phys.electron</Ucd>
364 <Cadence>PT4S</Cadence> 387 <Cadence>PT4S</Cadence>
365 <Units>km/s</Units> 388 <Units>km/s</Units>
@@ -406,7 +429,9 @@ @@ -406,7 +429,9 @@
406 <Parameter> 429 <Parameter>
407 <Name>heat_flux_gse</Name> 430 <Name>heat_flux_gse</Name>
408 <ParameterKey>c1_pea_flux</ParameterKey> 431 <ParameterKey>c1_pea_flux</ParameterKey>
409 - <Description>Cluster II Rumba Prime Parameter Plasma Electron and Current Experiment parallel electron heat flux at spin time resolution</Description> 432 + <Description>
  433 + Parallel electron heat flux at spin time resolution, in GSE
  434 + </Description>
410 <Ucd>phys.heatflux;phys.atmol.ionStage</Ucd> 435 <Ucd>phys.heatflux;phys.atmol.ionStage</Ucd>
411 <Cadence>PT4S</Cadence> 436 <Cadence>PT4S</Cadence>
412 <Units>microW/m^2</Units> 437 <Units>microW/m^2</Units>
@@ -440,7 +465,9 @@ @@ -440,7 +465,9 @@
440 <Parameter> 465 <Parameter>
441 <Name>pressure_gse</Name> 466 <Name>pressure_gse</Name>
442 <ParameterKey>c1_pea_press</ParameterKey> 467 <ParameterKey>c1_pea_press</ParameterKey>
443 - <Description>Cluster II Rumba Prime Parameter Plasma Electron and Current Experiment parallel pressure tensor at spin time resolution</Description> 468 + <Description>
  469 + Electron pressure tensor at spin time resolution, in GSE
  470 + </Description>
444 <Ucd>phys.pressure</Ucd> 471 <Ucd>phys.pressure</Ucd>
445 <Cadence>PT4S</Cadence> 472 <Cadence>PT4S</Cadence>
446 <Units>microW/m^2</Units> 473 <Units>microW/m^2</Units>
@@ -452,20 +479,50 @@ @@ -452,20 +479,50 @@
452 <DisplayType>TimeSeries</DisplayType> 479 <DisplayType>TimeSeries</DisplayType>
453 </RenderingHints> 480 </RenderingHints>
454 <Structure> 481 <Structure>
455 - <Size>3</Size> 482 + <Size>9</Size>
456 <Element> 483 <Element>
457 <Name>xx</Name> 484 <Name>xx</Name>
458 <Index>1</Index> 485 <Index>1</Index>
459 <ParameterKey>c1_pea_press(0)</ParameterKey> 486 <ParameterKey>c1_pea_press(0)</ParameterKey>
460 </Element> 487 </Element>
461 <Element> 488 <Element>
462 - <Name>yy</Name> 489 + <Name>xy</Name>
463 <Index>2</Index> 490 <Index>2</Index>
  491 + <ParameterKey>c1_pea_press(1)</ParameterKey>
  492 + </Element>
  493 + <Element>
  494 + <Name>xz</Name>
  495 + <Index>3</Index>
  496 + <ParameterKey>c1_pea_press(2)</ParameterKey>
  497 + </Element>
  498 + <Element>
  499 + <Name>yx</Name>
  500 + <Index>4</Index>
  501 + <ParameterKey>c1_pea_press(3)</ParameterKey>
  502 + </Element>
  503 + <Element>
  504 + <Name>yy</Name>
  505 + <Index>5</Index>
464 <ParameterKey>c1_pea_press(4)</ParameterKey> 506 <ParameterKey>c1_pea_press(4)</ParameterKey>
465 </Element> 507 </Element>
466 <Element> 508 <Element>
  509 + <Name>yz</Name>
  510 + <Index>6</Index>
  511 + <ParameterKey>c1_pea_press(5)</ParameterKey>
  512 + </Element>
  513 + <Element>
  514 + <Name>zx</Name>
  515 + <Index>7</Index>
  516 + <ParameterKey>c1_pea_press(6)</ParameterKey>
  517 + </Element>
  518 + <Element>
  519 + <Name>zy</Name>
  520 + <Index>8</Index>
  521 + <ParameterKey>c1_pea_press(7)</ParameterKey>
  522 + </Element>
  523 + <Element>
467 <Name>zz</Name> 524 <Name>zz</Name>
468 - <Index>3</Index> 525 + <Index>9</Index>
469 <ParameterKey>c1_pea_press(8)</ParameterKey> 526 <ParameterKey>c1_pea_press(8)</ParameterKey>
470 </Element> 527 </Element>
471 </Structure> 528 </Structure>
@@ -478,7 +535,9 @@ @@ -478,7 +535,9 @@
478 <Parameter> 535 <Parameter>
479 <Name>t_para</Name> 536 <Name>t_para</Name>
480 <ParameterKey>c1_pea_tpar</ParameterKey> 537 <ParameterKey>c1_pea_tpar</ParameterKey>
481 - <Description>Cluster II Rumba Prime Parameter Plasma Electron and Current Experiment parallel electron temperature at spin time resolution</Description> 538 + <Description>
  539 + Parallel electron temperature at spin time resolution
  540 + </Description>
482 <Ucd>phys.temperature;phys.electron</Ucd> 541 <Ucd>phys.temperature;phys.electron</Ucd>
483 <Cadence>PT4S</Cadence> 542 <Cadence>PT4S</Cadence>
484 <Units>eV</Units> 543 <Units>eV</Units>
@@ -495,7 +554,9 @@ @@ -495,7 +554,9 @@
495 <Parameter> 554 <Parameter>
496 <Name>t_perp</Name> 555 <Name>t_perp</Name>
497 <ParameterKey>c1_pea_tperp</ParameterKey> 556 <ParameterKey>c1_pea_tperp</ParameterKey>
498 - <Description>Cluster II Rumba Prime Parameter Plasma Electron and Current Experiment perpendicular electron temperature at spin time resolution</Description> 557 + <Description>
  558 + Perpendicular electron temperature at spin time resolution
  559 + </Description>
499 <Ucd>phys.temperature;phys.electron</Ucd> 560 <Ucd>phys.temperature;phys.electron</Ucd>
500 <Cadence>PT4S</Cadence> 561 <Cadence>PT4S</Cadence>
501 <Units>eV</Units> 562 <Units>eV</Units>
NumericalData/AMDA/Cluster/Cluster2/PEACE/clust2-pea-mom.xml
@@ -5,52 +5,61 @@ @@ -5,52 +5,61 @@
5 <ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster2/PEACE/clust2-pea-mom</ResourceID> 5 <ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster2/PEACE/clust2-pea-mom</ResourceID>
6 <ResourceHeader> 6 <ResourceHeader>
7 <ResourceName>electron moments</ResourceName> 7 <ResourceName>electron moments</ResourceName>
8 - <AlternateName>Cluster 2 Prime Parameter PEACE Data</AlternateName>  
9 - <ReleaseDate>2015-10-19T15:51:44Z</ReleaseDate>  
10 - <Description>The primary task of this instrument (PEACE: Plasma Electrons and Currents Experiment)  
11 - is to obtain the velocity moments of the distribution function of electrons as frequently and  
12 - as accurately as the spacecraft telemetry will allow. Detector counts are collected in energy,  
13 - polar-angle, and azimuth-angle bins to form a three-dimensional matrix.  
14 - Two sensors are used: LEEA (low-energy electron analyzer) and HEEA (high-energy electron analyzer).  
15 - The energy coverage is from 0.67 eV to 30 KeV in 92 levels. The first 16 levels are equally spaced linearly  
16 - up to 10.7 eV; the remainder are logarithmically spaced. Both sensors can use the full range, but the HEEA  
17 - will normally operate over a higher energy range than the LEEA. The LEEA specializes in coverage of the  
18 - energies from 0.7-10 eV, and has a geometric factor one fifth that of the HEAA. Both sensors consist of  
19 - hemispherical electrostatic analyzers of the top-hat type and a detector in the form of an annular  
20 - micro-channel plate with a position-sensitive readout. Each sensor covers the range 0-180 degrees  
21 - with respect to the spin axis, and they are mounted opposite each other with a view perpendicular  
22 - to the spin axis, thus covering the complete angular range in a half rotation of the spacecraft.  
23 - The field of view perpendicular to the fan is 2 degrees for the LEEA and 5.6 degrees for the HEEA.  
24 - Energy resolution (Delta-E)/E is 0.13 for LEEA and 0.16 for HEEA. There are four sweep modes,  
25 - synchronized to the spin period (4 s), to vary the azimuthal angular resolution.  
26 - The spin phasing can be made coincident with that of the CIS instrument, to ensure that the electron  
27 - and ion moments will be measured simultaneously. On-board processing is used to calculate the moments  
28 - of the distribution with an accuracy of 1% and to select suitable parts of the complete distribution  
29 - for transmission. The normal science data format is based on one spin period, and consists of core data  
30 - followed by other optional distributions as can be fit into the available telemetry for that spin.  
31 - The core data (moments, spacecraft potential, and pitch angle distribution) are always transmitted  
32 - (if the spin is nominal). The next distribution is transmitted if, before the end of the spin,  
33 - all the previous data have been sent. Thus the next spin of data will be transmitted slightly late,  
34 - but all of its core data will be transmitted before the following spin of data is started on.  
35 - Eventually the transmission will catch up and be able to transmit the distribution after the core again,  
36 - but only after some time. This applies at all telemetry rates. The instrument can adapt automatically to  
37 - six different telemetry rates: a basic 1.52 Kbps rate (CIS priority); a normal 2.52 Kbps rate;  
38 - an enhanced PEACE priority rate of 3.54 Kbps; and three burst mode rates, with a maximum of 15.98 Kbps.  
39 - For more details of the Cluster mission, the spacecraft, and its instruments,  
40 - see the report Cluster: mission, payload and supporting activities, March 1993, ESA SP-1159,  
41 - and the included article PEACE: a Plasma Electron and Current Experiment, by A. D. Johnstone et al.,  
42 - from which this information was obtained.</Description>  
43 - <Acknowledgement>NASA, Dr. Andrew N. Fazakerley, European Space Agency</Acknowledgement> 8 + <AlternateName>Cluster 2 electron moments</AlternateName>
  9 + <ReleaseDate>2016-10-16T16:51:44Z</ReleaseDate>
  10 + <Description> The CAA Moments data are electron density, velocity vector,
  11 + pressure tensor and heat flux vector. The vectors and tensors are provided in GSE coordinates. Velocity and temperature
  12 + are also provided as components perpendicular and parallel to the magnetic field.
  13 + The magnetic field data is taken from CSDS FGM PP data, at present. In a possible future
  14 + release we would ideally use CAA FGM data, but it is considered unlikely that there will be major differences except in
  15 + very weak field regions. Furthermore :
  16 + * T_perp and T_para are determined by projecting the pressure tensor along the magnetic field and dividing by the density and by Boltzmanns constant. T_perp is the average of the two perpendicular components.
