1. VGMO.NET Vladimir Papitashvili papita@umich.edu Anshuman Saxena anshuman.saxena @tcs.com Valeriy Petrov vpetrov@engin. umich.edu Robert Clauer rclauer@umich.edu Natalia Papitashvili natasha@mail630. gsfc.nasa.gov April 23, 2004 Page 1 of 15 ICESTAR A Workshop for Planning the SCAR Scientific Programme Interhemispheric Conjugacy Effects in Solar-Terrestrial and Aeronomy Research April 22-23, 2004, Villefranche sur Mer, France Vladimir Papitashvili, Anshuman Saxena*, Valeriy Petrov, Robert Clauer, and Natalia Papitashvili** Space Physics Research Laboratory University of Michigan, Ann Arbor, MI, U.S.A. http://maggy.engin.umich.edu/mist/vgmo.html * Now at TATA Consultancy Services, Bangalore, India ** NSSDC and QSS, Inc., NASA/GSFC, Greenbelt, MD, U.S.A. VGMO.NET A VIRTUAL GLOBAL MAGNETIC OBSERVATORY Concept and Realization

2. VGMO.NET Vladimir Papitashvili papita@umich.edu Anshuman Saxena anshuman.saxena @tcs.com Valeriy Petrov vpetrov@engin. umich.edu Robert Clauer rclauer@umich.edu Natalia Papitashvili natasha@mail630. gsfc.nasa.gov April 23, 2004 Page 2 of 15 ICESTAR 1.Search through a number of data centers, various institutions, observatories, contact colleagues… Hi, Bob, could you send me data? 3.Then ingest retrieved data into a local database… Ugh, done! 4.Process collected data using mostly proprietary codes, run models… and… Sounds “exciting”… right? Yes, searching and then converting data from various formats into something useful for local processing and analysis – this can be time consuming, labor intensive, and often frustrating if collected data do not deliver what you have expected! 2.Get data via snail-mail, air-mail, e-mail, Web… Oh, where are data? 5.Finally, get something meaningful or meaningless… Hurrah! To get scientific data from various, mostly distributed sources, a scientist may have to:

3. VGMO.NET Vladimir Papitashvili papita@umich.edu Anshuman Saxena anshuman.saxena @tcs.com Valeriy Petrov vpetrov@engin. umich.edu Robert Clauer rclauer@umich.edu Natalia Papitashvili natasha@mail630. gsfc.nasa.gov April 23, 2004 Page 3 of 15 ICESTAR Current Forms of Sharing Geomagnetic Data: Centralized distribution schemes – e.g., World Data Centers (WDC) Require persistent support for data acquisition, storage, and distribution Submission of data remains voluntary Often data are not suitable for submission – e.g., WDCs only accept absolute geomagnetic measurements; however, geomagnetic data collected outside of standard magnetic observatories are mostly variational in nature Personal Communication – exchange of discs, customized FTP access, etc. Communication overhead – significant delays between responses Any change in the structure of remote databases requires renegotiation for access Need to develop more contacts Remember - people often change their minds and responsibilities Publishing data through World Wide Web In order to avoid additional steps of data preparation for submission to WDC To achieve greater visibility amongst the scientific and user communities Increased computing power and bandwidth – lots of untapped potential at the edge of networking Such diversity of available geomagnetic databases argues for more sophisticated search engines capable of identifying geomagnetic data repositories and then retrieving data for scientific analyses

4. VGMO.NET Vladimir Papitashvili papita@umich.edu Anshuman Saxena anshuman.saxena @tcs.com Valeriy Petrov vpetrov@engin. umich.edu Robert Clauer rclauer@umich.edu Natalia Papitashvili natasha@mail630. gsfc.nasa.gov April 23, 2004 Page 4 of 15 ICESTAR VGMO.NET Virtual Global Magnetic Observatory VGMO.NET is a middleware architecture that provides a new way for the worldwide geomagnetic community to share data and functionality in a platform-independent and location-neutral environment Design Goals Identify prospective geomagnetic data repositories and provide transparent access to these remote databases through a common interface Perform online processing of the acquired data sets Ability to construct self-populating databases on individual machines; these self- populated sub-centers can be made available to other users through future request chains (i.e., building a GRID-type access and computing) FFMN A four-tier architecture of VGMO.NET LOCATION DISCOVERY (GeoMaC) IDLMatlab Simulink Lowest layer - Location Discovery Module, GeoMagnetic Crawler (GeoMaC), which continuously forages Web for prospective geomagnetic data repositories Data Acquisition downloads requested data from remote sites using specific site information from the shared data structures A2F converts downloaded data into a Flat- File Format (or even to a proprietary format) Integrated Visualization Layer, e.g., Flat File Manager (FFMN) or other tools, can be used to perform analysis of data DATA ACQUISITION (HTTP/FTP/OPeNDAP/….) FORMAT CONVERSION (A2F)

