Data Set Information
|
DATA_SET_NAME |
VL1/VL2 MARS METEOROLOGY RESAMPLED DAILY AVG PRESSURE V1.0
|
DATA_SET_ID |
VL1/VL2-M-MET-4-DAILY-AVG-PRESSURE-V1.0
|
NSSDC_DATA_SET_ID |
75-075C-07L
75-083C-07M
|
DATA_SET_TERSE_DESCRIPTION |
VL1/VL2 MARS METEOROLOGY RESAMPLED DAILY AVG PRESSURE
|
DATA_SET_DESCRIPTION |
Data Set Overview
=================
This data set contains summary pressure data obtained from the
Viking Meteorology Instrument System (VMIS) through the
duration of the Viking Lander 1 and 2 missions. The data are
derived from the ambient pressure sensor carried onboard the
Landers. The data set consists of the daily average pressure
values and relevant statistics presented on a sol by sol basis.
For further background information on the VMIS and results from
this experiment, see CHAMBERLAIN_ETAL1976, HESS_ETAL_1977,
TILLMAN_ETAL_1979, HESS_ETAL_1980, and SHARMAN_RYAN_1980. An
earlier version of this data set, including descriptive
documents and plots on microfiche, is archived at the NSSDC
(NSSDC ID 75-075C-07I, 75-075C-07J, 75-083C-07I, and
75-083C-07J).
This data set is composed of the following fields (listed as
the field name followed by a description):
SC_ID
Spacecraft id
SOL_LON
Areocentric longitude of the Sun (Ls), derived for the
beginning of each local day (sol)
VIKING_YEAR
Viking mission year, starting at 1 when the Viking
spacecraft reached Mars, and incremented at Ls = 0
every martian year
MARTIAN_DAY
The martian solar day (sol), starting at day 0 when
each Lander touched down
PRESS_MEAN
Daily average atmospheric pressure
PRESS_MIN
Minimum daily atmospheric pressure
PRESS_RANGE
Maximum variation in pressure during each day
PRESS_SIGMA
Standard deviation in the daily average pressure
MAX_TIME_GAP
Length of maximum time gap between two
measurements (hours)
BEG_GAP_HOUR
Local hour of maximum time gap start
BEG_GAP_MIN
Local minute of maximum time gap start
BEG_GAP_SEC
Local second of maximum time gap start
END_GAP_HOUR
Local hour at which maximum time gap ended
END_GAP_MIN
Local minute at which maximum time gap ended
END_GAP_SEC
Local second at which maximum time gap ended
BIT_ERR_RATE
Indicates quality of spacecraft to ground communications
WARNING_FLAG
Flags indicating number and length of time gaps
Processing Level Id : 4
Software Flag : Y
Processing Start Time : UNK
Processing Stop Time : UNK
Native Start Time : 97.1 AREOCENTRIC SOL LON,
EARTH YR 1976
Native Stop Time : 226.7 AREOCENTRIC SOL LON,
EARTH YR 1982
Parameters
==========
Data Set Parameter 'ATMOSPHERIC PRESSURE'
-----------------------------------------
The force per unit area exerted by an atmosphere, measured in
millibars (10**3 dyne cm**-2).
Data Set Parameter Name : ATMOSPHERIC PRESSURE
Data Set Parameter Unit : MILLIBAR
Sampling Parameter Name : TIME
Sampling Parameter Unit : MARS SOLAR DAY
Minimum Sampling Parameter : N/A
Maximum Sampling Parameter : N/A
Sampling Parameter Resolution : 1
Sampling Parameter Interval : 1
Minimum Available Sampling Int : 1
Noise Level : N/A
Source Instrument Parameters
============================
Instrument Host ID : VL1
Data Set Parameter Name : ATMOSPHERIC PRESSURE
Instrument Parameter Name : PRESSURE
Important Instrument Parameters : 1
Instrument Host ID : VL2
Data Set Parameter Name : ATMOSPHERIC PRESSURE
Instrument Parameter Name : PRESSURE
Important Instrument Parameters : 1
Processing
==========
Processing History
------------------
Source Data Set ID : VL1/VL2-M-MET-3-P-V1.0
Software : UNK
Product Data Set ID :
VL1/VL2-M-MET-4-DAILY-AVG-PRESSURE-V1.0
|
DATA_SET_RELEASE_DATE |
1989-11-01T00:00:00.000Z
|
START_TIME |
1976-07-20T12:00:00.000Z
|
STOP_TIME |
1982-11-13T12:00:00.000Z
|
MISSION_NAME |
VIKING
|
MISSION_START_DATE |
1975-08-20T12:00:00.000Z
|
MISSION_STOP_DATE |
1983-02-01T12:00:00.000Z
|
TARGET_NAME |
MARS
|
TARGET_TYPE |
PLANET
|
INSTRUMENT_HOST_ID |
VL1
VL2
|
INSTRUMENT_NAME |
VIKING METEOROLOGY INSTRUMENT SYSTEM
VIKING METEOROLOGY INSTRUMENT SYSTEM
|
INSTRUMENT_ID |
MET
MET
|
INSTRUMENT_TYPE |
METEOROLOGY
METEOROLOGY
|
NODE_NAME |
Planetary Atmospheres
|
ARCHIVE_STATUS |
ARCHIVED
|
CONFIDENCE_LEVEL_NOTE |
Overview
========
The pressure transducers were calibrated to approximately 0.01
to 0.02 millibars accuracy over the ranges expected for martian
atmospheric pressure variation. Calibrations to accuracies
