Data Set Information
|
DATA_SET_NAME |
VEGA2 PLASMAG-1 PLASMA ENERGY ANALYSER DATA V1.0
|
DATA_SET_ID |
VEGA2-C-PM1-2-RDR-HALLEY-V1.0
|
NSSDC_DATA_SET_ID |
XD-B3A
|
DATA_SET_TERSE_DESCRIPTION |
VEGA 2 satellite PLASMAG instrument energy analyzer data from
1P/Halley
|
DATA_SET_DESCRIPTION |
Data Set Overview
=================
The PLASMAG-1 instument package included six different sensors:
A0 plasma impact detector for measuring neutral particle flux,
(manufactured by R. Grard, ESA/ESTEC, Noordwijk, The Netherlands)
A1 Faraday cup for measuring integral ion flux from solar direction,
A2 Faraday cup for measuring integral ion flux and neutral particles
from ram direction,
A3 spherical electrostatic analyzer for measuring ions from ram direction
in the energy range of 15 eV - 3.6 keV in 120 logarithmically
spaced channels,
A4 spherical electrostatic analyzer for measuring ions from solar direction
in the energy range of 60 eV - 30 keV in 60 logarithmically
spaced channels,
A5 cylindrical electrostatic analyzer for measuring ions perpendicular
to the ecliptic plane in the energy range of 2 eV - 10 keV in
30 logarithmically spaced channels.
The sensitivity of the electron analyzer A5 was very
low. Detector A3 of Vega-2 was fatally damaged 2.5
min before closest approach. The channeltrons of A3
were saturating at higher count rates.
Field of view of the detectors:
A1: 90x90 deg (centered on solar direction),
A2: 26x26 deg (centered on ram direction),
A3: 32x12 deg (centered on ram direction),
A4: 36x32 deg (centered on solar direction),
A5: 7x7 deg (perpendicular to ecliptic plane).
Effective apperture: A1: 1.6 cm**2
A2: 0.93 cm**2
A3: 0.0193 cm**2
A4: 0.00455 cm**2
A5: 0.0036 cm**2
Energy resolution:
A3: 3.2 %
A4: 3.85%
A5: 7.5 %
One complete spectrum was taken by A3, A4, and A5 in every
second during the BRL (high telemery rate) seance.
Sampling times for each energy channel:
A3: 0.005 sec
A4: 0.005 sec
A5: 0.021 sec
During the cruise phase data were recorded by an
on-board magnetometer at lower telemetry rate.
The data were measured during the BRL seance on
March 9, 1986.
1. parameter: time in sec - end of a 10 sec averaging interval
(0 sec is 4:00 UT in spacecraft time)
2-30. parameters: count rates observed by A5 (electrons)
31-90. parameters: count rates observed by A4
(ions from solar direction)
91-210. parameters: count rates observed by A3
(ions from ram direction)
The energy levels for the 29 channels of detector A5 in eV:
1.9 2.9 3.8 5.8 7.7 10.6 14.9
19.2 25.9 35 0
47.0 61.0 84.5 113.3 168.2 229.7 311.3
410.9 553.0 744 8
999.2 1349.0 1804.8 2430.2 3225.2 4364.7 5869.9
7868.0 10571.0
The energy levels for the 60 channels of detector A4 in eV:
64.0 73.8 78.7 88.6 94.3 103.3 114.0 128.7
138.6 154 2
173.8 188.6 209.1 235.3 255.0 286.2 317.3 351.0
387.0 431 3
480.5 534.6 594.5 660.9 734.7 818.4 912.7 1014.3
1123.4 1246 4
1384.2 1531.8 1689.2 1877.8 2099.2 2341.1 2606.0 2896.2
3214.4 3575 2
3985.2 4436.2 4936.4 5494.0 6117.2 6724.0 6724.0 7544.0
8388.6 9290 6
10291.0 11439.0 12783.8 14268.0 15924.4 17728.4 19647.2 21861.2