  17 + * v_para = (v.b) b and v_perp = v - (v.b) b. where v is the velocity vector and b is the magnetic field unit vector.
  18 +
  19 + These data are produced on the ground using 3-D data and thus are available at time resolutions which are limited by the
  20 + rate at which 3-D data can be transmitted. The data source used to generate the mome
  21 + nts is always the best available resolution 3-D data; this means mainly 3DR data but in the case 3DX or 3DXP are available these
  22 + are used instead for the MOMENTS production (see Mode_DataOrigin_HEEA/LEEA). Choices on the best way to combine data from the two
  23 + sensors can be made in the moments production software; in the first release the moments are made using LEEA data in the
  24 + energy overlap region.
  25 + In some situations, use of both sensors together may be a better choice, for example in case
  26 + s where the distribution changes
  27 + during a spin as the method can resolve time aliasing errors. If resources allow, the Moments
  28 + product at CAA may be updated to take advantage of this possibility.
  29 + The advantage of these ground - calculated moments is that the best available
  30 + calibration data is used, a correction can be made for the spacecraft potential
  31 + measurements (collected by the EFW experiment), and spacecraft electrons can be
  32 + properly removed. The current release has been generated automatically
  33 + using default values to control the approach to
  34 + potential correction and photoelectron removal, and has not been systematically human
  35 + - validated, so some errors may exist.
  36 + Specifically, the spacecraft potential, Vsc, is set to be 1 V greater than the
  37 + measured probe - spacecraft potential provided by
  38 + the electric field experiment (EFW) and the lower energy cutoff for the moments
  39 + integration is set to reject the energy bin
  40 + containing the EFW potential and the one above that (which in practice
  41 + may also contain counts due to spacecraft electrons).
  42 + Sometimes cold electrons are present which can appear in the same energy bin as the spacecraft photoelectrons,
  43 + therefore both the cold electrons and spacecraft photoelectrons are removed resulting in underestimated electron densities.
  44 + Recent work
  45 + by the EFW team suggests a more accurate determination of from would be a term that increases linearly
  46 + above ~10 V (Cully et al., 2007) but this has not yet been
  47 + implemented in our CAA moments generation code.</Description>
  48 + <Acknowledgement>Principal Investigator: Andrew Fazakerley</Acknowledgement>
44 <Contact> 49 <Contact>
45 - <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>  
46 - <Role>TechnicalContact</Role>  
47 - </Contact>  
48 - 50 + <PersonID>spase://SMWG/Person/Andrew.N.Fazakerley</PersonID>
  51 + <Role>PrincipalInvestigator</Role>
  52 + </Contact>
49 <InformationURL> 53 <InformationURL>
50 - <Name>NSSDC Master Catalog listing for Cluster II Rumba Plasma Electron and Current Experiment (PEACE)</Name> 54 + <Name>ESA web page</Name>
  55 + <URL>http://www.cosmos.esa.int/web/csa/documentation</URL>
  56 + <Description>This site contains PEACE data documentation</Description>
  57 + </InformationURL>
  58 + <InformationURL>
  59 + <Name>NSSDC Master Catalog listing for Cluster II Salsa Plasma Electron and Current Experiment (PEACE)</Name>
51 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-05</URL> 60 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-05</URL>
52 <Description>This site provides information concerning the Cluster II Salsa Plasma Electron and Current Experiment Instrument.</Description> 61 <Description>This site provides information concerning the Cluster II Salsa Plasma Electron and Current Experiment Instrument.</Description>
53 - </InformationURL> 62 + </InformationURL>
54 </ResourceHeader> 63 </ResourceHeader>
55 <AccessInformation> 64 <AccessInformation>
56 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID> 65 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
@@ -60,19 +69,18 @@ @@ -60,19 +69,18 @@
60 <Name>AMDA at CDPP</Name> 69 <Name>AMDA at CDPP</Name>
61 <URL>http://amda.cdpp.eu</URL> 70 <URL>http://amda.cdpp.eu</URL>
62 </AccessURL> 71 </AccessURL>
63 - <Format>NetCDF</Format>  
64 - <Acknowledgement>NASA, Dr. Andrew N. Fazakerley</Acknowledgement> 72 + <Format>NetCDF</Format>
65 </AccessInformation> 73 </AccessInformation>
66 <ProviderName>CSA</ProviderName> 74 <ProviderName>CSA</ProviderName>
67 <ProcessingLevel>Calibrated</ProcessingLevel> 75 <ProcessingLevel>Calibrated</ProcessingLevel>
68 - <ProviderResourceName>Cluster II Salsa Prime Parameter Plasma Electron and Current Experiment (PEACE) Data</ProviderResourceName> 76 + <ProviderResourceName>C2_CP_PEA_MOMENTS</ProviderResourceName>
69 <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel> 77 <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
70 <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Salsa/PEACE</InstrumentID> 78 <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Salsa/PEACE</InstrumentID>
71 <MeasurementType>ThermalPlasma</MeasurementType> 79 <MeasurementType>ThermalPlasma</MeasurementType>
72 <TemporalDescription> 80 <TemporalDescription>
73 <TimeSpan> 81 <TimeSpan>
74 - <StartDate>2001-01-10T00:01:11Z</StartDate>  
75 - <StopDate>2013-06-30T23:59:40Z</StopDate> 82 + <StartDate>2001-01-10T00:02:11Z</StartDate>
  83 + <StopDate>2013-06-30T12:39:50Z</StopDate>
76 </TimeSpan> 84 </TimeSpan>
77 <Cadence_Min>PT4S</Cadence_Min> 85 <Cadence_Min>PT4S</Cadence_Min>
78 <Cadence_Max>PT160S</Cadence_Max> 86 <Cadence_Max>PT160S</Cadence_Max>
@@ -102,7 +110,9 @@ @@ -102,7 +110,9 @@
102 <Parameter> 110 <Parameter>
103 <Name>density</Name> 111 <Name>density</Name>
104 <ParameterKey>c2_pea_dens</ParameterKey> 112 <ParameterKey>c2_pea_dens</ParameterKey>
105 - <Description>Cluster II Salsa Prime Parameter Plasma Electron and Current Experiment electron number density at spin time resolution</Description> 113 + <Description>
  114 + Electron number density at spin time resolution
  115 + </Description>
106 <Ucd>phys.density;phys.electron</Ucd> 116 <Ucd>phys.density;phys.electron</Ucd>
107 <Cadence>PT4S</Cadence> 117 <Cadence>PT4S</Cadence>
108 <Units>cm^-3</Units> 118 <Units>cm^-3</Units>
@@ -125,7 +135,9 @@ @@ -125,7 +135,9 @@
125 <Parameter> 135 <Parameter>
126 <Name>v_gse</Name> 136 <Name>v_gse</Name>
127 <ParameterKey>c2_pea_vgse</ParameterKey> 137 <ParameterKey>c2_pea_vgse</ParameterKey>
128 - <Description>Cluster II Salsa Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 138 + <Description>
  139 + Electron velocity at spin time resolution
  140 + </Description>
129 <Ucd>phys.veloc;phys.electron</Ucd> 141 <Ucd>phys.veloc;phys.electron</Ucd>
130 <Cadence>PT4S</Cadence> 142 <Cadence>PT4S</Cadence>
131 <Units>km/s</Units> 143 <Units>km/s</Units>
@@ -172,7 +184,9 @@ @@ -172,7 +184,9 @@
172 <Parameter> 184 <Parameter>
173 <Name>v_gsm</Name> 185 <Name>v_gsm</Name>
174 <ParameterKey>c2_pea_vgsm</ParameterKey> 186 <ParameterKey>c2_pea_vgsm</ParameterKey>
175 - <Description>Cluster II Salsa Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 187 + <Description>
  188 + Electron velocity at spin time resolution, in GSM
  189 + </Description>
176 <Ucd>phys.veloc;phys.electron</Ucd> 190 <Ucd>phys.veloc;phys.electron</Ucd>
177 <Cadence>PT4S</Cadence> 191 <Cadence>PT4S</Cadence>
178 <Units>km/s</Units> 192 <Units>km/s</Units>
@@ -219,7 +233,9 @@ @@ -219,7 +233,9 @@
219 <Parameter> 233 <Parameter>
220 <Name>v_para_gse</Name> 234 <Name>v_para_gse</Name>
221 <ParameterKey>c2_pea_vpar</ParameterKey> 235 <ParameterKey>c2_pea_vpar</ParameterKey>
222 - <Description>Cluster II Salsa Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 236 + <Description>
  237 + Electron parallel velocity at spin time resolution, in GSE
  238 + </Description>
223 <Ucd>phys.veloc;phys.electron</Ucd> 239 <Ucd>phys.veloc;phys.electron</Ucd>
224 <Cadence>PT4S</Cadence> 240 <Cadence>PT4S</Cadence>
225 <Units>km/s</Units> 241 <Units>km/s</Units>
@@ -266,7 +282,9 @@ @@ -266,7 +282,9 @@
266 <Parameter> 282 <Parameter>
267 <Name>v_para_gsm</Name> 283 <Name>v_para_gsm</Name>
268 <ParameterKey>c2_pea_vpar_gsm</ParameterKey> 284 <ParameterKey>c2_pea_vpar_gsm</ParameterKey>
269 - <Description>Cluster II Salsa Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 285 + <Description>
  286 + Electron parallel velocity at spin time resolution, in GSM
  287 + </Description>
270 <Ucd>phys.veloc;phys.electron</Ucd> 288 <Ucd>phys.veloc;phys.electron</Ucd>
271 <Cadence>PT4S</Cadence> 289 <Cadence>PT4S</Cadence>
272 <Units>km/s</Units> 290 <Units>km/s</Units>
@@ -313,7 +331,9 @@ @@ -313,7 +331,9 @@
313 <Parameter> 331 <Parameter>
314 <Name>v_perp_gse</Name> 332 <Name>v_perp_gse</Name>
315 <ParameterKey>c2_pea_vperp</ParameterKey> 333 <ParameterKey>c2_pea_vperp</ParameterKey>
316 - <Description>Cluster II Salsa Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 334 + <Description>
  335 + Electron perpendicular velocity at spin time resolution, in GSE
  336 + </Description>
317 <Ucd>phys.veloc;phys.electron</Ucd> 337 <Ucd>phys.veloc;phys.electron</Ucd>
318 <Cadence>PT4S</Cadence> 338 <Cadence>PT4S</Cadence>
319 <Units>km/s</Units> 339 <Units>km/s</Units>
@@ -360,7 +380,9 @@ @@ -360,7 +380,9 @@
360 <Parameter> 380 <Parameter>
361 <Name>v_perp_gsm</Name> 381 <Name>v_perp_gsm</Name>
