The FIFE Surface Flux Baseline 92 Derived Data Set was compiled from the original surface flux data collected during FIFE (i.e., no measurements were made specifically for this data set). This data set contains data collected from mid-May through mid-October, 1987 at 21 stations located within 19 sitegrids spread throughout the FIFE study area. For a description of the theory behind the original surface flux measurements see the documentation for each of the original surface flux data sets.
Surface heat flux data routinely have erroneous jumps (i.e., spikes) in the latent and sensible heat flux time series in the early morning and evening hours due to small gradients in the measured data. A series of tests were developed to identify these spikes and flag them. Flux data obtained from Bowen ratio sites are also checked for energy imbalances. These data were also compared to model results. The consistency between these two methods is indicated in this data set.
Surface Flux Baseline 92 Derived (FIFE).
(Surface Flux Baseline 1992).
The FIFE Surface Flux Baseline 92 Derived Data Set was compiled from the original surface flux data collected during FIFE (i.e., no measurements were made specifically for this data set). This data set contains data collected from mid-May through mid-October, 1987 at 21 stations located within 19 sitegrids spread throughout the FIFE study area.
A standardized Surface Flux Baseline data set was produced to replace the Surface Flux Baseline July 1990 data set. In the data set described here 'spikes' and energy imbalances in the surface flux time series are flagged. In addition a model-based check on the reasonableness of the fluxes is provided.
Net radiation, sensible heat flux, latent heat flux, and ground heat flux.
Surface heat flux data routinely have erroneous jumps (i.e. spikes) in the latent and sensible heat flux time series in the early morning and evening hours due to small gradients in the measured data. A series of tests were developed to identify these spikes and flag them. Flux data obtained from Bowen ratio sites are also checked for energy imbalances. These data were also compared to model results. The consistency between these two methods is indicated in this data set. These data were collected from mid-May through mid-October, 1987 at 21 stations located within 19 sitegrids spread throughout the FIFE study area. During this time period measurements were made almost every day.
SURFACE_FLUX_BASELINE92_DERV.
Dr. Piers Sellers
Biospheric Sciences Branch
Surface Flux Baseline 1992.
Contact 1:
Mr. Mark Heiser
University of Maryland
College Park, MD
Telephone: (301) 405-5363
Email: heiser@atmos.umd.edu
The Surface Flux Baseline 1992 data were compiled at NASA Goddard Space Flight Center under the direction of Dr. P. Sellers. The dedicated effort of M. Heiser in the compilation of these data is particularly appreciated.
These data are compiled from the original surface flux data collected during FIFE. Consequently, no measurements were made specifically for this data set. For a description of the theory behind the original surface flux measurements see the documentation for each of the original surface data sets listed in the Related Data Sets Section above.
A desktop computer was used to identify and flag the 'spikes' in the data. In addition, this computer was used to compute the model results which were compared to the original, field-measured fluxes.
See the Sensor/Instrument Description Section.
See the Sensor/Instrument Description Section.
See the Sensor/Instrument Description Section.
Net radiation, sensible heat flux, latent heat flux, ground heat flux, and flags indicating spikes and agreement with model results.
See the Sensor/Instrument Description Section.
See the Sensor/Instrument Description Section.
Not available at this revision.
Calibration is not applicable to this data set since the data are compiled from the original surface flux data. A description of the calibration procedures used for each of these underlying data sets can be found in the individual documentation for the Bowen ratio and Eddy correlation surface flux data sets (see the Related Data Sets Section for a list of these data sets).
See the Calibration Section.
See the Calibration Section.
See the Calibration Section.
See the Calibration Section.
The surface flux data were acquired from the FIFE Information System. These data are available on FIFE CD-ROM Volume 1 in the DATA\SUR_FLUX\30_MIN\ subdirectory.
Not available.
Not applicable.
The FIFE study area, with areal extent of 15 km by 15 km, is located south of the Tuttle Reservoir and Kansas River, and about 10 km from Manhattan, Kansas, USA. The northwest corner of the area has UTM coordinates of 4,334,000 Northing and 705,000 Easting in UTM Zone 14.
Data were compiled from 21 surface flux stations located in 19 sitegrids scattered throughout the FIFE study area.
