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DAILY SOLAR GEOPHYSICAL DATA BROADCAST PROCESSOR
DATA BASE MANAGER - USERS MANUAL
VERSION 1.0
Copyright (c) 1991 Solar Terrestrial Dispatch
DAILY SOLAR GEOPHYSICAL DATA BROADCAST PROCESSOR
DATA BASE MANAGER - USERS MANUAL
VERSION 1.0
Copyright (c) 1991 Solar Terrestrial Dispatch
1. Introduction
The Solar Terrestrial Dispatch (STD) recently began providing a
comprehensive set of daily solar geophysical indices to the public in
the form of a product known as the "Daily Solar Geophysical Data
Broadcast" (SGDB). The data and indices contained in the SGDB are
very valuable to persons interested in ionospheric radio communica-
tions, solar activity, auroral activity, related geomagnetic events
and even atmospheric phenomena. The datsets are used by a large
number of professional research institutions and astronomical organi-
zations to aid in the study of such things as the Earths atmosphere,
the Earths magnetic field, solar and space research, etc.
It was clearly evident that such a large set of data would be
more useful if it could be archived and studied over time. In order
to satisfy this need, the Solar Terrestrial Dispatch began the
development of a software package which would automatically extract
all of the relevant data from the SGDBs and archive them to disk for
analysis and study. This software became known as "BCAST", the Solar
Geophysical Data BroadCAST Processor and Database Manager.
BCAST provides complete archive and database management capabili-
ties in a user-friendly and easily operated environment. It will
automatically maintain a fully sorted archive of the data sets for
instant recall or graphical analysis. It will also produce detailed
summaries of the datasets in laymans terms which may be printed out
and distributed or filed away.
BCAST also provides a powerful "batch" processing feature to
automatically archive large numbers of SGDBs in one simple step.
Included with the BCAST software is a complete copy of every SGDB
report produced since its inception to the date the BCAST software was
released. All of the SGDB reports are archived at several sites and
may also be obtained from our computer BBS at: (403) 756-3008. Using
the "batch" function of the BCAST software, you will easily be able to
create a complete archive of the data contained in these SGDB reports.
Also included with BCAST is our extensive document "Understanding
Solar Terrestrial Reports" and the supplement "Glossary of Solar Ter-
restrial Terms." These documents have helped many people better
November 13, 1991
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understand the impact the Sun has on phenomena and conditions here on
Earth as well as the language and jargon used to describe conditions.
The database generated and maintained by BCAST will let you
analyze and study the cyclical behavior of such things as solar
activity, geomagnetic activity, and ionospheric disturbances. You may
also be able to anticipate the future behavior of the indices. This
is invaluable to those who, for example, are interested in predicting
when radio communications will be optimum, or when auroral activity
may again be observed, or when the next group of hot solar regions is
due to rotate into view.
These, and other features of the BCAST software provide you with
all of the tools necessary to closely monitor conditions on your own.
2. The SGDB Data Sets
The Solar Geophysical Data Broadcasts (SGDBs) released daily by
the Solar Terrestrial Dispatch are composed of a number of compact
textual lines. In order to fully describe the meaning of each com-
ponent of each line in the SGDBs, a document was created which goes
through the data sets line by line, component by component.
A complete copy of this descriptive document may be found in the
file "SGDB.DOC". For those who are interested in understanding the
format of the SGDB reports, this document will be invaluable.
3. The Shareware Concept
Shareware is a unique method of distributing computer software.
Programs are developed and freely distributed throughout the world.
The programs provide you with an idea of their operation and their
features, but restrict access to certain key features until the person
interested pays for the software.
BCAST is not free. A considerable amount of our time and
resources have been expended to develop this software package, not to
mention the large number of resources which are regularly dedicated to
produce the daily data sets.
In order to be able to continue providing these daily data sets
and software to use them, it is important that we recover our costs
for providing these services. In order to accomplish this, we have
based the BCAST software on the shareware theme and will require pay-
ment from those who wish to use all of its capabilities.
The BCAST software package is freely distributed as "Unre-
gistered" software. To purchase the software so all of its features
may be used, it must be registered. The only way to accomplish this
is to send a cheque or money order for $28.00 dollars (in Canadian or
U.S. funds) to:
November 13, 1991
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Solar Terrestrial Dispatch
P.O. Box 357
Stirling, Alberta, Canada
T0K 2E0
All funds should be remitted to the "Solar Terrestrial Dispatch".