362 <ParameterKey>c2_pea_vperp_gsm</ParameterKey> 382 <ParameterKey>c2_pea_vperp_gsm</ParameterKey>
363 - <Description>Cluster II Salsa Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 383 + <Description>
  384 + Electron perpendicular velocity at spin time resolution, in GSM
  385 + </Description>
364 <Ucd>phys.veloc;phys.electron</Ucd> 386 <Ucd>phys.veloc;phys.electron</Ucd>
365 <Cadence>PT4S</Cadence> 387 <Cadence>PT4S</Cadence>
366 <Units>km/s</Units> 388 <Units>km/s</Units>
@@ -407,13 +429,15 @@ @@ -407,13 +429,15 @@
407 <Parameter> 429 <Parameter>
408 <Name>heat_flux_gse</Name> 430 <Name>heat_flux_gse</Name>
409 <ParameterKey>c2_pea_flux</ParameterKey> 431 <ParameterKey>c2_pea_flux</ParameterKey>
410 - <Description>Cluster II Salsa Prime Parameter Plasma Electron and Current Experiment parallel electron heat flux at spin time resolution</Description> 432 + <Description>
  433 + Parallel electron heat flux at spin time resolution, in GSE
  434 + </Description>
411 <Ucd>phys.heatflux;phys.atmol.ionStage</Ucd> 435 <Ucd>phys.heatflux;phys.atmol.ionStage</Ucd>
412 <Cadence>PT4S</Cadence> 436 <Cadence>PT4S</Cadence>
413 - <Units>microW/m^2</Units> 437 + <Units>microW/m^2</Units>
414 <RenderingHints> 438 <RenderingHints>
415 <DisplayType>TimeSeries</DisplayType> 439 <DisplayType>TimeSeries</DisplayType>
416 - </RenderingHints> 440 + </RenderingHints>
417 <Structure> 441 <Structure>
418 <Size>3</Size> 442 <Size>3</Size>
419 <Element> 443 <Element>
@@ -441,7 +465,9 @@ @@ -441,7 +465,9 @@
441 <Parameter> 465 <Parameter>
442 <Name>pressure_gse</Name> 466 <Name>pressure_gse</Name>
443 <ParameterKey>c2_pea_press</ParameterKey> 467 <ParameterKey>c2_pea_press</ParameterKey>
444 - <Description>Cluster II Salsa Prime Parameter Plasma Electron and Current Experiment parallel pressure tensor at spin time resolution</Description> 468 + <Description>
  469 + Electron pressure tensor at spin time resolution, in GSE
  470 + </Description>
445 <Ucd>phys.pressure</Ucd> 471 <Ucd>phys.pressure</Ucd>
446 <Cadence>PT4S</Cadence> 472 <Cadence>PT4S</Cadence>
447 <Units>microW/m^2</Units> 473 <Units>microW/m^2</Units>
@@ -451,22 +477,52 @@ @@ -451,22 +477,52 @@
451 </CoordinateSystem> 477 </CoordinateSystem>
452 <RenderingHints> 478 <RenderingHints>
453 <DisplayType>TimeSeries</DisplayType> 479 <DisplayType>TimeSeries</DisplayType>
454 - </RenderingHints> 480 + </RenderingHints>
455 <Structure> 481 <Structure>
456 - <Size>3</Size> 482 + <Size>9</Size>
457 <Element> 483 <Element>
458 <Name>xx</Name> 484 <Name>xx</Name>
459 <Index>1</Index> 485 <Index>1</Index>
460 <ParameterKey>c2_pea_press(0)</ParameterKey> 486 <ParameterKey>c2_pea_press(0)</ParameterKey>
461 </Element> 487 </Element>
462 <Element> 488 <Element>
463 - <Name>yy</Name> 489 + <Name>xy</Name>
464 <Index>2</Index> 490 <Index>2</Index>
  491 + <ParameterKey>c2_pea_press(1)</ParameterKey>
  492 + </Element>
  493 + <Element>
  494 + <Name>xz</Name>
  495 + <Index>3</Index>
  496 + <ParameterKey>c2_pea_press(2)</ParameterKey>
  497 + </Element>
  498 + <Element>
  499 + <Name>yx</Name>
  500 + <Index>4</Index>
  501 + <ParameterKey>c2_pea_press(3)</ParameterKey>
  502 + </Element>
  503 + <Element>
  504 + <Name>yy</Name>
  505 + <Index>5</Index>
465 <ParameterKey>c2_pea_press(4)</ParameterKey> 506 <ParameterKey>c2_pea_press(4)</ParameterKey>
466 </Element> 507 </Element>
467 <Element> 508 <Element>
  509 + <Name>yz</Name>
  510 + <Index>6</Index>
  511 + <ParameterKey>c2_pea_press(5)</ParameterKey>
  512 + </Element>
  513 + <Element>
  514 + <Name>zx</Name>
  515 + <Index>7</Index>
  516 + <ParameterKey>c2_pea_press(6)</ParameterKey>
  517 + </Element>
  518 + <Element>
  519 + <Name>zy</Name>
  520 + <Index>8</Index>
  521 + <ParameterKey>c2_pea_press(7)</ParameterKey>
  522 + </Element>
  523 + <Element>
468 <Name>zz</Name> 524 <Name>zz</Name>
469 - <Index>3</Index> 525 + <Index>9</Index>
470 <ParameterKey>c2_pea_press(8)</ParameterKey> 526 <ParameterKey>c2_pea_press(8)</ParameterKey>
471 </Element> 527 </Element>
472 </Structure> 528 </Structure>
@@ -479,7 +535,9 @@ @@ -479,7 +535,9 @@
479 <Parameter> 535 <Parameter>
480 <Name>t_para</Name> 536 <Name>t_para</Name>
481 <ParameterKey>c2_pea_tpar</ParameterKey> 537 <ParameterKey>c2_pea_tpar</ParameterKey>
482 - <Description>Cluster II Salsa Prime Parameter Plasma Electron and Current Experiment parallel electron temperature at spin time resolution</Description> 538 + <Description>
  539 + Parallel electron temperature at spin time resolution
  540 + </Description>
483 <Ucd>phys.temperature;phys.electron</Ucd> 541 <Ucd>phys.temperature;phys.electron</Ucd>
484 <Cadence>PT4S</Cadence> 542 <Cadence>PT4S</Cadence>
485 <Units>eV</Units> 543 <Units>eV</Units>
@@ -496,14 +554,15 @@ @@ -496,14 +554,15 @@
496 <Parameter> 554 <Parameter>
497 <Name>t_perp</Name> 555 <Name>t_perp</Name>
498 <ParameterKey>c2_pea_tperp</ParameterKey> 556 <ParameterKey>c2_pea_tperp</ParameterKey>
499 - <Description>Cluster II Salsa Prime Parameter Plasma Electron and Current Experiment perpendicular electron temperature at spin time resolution</Description> 557 + <Description>
  558 + Perpendicular electron temperature at spin time resolution
  559 + </Description>
500 <Ucd>phys.temperature;phys.electron</Ucd> 560 <Ucd>phys.temperature;phys.electron</Ucd>
501 <Cadence>PT4S</Cadence> 561 <Cadence>PT4S</Cadence>
502 <Units>eV</Units> 562 <Units>eV</Units>
503 <RenderingHints> 563 <RenderingHints>
504 <DisplayType>TimeSeries</DisplayType> 564 <DisplayType>TimeSeries</DisplayType>
505 </RenderingHints> 565 </RenderingHints>
506 - <FillValue>-1.0000e+31</FillValue>  
507 <Particle> 566 <Particle>
508 <ParticleType>Electron</ParticleType> 567 <ParticleType>Electron</ParticleType>
509 <Qualifier>Scalar</Qualifier> 568 <Qualifier>Scalar</Qualifier>
NumericalData/AMDA/Cluster/Cluster3/PEACE/clust3-pea-mom.xml
@@ -5,52 +5,61 @@ @@ -5,52 +5,61 @@
5 <ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster3/PEACE/clust3-pea-mom</ResourceID> 5 <ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster3/PEACE/clust3-pea-mom</ResourceID>
6 <ResourceHeader> 6 <ResourceHeader>
7 <ResourceName>electron moments</ResourceName> 7 <ResourceName>electron moments</ResourceName>
8 - <AlternateName>Cluster 3 Prime Parameter PEACE Data</AlternateName>  
9 - <ReleaseDate>2015-10-19T15:51:44Z</ReleaseDate>  
10 - <Description>The primary task of this instrument (PEACE: Plasma Electrons and Currents Experiment)  
11 - is to obtain the velocity moments of the distribution function of electrons as frequently and  
12 - as accurately as the spacecraft telemetry will allow. Detector counts are collected in energy,  
13 - polar-angle, and azimuth-angle bins to form a three-dimensional matrix.  
14 - Two sensors are used: LEEA (low-energy electron analyzer) and HEEA (high-energy electron analyzer).  
15 - The energy coverage is from 0.67 eV to 30 KeV in 92 levels. The first 16 levels are equally spaced linearly  
16 - up to 10.7 eV; the remainder are logarithmically spaced. Both sensors can use the full range, but the HEEA  
17 - will normally operate over a higher energy range than the LEEA. The LEEA specializes in coverage of the  
18 - energies from 0.7-10 eV, and has a geometric factor one fifth that of the HEAA. Both sensors consist of  
19 - hemispherical electrostatic analyzers of the top-hat type and a detector in the form of an annular  
20 - micro-channel plate with a position-sensitive readout. Each sensor covers the range 0-180 degrees  
21 - with respect to the spin axis, and they are mounted opposite each other with a view perpendicular  
22 - to the spin axis, thus covering the complete angular range in a half rotation of the spacecraft.  
23 - The field of view perpendicular to the fan is 2 degrees for the LEEA and 5.6 degrees for the HEEA.  
24 - Energy resolution (Delta-E)/E is 0.13 for LEEA and 0.16 for HEEA. There are four sweep modes,  
25 - synchronized to the spin period (4 s), to vary the azimuthal angular resolution.  
26 - The spin phasing can be made coincident with that of the CIS instrument, to ensure that the electron  
27 - and ion moments will be measured simultaneously. On-board processing is used to calculate the moments  
28 - of the distribution with an accuracy of 1% and to select suitable parts of the complete distribution  
29 - for transmission. The normal science data format is based on one spin period, and consists of core data  
30 - followed by other optional distributions as can be fit into the available telemetry for that spin.  
31 - The core data (moments, spacecraft potential, and pitch angle distribution) are always transmitted  
32 - (if the spin is nominal). The next distribution is transmitted if, before the end of the spin,  
33 - all the previous data have been sent. Thus the next spin of data will be transmitted slightly late,  
34 - but all of its core data will be transmitted before the following spin of data is started on.  
35 - Eventually the transmission will catch up and be able to transmit the distribution after the core again,  
36 - but only after some time. This applies at all telemetry rates. The instrument can adapt automatically to  
37 - six different telemetry rates: a basic 1.52 Kbps rate (CIS priority); a normal 2.52 Kbps rate;  
38 - an enhanced PEACE priority rate of 3.54 Kbps; and three burst mode rates, with a maximum of 15.98 Kbps.  