SITEGRID STN_ID NORTHING EASTING LATITUDE LONGITUDE ELEV -------- ------ -------- ------- -------- --------- ---- 1246-BRL 40 4331666 714212 39 06 35 -96 31 21 365 1445-BRL 42 4331160 714090 39 06 19 -96 31 27 400 1478-BRS 38 4331216 720603 39 06 15 -96 26 56 350 1916-BRS 2 4330296 708270 39 05 56 -96 35 30 340 2043-BRL 44 4330003 713536 39 05 42 -96 31 51 415 2516-BRK 14 4328956 708102 39 05 12 -96 35 38 405 2655-BRL 36 4328787 716070 39 05 00 -96 30 07 367 2731-ECA 4 4328678 711110 39 05 01 -96 33 34 446 2915-BRK 12 4328167 708028 39 04 47 -96 35 42 415 3129-BRK 8 4327702 710711 39 04 30 -96 33 51 430 3414-BRK 10 4327286 707854 39 04 19 -96 35 51 410 3479-BRL 34 4327134 720890 39 04 02 -96 26 49 420 4268-ECG 30 4325626 718574 39 03 15 -96 28 27 445 4268-BRK 32 4325626 718579 39 03 15 -96 28 27 445 4439-ECV 16 4325215 712794 39 03 07 -96 32 28 445 4439-BRV 18 4325218 712792 39 03 07 -96 32 28 445 4609-ECW 22 4324890 706705 39 03 02 -96 36 41 390 6340-BRL 20 4321484 713000 39 01 06 -96 32 23 410 6912-BRW 24 4320111 707336 39 00 26 -96 36 20 397 6943-ECW 28 4320147 713500 39 00 22 -96 32 04 415 8739-ECB 26 4316699 712845 38 58 31 -96 32 35 442
Not available.
Not available.
Not available.
Surface fluxes were measured from May 26 to October 16 in 1987.
Not available.
Surface fluxes were reported at 30 minute intervals for all sites except for site 8739-ECB (site 26) which reported the data at 1 hour intervals.
The SQL definition for this table is found in the SF_BL92.TDF file located on FIFE CD-ROM Volume 1.
Parameter/Variable Name
Parameter/Variable Description Range Units Source
SITEGRID_ID This is a FIS grid location code. Site grid codes (SSEE-III) give the south (SS) and the east (EE) cell number in a 100 x 100 array of 200 m square cells. The last 3 characters (III) are an instrument identifier.
STATION_ID The station ID designating the location of the observations.
OBS_DATE The date of the observations, in the format (DD-mmm-YY).
OBS_TIME The time that the observation [GMT] was taken in GMT. The format is (HHMM).
NET_RADTN The Net Radiation. ** [Watts] [meter^-2]
LATENT_HEAT_FLUX The Latent Heat flux. ** [Watts] [meter^-2]
SENSIBLE_HEAT_FLUX The Sensible Heat flux. ** [Watts] [meter^-2]
SOIL_HEAT_FLUX The Surface Soil Heat flux. ** [Watts] [meter^-2]
SPIKE_FLAG A flag indicating if this data is considered "spike" (or glich) data. 0 means good data, 1 means spike data, 2 means available energy does not balance, 3 means both 1 and 2.
IDF_FLAG A flag showing the reasonableness of the data (lower is better) based on comparisons with model results. See the Processing Steps Section of the document for the meaning of the values.
FIFE_DATA_CRTFCN_CODE The FIFE Certification Code for * the data, in the following format: CPI (Certified by PI), CPI-??? (CPI - questionable data).
LAST_REVISION_DATE in the format (DD-MMM-YY).
Footnotes:
* Valid levels
The primary certification codes are:
EXM Example or Test data (not for release) PRE Preliminary (unchecked, use at your own risk) CPI Checked by Principal Investigator (reviewed for quality) CGR Checked by a group and reconciled (data comparisons and cross checks)
The certification code modifiers are:
PRE-NFP Preliminary - Not for publication, at the request of investigator. CPI-MRG PAMS data that is "merged" from two separate receiving stations to eliminate transmission errors. CPI-??? Investigator thinks data item may be questionable.