U.S. cheques or money orders are acceptable. A sample registration
form is contained with this software package under the filename
"REGISTER.DOC". You may print out a copy and mail it to us with your
payment, if desired.
Upon receipt of your registration request and payment, we will
immediately send you the necessary instructions to make your copy of
the BCAST software a registered copy, along with your unique registra-
tion I.D. number. Thereafter, you will be able to use the BCAST
software without limitation.
If you have an email address on one of the larger INTERNET or
BITNET networks, include your address(es) with your registration
request so we can contact you through e-mail. If you don't have an
e-mail address or if you fail to include it with your payment, we will
notify you through postal mail.
4. Starting Up BCAST
There are two ways you can invoke BCAST. The easiest method is
simply to type "BCAST" at your DOS command line prompt. This will
immediately load the program and execute it. The second method of
invoking BCAST is through the use of the "batch" feature for process-
ing multiple SGDB data sets quickly and easily. This feature will be
described later.
In order for BCAST to be able to find the various support files
it requires for normal operation (ex. the database file), you should
execute BCAST in the directory where the BCAST database file exists.
When you are maintaining a database, BCAST expects to find the data-
base file with the filename: "DATASETS.DAT". BCAST will not utilize
the database if this file cannot be found in the same directory that
you execute BCAST.
After you have executed BCAST, a title page should appear on-
screen. If you have registered your copy of BCAST, the word
"Registered" will appear on the title page. If you have not yet
registered your copy of BCAST, the word "Unregistered" will be
displayed. Unregistered copies of BCAST are heavily limited in the
number of functions which may be performed, in order to help encourage
payment for the program.
Pressing any key will move you from the title page screen to the
main menu screen. This screen has four major functions which may be
selected using the arrow keys. Each function is discussed below.
November 13, 1991
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4.1. Processing Data Sets
To select this function, use the left or right arrow keys until
the function "Process Data Sets" is highlighted, then hit the down
arrow key or press ENTER.
This function simply extracts all of the information from the
textual SGDB file and converts the data into a form which can be more
easily used by the computer.
Use this function when you need to incorporate a new SGDB data
set into your database, or to extract the information for display
using the second function of the main menu (Review Data Set).
You will be asked for the name of the file containing the SGDB
data set. Simply supply the name of the file and press ENTER. BCAST
will automatically find the dataset (even if the dataset is buried in
another text file such as a mail message or a descriptive report) and
process it.
During the processing phase, BCAST checks to make sure that you
are using a version of BCAST which is compatible with the SGDB data
set being processed. It also checks every line of the SGDB report to
ensure that it is properly formatted. If BCAST finds anything unex-
pected or anomalous with the data set it is processing, it reports it
on-screen. Depending on the severity of the anomaly detected, BCAST
may terminate with a Fatal Error (ex. return you to the DOS prompt
with an explanation) or simply warn you and continue processing the
data set.
If all goes well, BCAST will almost instantly load the textual
SGDB data set into memory. Once the data set has been processed, you
are free to do a number of things. You may display the dataset in an
easier to understand format on-screen. Or you may wish to save the
dataset to your database for future analysis. You may also want BCAST
to create a detailed summary of the data set on disk, or graphically
analyze the data. Once you have loaded a dataset into memory, you are
free to do almost anything.
4.2. Displaying Data Sets On-Screen
After a SGDB dataset has been loaded from disk into memory, you
may choose to display the data on-screen in a much friendlier format.
The second main menu function, "Display Data Set" provides you with
this capability.
This feature automatically decodes the various acronyms used in
the textual SGDB reports and displays their meanings on-screen in lay-
mans terms. It provides screenful upon screenful of useful informa-
tion regarding the dataset by interpreting the contents and explaining
or displaying them.
The first and possibly second screens displayed by BCAST are sum-
maries of the warnings and alerts which were in progress at the time
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the SGDB data set was compiled at the Solar Terrestrial Dispatch.