39 - For more details of the Cluster mission, the spacecraft, and its instruments,  
40 - see the report Cluster: mission, payload and supporting activities, March 1993, ESA SP-1159,  
41 - and the included article PEACE: a Plasma Electron and Current Experiment, by A. D. Johnstone et al.,  
42 - from which this information was obtained.</Description>  
43 - <Acknowledgement>NASA, Dr. Andrew N. Fazakerley, European Space Agency</Acknowledgement> 8 + <AlternateName>Cluster 3 electron moments</AlternateName>
  9 + <ReleaseDate>2016-10-16T16:51:44Z</ReleaseDate>
  10 + <Description> The CAA Moments data are electron density, velocity vector,
  11 + pressure tensor and heat flux vector. The vectors and tensors are provided in GSE coordinates. Velocity and temperature
  12 + are also provided as components perpendicular and parallel to the magnetic field.
  13 + The magnetic field data is taken from CSDS FGM PP data, at present. In a possible future
  14 + release we would ideally use CAA FGM data, but it is considered unlikely that there will be major differences except in
  15 + very weak field regions. Furthermore :
  16 + * T_perp and T_para are determined by projecting the pressure tensor along the magnetic field and dividing by the density and by Boltzmanns constant. T_perp is the average of the two perpendicular components.
  17 + * v_para = (v.b) b and v_perp = v - (v.b) b. where v is the velocity vector and b is the magnetic field unit vector.
  18 +
  19 + These data are produced on the ground using 3-D data and thus are available at time resolutions which are limited by the
  20 + rate at which 3-D data can be transmitted. The data source used to generate the mome
  21 + nts is always the best available resolution 3-D data; this means mainly 3DR data but in the case 3DX or 3DXP are available these
  22 + are used instead for the MOMENTS production (see Mode_DataOrigin_HEEA/LEEA). Choices on the best way to combine data from the two
  23 + sensors can be made in the moments production software; in the first release the moments are made using LEEA data in the
  24 + energy overlap region.
  25 + In some situations, use of both sensors together may be a better choice, for example in case
  26 + s where the distribution changes
  27 + during a spin as the method can resolve time aliasing errors. If resources allow, the Moments
  28 + product at CAA may be updated to take advantage of this possibility.
  29 + The advantage of these ground - calculated moments is that the best available
  30 + calibration data is used, a correction can be made for the spacecraft potential
  31 + measurements (collected by the EFW experiment), and spacecraft electrons can be
  32 + properly removed. The current release has been generated automatically
  33 + using default values to control the approach to
  34 + potential correction and photoelectron removal, and has not been systematically human
  35 + - validated, so some errors may exist.
  36 + Specifically, the spacecraft potential, Vsc, is set to be 1 V greater than the
  37 + measured probe - spacecraft potential provided by
  38 + the electric field experiment (EFW) and the lower energy cutoff for the moments
  39 + integration is set to reject the energy bin
  40 + containing the EFW potential and the one above that (which in practice
  41 + may also contain counts due to spacecraft electrons).
  42 + Sometimes cold electrons are present which can appear in the same energy bin as the spacecraft photoelectrons,
  43 + therefore both the cold electrons and spacecraft photoelectrons are removed resulting in underestimated electron densities.
  44 + Recent work
  45 + by the EFW team suggests a more accurate determination of from would be a term that increases linearly
  46 + above ~10 V (Cully et al., 2007) but this has not yet been
  47 + implemented in our CAA moments generation code.</Description>
  48 + <Acknowledgement>Principal Investigator: Andrew Fazakerley</Acknowledgement>
44 <Contact> 49 <Contact>
45 - <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>  
46 - <Role>TechnicalContact</Role>  
47 - </Contact>  
48 - 50 + <PersonID>spase://SMWG/Person/Andrew.N.Fazakerley</PersonID>
  51 + <Role>PrincipalInvestigator</Role>
  52 + </Contact>
49 <InformationURL> 53 <InformationURL>
50 - <Name>NSSDC Master Catalog listing for Cluster II Rumba Plasma Electron and Current Experiment (PEACE)</Name> 54 + <Name>ESA web page</Name>
  55 + <URL>http://www.cosmos.esa.int/web/csa/documentation</URL>
  56 + <Description>This site contains PEACE data documentation</Description>
  57 + </InformationURL>
  58 + <InformationURL>
  59 + <Name>NSSDC Master Catalog listing for Cluster II Salsa Plasma Electron and Current Experiment (PEACE)</Name>
51 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-05</URL> 60 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-05</URL>
52 - <Description>This site provides information concerning the Cluster II Rumba Plasma Electron and Current Experiment Instrument.</Description>  
53 - </InformationURL> 61 + <Description>This site provides information concerning the Cluster II Salsa Plasma Electron and Current Experiment Instrument.</Description>
  62 + </InformationURL>
54 </ResourceHeader> 63 </ResourceHeader>
55 <AccessInformation> 64 <AccessInformation>
56 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID> 65 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
@@ -60,19 +69,18 @@ @@ -60,19 +69,18 @@
60 <Name>AMDA at CDPP</Name> 69 <Name>AMDA at CDPP</Name>
61 <URL>http://amda.cdpp.eu</URL> 70 <URL>http://amda.cdpp.eu</URL>
62 </AccessURL> 71 </AccessURL>
63 - <Format>NetCDF</Format>  
64 - <Acknowledgement>NASA, Dr. Andrew N. Fazakerley</Acknowledgement> 72 + <Format>NetCDF</Format>
65 </AccessInformation> 73 </AccessInformation>
66 <ProviderName>CSA</ProviderName> 74 <ProviderName>CSA</ProviderName>
67 <ProcessingLevel>Calibrated</ProcessingLevel> 75 <ProcessingLevel>Calibrated</ProcessingLevel>
68 - <ProviderResourceName>Cluster II Samba Prime Parameter Plasma Electron and Current Experiment (PEACE) Data</ProviderResourceName> 76 + <ProviderResourceName>C3_CP_PEA_MOMENTS</ProviderResourceName>
69 <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel> 77 <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
70 - <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Samba/PEACE</InstrumentID> 78 + <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Salsa/PEACE</InstrumentID>
71 <MeasurementType>ThermalPlasma</MeasurementType> 79 <MeasurementType>ThermalPlasma</MeasurementType>
72 <TemporalDescription> 80 <TemporalDescription>
73 <TimeSpan> 81 <TimeSpan>
74 - <StartDate>2001-01-09T15:15:12Z</StartDate>  
75 - <StopDate>2013-06-30T23:59:39Z</StopDate> 82 + <StartDate>2001-01-10T00:02:11Z</StartDate>
  83 + <StopDate>2013-06-30T12:39:50Z</StopDate>
76 </TimeSpan> 84 </TimeSpan>
77 <Cadence_Min>PT4S</Cadence_Min> 85 <Cadence_Min>PT4S</Cadence_Min>
78 <Cadence_Max>PT160S</Cadence_Max> 86 <Cadence_Max>PT160S</Cadence_Max>
@@ -101,8 +109,10 @@ @@ -101,8 +109,10 @@
101 <Keyword>lobe</Keyword> 109 <Keyword>lobe</Keyword>
102 <Parameter> 110 <Parameter>
103 <Name>density</Name> 111 <Name>density</Name>
104 - <ParameterKey>c3_pea_dens</ParameterKey>  
105 - <Description>Cluster II Samba Prime Parameter Plasma Electron and Current Experiment electron number density at spin time resolution</Description> 112 + <ParameterKey>c2_pea_dens</ParameterKey>
  113 + <Description>
  114 + Electron number density at spin time resolution
  115 + </Description>
106 <Ucd>phys.density;phys.electron</Ucd> 116 <Ucd>phys.density;phys.electron</Ucd>
107 <Cadence>PT4S</Cadence> 117 <Cadence>PT4S</Cadence>
108 <Units>cm^-3</Units> 118 <Units>cm^-3</Units>
@@ -124,8 +134,10 @@ @@ -124,8 +134,10 @@
124 </Parameter> 134 </Parameter>
125 <Parameter> 135 <Parameter>
126 <Name>v_gse</Name> 136 <Name>v_gse</Name>
127 - <ParameterKey>c3_pea_vgse</ParameterKey>  
128 - <Description>Cluster II Samba Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 137 + <ParameterKey>c2_pea_vgse</ParameterKey>
  138 + <Description>
  139 + Electron velocity at spin time resolution
  140 + </Description>
129 <Ucd>phys.veloc;phys.electron</Ucd> 141 <Ucd>phys.veloc;phys.electron</Ucd>
130 <Cadence>PT4S</Cadence> 142 <Cadence>PT4S</Cadence>
131 <Units>km/s</Units> 143 <Units>km/s</Units>
@@ -145,19 +157,19 @@ @@ -145,19 +157,19 @@
145 <Name>vx</Name> 157 <Name>vx</Name>
146 <Qualifier>Component.I</Qualifier> 158 <Qualifier>Component.I</Qualifier>
147 <Index>1</Index> 159 <Index>1</Index>
148 - <ParameterKey>c3_pea_vgse(0)</ParameterKey> 160 + <ParameterKey>c2_pea_vgse(0)</ParameterKey>
149 </Element> 161 </Element>
150 <Element> 162 <Element>
151 <Name>vy</Name> 163 <Name>vy</Name>
152 <Qualifier>Component.J</Qualifier> 164 <Qualifier>Component.J</Qualifier>