** Missing values are reported as -9999 or -8888.
SITEGRID_ID STATION_ID OBS_DATE OBS_TIME NET_RADTN LATENT_HEAT_FLUX ----------- ---------- --------- -------- --------- ---------------- 1916-BRS 2 27-MAY-87 515 -1.280 -55.390 1916-BRS 2 27-MAY-87 545 -2.190 -37.160 1916-BRS 2 27-MAY-87 615 -4.030 -30.740 1916-BRS 2 27-MAY-87 645 -6.610 -26.600 SENSIBLE_HEAT_FLUX SOIL_HEAT_FLUX SPIKE_FLAG IDF_FLAG ------------------ -------------- ---------- -------- 42.650 14.020 25.270 14.080 18.750 16.020 11.440 21.770 FIFE_DATA_CRTFCN_CODE LAST_REVISION_DATE --------------------- ------------------ CGR 04-JAN-94 CGR 04-JAN-94 CGR 04-JAN-94 CGR 04-JAN-94
The surface fluxes for each station are representative of an area extending approximately 100 meters upwind from the surface flux equipment. Surface fluxes were reported at 30 minute intervals for all sites except for site 8739-ECB (site 26) which reported the data at 1 hour intervals.
A general description of data granularity as it applies to the IMS appears in the EOSDIS Glossary.
The CD-ROM file format consists of numerical and character fields of varying length separated by commas. The character fields are enclosed with a single apostrophe. There are no spaces between the fields. Each file begins with five header records. Header records contain the following information:
Record 1 Name of this file, its table name, number of records in this file, path and name of the document that describes the data in this file, and name of principal investigator for these data. Record 2 Path and filename of the previous data set, and path and filename of the next data set. (Path and filenames for files that contain another set of data taken at the same site on the same day.) Record 3 Path and filename of the previous site, and path and filename of the next site. (Path and filenames for files of the same data set taken on the same day for the previous and next sites (sequentially numbered by SITEGRID_ID)). Record 4 Path and filename of the previous date, and path and filename of the next date. (Path and filenames for files of the same data set taken at the same site for the previous and next date.) Record 5 Column names for the data within the file, delimited by commas. Record 6 Data records begin. Each field represents one of the attributes listed in the chart in the Data Characteristics Section and described in detail in the TDF file. These fields are in the same order as in the chart.
At a given time, Bowen ratio stations should have equal available energies since RN and GH are used to calculate LE and SH. Flux data for Bowen ratio stations will fail the test if the absolute value of DELTA is greater than 1 [watts][m^-2]. Since eddy correlation stations measure LE and SH directly with RN and GH measured by other instruments, one would not expect the available energies to be equal. If they are equal it is assumed that the GH is computed as a residual. Therefore, if the absolute value of DELTA is less than 1 [watts][m^-2], GH is set to an undefined value.
Spikes have been observed in some ground heat flux data records. This can result in incorrect values for latent and sensible heat fluxes at Bowen ratio sites due to the manner in which these fluxes are derived. These points are flagged as being a spike when the absolute value of the rate of change of the ground heat
flux exceeds 1.5 times the rate of change of the net radiation or 50.0 [watts][m^-2][hour^-1] (whichever is greater). This test is applied only to Bowen Ratio stations when the net radiation exceeds 100 [watts][m^-2] and must be true for both the time period leading up to and immediately following the time of the observation.
As an initial spike identification test, the following conditions must be satisfied. The sensible heat flux must be either less than or greater than the values reported before and after the time in question.
AND
The latent heat flux must be either less than or greater than the values reported before and after the time in question.
The 2nd derivatives with respect to time of the latent and sensible heat fluxes must have opposite signs for a point to be a spike.
Both the sensible and latent heat fluxes must exceed the average of the observations immediately preceding and following the flux observation time by LIM1 or 25 [watts][m^-2] (whichever is greater) for a point to be a spike. This test forces spike checking on points that deviate from the mean by at least 25 [watts][m^-2] thus preserving small variations in the flux time series that otherwise might be eliminated.
In the early morning and evening hours, there are sometimes large absolute differences between the sensible and latent heat fluxes that are unrealistic. These points are eliminated if the absolute value of the difference between the sensible and latent heat flux exceeds 100 [watts][m^-2]. This test is only applied when the sum of the latent and sensible heat flux is less than 25 [watts][m^-2].