These warnings and alerts which are displayed do not go into any sig-
nificant detail. In fact, this section of the SGDB report is the only
section which is not copied verbosely into the computer during the
processing phase. In other words, the details of each warning and/or
alert are not processed. The reason for this is to keep the BCAST
database file down to a minimal size. The smaller each BCAST database
record is, the more information you will be able to store in a given
amount of disk space. If all of the possible details of every various
warning and alert were processed, each database record would be much
larger than needed, more difficult to process and would be wasteful
with disk space. All that is really required is knowledge of the
basic warnings and alerts which are in effect during each day. The
details of the warnings or alerts aren't as important. If the details
are important, you are encouraged to obtain one of the extensive
monthly summaries of activity produced by the Solar Terrestrial
Dispatch, or made available on our computer BBS system.
The screens following the warnings and alerts summarize in great
detail the data which was loaded from the textual SGDB report. All of
the various indices are listed. Many of them are interpreted for you
so you can better understand their meaning.
This feature may be executed by those who have not registered the
BCAST software package with us.
4.3. The Archive and Analysis Menu
The third function of the BCAST main menu represents the heart of
BCAST: the archive and analysis features. This is an extensive menu
containing all of the functions necessary to maintain the database,
archive new data to disk, generate reports, and graphically analyze
the data in the database.
In order to encourage payment for this program, this section of
BCAST is not available to those who have not registered their copy of
BCAST with us. In order to develop and maintain your own database of
records, you will need to purchase your copy of the program by sending
a cheque or money order for $28.00 in either Canadian or U.S. funds to
the Solar Terrestrial Dispatch (our address was given in "The
Shareware Concept" section of this manual). After your unique regis-
tration number has been returned to you with the simple instructions
for making your copy of BCAST a registered copy, you will be able to
access and use this section of BCAST at your leisure.
4.3.1. Saving Loaded Data Sets to the Database
BCAST expects to find its database file in the same directory
that you execute BCAST and with a filename of "DATASETS.DAT". If you
execute BCAST in a directory where this file does not exist, BCAST
will not use the database. This behavior allows you to maintain
separate databases in different directories. To use a specific data-
base, simply move to the directory containing the database and execute
BCAST.
November 13, 1991
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There are two methods of adding datasets to your database. The
first is the "batch" processing method which automatically archives
large numbers of SGDB datasets to your database in a single command.
The second method, and the one which will be discussed now, archives a
single SGDB dataset to your database.
Before this option can be executed, you must first load a dataset
into memory using the first option (Process Data Set) of the main
menu. After you have loaded a dataset into memory, you may archive
that dataset to your database file using this option of the Archive
Menu. To execute this option, simply select the "Save Data Set"
option in the Archive Menu using the Up and Down arrow keys. After
you have highlighted the "Save Data Set" option, press ENTER.
Before writing the new data set to the database file, BCAST
checks to make sure that no other records in the database match the
one you are attempting to archive. If it finds a record in the data-
base with the same date as the dataset you are attempting to archive,
a warning is displayed on-screen giving you three options. You may
overwrite the record, which is useful when you need to correct or
modify a record in your database. You may skip the record, which will
force BCAST to write the dataset to the database. In this case, noth-
ing is overwritten. New space within the database is created for the
dataset you are saving. If this option is chosen, there will be two
records in your database with identical dates. The last option lets
you abort the save procedure altogether. In this case, the database
is left unchanged. Nothing is written to the database.
When BCAST saves datasets to the database file, it automatically
archives the dataset fully sorted with the existing records in the
database. It sorts the database according to dates. For this reason,
records which are archived near the "front" of the database (ex. a
dataset which has a date earlier than anything presently existing in
the database) will take longer to save to disk than a dataset which
has a date close to the present date. The sorting process occurs
sequentially from the lowest to the highest dates. That is, a dataset
dated January 1, 1991 would appear BEFORE a dataset dated January 2,
1991. Conversely, a dataset dated December 31, 1990 (note the year)
would appear BEFORE the datasets dated January 1 and 2, 1991 in the
database file.
This automatic sorting feature significantly simplifies and
speeds up many of the functions available in this program.
If the dataset is successfully archived to the database, an
"operation successful" message is displayed on your screen. If an
error occurs, you may be returned to DOS depending on the severity of
the error. All disk errors result in a Fatal Error message which
immediately returns you to the DOS prompt with an explanation.