153 <Index>2</Index> 165 <Index>2</Index>
154 - <ParameterKey>c3_pea_vgse(1)</ParameterKey> 166 + <ParameterKey>c2_pea_vgse(1)</ParameterKey>
155 </Element> 167 </Element>
156 <Element> 168 <Element>
157 <Name>vz</Name> 169 <Name>vz</Name>
158 <Qualifier>Component.K</Qualifier> 170 <Qualifier>Component.K</Qualifier>
159 <Index>3</Index> 171 <Index>3</Index>
160 - <ParameterKey>c3_pea_vgse(2)</ParameterKey> 172 + <ParameterKey>c2_pea_vgse(2)</ParameterKey>
161 </Element> 173 </Element>
162 </Structure> 174 </Structure>
163 <ValidMin>-10000</ValidMin> 175 <ValidMin>-10000</ValidMin>
@@ -171,8 +183,10 @@ @@ -171,8 +183,10 @@
171 </Parameter> 183 </Parameter>
172 <Parameter> 184 <Parameter>
173 <Name>v_gsm</Name> 185 <Name>v_gsm</Name>
174 - <ParameterKey>c3_pea_vgsm</ParameterKey>  
175 - <Description>Cluster II Samba Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 186 + <ParameterKey>c2_pea_vgsm</ParameterKey>
  187 + <Description>
  188 + Electron velocity at spin time resolution, in GSM
  189 + </Description>
176 <Ucd>phys.veloc;phys.electron</Ucd> 190 <Ucd>phys.veloc;phys.electron</Ucd>
177 <Cadence>PT4S</Cadence> 191 <Cadence>PT4S</Cadence>
178 <Units>km/s</Units> 192 <Units>km/s</Units>
@@ -192,19 +206,19 @@ @@ -192,19 +206,19 @@
192 <Name>vx</Name> 206 <Name>vx</Name>
193 <Qualifier>Component.I</Qualifier> 207 <Qualifier>Component.I</Qualifier>
194 <Index>1</Index> 208 <Index>1</Index>
195 - <ParameterKey>c3_pea_vgsm(0)</ParameterKey> 209 + <ParameterKey>c2_pea_vgsm(0)</ParameterKey>
196 </Element> 210 </Element>
197 <Element> 211 <Element>
198 <Name>vy</Name> 212 <Name>vy</Name>
199 <Qualifier>Component.J</Qualifier> 213 <Qualifier>Component.J</Qualifier>
200 <Index>2</Index> 214 <Index>2</Index>
201 - <ParameterKey>c3_pea_vgsm(1)</ParameterKey> 215 + <ParameterKey>c2_pea_vgsm(1)</ParameterKey>
202 </Element> 216 </Element>
203 <Element> 217 <Element>
204 <Name>vz</Name> 218 <Name>vz</Name>
205 <Qualifier>Component.K</Qualifier> 219 <Qualifier>Component.K</Qualifier>
206 <Index>3</Index> 220 <Index>3</Index>
207 - <ParameterKey>c3_pea_vgsm(2)</ParameterKey> 221 + <ParameterKey>c2_pea_vgsm(2)</ParameterKey>
208 </Element> 222 </Element>
209 </Structure> 223 </Structure>
210 <ValidMin>-10000</ValidMin> 224 <ValidMin>-10000</ValidMin>
@@ -218,8 +232,10 @@ @@ -218,8 +232,10 @@
218 </Parameter> 232 </Parameter>
219 <Parameter> 233 <Parameter>
220 <Name>v_para_gse</Name> 234 <Name>v_para_gse</Name>
221 - <ParameterKey>c3_pea_vpar</ParameterKey>  
222 - <Description>Cluster II Samba Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 235 + <ParameterKey>c2_pea_vpar</ParameterKey>
  236 + <Description>
  237 + Electron parallel velocity at spin time resolution, in GSE
  238 + </Description>
223 <Ucd>phys.veloc;phys.electron</Ucd> 239 <Ucd>phys.veloc;phys.electron</Ucd>
224 <Cadence>PT4S</Cadence> 240 <Cadence>PT4S</Cadence>
225 <Units>km/s</Units> 241 <Units>km/s</Units>
@@ -239,19 +255,19 @@ @@ -239,19 +255,19 @@
239 <Name>vx</Name> 255 <Name>vx</Name>
240 <Qualifier>Component.I</Qualifier> 256 <Qualifier>Component.I</Qualifier>
241 <Index>1</Index> 257 <Index>1</Index>
242 - <ParameterKey>c3_pea_vpar(0)</ParameterKey> 258 + <ParameterKey>c2_pea_vpar(0)</ParameterKey>
243 </Element> 259 </Element>
244 <Element> 260 <Element>
245 <Name>vy</Name> 261 <Name>vy</Name>
246 <Qualifier>Component.J</Qualifier> 262 <Qualifier>Component.J</Qualifier>
247 <Index>2</Index> 263 <Index>2</Index>
248 - <ParameterKey>c3_pea_vpar(1)</ParameterKey> 264 + <ParameterKey>c2_pea_vpar(1)</ParameterKey>
249 </Element> 265 </Element>
250 <Element> 266 <Element>
251 <Name>vz</Name> 267 <Name>vz</Name>
252 <Qualifier>Component.K</Qualifier> 268 <Qualifier>Component.K</Qualifier>
253 <Index>3</Index> 269 <Index>3</Index>
254 - <ParameterKey>c3_pea_vpar(2)</ParameterKey> 270 + <ParameterKey>c2_pea_vpar(2)</ParameterKey>
255 </Element> 271 </Element>
256 </Structure> 272 </Structure>
257 <ValidMin>-10000</ValidMin> 273 <ValidMin>-10000</ValidMin>
@@ -265,8 +281,10 @@ @@ -265,8 +281,10 @@
265 </Parameter> 281 </Parameter>
266 <Parameter> 282 <Parameter>
267 <Name>v_para_gsm</Name> 283 <Name>v_para_gsm</Name>
268 - <ParameterKey>c3_pea_vpar_gsm</ParameterKey>  
269 - <Description>Cluster II Samba Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 284 + <ParameterKey>c2_pea_vpar_gsm</ParameterKey>
  285 + <Description>
  286 + Electron parallel velocity at spin time resolution, in GSM
  287 + </Description>
270 <Ucd>phys.veloc;phys.electron</Ucd> 288 <Ucd>phys.veloc;phys.electron</Ucd>
271 <Cadence>PT4S</Cadence> 289 <Cadence>PT4S</Cadence>
272 <Units>km/s</Units> 290 <Units>km/s</Units>
@@ -286,19 +304,19 @@ @@ -286,19 +304,19 @@
286 <Name>vx</Name> 304 <Name>vx</Name>
287 <Qualifier>Component.I</Qualifier> 305 <Qualifier>Component.I</Qualifier>
288 <Index>1</Index> 306 <Index>1</Index>
289 - <ParameterKey>c3_pea_vpar_gsm(0)</ParameterKey> 307 + <ParameterKey>c2_pea_vpar_gsm(0)</ParameterKey>
290 </Element> 308 </Element>
291 <Element> 309 <Element>
292 <Name>vy</Name> 310 <Name>vy</Name>
293 <Qualifier>Component.J</Qualifier> 311 <Qualifier>Component.J</Qualifier>
294 <Index>2</Index> 312 <Index>2</Index>
295 - <ParameterKey>c3_pea_vpar_gsm(1)</ParameterKey> 313 + <ParameterKey>c2_pea_vpar_gsm(1)</ParameterKey>
296 </Element> 314 </Element>
297 <Element> 315 <Element>
298 <Name>vz</Name> 316 <Name>vz</Name>
299 <Qualifier>Component.K</Qualifier> 317 <Qualifier>Component.K</Qualifier>
300 <Index>3</Index> 318 <Index>3</Index>
301 - <ParameterKey>c3_pea_vpar_gsm(2)</ParameterKey> 319 + <ParameterKey>c2_pea_vpar_gsm(2)</ParameterKey>
302 </Element> 320 </Element>
303 </Structure> 321 </Structure>
304 <ValidMin>-10000</ValidMin> 322 <ValidMin>-10000</ValidMin>
@@ -312,8 +330,10 @@ @@ -312,8 +330,10 @@
312 </Parameter> 330 </Parameter>
313 <Parameter> 331 <Parameter>
314 <Name>v_perp_gse</Name> 332 <Name>v_perp_gse</Name>
315 - <ParameterKey>c3_pea_vperp</ParameterKey>  
316 - <Description>Cluster II Samba Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 333 + <ParameterKey>c2_pea_vperp</ParameterKey>
  334 + <Description>
  335 + Electron perpendicular velocity at spin time resolution, in GSE
  336 + </Description>
317 <Ucd>phys.veloc;phys.electron</Ucd> 337 <Ucd>phys.veloc;phys.electron</Ucd>
318 <Cadence>PT4S</Cadence> 338 <Cadence>PT4S</Cadence>
319 <Units>km/s</Units> 339 <Units>km/s</Units>
@@ -333,19 +353,19 @@ @@ -333,19 +353,19 @@
333 <Name>vx</Name> 353 <Name>vx</Name>
334 <Qualifier>Component.I</Qualifier> 354 <Qualifier>Component.I</Qualifier>
335 <Index>1</Index> 355 <Index>1</Index>
336 - <ParameterKey>c3_pea_vperp(0)</ParameterKey> 356 + <ParameterKey>c2_pea_vperp(0)</ParameterKey>
337 </Element> 357 </Element>
338 <Element> 358 <Element>
339 <Name>vy</Name> 359 <Name>vy</Name>
340 <Qualifier>Component.J</Qualifier> 360 <Qualifier>Component.J</Qualifier>
341 <Index>2</Index> 361 <Index>2</Index>
342 - <ParameterKey>c3_pea_vperp(1)</ParameterKey> 362 + <ParameterKey>c2_pea_vperp(1)</ParameterKey>
343 </Element> 363 </Element>
344 <Element> 364 <Element>
345 <Name>vz</Name> 365 <Name>vz</Name>
346 <Qualifier>Component.K</Qualifier> 366 <Qualifier>Component.K</Qualifier>
347 <Index>3</Index> 367 <Index>3</Index>
348 - <ParameterKey>c3_pea_vperp(2)</ParameterKey> 368 + <ParameterKey>c2_pea_vperp(2)</ParameterKey>
349 </Element> 369 </Element>
350 </Structure> 370 </Structure>
351 <ValidMin>-10000</ValidMin> 371 <ValidMin>-10000</ValidMin>
@@ -359,8 +379,10 @@ @@ -359,8 +379,10 @@
359 </Parameter> 379 </Parameter>
360 <Parameter> 380 <Parameter>
361 <Name>v_perp_gsm</Name> 381 <Name>v_perp_gsm</Name>
362 - <ParameterKey>c3_pea_vperp_gsm</ParameterKey>  
363 - <Description>Cluster II Samba Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 382 + <ParameterKey>c2_pea_vperp_gsm</ParameterKey>
  383 + <Description>
  384 + Electron perpendicular velocity at spin time resolution, in GSM
  385 + </Description>
364 <Ucd>phys.veloc;phys.electron</Ucd> 386 <Ucd>phys.veloc;phys.electron</Ucd>
365 <Cadence>PT4S</Cadence> 387 <Cadence>PT4S</Cadence>
366 <Units>km/s</Units> 388 <Units>km/s</Units>
@@ -380,19 +402,19 @@ @@ -380,19 +402,19 @@
380 <Name>vx</Name> 402 <Name>vx</Name>
381 <Qualifier>Component.I</Qualifier> 403 <Qualifier>Component.I</Qualifier>
382 <Index>1</Index> 404 <Index>1</Index>
383 - <ParameterKey>c3_pea_vperp_gsm(0)</ParameterKey> 405 + <ParameterKey>c2_pea_vperp_gsm(0)</ParameterKey>
384 </Element> 406 </Element>
385 <Element> 407 <Element>
386 <Name>vy</Name> 408 <Name>vy</Name>
387 <Qualifier>Component.J</Qualifier> 409 <Qualifier>Component.J</Qualifier>
388 <Index>2</Index> 410 <Index>2</Index>
389 - <ParameterKey>c3_pea_vperp_gsm(1)</ParameterKey> 411 + <ParameterKey>c2_pea_vperp_gsm(1)</ParameterKey>
390 </Element> 412 </Element>