24403.2 27191 2
The energy levels for the 120 channels of detector A3 in eV:
15.6 17.2 18.9 19.7 20.5 22.1 23.0 24.6
27.1 28 3
29.5 30.8 32.0 33.2 34.4 35.7 36.9 38.1
39.4 40 6
41.8 43.5 45.1 45.9 46.7 48.0 50.0 51.3
52.5 54 9
57.4 59.4 61.5 64.0 66.8 69.7 73.0 76.7
80.8 84 9
89.4 93.9 98.4 102.9 107.4 112.3 117.7 123.0
128.7 134 5
140.6 147.2 154.2 161.5 169.3 177.1 185.3 194.3
203.8 213 2
223.0 234.1 245.6 257.5 269.8 282.9 296.4 310.0
323.9 337 8
352.2 366.5 381.3 398.5 418.2 440.3 464.1 487.9
512.5 537 1
561.7 587.9 615.8 645.3 676.5 710.9 747.8 787.2
828.2 870 8
914.3 959.4 1005.3 1052.9 1102.1 1152.1 1203.8 1262.0
1325.1 1393 1
1466.2 1539.1 1612.9 1687.6 1763.0 1845.0 1935.2 2033.6
2140.2 2248 4
2358.3 2469.8 2583.8 2702.7 2829.8 2966.8 3112.7 3268.5
3432.5 3604 7
Measurements were performed in every sec, data
provided here are 10 sec averages.
Time of first observation: 4:13:00 UT
Time of first data in file: 4:13:10 UT (790 sec)
Time of last observation: 8:40:00 UT
Time of last data in file: 8:40:00 UT (16800 sec)
There was a data gap between 7:17:30 UT (11850 sec) and 7:45:10
(13510 sec).
Missing or bad data: -99
The detector A3 was fatally damaged at 7:17:31 UT
when the telemetry connection also broke down. At
7:45:10 UT the connection with the instrument was
re-established.
|
DATA_SET_RELEASE_DATE |
3000-01-01T00:00:00.000Z
|
START_TIME |
1986-03-09T04:13:00.000Z
|
STOP_TIME |
1986-03-09T08:40:00.000Z
|
MISSION_NAME |
VEGA 2
|
MISSION_START_DATE |
1984-12-21T12:00:00.000Z
|
MISSION_STOP_DATE |
1986-04-01T12:00:00.000Z
|
TARGET_NAME |
HALLEY
|
TARGET_TYPE |
COMET
|
INSTRUMENT_HOST_ID |
VEGA2
|
INSTRUMENT_NAME |
PLASMA ENERGY ANALYZER
|
INSTRUMENT_ID |
PM1
|
INSTRUMENT_TYPE |
ELECTROSTATIC ANALYZER
|
NODE_NAME |
Small Bodies
|
ARCHIVE_STATUS |
ARCHIVED
|
CONFIDENCE_LEVEL_NOTE |
Confidence Level Overview
=========================
N/A
|
CITATION_DESCRIPTION |
Dyachkov, A. V., VEGA2 PLASMAG-1 PLASMA ENERGY ANALYSER DATA
V1.0, VEGA2-C-PM1-2-RDR-HALLEY-V1.0, NASA Planetary Data System,
1997
|
ABSTRACT_TEXT |
The PLASMAG-1 instument package included six different sensors:
A0 plasma impact detector for measuring neutral particle flux,
(manufactured by R. Grard, ESA/ESTEC, Noordwijk, The Netherlands)
A1 Faraday cup for measuring integral ion flux from solar
direction, A2 Faraday cup for measuring integral ion flux and
neutral particles from ram direction, A3 spherical electrostatic
analyzer for measuring ions from ram direction in the energy
range of 15 eV - 3.6 keV in 120 logarithmically spaced channels,
A4 spherical electrostatic analyzer for measuring ions from solar
direction in the energy range of 60 eV - 30 keV in 60
logarithmically spaced channels, A5 cylindrical electrostatic
analyzer for measuring ions perpendicular to the ecliptic plane
in the energy range of 2 eV - 10 keV in 30 logarithmically spaced
channels.
|
PRODUCER_FULL_NAME |
INTERNATIONAL HALLEY WATCH
|
SEARCH/ACCESS DATA |
SBN Comet Website
|
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