5. VGMO.NET Vladimir Papitashvili papita@umich.edu Anshuman Saxena anshuman.saxena @tcs.com Valeriy Petrov vpetrov@engin. umich.edu Robert Clauer rclauer@umich.edu Natalia Papitashvili natasha@mail630. gsfc.nasa.gov April 23, 2004 Page 5 of 15 ICESTAR VGMO.NET - The Local Database oGeomagnetic data are published in widely different, often proprietary formats oWe convert all downloaded data sets into a Flat-File database oDatabases built via VGMO.NET conform to the Flat-File DBMS architecture Flat DBMS revisited [A. Smith, C. R. Clauer, 1984] oEach dataset consists of two files: a header file, which is an ASCII description of the dataset and a binary data file that is the data itself oLeverages advantages of ASCII presentation (readable and editable data description), as well as binary presentation (compact data storage and fast random access) oA sample header file: Name of header and data files: VOS01 Date files created: 13-May-2002 Record length of data file, in bytes: 20 Number of columns: 4 Number of rows: 3137310 Flag for missing data: -0.10E+33 # name units source type loc 1 Time seconds T 1 2 VOCE nT Antarctic magnetometer R 9 3 VOSH nT Antarctic magnetometer R 13 4 VOSZ nT Antarctic magnetometer R 17 NOTES: Start time = 01-JAN-01 00:02:00.000 End time = 31-DEC-01 23:58:00.000 Antarctic magnetometer high resolution data END Note that the local database might hold a mixture of various data (flat files): the interplanetary magnetic field/solar wind data, ionospheric data, etc.

6. VGMO.NET Vladimir Papitashvili papita@umich.edu Anshuman Saxena anshuman.saxena @tcs.com Valeriy Petrov vpetrov@engin. umich.edu Robert Clauer rclauer@umich.edu Natalia Papitashvili natasha@mail630. gsfc.nasa.gov April 23, 2004 Page 6 of 15 ICESTAR VGMO.NET - The Local Database (cont’d) File Name consists of three parts – a station IAGA 3-letter code, followed by a timestamp in YYYYMMDD format and some special tags that are attached for housekeeping purposes: Special Tags: absolute measurements: a variation measurements: v public access: p restricted access: r rate of data sampling (in sec): 60/30/1/ For example, a publicly accessible dataset consisting of 60-sec samples of absolute geomagnetic measurements from Antarctic magnetic observatory VOSTOK for December 2002 will be stored in the flat files named: \2000\06\MAG\VOS2000600_60pa.hed VOS2000600_60pa.dat Directory structure and naming convention

7. VGMO.NET Vladimir Papitashvili papita@umich.edu Anshuman Saxena anshuman.saxena @tcs.com Valeriy Petrov vpetrov@engin. umich.edu Robert Clauer rclauer@umich.edu Natalia Papitashvili natasha@mail630. gsfc.nasa.gov April 23, 2004 Page 7 of 15 ICESTAR VGMO.NET - Architecture Unleashed Remote Site Info Format Info Conversion Pointer ftp.iki.rssi.ru--- ftp.abs.xyz.edu---. Remote Site Info Format Info Conversion Pointer ftp.dmi.dk1980- 2002 /pub/wdcc1/obsdata/1minval / YYYY/ ftp.ngdc. noaa.gov 1970- 2002 /STP/GEOMAGNETIC_DATA/ONE_ MINUTE_VALUES/YYYY/ …………………………………………………………………… Active Section Prospective Section Geo Magnetic Crawler (GeoMaC) LOOKUP TABLE A2F - Any to Flat File Conversion Module FFMN Flat File Manager INTERNET