391 <Element> 413 <Element>
392 <Name>vz</Name> 414 <Name>vz</Name>
393 <Qualifier>Component.K</Qualifier> 415 <Qualifier>Component.K</Qualifier>
394 <Index>3</Index> 416 <Index>3</Index>
395 - <ParameterKey>c3_pea_vperp_gsm(2)</ParameterKey> 417 + <ParameterKey>c2_pea_vperp_gsm(2)</ParameterKey>
396 </Element> 418 </Element>
397 </Structure> 419 </Structure>
398 <ValidMin>-10000</ValidMin> 420 <ValidMin>-10000</ValidMin>
@@ -406,11 +428,13 @@ @@ -406,11 +428,13 @@
406 </Parameter> 428 </Parameter>
407 <Parameter> 429 <Parameter>
408 <Name>heat_flux_gse</Name> 430 <Name>heat_flux_gse</Name>
409 - <ParameterKey>c3_pea_flux</ParameterKey>  
410 - <Description>Cluster II Samba Prime Parameter Plasma Electron and Current Experiment parallel electron heat flux at spin time resolution</Description> 431 + <ParameterKey>c2_pea_flux</ParameterKey>
  432 + <Description>
  433 + Parallel electron heat flux at spin time resolution, in GSE
  434 + </Description>
411 <Ucd>phys.heatflux;phys.atmol.ionStage</Ucd> 435 <Ucd>phys.heatflux;phys.atmol.ionStage</Ucd>
412 <Cadence>PT4S</Cadence> 436 <Cadence>PT4S</Cadence>
413 - <Units>microW/m^2</Units> 437 + <Units>microW/m^2</Units>
414 <RenderingHints> 438 <RenderingHints>
415 <DisplayType>TimeSeries</DisplayType> 439 <DisplayType>TimeSeries</DisplayType>
416 </RenderingHints> 440 </RenderingHints>
@@ -419,17 +443,17 @@ @@ -419,17 +443,17 @@
419 <Element> 443 <Element>
420 <Name>flux_x</Name> 444 <Name>flux_x</Name>
421 <Index>1</Index> 445 <Index>1</Index>
422 - <ParameterKey>c3_pea_flux(0)</ParameterKey> 446 + <ParameterKey>c2_pea_flux(0)</ParameterKey>
423 </Element> 447 </Element>
424 <Element> 448 <Element>
425 <Name>flux_y</Name> 449 <Name>flux_y</Name>
426 <Index>1</Index> 450 <Index>1</Index>
427 - <ParameterKey>c3_pea_flux(1)</ParameterKey> 451 + <ParameterKey>c2_pea_flux(1)</ParameterKey>
428 </Element> 452 </Element>
429 <Element> 453 <Element>
430 <Name>flux_z</Name> 454 <Name>flux_z</Name>
431 <Index>1</Index> 455 <Index>1</Index>
432 - <ParameterKey>c3_pea_flux(2)</ParameterKey> 456 + <ParameterKey>c2_pea_flux(2)</ParameterKey>
433 </Element> 457 </Element>
434 </Structure> 458 </Structure>
435 <Particle> 459 <Particle>
@@ -440,8 +464,10 @@ @@ -440,8 +464,10 @@
440 </Parameter> 464 </Parameter>
441 <Parameter> 465 <Parameter>
442 <Name>pressure_gse</Name> 466 <Name>pressure_gse</Name>
443 - <ParameterKey>c3_pea_press</ParameterKey>  
444 - <Description>Cluster II Samba Prime Parameter Plasma Electron and Current Experiment parallel pressure tensor at spin time resolution</Description> 467 + <ParameterKey>c2_pea_press</ParameterKey>
  468 + <Description>
  469 + Electron pressure tensor at spin time resolution, in GSE
  470 + </Description>
445 <Ucd>phys.pressure</Ucd> 471 <Ucd>phys.pressure</Ucd>
446 <Cadence>PT4S</Cadence> 472 <Cadence>PT4S</Cadence>
447 <Units>microW/m^2</Units> 473 <Units>microW/m^2</Units>
@@ -453,21 +479,51 @@ @@ -453,21 +479,51 @@
453 <DisplayType>TimeSeries</DisplayType> 479 <DisplayType>TimeSeries</DisplayType>
454 </RenderingHints> 480 </RenderingHints>
455 <Structure> 481 <Structure>
456 - <Size>3</Size> 482 + <Size>9</Size>
457 <Element> 483 <Element>
458 <Name>xx</Name> 484 <Name>xx</Name>
459 <Index>1</Index> 485 <Index>1</Index>
460 - <ParameterKey>c3_pea_press(0)</ParameterKey> 486 + <ParameterKey>c2_pea_press(0)</ParameterKey>
461 </Element> 487 </Element>
462 <Element> 488 <Element>
463 - <Name>yy</Name> 489 + <Name>xy</Name>
464 <Index>2</Index> 490 <Index>2</Index>
465 - <ParameterKey>c3_pea_press(4)</ParameterKey> 491 + <ParameterKey>c2_pea_press(1)</ParameterKey>
466 </Element> 492 </Element>
467 <Element> 493 <Element>
468 - <Name>zz</Name> 494 + <Name>xz</Name>
469 <Index>3</Index> 495 <Index>3</Index>
470 - <ParameterKey>c3_pea_press(8)</ParameterKey> 496 + <ParameterKey>c2_pea_press(2)</ParameterKey>
  497 + </Element>
  498 + <Element>
  499 + <Name>yx</Name>
  500 + <Index>4</Index>
  501 + <ParameterKey>c2_pea_press(3)</ParameterKey>
  502 + </Element>
  503 + <Element>
  504 + <Name>yy</Name>
  505 + <Index>5</Index>
  506 + <ParameterKey>c2_pea_press(4)</ParameterKey>
  507 + </Element>
  508 + <Element>
  509 + <Name>yz</Name>
  510 + <Index>6</Index>
  511 + <ParameterKey>c2_pea_press(5)</ParameterKey>
  512 + </Element>
  513 + <Element>
  514 + <Name>zx</Name>
  515 + <Index>7</Index>
  516 + <ParameterKey>c2_pea_press(6)</ParameterKey>
  517 + </Element>
  518 + <Element>
  519 + <Name>zy</Name>
  520 + <Index>8</Index>
  521 + <ParameterKey>c2_pea_press(7)</ParameterKey>
  522 + </Element>
  523 + <Element>
  524 + <Name>zz</Name>
  525 + <Index>9</Index>
  526 + <ParameterKey>c2_pea_press(8)</ParameterKey>
471 </Element> 527 </Element>
472 </Structure> 528 </Structure>
473 <Particle> 529 <Particle>
@@ -478,8 +534,10 @@ @@ -478,8 +534,10 @@
478 </Parameter> 534 </Parameter>
479 <Parameter> 535 <Parameter>
480 <Name>t_para</Name> 536 <Name>t_para</Name>
481 - <ParameterKey>c3_pea_tpar</ParameterKey>  
482 - <Description>Cluster II Samba Prime Parameter Plasma Electron and Current Experiment parallel electron temperature at spin time resolution</Description> 537 + <ParameterKey>c2_pea_tpar</ParameterKey>
  538 + <Description>
  539 + Parallel electron temperature at spin time resolution
  540 + </Description>
483 <Ucd>phys.temperature;phys.electron</Ucd> 541 <Ucd>phys.temperature;phys.electron</Ucd>
484 <Cadence>PT4S</Cadence> 542 <Cadence>PT4S</Cadence>
485 <Units>eV</Units> 543 <Units>eV</Units>
@@ -495,15 +553,16 @@ @@ -495,15 +553,16 @@
495 </Parameter> 553 </Parameter>
496 <Parameter> 554 <Parameter>
497 <Name>t_perp</Name> 555 <Name>t_perp</Name>
498 - <ParameterKey>c3_pea_tperp</ParameterKey>  
499 - <Description>Cluster II Samba Prime Parameter Plasma Electron and Current Experiment perpendicular electron temperature at spin time resolution</Description> 556 + <ParameterKey>c2_pea_tperp</ParameterKey>
  557 + <Description>
  558 + Perpendicular electron temperature at spin time resolution
  559 + </Description>
500 <Ucd>phys.temperature;phys.electron</Ucd> 560 <Ucd>phys.temperature;phys.electron</Ucd>
501 <Cadence>PT4S</Cadence> 561 <Cadence>PT4S</Cadence>
502 <Units>eV</Units> 562 <Units>eV</Units>
503 <RenderingHints> 563 <RenderingHints>
504 <DisplayType>TimeSeries</DisplayType> 564 <DisplayType>TimeSeries</DisplayType>
505 </RenderingHints> 565 </RenderingHints>
506 - <FillValue>-1.0000e+31</FillValue>  
507 <Particle> 566 <Particle>
508 <ParticleType>Electron</ParticleType> 567 <ParticleType>Electron</ParticleType>
509 <Qualifier>Scalar</Qualifier> 568 <Qualifier>Scalar</Qualifier>
NumericalData/AMDA/Cluster/Cluster4/PEACE/clust4-pea-mom.xml
@@ -5,51 +5,61 @@ @@ -5,51 +5,61 @@
5 <ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster4/PEACE/clust4-pea-mom</ResourceID> 5 <ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster4/PEACE/clust4-pea-mom</ResourceID>
6 <ResourceHeader> 6 <ResourceHeader>
7 <ResourceName>electron moments</ResourceName> 7 <ResourceName>electron moments</ResourceName>
8 - <AlternateName>Cluster 4 Prime Parameter PEACE Data</AlternateName>  
9 - <ReleaseDate>2015-10-16T16:51:44Z</ReleaseDate>  
10 - <Description>The primary task of this instrument (PEACE: Plasma Electrons and Currents Experiment)  
11 - is to obtain the velocity moments of the distribution function of electrons as frequently and  
12 - as accurately as the spacecraft telemetry will allow. Detector counts are collected in energy,  
13 - polar-angle, and azimuth-angle bins to form a three-dimensional matrix.  
14 - Two sensors are used: LEEA (low-energy electron analyzer) and HEEA (high-energy electron analyzer).  
15 - The energy coverage is from 0.67 eV to 30 KeV in 92 levels. The first 16 levels are equally spaced linearly  
16 - up to 10.7 eV; the remainder are logarithmically spaced. Both sensors can use the full range, but the HEEA  
17 - will normally operate over a higher energy range than the LEEA. The LEEA specializes in coverage of the  
18 - energies from 0.7-10 eV, and has a geometric factor one fifth that of the HEAA. Both sensors consist of  
19 - hemispherical electrostatic analyzers of the top-hat type and a detector in the form of an annular  
20 - micro-channel plate with a position-sensitive readout. Each sensor covers the range 0-180 degrees  
21 - with respect to the spin axis, and they are mounted opposite each other with a view perpendicular  
22 - to the spin axis, thus covering the complete angular range in a half rotation of the spacecraft.  
23 - The field of view perpendicular to the fan is 2 degrees for the LEEA and 5.6 degrees for the HEEA.  
24 - Energy resolution (Delta-E)/E is 0.13 for LEEA and 0.16 for HEEA. There are four sweep modes,  
25 - synchronized to the spin period (4 s), to vary the azimuthal angular resolution.  
