Commit b5bbcfeb9f7d5561afec0c111c7056c0d77b2e83
1 parent
8d31ce32
Exists in
master
and in
11 other branches
pas err
Showing
4 changed files
with
74 additions
and
1 deletions
Show diff stats
... | ... | @@ -0,0 +1,39 @@ |
1 | +<?xml version="1.0" encoding="UTF-8"?> | |
2 | +<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" xsi:schemaLocation="http://www.spase-group.org/data/schema http://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd"> | |
3 | + <Version>2.3.1</Version> | |
4 | + <Instrument> | |
5 | + <ResourceID>spase://CNES/Instrument/CDPP-AMDA/Interball-1/DOK2</ResourceID> | |
6 | + <ResourceHeader> | |
7 | + <ResourceName>DOK2</ResourceName> | |
8 | + <AlternateName/> | |
9 | + <ReleaseDate>2010-02-04T12:34:56.789</ReleaseDate> | |
10 | + <Description>DOK-2 uses two pairs of energetic particle telescopes. | |
11 | + Each telescope has a single, passively cooled, totally depleted, surface-barrier silicon detector. | |
12 | + One detector of each pair (1e,2e) is of 0.3 mm thick. Thin foil in front of detector absorbes protons with energies E less than 400 keV so | |
13 | + this detector measures electron spectrum in 20 - 420 keV range. The second detector (1p,2p) of 0.15 mm thick is supplied with a broom magnet, deflecting electrons up to 1500 keV . It measures spectrum of ions (protons) in 20-850 keV range. | |
14 | + Full aperture angles and geometric factors of electron telescopes are of 27° and 0.066. | |
15 | + For proton telescopes these values are 12.7° and 0.015. Particle flux angular distribution is measured using spacecraft rotation with a ~2 min | |
16 | + period around the axis directed to the Sun (the angle ) and mechanical scanning of the second telescope pair in a plane containing the rotation | |
17 | + axis (the angle). So 3-dimensional particle distribution function is measured during each 2 min rotation period. | |
18 | + About seven full scanning cycles are carried out for every rotation. The first detector pair (1e,1p) is fixed in the antisolar direction. | |
19 | + Moving detector pair (2e,2p) can either scan from 45° to 180° (to a Sun direction) or stay in one of 4 positions: 45, 90, 135 and 180°. | |
20 | + </Description> | |
21 | + <Contact> | |
22 | + <PersonID>spase://CNES/Person/Volt.Lutsenko</PersonID> | |
23 | + <Role>PrincipalInvestigator</Role> | |
24 | + </Contact> | |
25 | + <Contact> | |
26 | + <PersonID>spase://CNES/Person/Karel.Kudela</PersonID> | |
27 | + <Role>PrincipalInvestigator</Role> | |
28 | + </Contact> | |
29 | + <InformationURL> | |
30 | + <Name>DOK2 Home Page at IKI</Name> | |
31 | + <URL>http://www.iki.rssi.ru/interball/dok.html</URL> | |
32 | + <Description></Description> | |
33 | + </InformationURL> | |
34 | + </ResourceHeader> | |
35 | + <InstrumentType>SolidStateDetector</InstrumentType> | |
36 | + <InvestigationName/> | |
37 | + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/Interball-Tail</ObservatoryID> | |
38 | + </Instrument> | |
39 | +</Spase> | |
... | ... |
NumericalData/CDPP-AMDA/Solar_Orbiter/PAS/so-pas-momgr.xml
... | ... | @@ -52,7 +52,14 @@ |
52 | 52 | <Description/> |
53 | 53 | <Ucd/> |
54 | 54 | <Units>cm**-3</Units> |
55 | - </Parameter> | |
55 | + </Parameter> | |
56 | + <Parameter> | |
57 | + <Name>density : err</Name> | |
58 | + <ParameterKey>pas_momgr_n_err</ParameterKey> | |
59 | + <Description/> | |
60 | + <Ucd/> | |
61 | + <Units>cm**-3</Units> | |
62 | + </Parameter> | |
56 | 63 | <Parameter> |
57 | 64 | <Name>v_s/c</Name> |
58 | 65 | <ParameterKey>pas_momgr_v</ParameterKey> |
... | ... | @@ -85,6 +92,13 @@ |
85 | 92 | </Structure> |
86 | 93 | </Parameter> |
87 | 94 | <Parameter> |
95 | + <Name>|v_sc|</Name> | |
96 | + <ParameterKey>pas_momgr_v_tot</ParameterKey> | |
97 | + <Description/> | |
98 | + <Ucd/> | |
99 | + <Units>km/s</Units> | |
100 | + </Parameter> | |
101 | + <Parameter> | |
88 | 102 | <Name>t_av</Name> |
89 | 103 | <ParameterKey>pas_momgr_tav</ParameterKey> |
90 | 104 | <Description/> |
... | ... |
... | ... | @@ -0,0 +1,10 @@ |
1 | +<?xml version="1.0" encoding="UTF-8"?> | |
2 | +<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_2_0.xsd"> | |
3 | + <Version>2.2.0</Version> | |
4 | + <Person> | |
5 | + <ResourceID>spase://CNES/Person/Karel.Kudela</ResourceID> | |
6 | + <PersonName>Dr. Karel Kudela</PersonName> | |
7 | + <OrganizationName>Institute of Experim. Physics. SAS, Kosice, Slovakia</OrganizationName> | |
8 | + <Email/> | |
9 | + </Person> | |
10 | +</Spase> | |
... | ... |
... | ... | @@ -0,0 +1,10 @@ |
1 | +<?xml version="1.0" encoding="UTF-8"?> | |
2 | +<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_2_0.xsd"> | |
3 | + <Version>2.2.0</Version> | |
4 | + <Person> | |
5 | + <ResourceID>spase://CNES/Person/Volt.Lutsenko</ResourceID> | |
6 | + <PersonName>Dr. Volt N. Lutsenko</PersonName> | |
7 | + <OrganizationName>Space Research Institute, Moscow, Russia</OrganizationName> | |
8 | + <Email>vlutsenk@volt.iki.rssi.ru</Email> | |
9 | + </Person> | |
10 | +</Spase> | |
... | ... |