4.3.2. Loading a Dataset from the Database
This option loads a dataset which you previously archived to the
database. Using this option, you can examine (via the main menu
November 13, 1991
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option "Review Data Sets") the conditions and indices which were
observed for any date contained in your database file.
You are simply prompted for the date of the dataset you wish to
load from the database. After specifying a date, BCAST searches
through the database until it finds the requested dataset. If the
date you specify is either invalid or cannot be found in the database,
an error message is displayed which then returns you to the Archive
Menu.
This option has a secondary side-effect which may not be clearly
apparent at first. When BCAST graphically analyzes the datasets in
the database file, it always attempts to graphically display the vari-
ous datasets with respect to the date of the currently loaded dataset.
In other words, all graphs or charts produced by BCAST will be
displayed so that the LAST line of the graph or chart is the graph
line of the dataset which you have currently loaded in memory. If you
do not have a specific dataset loaded in memory, all graphs are pro-
duced with the last dataset of the database (ex. the most recently
archived dataset) displayed as the last graph line on the screen.
To better explain this feature, let's assume that you have 200
datasets archived to your database and you wish to graphically analyze
them. Since BCAST can only fit 70 datasets on-screen at one time, it
is necessary to select a portion of the 200 datasets to graphically
analyze. This is achieved by loading datasets for specific dates into
memory. If a dataset is loaded into memory, the date of that dataset
is used to determine which portion of the 200 datasets to graphically
display on-screen. For example, if the 200 datasets in your database
were sequentially dated from January 1, 1991 to July 19, 1991 (200
consecutive days), and you loaded a dataset into memory which was
dated March 11, 1991, BCAST would only graphically analyze the
datasets from January 1, 1991 to March 11, 1991 (70 days). The
dataset for March 11, 1991 would be the last graph line displayed on-
screen. Similarly, if you wanted to graphically display the last 70
datasets on-screen, you would load the dataset which was dated July
19, 1991 into memory. All graphical charts produced by BCAST follow
this procedure.
For these reasons, this option is important for positioning the
graphical charts produced by BCAST. The graphical analysis features
are presented next.
4.3.3. The Graphical Analysis Options
BCAST provides a set of valuable graphical analysis tools which
will help you better analyze the cyclical behavior or other parameters
of the datasets in your database.
Almost all of the various data contained in the SGDB reports can
be graphically analyzed using BCAST. The only items which are not
analyzed are the Boulder and Planetary K-indices. For these indices,
we have developed an impressive three-dimensional graphics analysis
package which will read the database generated by BCAST to analyze the
November 13, 1991
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Boulder and Planetary K indices. It will also generate self-contained
GIF images of the graphs you produce on-screen for future study,
reference, archiving, transmission, or for hard-copy production using
GIF image viewers. This VGA-compatible graphical analysis package may
be purchased from the Solar Terrestrial Dispatch. Those of you who
are interested may wish to purchase this program at the same time you
register your copy of BCAST. This three-dimensional graphical
analysis software is a handsome complement to the BCAST software pack-
age. For more information regarding this program and for purchase
information, consult the file "SOFTWARE.DOC".
To analyze a specific set of data, simply select the appropriate
option from the Archive Menu and press ENTER.
BCAST produces two types of graphical charts depending on what
type of data you are analyzing. Linear data, such as the 10.7 cm
solar radio flux or the geomagnetic data, use the linear graphical
functions. Other datasets such as the proton fluence or x-ray statis-
tics are analyzed and graphed using logarithmic graphical charts.
This significantly improves the detail of the graphs.
There are two important functions which can be executed while
graphs of datasets are displayed on-screen. The first is the ability
to move through the graph, line by line, using the left and right
arrow keys. As you use the arrow keys, each new graph line you move
to is highlighted. Using the left arrow keys moves the highlighted
area to the left. The right arrow key moves the highlighted area to
the right. In addition, the date of the highlighted graph line as
well as the exact value producing that line is displayed at the bottom
of the screen. This lets you examine each line of the graph in great
detail.
The second important function which can be executed while a
graphical chart is displayed, is the ability to save the currently
displayed graph to a text ASCII file on disk. After a graph has been
saved to disk, you may print it out on a printer or transfer them
electronically to other locations.