If both the latent and sensible heat fluxes preceding and following an observation time are undefined or flagged as a spike, the latent and sensible heat flux at the observation time is considered unreliable and flagged as a spike.
Do this for all available times before moving onto the next step (see the Derivation Techniques and Algorithms Section.
Do this for all available times before moving onto the next step (see the Special Corrections/Adjustments Section.
This test for spikes is applied to the data for each observation time except for the first and last observations since the filter requires data preceding and following the time of the observation. The tests are run beginning with the second available observation time and ending with the next to last available observation time. both latent and sensible heat fluxes must be present at the time of the observation as well as at the immediately preceding or following times for these tests to be applied. If there are any absent data, the program moves on to the next observation time. (see the Derivation Techniques and Algorithms Section.
For each observation apply:
Do this for all available times before moving onto the next step (see the Derivation Techniques and Algorithms Section.
Since this filter requires data preceding and following the time of the observation, these tests are run beginning with the second available observation time and ending with the next to last available observation time (see the Derivation Techniques and Algorithms Section.
Do this for each Intensive Field Campaign day in 1987 (see the Confidence Level/Accuracy Judgment Section.
None.
Net Radiation Adjustments
The net radiation for sites 1916-BRS (site 2), 8739-ECB (site 26) and 1478-BRS (site 38) is adjusted to correspond to the 'site mean' net radiation measured using Q*6 radiometers. The latent and sensible heat fluxes are also adjusted accordingly and the ground heat flux is left unchanged. Only these sites are adjusted but adjustment parameters for all stations have been included in the table below for comparison purposes. <RN> Site averaged Q*6 net radiation RN measured net radiation GH measured ground heat flux LE measured latent heat flux SH measured sensible heat flux XRN <RN> = 325 [watts][m^-2] YRN value of RN when <RN> = 325 [watts][m^-2] ARN adjusted net radiation ALE adjusted latent heat flux ASH adjusted sensible heat flux
A plot of the net radiation measured at each flux site against the site averaged Q*6 net radiation revealed that a regression using two linear functions would do the best job at adjusting the net radiation. One function describes the adjustment when RN is between 0 and YRN and the second function describes the adjustment when RN is greater than YRN. There is no adjustment made when RN is less than zero. Using the values in the table below, RN is adjusted as follows:
Allowing the ground heat flux to keep its original value, corresponding adjustments are then made to the sensible and latent heat fluxes using a ratio of the adjusted available energy to the original available energy.
----------1987
----------
STN_ID SITEGRID XRN YRN SLOPE 1 YINT1 SLOPE 2 YINT2 ------ -------- ------ ------ ------- ----- ------- ------- 2 1916-BRS 325.00 331.55 1.020 0.000 1.170 -48.70 6 2132-BRK 325.00 338.45 1.041 0.000 0.973 22.23 8 3129-BRK 325.00 327.38 1.007 0.000 0.969 12.46 10 3414-BRK 325.00 330.92 1.018 0.000 0.973 14.70 12 2915-BRK 325.00 349.73 1.076 0.000 0.976 32.53 14 2516-BRK 325.00 339.82 1.046 0.000 0.934 36.27 16 4439-ECV 325.00 305.00 0.938 0.000 1.000 -20.00 18 4439-BRV 325.00 304.44 0.937 0.000 1.024 -28.36 20 6340-BRL 325.00 333.66 1.027 0.000 0.977 16.14 22 4609-ECW 325.00 323.62 0.996 0.000 0.955 13.25 24 6912-BRW 325.00 338.50 1.042 0.000 1.039 0.83 26 8739-ECB 325.00 344.68 1.061 0.000 1.060 0.18 28 6943-ECW 325.00 321.30 0.989 0.000 0.969 6.38 30 4268-ECG 325.00 310.83 0.956 0.000 1.085 -41.79 32 4268-BRK 325.00 327.03 1.006 0.000 0.978 9.18 34 3479-BRL 325.00 316.66 0.974 0.000 0.998 -7.69 36 2655-BRL 325.00 322.25 0.992 0.000 1.047 -18.02 38 1478-BRS 325.00 345.93 1.064 0.000 1.106 -13.52 40 1246-BRL 325.00 323.19 0.994 0.000 0.990 1.44 42 1445-BRL 325.00 322.27 0.992 0.000 1.016 -7.93 44 2043-BRL 325.00 315.61 0.971 0.000 1.077 -34.41
None.