8. VGMO.NET Vladimir Papitashvili papita@umich.edu Anshuman Saxena anshuman.saxena @tcs.com Valeriy Petrov vpetrov@engin. umich.edu Robert Clauer rclauer@umich.edu Natalia Papitashvili natasha@mail630. gsfc.nasa.gov April 23, 2004 Page 8 of 15 ICESTAR Two Implementations of VGMO.NET Web-Based Portal – available at http://maggy.engin.umich.edu/mist/vgmo.html  A secure, scalable, platform independent, and user-friendly software framework for remote access to VGMO.NET Flat File Manager  The Flat File Manager Client is written to the Java 2 platform that requires a Java Web Start (JNLP - Java Network Launching Protocol) Self-Populating Standalone Version - available for download from above Web site  An alternate standalone version to create, manage, and populate local geomagnetic databases from INTERNET; aims on building a geomagnetic GRID access

9. VGMO.NET Vladimir Papitashvili papita@umich.edu Anshuman Saxena anshuman.saxena @tcs.com Valeriy Petrov vpetrov@engin. umich.edu Robert Clauer rclauer@umich.edu Natalia Papitashvili natasha@mail630. gsfc.nasa.gov April 23, 2004 Page 9 of 15 ICESTAR VGMO.NET Highlights http://maggy.engin.umich.edu/mist/vgmo.html Remote (Client) Machine Requirements Java Runtime Environment (JRE), version 1.2.2 or later Java Web Start (available for Windows 98/ME/NT/2000/XP, Linux, and Solaris OE) The library and “Java thin client” for the FFMN Client Server Requirements Any standard Web server configured for JNLP ( Java Network Launching Protocol) Flat File Manager DLLs and Flat File Manager Server software Platform Independence FFMN Server can be deployed on a wide-variety of platforms (Linux, Solaris OE, Windows 98/ME/NT/2000/XP) and launched remotely from any platform Client Side Security and Notification of Application’s Origin The FFMN service provider signs the downloadable code to ensure that no other party can impersonate the application on the Web; thus, the VGMO framework provides flexibility without compromising security. The user is shown a dialog displaying the application's origin (based on the signer's certificate) before the application is launched; thereby, the user can make an informed decision whether to grant additional privileges to the downloaded code If the user trusts the FFMN service provider, he/she can choose to grant additional system privileges, such as a write access to a local disk

10. VGMO.NET Vladimir Papitashvili papita@umich.edu Anshuman Saxena anshuman.saxena @tcs.com Valeriy Petrov vpetrov@engin. umich.edu Robert Clauer rclauer@umich.edu Natalia Papitashvili natasha@mail630. gsfc.nasa.gov April 23, 2004 Page 10 of 15 ICESTAR Launching VGMO.NET http://maggy.engin.umich.edu/mist/vgmo.html  The very first initiation of FFMN is through a Web browser. As initiated, the remote machine is checked for necessary software (e.g., JRE, the Java Runtime Environment). If that software is not found, the user can choose an option of “One Click” installation or download various components manually and launch FFMN later. However, the “One Click” option requires least manual intervention and prepares the platform to launch FFMN remotely.  As the FFMN client software is downloaded from the Web server, it is launched locally via JNLP (Java Network Launch Protocol). Note that the downloaded application runs at the remote machine in a protective environment (“sandbox”).  The “Java thin client” opens a control connection (out-of band signaling) with the FFMN Server and instructs the server to run Flat File Manager locally but the output is posted at the remote machine. Later this control connection initiates FTP sessions on demand and allows users to download requested files.  Subsequent initiations of FFMN from the remote machine can be independent of a Web browser; the application can be launched through desktop shortcuts, making launching the Web-deployed application similar to launching a native application. The user is prompted for creating a desktop shortcut in Step (1).