26 - The spin phasing can be made coincident with that of the CIS instrument, to ensure that the electron  
27 - and ion moments will be measured simultaneously. On-board processing is used to calculate the moments  
28 - of the distribution with an accuracy of 1% and to select suitable parts of the complete distribution  
29 - for transmission. The normal science data format is based on one spin period, and consists of core data  
30 - followed by other optional distributions as can be fit into the available telemetry for that spin.  
31 - The core data (moments, spacecraft potential, and pitch angle distribution) are always transmitted  
32 - (if the spin is nominal). The next distribution is transmitted if, before the end of the spin,  
33 - all the previous data have been sent. Thus the next spin of data will be transmitted slightly late,  
34 - but all of its core data will be transmitted before the following spin of data is started on.  
35 - Eventually the transmission will catch up and be able to transmit the distribution after the core again,  
36 - but only after some time. This applies at all telemetry rates. The instrument can adapt automatically to  
37 - six different telemetry rates: a basic 1.52 Kbps rate (CIS priority); a normal 2.52 Kbps rate;  
38 - an enhanced PEACE priority rate of 3.54 Kbps; and three burst mode rates, with a maximum of 15.98 Kbps.  
39 - For more details of the Cluster mission, the spacecraft, and its instruments,  
40 - see the report Cluster: mission, payload and supporting activities, March 1993, ESA SP-1159,  
41 - and the included article PEACE: a Plasma Electron and Current Experiment, by A. D. Johnstone et al.,  
42 - from which this information was obtained.</Description>  
43 - <Acknowledgement>NASA, Dr. Andrew N. Fazakerley, European Space Agency</Acknowledgement> 8 + <AlternateName>Cluster 4 electron moments</AlternateName>
  9 + <ReleaseDate>2016-10-16T16:51:44Z</ReleaseDate>
  10 + <Description> The CAA Moments data are electron density, velocity vector,
  11 + pressure tensor and heat flux vector. The vectors and tensors are provided in GSE coordinates. Velocity and temperature
  12 + are also provided as components perpendicular and parallel to the magnetic field.
  13 + The magnetic field data is taken from CSDS FGM PP data, at present. In a possible future
  14 + release we would ideally use CAA FGM data, but it is considered unlikely that there will be major differences except in
  15 + very weak field regions. Furthermore :
  16 + * T_perp and T_para are determined by projecting the pressure tensor along the magnetic field and dividing by the density and by Boltzmanns constant. T_perp is the average of the two perpendicular components.
  17 + * v_para = (v.b) b and v_perp = v - (v.b) b. where v is the velocity vector and b is the magnetic field unit vector.
  18 +
  19 + These data are produced on the ground using 3-D data and thus are available at time resolutions which are limited by the
  20 + rate at which 3-D data can be transmitted. The data source used to generate the mome
  21 + nts is always the best available resolution 3-D data; this means mainly 3DR data but in the case 3DX or 3DXP are available these
  22 + are used instead for the MOMENTS production (see Mode_DataOrigin_HEEA/LEEA). Choices on the best way to combine data from the two
  23 + sensors can be made in the moments production software; in the first release the moments are made using LEEA data in the
  24 + energy overlap region.
  25 + In some situations, use of both sensors together may be a better choice, for example in case
  26 + s where the distribution changes
  27 + during a spin as the method can resolve time aliasing errors. If resources allow, the Moments
  28 + product at CAA may be updated to take advantage of this possibility.
  29 + The advantage of these ground - calculated moments is that the best available
  30 + calibration data is used, a correction can be made for the spacecraft potential
  31 + measurements (collected by the EFW experiment), and spacecraft electrons can be
  32 + properly removed. The current release has been generated automatically
  33 + using default values to control the approach to
  34 + potential correction and photoelectron removal, and has not been systematically human
  35 + - validated, so some errors may exist.
  36 + Specifically, the spacecraft potential, Vsc, is set to be 1 V greater than the
  37 + measured probe - spacecraft potential provided by
  38 + the electric field experiment (EFW) and the lower energy cutoff for the moments
  39 + integration is set to reject the energy bin
  40 + containing the EFW potential and the one above that (which in practice
  41 + may also contain counts due to spacecraft electrons).
  42 + Sometimes cold electrons are present which can appear in the same energy bin as the spacecraft photoelectrons,
  43 + therefore both the cold electrons and spacecraft photoelectrons are removed resulting in underestimated electron densities.
  44 + Recent work
  45 + by the EFW team suggests a more accurate determination of from would be a term that increases linearly
  46 + above ~10 V (Cully et al., 2007) but this has not yet been
  47 + implemented in our CAA moments generation code.</Description>
  48 + <Acknowledgement>Principal Investigator: Andrew Fazakerley</Acknowledgement>
44 <Contact> 49 <Contact>
45 - <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>  
46 - <Role>TechnicalContact</Role>  
47 - </Contact> 50 + <PersonID>spase://SMWG/Person/Andrew.N.Fazakerley</PersonID>
  51 + <Role>PrincipalInvestigator</Role>
  52 + </Contact>
  53 + <InformationURL>
  54 + <Name>ESA web page</Name>
  55 + <URL>http://www.cosmos.esa.int/web/csa/documentation</URL>
  56 + <Description>This site contains PEACE data documentation</Description>
  57 + </InformationURL>
48 <InformationURL> 58 <InformationURL>
49 <Name>NSSDC Master Catalog listing for Cluster II Tango Plasma Electron and Current Experiment (PEACE)</Name> 59 <Name>NSSDC Master Catalog listing for Cluster II Tango Plasma Electron and Current Experiment (PEACE)</Name>
50 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-05</URL> 60 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-05</URL>
51 <Description>This site provides information concerning the Cluster II Tango Plasma Electron and Current Experiment Instrument.</Description> 61 <Description>This site provides information concerning the Cluster II Tango Plasma Electron and Current Experiment Instrument.</Description>
52 - </InformationURL> 62 + </InformationURL>
53 </ResourceHeader> 63 </ResourceHeader>
54 <AccessInformation> 64 <AccessInformation>
55 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID> 65 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
@@ -59,19 +69,18 @@ @@ -59,19 +69,18 @@
59 <Name>AMDA at CDPP</Name> 69 <Name>AMDA at CDPP</Name>
60 <URL>http://amda.cdpp.eu</URL> 70 <URL>http://amda.cdpp.eu</URL>
61 </AccessURL> 71 </AccessURL>
62 - <Format>NetCDF</Format>  
63 - <Acknowledgement>NASA, Dr. Andrew N. Fazakerley</Acknowledgement> 72 + <Format>NetCDF</Format>
64 </AccessInformation> 73 </AccessInformation>
65 <ProviderName>CSA</ProviderName> 74 <ProviderName>CSA</ProviderName>
66 <ProcessingLevel>Calibrated</ProcessingLevel> 75 <ProcessingLevel>Calibrated</ProcessingLevel>
67 - <ProviderResourceName>Cluster II Tango Prime Parameter Plasma Electron and Current Experiment (PEACE) Data</ProviderResourceName> 76 + <ProviderResourceName>C4_CP_PEA_MOMENTS</ProviderResourceName>
68 <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel> 77 <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
69 <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Tango/PEACE</InstrumentID> 78 <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Tango/PEACE</InstrumentID>
70 <MeasurementType>ThermalPlasma</MeasurementType> 79 <MeasurementType>ThermalPlasma</MeasurementType>
71 <TemporalDescription> 80 <TemporalDescription>
72 <TimeSpan> 81 <TimeSpan>
73 - <StartDate>2001-01-09T15:15:32Z</StartDate>  
74 - <StopDate>2013-06-30T12:59:57Z</StopDate> 82 + <StartDate>2001-01-10T00:02:11Z</StartDate>
  83 + <StopDate>2013-06-30T12:39:50Z</StopDate>
75 </TimeSpan> 84 </TimeSpan>
76 <Cadence_Min>PT4S</Cadence_Min> 85 <Cadence_Min>PT4S</Cadence_Min>
77 <Cadence_Max>PT160S</Cadence_Max> 86 <Cadence_Max>PT160S</Cadence_Max>
@@ -101,8 +110,11 @@ @@ -101,8 +110,11 @@
101 <Parameter> 110 <Parameter>
102 <Name>density</Name> 111 <Name>density</Name>
103 <ParameterKey>c4_pea_dens</ParameterKey> 112 <ParameterKey>c4_pea_dens</ParameterKey>
104 - <Description>Cluster II Tango Prime Parameter Plasma Electron and Current Experiment electron number density at spin time resolution</Description> 113 + <Description>
  114 + Electron number density at spin time resolution
  115 + </Description>
105 <Ucd>phys.density;phys.electron</Ucd> 116 <Ucd>phys.density;phys.electron</Ucd>
  117 + <Cadence>PT4S</Cadence>
106 <Units>cm^-3</Units> 118 <Units>cm^-3</Units>
107 <UnitsConversion>1.0e6&gt;m^-3</UnitsConversion> 119 <UnitsConversion>1.0e6&gt;m^-3</UnitsConversion>
108 <RenderingHints> 120 <RenderingHints>
@@ -123,8 +135,11 @@ @@ -123,8 +135,11 @@
123 <Parameter> 135 <Parameter>
124 <Name>v_gse</Name> 136 <Name>v_gse</Name>