See the Quality Assessment Section below.
It was recognized early in the study that standardization of "constants" (e.g. physical constants of the air, psychrometic constant, etc.), methods of computation, integration and reporting time, etc. were necessary. These were agreed upon in planning sessions. Preliminary data sets were compared among stations and instruments from different manufacturers for estimating net radiation, soil heat flux, water vapor density, temperature, solar radiation, and wind speed, it was necessary to have confidence that differences in observations were due to site differences and not due to instrumentation.
The hydrological Science Branch at NASA Goddard Space Flight Center was given the responsibility to compare flux data from all flux stations. This served two purposes: 1) as a data quality check, and 2) a preliminary analysis of site differences.
Model dependent flags by station and Intensive Field Campaign
This flag is computed based on computer runs using the Simple Biosphere (SiB) model. It gives an indication of the model's ability to reproduce the observed latent and sensible heat flux time series. A comparison of the canopy conductance computed for each IFC provides another check on the reasonableness of the data. Theory and observations suggest that this quantity should decrease from IFC-2 to IFC-4 as the site dries out. IFC-1 is disregarded since it was a wet period with high soil moisture contributions to the heat flux that would contaminate the calculated values of the canopy conductance.
Contradictions to this expectation are noted. Finally, a high canopy conductance in IFC-4 when the site was dry points to a bias in the data and is noted in the IDF_FLAG descriptor.
SIGH = standard deviation between the observed and calculated sensible heat flux over a given day
SIGE = standard deviation between the observed and calculated latent heat flux over a given day
ABAR = average observed available energy for a given day
SUM2 = SIGH * SIGH + SIGE * SIGE
The error is computed by taking the square root of SUM2 and dividing that by ABAR.
IDF DEFINITION--- ----------
0 Good data
1 The model did not have a good fit to the observed latent and sensible heat fluxes for that day. This condition was considered met when the error was greater than or equal to 0.10 for a particular IFC.
2 The results are contrary to the expectation of decreasing values of DF through IFC's 2, 3, 4 as suggested by theory and observations.
3 Error conditions 1 and 2 are met.
4 Abnormally high values of DF in IFC-4 suggest a bias in the data. Any values of DF in IFC-4 greater than 1.29e-5 (m^3/joules) (the average DF plus one standard deviation) were considered abnormally high.
5 Error conditions 1 and 4 are met.
6 Error conditions 2 and 4 are met.
7 Error conditions 1, 2 and 4 are met.
NOTE: IDF condition 1 is added only to that IFC.
IDF condition 2 is added to all IFCs.
IDF condition 4 is added to all IFCs.
STN_ID SITEGRID IFC DF ERROR IDF ------ -------- --- ---- ------ --- 2 1916-BRS 1 2.58 0.041 0 2 1916-BRS 2 2.43 0.105 1 2 1916-BRS 3 1.18 0.049 0 2 1916-BRS 4 1.13 0.046 0 10 3414-BRK 1 -9.99 -9.990 0 10 3414-BRK 2 4.30 0.067 0 10 3414-BRK 3 3.15 0.080 0 10 3414-BRK 4 0.87 0.028 0 12 2915-BRK 1 1.78 0.060 0 12 2915-BRK 2 3.35 0.025 0 12 2915-BRK 3 1.23 0.072 0 12 2915-BRK 4 0.30 0.045 0 14 2516-BRK 1 0.75 0.025 0 14 2516-BRK 2 1.79 0.033 0 14 2516-BRK 3 1.20 0.041 0 14 2516-BRK 4 0.73 0.036 0 16 4439-ECV 1 3.57 0.093 0 16 4439-ECV 