To invoke this disk saving function, simply press "S" (for
"S"ave) while any graphical chart is displayed on-screen. The screen
will immediately be converted to ASCII format and saved to disk under
the file name "GRAPH.TXT". Each time you press "S", the graphical
chart displayed on-screen is APPENDED to (or written to the end of)
the GRAPH.TXT file. This lets you compile an extensive set of graphs
simply by graphically analyzing those datasets you need and pressing
the "S" key. After you have finished and exited the BCAST program to
the DOS prompt, you may display the GRAPH.TXT file, edit it using your
favorite word processor, print it out, transfer it elsewhere, or do
whatever you see fit to do with it.
To continue to view other datasets, press ENTER when you have
finished viewing a specific graphical chart. To abort the procedure
and return to the archive menu, press the ESCape key.
November 13, 1991
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4.3.4. Generating an Activity Summary Report
This option of the Archive Menu analyzes the currently loaded
dataset and writes a summary report to the file "SUMMARY.TXT" on disk.
All of the indices contained in that dataset are written to the file,
along with the various warnings and alerts which were in effect, etc.
This report-generation feature is most useful when data from the SGDB
reports are to be distributed throughout an organization, or
transfered to other locations through e-mail or modem. This is also
an invaluable tool for producing hard-copy summaries of the dataset
you have loaded in memory. This file may then be printed out and
filed away for future reference.
If the file "SUMMARY.TXT" already exists when you execute this
function, the contents of the file will NOT be overwritten. All
information is appended to the SUMMARY.TXT file. You will therefore
be able to store multiple summaries in a single file, if so desired.
4.3.5. Generating a Standard SGDB File & Modifying Records
BCAST has the ability to recreate a standard Solar Geophysical
Data Broadcast format file. This is an important function if you need
to modify certain indices or values of a specific dataset in your
archive.
To use this feature, you must have a dataset loaded in memory
(either using the first option of the Main Menu [Process Data Set], or
the second option of the Archive Menu [Load a Data Set]). After a
dataset has been loaded in memory, a precisely formatted SGDB file can
be created using this function.
Why would you need to create a standard SGDB file in the first
place? There are a number of reasons. You may need to transfer a
specific dataset you have in your archive to a friend who is missing
that particular dataset. You could transfer the SUMMARY.TXT file,
although this file is not in the correct format to be processed by
others using BCAST. Using this function, you can recreate a copy of
the SGDB for any dataset in your archive, which may then be shared
with others who are using BCAST to archive and analyze data.
One of the primary reasons for requiring this function is to per-
mit the easy modification of specific datasets in your database. For
example, lets assume that one of your datasets in your database is
corrupt. Lets say that one of your datasets in your database has a
bad value for the 10.7 cm solar radio flux and you need to correct it.
All you need to do is load that dataset into memory using the second
option of the Archive Menu (Load a Data Set), and generate a standard
SGDB file for that dataset. The incorrect 10.7 cm solar radio flux
value will be written to the SGDB.TXT file. Simply exit BCAST, edit
the SGDB.TXT file to correct the 10.7 cm solar radio flux value. Then
reload BCAST, reprocess the SGDB.TXT file so that the corrected
dataset is reloaded into memory (using the "Process Data Set" option
of the Main Menu), and save the corrected dataset to your database
using the "Save Data Set" option of the Archive Menu. BCAST will
November 13, 1991
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detect the corrupted dataset by realizing that the dataset you have
loaded into memory has the same date as the bad dataset in your
archive. It will then ask whether or not you want to overwrite the
dataset. By responding so that BCAST overwrites the incorrect
dataset, you can effectively correct the bad solar flux value in your
database.
This procedure can be carried out for any of the values in your
database. It is a quick and easy method of modifying any dataset in
your archive. To summarize, simply extract the dataset you need to
correct to a standard SGDB file, edit it using a word processor,
reprocess it using BCAST and resave it to your database file using the
"O"verwrite option which will appear.
This function will not overwrite any existing data in the
SGDB.TXT file if it already exists when you attempt to produce the
standard SGDB file. All data is appended to the SGDB.TXT file. You
may therefore create multiple SGDB reports in a single file, if
desired.
