Data Set Information
|
DATA_SET_NAME |
GIOTTO DUST IMPACT DETECTOR SYSTEM DATA V1.0
|
DATA_SET_ID |
GIO-C-DID-3-RDR-HALLEY-V1.0
|
NSSDC_DATA_SET_ID |
XD-B3A
|
DATA_SET_TERSE_DESCRIPTION |
GIOTTO Dust Detector (DID) observations of 1P/Halley
|
DATA_SET_DESCRIPTION |
Data Set Overview
=================
Dust Impact Detection System (DIDSY) consists of six
independent subsystems with the primary aim of
registering the impacts of all particulates of
significant mass incident on the probe during the
post-perihelion encounter with Comet Halley in 1986.
Mounted on Giotto's front dust shield, the detectors
will determine the mass spectrum of the dust, with a
limiting sensitivity of some 10^^-17^^ g, increasing
to the largest grain masses encountered along
Giotto's trajectory through the cometary environment
with an ultimate spatial resolution of some 70 km.
An additional detector is located on the rear shield
to monitor those dust particles (m > ~ 5 X 10^^-7^^
g) that are able to penetrate the front dust shield.
An ambient plasma monitor is also incorporated into
DIDSY to measure the inJpact plasma generated by both
dust and gas impacts on the spacecraft. The system
is controlled and its data processed by a
microprocessor-based system that allows the wide
range of anticipated impact rates (varying from a few
per minute, to ~ 10^6 s^^-1^^ at closest approach) to
be handled. The instrument weighs 2.26 kg and
consumes 1.9 W of power during normal operation.
Sampling parameter : TIME
Sampling parameter unit : SECOND
Data set parameter : MASS
Data set parameter unit : COUNTS
|
DATA_SET_RELEASE_DATE |
1992-04-30T00:00:00.000Z
|
START_TIME |
1986-03-13T11:01:00.900Z
|
STOP_TIME |
1986-03-14T01:00:13.900Z
|
MISSION_NAME |
GIOTTO
|
MISSION_START_DATE |
1985-07-02T12:00:00.000Z
|
MISSION_STOP_DATE |
1992-07-10T12:00:00.000Z
|
TARGET_NAME |
HALLEY
|
TARGET_TYPE |
COMET
|
INSTRUMENT_HOST_ID |
GIO
|
INSTRUMENT_NAME |
DUST IMPACT DETECTOR
|
INSTRUMENT_ID |
DID
|
INSTRUMENT_TYPE |
DUST DETECTOR
|
NODE_NAME |
Small Bodies
|
ARCHIVE_STATUS |
ARCHIVED
|
CONFIDENCE_LEVEL_NOTE |
Confidence Level Overview
=========================
N/A
|
CITATION_DESCRIPTION |
McDonnell, J. A. M, GIOTTO DUST IMPACT DETECTOR SYSTEM DATA V1.0,
GIO-C-DID-3-RDR-HALLEY-V1.0, NASA Planetary Data System, 1992.
|
ABSTRACT_TEXT |
Dust Impact Detection System (DIDSY) consists of six independent
subsystems with the primary aim of registering the impacts of all
particulates of significant mass incident on the probe during the
post-perihelion encounter with Comet Halley in 1986. Mounted on
Giotto's front dust shield, the detectors will determine the
mass spectrum of the dust, with a limiting sensitivity of some
10^^-17^^ g, increasing to the largest grain masses encountered
along Giotto's trajectory through the cometary environment
with an ultimate spatial resolution of some 70 km. An additional
detector is located on the rear shield to monitor those dust
particles (m > ~ 5 X 10^^-7^^ g) that are able to penetrate
the front dust shield. An ambient plasma monitor is also
incorporated into DIDSY to measure the inJpact plasma generated
by both dust and gas impacts on the spacecraft. The system is
controlled and its data processed by a microprocessor-based
system that allows the wide range of anticipated impact rates
(varying from a few per minute, to ~ 10^6 s^^-1^^ at closest
approach) to be handled. The instrument weighs 2.26 kg and
consumes 1.9 W of power during normal operation.
|
PRODUCER_FULL_NAME |
INTERNATIONAL HALLEY WATCH
|
SEARCH/ACCESS DATA |
SBN Comet Website
|