2 3.38 0.067 0 16 4439-ECV 3 1.53 0.085 0 16 4439-ECV 4 0.62 0.033 0 18 4439-BRV 1 2.95 0.054 0 18 4439-BRV 2 2.97 0.066 0 18 4439-BRV 3 1.56 0.088 0 18 4439-BRV 4 0.76 0.043 0 20 6340-BRL 1 7.45 0.113 1 20 6340-BRL 2 3.35 0.062 0 20 6340-BRL 3 1.53 0.050 0 20 6340-BRL 4 0.94 0.049 0 22 4609-ECW 1 4.37 0.085 0 22 4609-ECW 2 3.20 0.068 0 22 4609-ECW 3 1.54 0.044 0 22 4609-ECW 4 0.44 0.029 0 24 6912-BRW 1 6.45 0.145 1 24 6912-BRW 2 4.18 0.111 1 24 6912-BRW 3 2.63 0.066 0 24 6912-BRW 4 0.43 0.033 0 26 8739-ECB 1 4.40 0.056 0 26 8739-ECB 2 4.72 0.070 0 26 8739-ECB 3 1.66 0.031 0 26 8739-ECB 4 1.03 0.083 0 28 6943-ECW 1 2.34 0.087 0 28 6943-ECW 2 1.66 0.068 0 28 6943-ECW 3 1.30 0.113 1 28 6943-ECW 4 1.04 0.104 1 32 4268-BRK 1 -9.99 -9.990 6 32 4268-BRK 2 2.34 0.065 6 32 4268-BRK 3 2.74 0.120 7 32 4268-BRK 4 1.37 0.039 6 34 3479-BRL 1 3.42 0.087 0 34 3479-BRL 2 1.85 0.113 1 34 3479-BRL 3 1.49 0.133 1 34 3479-BRL 4 1.10 0.232 1 36 2655-BRL 1 5.98 0.104 1 36 2655-BRL 2 4.80 0.076 0 36 2655-BRL 3 2.37 0.037 0 36 2655-BRL 4 0.85 0.048 0 38 1478-BRS 1 4.40 0.111 1 38 1478-BRS 2 3.42 0.072 0 38 1478-BRS 3 1.96 0.066 0 38 1478-BRS 4 0.33 0.037 0 40 1246-BRL 1 3.21 0.061 4 40 1246-BRL 2 3.01 0.045 4 40 1246-BRL 3 2.62 0.076 4 40 1246-BRL 4 1.40 0.086 4 42 1445-BRL 1 3.43 0.052 2 42 1445-BRL 2 1.76 0.077 2 42 1445-BRL 3 1.07 0.042 2 42 1445-BRL 4 1.17 0.103 3 44 2043-BRL 1 3.37 0.035 4 44 2043-BRL 2 5.00 0.053 4 44 2043-BRL 3 3.03 0.070 4 44 2043-BRL 4 1.73 0.047 4
The errors associated with the original flux measurements are described in the documents describing the original data sets. See the documents listed in the Related Data Sets Section for this information.
FIS staff applied a general QA procedure to the data to identify inconsistencies and problems for potential users. As a general procedure, the FIS QA consisted of examining the maximum, minimum, average, and standard deviation for each numerical field in the data table. Inconsistencies and problems found in the QA check are described in the Known Problems with the Data Section.
The data verification performed by the ORNL DAAC deals with the quality of the data format, media, and readability. The ORNL DAAC does not make an assessment of the quality of the data itself except during the course of performing other QA procedures as described below.
The FIFE data were transferred to the ORNL DAAC via CD-ROM. These CD-ROMs are distributed by the ORNL DAAC unmodified as a set or in individual volumes, as requested. In addition, the DAAC has incorporated each of the 98 FIFE tabular datasets from the CD-ROMs into its online data holdings. Incorporation of these data involved the following steps:
Each distinct type of data (i.e. "data set" on the CD-ROM), is accompanied by a documentation file (i.e., .doc file) and a data format/structure definition file (i.e., .tdf file). The data format files on the CD-ROM are Oracle SQL commands (e.g., "create table") that can be used to set up a relational database table structure. This file provides column/variable names, character/numeric type, length, and format, and labels/comments. These SQL commands were converted to SAS code and were used to create SAS data sets and subsequently to input data files directly from the CD-ROM into a SAS dataset. During this process, file names and directory paths were captured and metadata was extracted to the extent possible electronically. No files were found to be corrupted or unreadable during the conversion process.
