SPADE
(1994-01-12 - pgh)
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Introduction
This CD-ROM contains the data pertaining to the Stratospheric
Photochemistry, Aerosols and Dynamics Expedition (SPADE) which was
based at Ames Research Center in California during portions of 1992
and 1993. Most of the data are in essentially final form, however
additional calibration work is being done for some of the instruments.
None of the instrument data is expected to change significantly from
the values reported here. A second edition incorporating updates and/or
changes to the data is anticipated in late 1994 or early 1995.
The data consist of measurements collected onboard the
NASA ER-2 aircraft, and selected radiosonde soundings from stations
in the region of the experiment. Flights were conducted during October
and November of 1992, April and May of 1993, and October of 1993.
Theory team products come in two forms -- as quantities
evaluated along flight tracks and as global or hemispheric fields.
Meteorological quantities, such as temperature, geopotential, and
potential vorticity are available in both forms. They are based on
analyses from both the U.S. National Meteorological Center and from
the Assimilation Model of NASA's Goddard Space Flight Center. Other
quantities, available along flight tracks only, include visible reflectivity,
cloud height, UV reflectivity, and total ozone. The first two are
derived from GOES imagery, the last two from the Meteor TOMS sensor.
Finally, calculations of mixing ratios of selected chemical species
using a photochemical steady state model are available along the flight
track.
All files within this release are standard ASCII files
with variable length records terminated by a carriage return/line
feed pair (, ASCII decimal values 13 and 10). Therefore, MS-DOS users
should be able to read them as they are, but UNIX and Mac users will
have to strip off either the or the from each line to convert them
to standard UNIX or Mac files. Commercially available software, such
as dos2unix and Apple File Exchange, exists to convert MS-DOS files
to both UNIX and Mac files. VMS users can define the files to have
STREAM record formats.
The file naming convention uses a two-character prefix
to identify the measurement, followed by a six digit number (yymmdd)
giving the year, month, and day (UT) of the flight, balloon launch,
or model result. To identify the measurement platform, a three character
extension of EA1, Bhh, or Ghh is used to denote the data is from the
ER-2, balloon, or grid point model output (hh denotes the UT hour
of balloon launch or model result).
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Directories
2.1 The DOCUMENT directory contains several files documenting
the contents of this edition.
Files:
- 2.1.1 CONTACT.DOC contains an updated list of names, addresses,
and phone numbers of the principal investigators responsible for
generating the datasets in this release.
- 2.1.2 ER2TABLE.DOC contains a record of the available ER-2 datasets
in tabular format.
- 2.1.3 FORSPEC1.PS and FORSPEC2.PS are PostScript files of the
document entitled "Format Specification for Data Exchange"
which defines the standard file formats in which all data are
recorded. These two PostScript files can be printed on any printer
that understands PostScript. FORSPEC1.PS contains the title page
and table of contents; FORSPEC2.PS contains the bulk of the document.
- 2.1.4 UV_VIS.DOC contains a detailed description of the UV-Vis
experiment, also known as the Composition and Photodissociative
Flux Measurement (CPFM). Note that the file name contains an underscore,
not a hyphen, to conform to the ISO 9660 file naming standards.
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Directory Structure for this CD-ROM is as follows:
- README.DOC in top level directory
>
- DOCUMENT
- DATA
- |-- ER2
- |-- MODEL
- |-- RAOB
This documentation and the accompanying data files were
compiled by:
Steven Gaines
NASA Ames Research Center
M/S 245-3
Moffett Field, CA 94035-1000
Patti Hathaway
NASA Ames Research Center
M/S 245-5
Moffett Field, CA 94035-1000
Steve Hipskind
NASA Ames Research Center
M/S 245-5
Moffett Field, CA 94035-1000
We have left the quality control of the data to the principal
investigators and have checked only the format of the data files. Therefore,
if problems with the data are encountered, please inform us or the appropriate
principal investigator.
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