125 <ParameterKey>c4_pea_vgse</ParameterKey> 137 <ParameterKey>c4_pea_vgse</ParameterKey>
126 - <Description>Cluster II Tango Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 138 + <Description>
  139 + Electron velocity at spin time resolution
  140 + </Description>
127 <Ucd>phys.veloc;phys.electron</Ucd> 141 <Ucd>phys.veloc;phys.electron</Ucd>
  142 + <Cadence>PT4S</Cadence>
128 <Units>km/s</Units> 143 <Units>km/s</Units>
129 <UnitsConversion>1.0e3&gt;m s^-1</UnitsConversion> 144 <UnitsConversion>1.0e3&gt;m s^-1</UnitsConversion>
130 <CoordinateSystem> 145 <CoordinateSystem>
@@ -169,8 +184,11 @@ @@ -169,8 +184,11 @@
169 <Parameter> 184 <Parameter>
170 <Name>v_gsm</Name> 185 <Name>v_gsm</Name>
171 <ParameterKey>c4_pea_vgsm</ParameterKey> 186 <ParameterKey>c4_pea_vgsm</ParameterKey>
172 - <Description>Cluster II Tango Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 187 + <Description>
  188 + Electron velocity at spin time resolution, in GSM
  189 + </Description>
173 <Ucd>phys.veloc;phys.electron</Ucd> 190 <Ucd>phys.veloc;phys.electron</Ucd>
  191 + <Cadence>PT4S</Cadence>
174 <Units>km/s</Units> 192 <Units>km/s</Units>
175 <UnitsConversion>1.0e3&gt;m s^-1</UnitsConversion> 193 <UnitsConversion>1.0e3&gt;m s^-1</UnitsConversion>
176 <CoordinateSystem> 194 <CoordinateSystem>
@@ -215,8 +233,11 @@ @@ -215,8 +233,11 @@
215 <Parameter> 233 <Parameter>
216 <Name>v_para_gse</Name> 234 <Name>v_para_gse</Name>
217 <ParameterKey>c4_pea_vpar</ParameterKey> 235 <ParameterKey>c4_pea_vpar</ParameterKey>
218 - <Description>Cluster II Tango Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 236 + <Description>
  237 + Electron parallel velocity at spin time resolution, in GSE
  238 + </Description>
219 <Ucd>phys.veloc;phys.electron</Ucd> 239 <Ucd>phys.veloc;phys.electron</Ucd>
  240 + <Cadence>PT4S</Cadence>
220 <Units>km/s</Units> 241 <Units>km/s</Units>
221 <UnitsConversion>1.0e3&gt;m s^-1</UnitsConversion> 242 <UnitsConversion>1.0e3&gt;m s^-1</UnitsConversion>
222 <CoordinateSystem> 243 <CoordinateSystem>
@@ -261,8 +282,11 @@ @@ -261,8 +282,11 @@
261 <Parameter> 282 <Parameter>
262 <Name>v_para_gsm</Name> 283 <Name>v_para_gsm</Name>
263 <ParameterKey>c4_pea_vpar_gsm</ParameterKey> 284 <ParameterKey>c4_pea_vpar_gsm</ParameterKey>
264 - <Description>Cluster II Tango Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 285 + <Description>
  286 + Electron parallel velocity at spin time resolution, in GSM
  287 + </Description>
265 <Ucd>phys.veloc;phys.electron</Ucd> 288 <Ucd>phys.veloc;phys.electron</Ucd>
  289 + <Cadence>PT4S</Cadence>
266 <Units>km/s</Units> 290 <Units>km/s</Units>
267 <UnitsConversion>1.0e3&gt;m s^-1</UnitsConversion> 291 <UnitsConversion>1.0e3&gt;m s^-1</UnitsConversion>
268 <CoordinateSystem> 292 <CoordinateSystem>
@@ -307,8 +331,11 @@ @@ -307,8 +331,11 @@
307 <Parameter> 331 <Parameter>
308 <Name>v_perp_gse</Name> 332 <Name>v_perp_gse</Name>
309 <ParameterKey>c4_pea_vperp</ParameterKey> 333 <ParameterKey>c4_pea_vperp</ParameterKey>
310 - <Description>Cluster II Tango Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 334 + <Description>
  335 + Electron perpendicular velocity at spin time resolution, in GSE
  336 + </Description>
311 <Ucd>phys.veloc;phys.electron</Ucd> 337 <Ucd>phys.veloc;phys.electron</Ucd>
  338 + <Cadence>PT4S</Cadence>
312 <Units>km/s</Units> 339 <Units>km/s</Units>
313 <UnitsConversion>1.0e3&gt;m s^-1</UnitsConversion> 340 <UnitsConversion>1.0e3&gt;m s^-1</UnitsConversion>
314 <CoordinateSystem> 341 <CoordinateSystem>
@@ -353,8 +380,11 @@ @@ -353,8 +380,11 @@
353 <Parameter> 380 <Parameter>
354 <Name>v_perp_gsm</Name> 381 <Name>v_perp_gsm</Name>
355 <ParameterKey>c4_pea_vperp_gsm</ParameterKey> 382 <ParameterKey>c4_pea_vperp_gsm</ParameterKey>
356 - <Description>Cluster II Tango Prime Parameter Plasma Electron and Current Experiment electron velocity at spin time resolution</Description> 383 + <Description>
  384 + Electron perpendicular velocity at spin time resolution, in GSM
  385 + </Description>
357 <Ucd>phys.veloc;phys.electron</Ucd> 386 <Ucd>phys.veloc;phys.electron</Ucd>
  387 + <Cadence>PT4S</Cadence>
358 <Units>km/s</Units> 388 <Units>km/s</Units>
359 <UnitsConversion>1.0e3&gt;m s^-1</UnitsConversion> 389 <UnitsConversion>1.0e3&gt;m s^-1</UnitsConversion>
360 <CoordinateSystem> 390 <CoordinateSystem>
@@ -399,9 +429,12 @@ @@ -399,9 +429,12 @@
399 <Parameter> 429 <Parameter>
400 <Name>heat_flux_gse</Name> 430 <Name>heat_flux_gse</Name>
401 <ParameterKey>c4_pea_flux</ParameterKey> 431 <ParameterKey>c4_pea_flux</ParameterKey>
402 - <Description>Cluster II Tango Prime Parameter Plasma Electron and Current Experiment parallel electron heat flux at spin time resolution</Description> 432 + <Description>
  433 + Parallel electron heat flux at spin time resolution, in GSE
  434 + </Description>
403 <Ucd>phys.heatflux;phys.atmol.ionStage</Ucd> 435 <Ucd>phys.heatflux;phys.atmol.ionStage</Ucd>
404 - <Units>microW/m^2</Units> 436 + <Cadence>PT4S</Cadence>
  437 + <Units>microW/m^2</Units>
405 <RenderingHints> 438 <RenderingHints>
406 <DisplayType>TimeSeries</DisplayType> 439 <DisplayType>TimeSeries</DisplayType>
407 </RenderingHints> 440 </RenderingHints>
@@ -432,8 +465,11 @@ @@ -432,8 +465,11 @@
432 <Parameter> 465 <Parameter>
433 <Name>pressure_gse</Name> 466 <Name>pressure_gse</Name>
434 <ParameterKey>c4_pea_press</ParameterKey> 467 <ParameterKey>c4_pea_press</ParameterKey>
435 - <Description>Cluster II Tango Prime Parameter Plasma Electron and Current Experiment parallel pressure tensor at spin time resolution</Description> 468 + <Description>
  469 + Electron pressure tensor at spin time resolution, in GSE
  470 + </Description>
436 <Ucd>phys.pressure</Ucd> 471 <Ucd>phys.pressure</Ucd>
  472 + <Cadence>PT4S</Cadence>
437 <Units>microW/m^2</Units> 473 <Units>microW/m^2</Units>
438 <CoordinateSystem> 474 <CoordinateSystem>
439 <CoordinateRepresentation>Cartesian</CoordinateRepresentation> 475 <CoordinateRepresentation>Cartesian</CoordinateRepresentation>
@@ -443,20 +479,50 @@ @@ -443,20 +479,50 @@
443 <DisplayType>TimeSeries</DisplayType> 479 <DisplayType>TimeSeries</DisplayType>
444 </RenderingHints> 480 </RenderingHints>
445 <Structure> 481 <Structure>
446 - <Size>3</Size> 482 + <Size>9</Size>
447 <Element> 483 <Element>
448 <Name>xx</Name> 484 <Name>xx</Name>
449 <Index>1</Index> 485 <Index>1</Index>
450 <ParameterKey>c4_pea_press(0)</ParameterKey> 486 <ParameterKey>c4_pea_press(0)</ParameterKey>
451 </Element> 487 </Element>
452 <Element> 488 <Element>
453 - <Name>yy</Name> 489 + <Name>xy</Name>
454 <Index>2</Index> 490 <Index>2</Index>
  491 + <ParameterKey>c4_pea_press(1)</ParameterKey>
  492 + </Element>
  493 + <Element>
  494 + <Name>xz</Name>
  495 + <Index>3</Index>
  496 + <ParameterKey>c4_pea_press(2)</ParameterKey>
  497 + </Element>
  498 + <Element>
  499 + <Name>yx</Name>
  500 + <Index>4</Index>
  501 + <ParameterKey>c4_pea_press(3)</ParameterKey>
  502 + </Element>
  503 + <Element>
  504 + <Name>yy</Name>
  505 + <Index>5</Index>
455 <ParameterKey>c4_pea_press(4)</ParameterKey> 506 <ParameterKey>c4_pea_press(4)</ParameterKey>
456 </Element> 507 </Element>
457 <Element> 508 <Element>
  509 + <Name>yz</Name>
  510 + <Index>6</Index>
  511 + <ParameterKey>c4_pea_press(5)</ParameterKey>
  512 + </Element>
  513 + <Element>
  514 + <Name>zx</Name>
  515 + <Index>7</Index>
  516 + <ParameterKey>c4_pea_press(6)</ParameterKey>
  517 + </Element>
  518 + <Element>
  519 + <Name>zy</Name>
  520 + <Index>8</Index>
  521 + <ParameterKey>c4_pea_press(7)</ParameterKey>
  522 + </Element>
  523 + <Element>
458 <Name>zz</Name> 524 <Name>zz</Name>
459 - <Index>3</Index> 525 + <Index>9</Index>
460 <ParameterKey>c4_pea_press(8)</ParameterKey> 526 <ParameterKey>c4_pea_press(8)</ParameterKey>
461 </Element> 527 </Element>
462 </Structure> 528 </Structure>
@@ -469,8 +535,11 @@ @@ -469,8 +535,11 @@
469 <Parameter> 535 <Parameter>
470 <Name>t_para</Name> 536 <Name>t_para</Name>
471 <ParameterKey>c4_pea_tpar</ParameterKey> 537 <ParameterKey>c4_pea_tpar</ParameterKey>
472 - <Description>Cluster II Tango Prime Parameter Plasma Electron and Current Experiment parallel electron temperature at spin time resolution</Description> 538 + <Description>
  539 + Parallel electron temperature at spin time resolution
  540 + </Description>
473 <Ucd>phys.temperature;phys.electron</Ucd> 541 <Ucd>phys.temperature;phys.electron</Ucd>
  542 + <Cadence>PT4S</Cadence>
474 <Units>eV</Units> 543 <Units>eV</Units>
475 <RenderingHints> 544 <RenderingHints>
476 <DisplayType>TimeSeries</DisplayType> 545 <DisplayType>TimeSeries</DisplayType>
@@ -485,8 +554,11 @@ @@ -485,8 +554,11 @@
485 <Parameter> 554 <Parameter>
486 <Name>t_perp</Name> 555 <Name>t_perp</Name>
487 <ParameterKey>c4_pea_tperp</ParameterKey> 556 <ParameterKey>c4_pea_tperp</ParameterKey>
488 - <Description>Cluster II Tango Prime Parameter Plasma Electron and Current Experiment perpendicular electron temperature at spin time resolution</Description> 557 + <Description>
  558 + Perpendicular electron temperature at spin time resolution
  559 + </Description>
489 <Ucd>phys.temperature;phys.electron</Ucd> 560 <Ucd>phys.temperature;phys.electron</Ucd>
  561 + <Cadence>PT4S</Cadence>
490 <Units>eV</Units> 562 <Units>eV</Units>
491 <RenderingHints> 563 <RenderingHints>
492 <DisplayType>TimeSeries</DisplayType> 564 <DisplayType>TimeSeries</DisplayType>