11. VGMO.NET Vladimir Papitashvili papita@umich.edu Anshuman Saxena anshuman.saxena @tcs.com Valeriy Petrov vpetrov@engin. umich.edu Robert Clauer rclauer@umich.edu Natalia Papitashvili natasha@mail630. gsfc.nasa.gov April 23, 2004 Page 11 of 15 ICESTAR VGMO.NET at Work http://maggy.engin.umich.edu/mist/vgmo.html FFMN Main Menu allows the user to select up to three data sets (File), then do certain operations with selected data sets (Action) by setting Options The File item allows the user to open the server database files or to create a temporary data set for the selected geomagnetic stations (selected either by names or geographic location) If the selected data are found in the server’s database, then the FFMN Server retrieves requested data for the plotting (and possible uploading) to the remote, FFMN client machine In addition, if the “Search worldwide” box is checked, the FFMN Server will look for the selected data on a number of remote FTP sites (listed in the FFMN Lookup File); these data are then downloaded, converted to flat files, and added to the FFMN server database When new FTP sites with geomagnetic data are found, they can be easily linked through additions to the FFMN Lookup File

12. VGMO.NET Vladimir Papitashvili papita@umich.edu Anshuman Saxena anshuman.saxena @tcs.com Valeriy Petrov vpetrov@engin. umich.edu Robert Clauer rclauer@umich.edu Natalia Papitashvili natasha@mail630. gsfc.nasa.gov April 23, 2004 Page 12 of 15 ICESTAR VGMO.NET Actions http://maggy.engin.umich.edu/mist/vgmo.html Plot –a stack of magnetograms plotted in accordance with the changeable Options menu Download – save the selected dataset to a file (in various formats, including IAGA-2002) and then download this file to the remote machine via FTP. If there were a few opened files on the server, then all selected data will be combined into a single file Merge rows – merge two similar data sets with interlaced time intervals Filter – apply the low, high, or band- pass filter to the selected data Calculate – enter a formula to compute new physical quantity from the given columns in the opened data files (e.g., compute the total geomagnetic field intensity from three orthogonal components) Shift time – to change timing in one of the data sets for the plotting purposes (e.g., showing delays between data) FFMN Client shows all data available from the Server (that is, included in the temporary data set for the selected time interval) and then the user can Select All or mark (+) the data subset for Action

13. VGMO.NET Vladimir Papitashvili papita@umich.edu Anshuman Saxena anshuman.saxena @tcs.com Valeriy Petrov vpetrov@engin. umich.edu Robert Clauer rclauer@umich.edu Natalia Papitashvili natasha@mail630. gsfc.nasa.gov April 23, 2004 Page 13 of 15 ICESTAR VGMO.NET Search and Plot Example http://maggy.engin.umich.edu/mist/vgmo.html

14. VGMO.NET Vladimir Papitashvili papita@umich.edu Anshuman Saxena anshuman.saxena @tcs.com Valeriy Petrov vpetrov@engin. umich.edu Robert Clauer rclauer@umich.edu Natalia Papitashvili natasha@mail630. gsfc.nasa.gov April 23, 2004 Page 14 of 15 ICESTAR VGMO.NET: World Wide Web Search http://maggy.engin.umich.edu/mist/vgmo.html By default all the sites presented in the list are contacted for world wide search The user can drop some sites from the list by making appropriate selections Each site remains in one of the following states Not connected : Site has not yet been contacted Connecting : Synchronization with the site is in progress Completed : Synchronization with the site has been completed The list of matching stations found are listed against each site

15. VGMO.NET Vladimir Papitashvili papita@umich.edu Anshuman Saxena anshuman.saxena @tcs.com Valeriy Petrov vpetrov@engin. umich.edu Robert Clauer rclauer@umich.edu Natalia Papitashvili natasha@mail630. gsfc.nasa.gov April 23, 2004 Page 15 of 15 ICESTAR  Existing World Data Centers continue to serve the worldwide scientific community in providing free access to global geophysical databases  Recently many digital geomagnetic datasets have been placed on the Web, often in near-real time, but some of these data are not even submitted to any data center  In this study, we formulated a concept and developed a prototype of a Virtual Global Magnetic Observatory (VGMO) that uses a pre-set list of FTP-based geomagnetic data holders to retrieve requested data  Saving retrieved data locally over multiple requests, a VGMO user begins to build his/her own data sub-center, which does not need searching the Web if a new data interval is within a span of earlier downloaded data  At the same time, these self-sustained sub-centers become available to other VGMO users - this network of “GEOMAGstered” users establishes VGMO.NET where Web data-crawling becomes transparent to the users  However, more studies are needed to help identifying newly “Webbed” digital geomagnetic data – and Semantic Web is the most promising approach Summary