greater than allowed by the digitizing system were accomplished
by test support instrumentation. Repeatability from year to
year of the daily average pressures indicates that the
transducers have remained stable to significantly better than
0.04 millibars throughout the mission, possibly maintaining
stabilities on the order of 0.01 millibars. The pressure
measurements were digitized into 255 approximately equal
increments (digital numbers or DNs), giving a basic pressure
digitization interval of 0.088 millibars. Raw DNs between 0
and 255 were converted to pressures by linear interpolation
between calibration points. Due to the limited pressure range
on Mars, the only calibration points used are those for DNs
100, 120, and 160. DN 140 was left out of the calibration
table, producing a maximum error of 0.0425 millibar for VL1 and
0.008 millibar for VL2; corrections have been applied to the
data set to correct for this missing calibration point.
As the output of the pressure transducer is quantized in 0.088
millibar increments, the resolution of a single measurement is
limited to 0.088 millibar. On average, half of the
measurements producing a given pressure value are at least one
half a quantum above the indicated value and that value is
actually the lower bound of the actual value. By adding 0.044
millibar to each measurement, any estimate of the average
pressure (generally having greater resolution than one DN) will
not be biased (see HESS_ETAL_1980). Such accuracy is important
as features of the annual pressure cycle repeat within 0.02
millibar or less and it is important to establish the actual
value for comparison between years and for future missions to
Mars.
The pressure measurements are presented in the form of sol
averages and sol range. The sol average is obtained by
weighting each measurement according to the period that it
represents. The sol range is determined by subtracting the
minimum from the maximum pressure on each sol. With sampling
intervals of less than approximately two hours, the average
very closely approximates the true average. Each sol is
checked for the maximum period between samples and when this
value exceeds approximately three hours, the raw data are
manually edited. The editing determines the validity of the
data for each of the several functions which are separately
flagged. For example, the data may be adequate to form a daily
average but not a daily range. Since the pressure quantization
is 0.088 millibar, the daily range has discrete jumps and
fluctuates by one quantum. Gaps in the data indicate missing
sols or sols for which the sampling is too infrequent to obtain
a meaningful value. In addition, bit error rate information is
tabulated on a sol by sol basis so that errors on the
communication link can be quantified.
The data set contains the following fields related to
confidence level (listed as the field name followed by a
MAX_TIME_GAP
Length of maximum time gap between two
measurements (hours)
BEG_GAP_HOUR
Local hour of maximum time gap start
BEG_GAP_MIN
Local minute of maximum time gap start
BEG_GAP_SEC
Local second of maximum time gap start
END_GAP_HOUR
Local hour at which maximum time gap ended
END_GAP_MIN
Local minute at which maximum time gap ended
END_GAP_SEC
Local second at which maximum time gap ended
BIT_ERR_RATE
Indicates quality of spacecraft to ground communications
WARNING_FLAG
Flags indicating number and length of time gaps
|
CITATION_DESCRIPTION |
Citation TBD
|
ABSTRACT_TEXT |
This data set contains summary pressure data obtained from the
Viking Meteorology Instrument System (VMIS) through the duration
of the Viking Lander 1 and 2 missions. The data are derived from
the ambient pressure sensor carried onboard the Landers. The data
set consists of the daily average pressure values and relevant
statistics presented on a sol by sol basis. For further
background information on the VMIS and results from this
experiment, see CHAMBERLAIN_ETAL1976, HESS_ETAL_1977,
TILLMAN_ETAL_1979, HESS_ETAL_1980, and SHARMAN_RYAN_1980. An
earlier version of this data set, including descriptive documents
and plots on microfiche, is archived at the NSSDC (NSSDC ID
75-075C-07I, 75-075C-07J, 75-083C-07I, and 75-083C-07J).
|
PRODUCER_FULL_NAME |
JAMES E. TILLMAN
|
SEARCH/ACCESS DATA |
Atmospheres Online Archives
Atmospheres Online Archives
|
|