4.3.6. Dumping Data Sets to an ASCII File
This powerful function lets you dump the entire contents of your
database to a text ASCII file with the name "DATASETS.TXT". Use this
function with caution, since very large text files can be created in
the process.
During this procedure, BCAST runs through your database file mul-
tiple times, extracting each of the datasets from the database and
saving them to the DATASETS.TXT file. The resulting text file is a
well-ordered, fully sorted, textual representation of every set of
data in your database.
This feature becomes particularly important when you need to
analyze the data externally using something like a statistical com-
puter program or a spreadsheet. Also, since the data is dumped in a
pure ASCII format, you can edit the text file and extract only the
information you require.
4.3.7. Deleting Datasets from the Database
The only other function required to provide complete management
control over your database is a method of deleting datasets from your
database. That is the purpose of this Archive Menu function.
To delete a specific dataset from your archive, simply select
this function. BCAST will prompt you for the date of the dataset to
delete. After typing in the date, BCAST will search through the data-
base until it finds a dataset with a matching date. It will then
request confirmation from you. If you respond in the affirmative,
BCAST will delete the dataset from your database. If you do not con-
firm deletion, BCAST will abort the procedure and leave your database
untouched.
November 13, 1991
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It is important to note that after you have confirmed deletion,
BCAST will delete ALL datasets with dates matching the one you sup-
plied, not only the one which BCAST first detects. Therefore, using
this command you can delete accidental redundant datasets from your
database (as can occur if you save a dataset to your archive which
already exists).
4.3.8. Returning to the Main Menu
You can return from the Archive Menu to the main menu at any time
by either pressing the ESCape key, or selecting the "Return to the
Main Menu" option. When running BCAST, the ESCape key serves as the
"abort" key. It will abort almost any process and return you to a
menu.
4.4. Exiting BCAST and Returning to DOS
To exit BCAST and return to the DOS prompt, either select the
"Exit Program" command of the Main Menu or press the ESCape key at the
Main Menu prompt. Either method will terminate the program and return
you to the DOS prompt.
5. The Batch Processing Feature of BCAST
BCAST provides a powerful batch processing function which can
only be invoked at the command line. This function will automatically
process large numbers of SGDB report files and archive them to your
database. All SGDB files processed in this manner are automatically
and accurately saved to your database fully sorted.
To execute this command, simply execute BCAST with the command
line parameter "-b" (or "-B", it is not case sensitive) followed by
the name(s) of the files you want to be processed and archived. Wild-
cards in the filenames are permitted.
For example, to create an extensive archive of every SGDB report
included with this software package, simply type: "BCAST -B *.DLY"
(excluding the parenthesis, of course) and press ENTER. BCAST will
automatically begin processing and archiving every file containing the
extension ".DLY". As each file is processed, it's name is displayed
on-screen so you can monitor the progress of the processing. It does
not matter which order you specify files to be processed. BCAST
automatically sorts the database so that all added datasets are placed
in the proper position in the archive.
During the batch processing phase, if BCAST attempts to process a
dataset which already exists in your archive (ex. a dataset with the
same date), BCAST discards the dataset and processes the next file.
You may therefore process a group of files without needing to worry
about accidentally processing a duplicate dataset. BCAST will not
batch process a dataset which already exist in your database.
After all of the files have been processed, BCAST loads and
displays the title page, followed by the Main Menu, etc.
November 13, 1991
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Please note that the last file processed will reside in memory
while BCAST executes. As a result, if you graphically analyze your
database after executing the batch processing feature, the graphical
charts will be displayed according to the date of the last dataset
processed. Consult the section on "Loading a Data Set from the Data-
base" for more information regarding this feature.
This feature is only available to those who have registered their
copy of BCAST with us (consult "The Shareware Concept" section of this
manual or the file "REGISTER.DOC" for more information regarding
registration).
6. Alternate Method of Executing BCAST
You can run BCAST and process a textual SGDB dataset at the same
time by executing BCAST with an extra parameter specifying the name of
the file to process. For example, to execute BCAST and automatically
process the file "SGDB.TXT" so that the dataset contained in that file
is loaded in memory, simply execute BCAST using the command:
"BCAST SGDB.TXT". This will run BCAST as usual, but will force it to
process the file SGDB.TXT before the main menu appears.