Additional Quality Assurance procedures were performed as follows:
As errors are discovered in the online tabular data by investigators, users, or DAAC staff, corrections are made in cooperation with the principal investigators. These corrections are then distributed to users. CD-ROM data are corrected when re-mastering occurs for replenishment of CD-ROM stock.
Not available.
The following problem were encountered by the FIS staff during their general QA procedures:
Not available at this revision.
Not available at this revision.
Not available at this revision.
The FIFE field campaigns were held in 1987 and 1989 and there are no plans for new data collection. Field work continues near the FIFE site at the Long-Term Ecological Research (LTER) Network Konza research site (i.e., LTER continues to monitor the site). The FIFE investigators are continuing to analyze and model the data from the field campaigns to produce new data products.
Software to access the data set is available on the all volumes of the FIFE CD-ROM set. For a detailed description of the available software see the Software Description Document.
ORNL DAAC User Services
Oak Ridge National Laboratory
Telephone: (865) 241-3952
FAX: (865) 574-4665
Email: ornldaac@ornl.gov
ORNL Distributed Active Archive Center
Oak Ridge National Laboratory
USA
Telephone: (865) 241-3952
FAX: (865) 574-4665
Email: ornldaac@ornl.gov
Users may place requests by telephone, electronic mail, or FAX. Data is also available via the World Wide Web at http://daac.ornl.gov.
FIFE data are available from the ORNL DAAC. Please contact the ORNL DAAC User Services Office for the most current information about these data.
The Surface Flux Baseline 1992 data are available on FIFE CD-ROM Volume 1. The CD-ROM filename is as follows:
\DATA\SUR_FLUX\BASEL_92\GRIDxxxx\YyyMmm\ydddgrid.SFB
Where xxxx is the four digit code for the location within the FIFE site grid, yy is the last two digits of the year (e.g. Y87 = 1987), mm is the month of the year (e.g. M12 = December), and ddd is the day of the year, (e.g. 061 = sixty-first day in the year). Note: capital letters indicate fixed values that appear on the CD-ROM exactly as shown here, lower case indicates characters (values) that change for each path and file.
The format used for the filenames is: ydddgrid.sfx, where grid is the four-number code for the location within the FIFE site grid, y is the last digit of the year (e.g. 7 = 1987, and 9 = 1989), and ddd is the day of the year. The filename extension (.sfx), identifies the data set content for the file (see the Data Characteristics Section and is equal to .SFB for this data set.
Not available at this revision.
Sellers, P.J., M.D. Heiser and F.G. Hall. 1992. Relations between surface conductance and spectral vegetation indices at intermediate (100 [m^2] - 15 [km^2]) length scales. J. Geophys. Res. 97:19,033-19,059.
Contact the EOS Distributed Active Archive Center (DAAC) at Oak Ridge National Laboratory (ORNL), Oak Ridge, Tennessee (see the Data Center Identification Section). Documentation about using the archive and/or online access to the data at the ORNL DAAC is not available at this revision.
A general glossary for the DAAC is located at Glossary.
A general list of acronyms for the DAAC is available at Acronyms.
April 26, 1994 (citation revised on October 15, 2002).
Warning: This document has not been checked for technical or editorial accuracy by the FIFE Information Scientist. There may be inconsistencies with other documents, technical or editorial errors that were inadvertently introduced when the document was compiled, or references to preliminary data that were not included on the final CD-ROM. Previous versions of this document have been reviewed by the Principal Investigator, the person who transmitted the data to FIS, a FIS staff member, or a FIFE scientist generally familiar with the data.
October 29, 1996.
ORNL-FIFE_SF_BL92.
Sellers, P. 1994. Surface Flux Baseline 92 Derived (FIFE). Data set. Available on-line [http://www.daac.ornl.gov] from Oak Ridge National Laboratory Distributed Active Archive Center, Oak Ridge, Tennessee, U.S.A. doi:10.3334/ORNLDAAC/121. Also published in D. E. Strebel, D. R. Landis, K. F. Huemmrich, and B. W. Meeson (eds.), Collected Data of the First ISLSCP Field Experiment, Vol. 1: Surface Observations and Non-Image Data Sets. CD-ROM. National Aeronautics and Space Administration, Goddard Space Flight Center, Greenbelt, Maryland, U.S.A. (available from http://www.daac.ornl.gov).