This speeds up the procedure for processing and analyzing the
dataset. Normally, you would need to select the "Process Data Set"
function of the Main Menu before you could review or archive the
dataset. By specifying the name of the SGDB file to process on the
command line, you effectively skip this step.
Please note that the dataset loaded in this manner is NOT
archived to your database. It is simply loaded in memory. If you
want to archive the dataset to your database, you will need to include
the "-B" (batch processing) parameter on the command line or expli-
citly save the loaded dataset to your database using the appropriate
Archive Menu function.
This function may be used on unregistered copies of BCAST.
7. Future Software Releases & BCAST Revisions
The Solar Terrestrial Dispatch reserves the right to change at
any time, and without prior warning, the format of the daily Solar
Geophysical Data Broadcasts. However, before any changes are made, we
will make sure that compatible versions of this BCAST program are
available. To ensure the proper operation of BCAST with the SGDB
datasets, the version numbers of both the SGDB datasets and the BCAST
software must match. If they don't match, you run the risk of
experiencing problems in processing the datasets.
Also, before any changes to the SGDB dataset formats are made, we
will ensure that future revisions or releases of BCAST contain
appropriate software to convert existing databases to the new format.
The Daily Solar Geophysical Data Broadcasts are used world-wide
by an increasing number of professional research institutions and
November 13, 1991
- 13 -
interested amateurs. It is therefore important that we maintain a
format which is as consistent and stable as possible.
All those who register the BCAST program with us will be able to
use future revisions or updates of BCAST without additional charges,
provided you continue to remain registered with us. Registrations
expire after one year. Registered persons who let their registrations
expire will still be able to use their software without limitation.
However, they will not qualify to use future updates of BCAST free
of charge, or be granted special priviledges to future software
releases. The most recent versions of BCAST may be ordered directly
from us at the address given earlier (read the file "ORDERS.DOC" for
procedures), or may be downloaded directly from our BBS in a
compressed format in the "Utilities" file section.
Although we have taken every measure to try to ensure the proper
operation of this software, there is always the chance that bugs were
overlooked. In the unfortunate event a bug is observed, please make a
note of it along with details which may help us to reproduce the
error. All bug reports should either be mailed to the Solar Terres-
trial Dispatch, or be sent via e-mail to: Oler@Hg.Uleth.CA, or to:
COler@Solar.Stanford.Edu. We will make every effort to correct any
problems with the software as soon as possible.
All future software which we develop may require the database
generated by the BCAST software to operate properly. We are presently
in the process of developing a large solar terrestrial software pack-
age which will use the database generated and maintained by BCAST to
produce regionalized forecasts for any area of the world. Although
still being developed, this software package should prove to be a sig-
nificant aid to those interested in observing auroral activity,
exploiting optimum radio communication conditions, or studying the
disturbance zones in interplanetary space. This software package will
be easy to use and understand by the layman.
A software package to graphically analyze the Boulder and Plane-
tary K-indices in three-dimensions from the records created by BCAST,
is (or soon will be) available from the Solar Terrestrial Dispatch.
This software requires the database generated by BCAST to work
properly. For those who are now registered with us, please note that
special discounts apply. Consult the file "SOFTWARE.DOC" for details.
November 13, 1991
- i -
Table of Contents
Introduction .................................................... 1
The SGDB Data Sets .............................................. 2
The Shareware Concept ........................................... 2
Starting Up BCAST ............................................... 3
Processing Data Sets ............................................ 4
Displaying Data Sets On-Screen .................................. 4
The Archive and Analysis Menu ................................... 5
Saving Loaded Data Sets to the Database ......................... 5
Loading a Dataset from the Database ............................. 6
The Graphical Analysis Options .................................. 7
Generating an Activity Summary Report ........................... 9
Generating a Standard SGDB File & Modifying Records ............. 9
Dumping Data Sets to an ASCII File .............................. 10
Deleting Datasets from the Database ............................. 10
Returning to the Main Menu ...................................... 11
Exiting BCAST and Returning to DOS .............................. 11
The Batch Processing Feature of BCAST ........................... 11
Alternate Method of Executing BCAST ............................. 12
Future Software Releases & BCAST Revisions ...................... 12
November 13, 1991