The Neutron Monitor Database Project. e-infrastructure. Report of the Rome Activity (January- June 2008)

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1 The Neutron Monitor Database Project e-infrastructure Report of the Rome Activity (January- June 2008) SVIRCO OBSERVATORY and TERRESTRIAL PHYSICS LABORATORY Via della Vasca Navale, Roma - Italy

2 CONTENT 1. SVIRCO Data: Status report SVIRCO server NM Data Inventory SVIRCO Data Reports min Data Recovery 2. Work for SVIRCO Data Delivery Preparation of the SVIRCO questionnaire for WP Meetings at the RomaTre Computing Center Preparation of the needed software for data transmission from the SVIRCO Observatory Server to the RomaTre Server Data file preparation with the requested NMDB format 3. Cosmic Ray Fluctuations: Status report for WP Inventory of past works Selection of two events for Kosice Meeting 4. Training & dissemination for WP INAF/UNIRomaTre Synergies for NMDB Concepts for PO site

3 1 - SVIRCO Data: Status report 1.1 -SVIRCO server NM Data Inventory The status of the neutron monitor data recorded by the Rome detector since July 1957 is reported in the following table: SVIRCO OBSERVATORY & TPL NM DATA INVENTORY ( ) ROME (ITALY) DEPUTY STAFF: Prof. M. PARISI TIME PERIOD DETECTOR MONTHLY DATA^ DAILY DATA^ Bi-hourly DATA^ Hourly DATA^ 5-min DATA 1-min DATA Jul Apr IGY May 1 Jul. 14, NM-64 Jul. 15 May 7, NM-64 May 8, 1969 Dec. 31, NM-64 Jan. 1, 1981 May 31, NM-64 Jun. 1, 1984 Dec. 31, NM-64 Jan. 1, 1988 May 20, NM-64 Possible recovery May 21, 1997 Jan. 6, NM-64 validated data (*) Jan. 7, 2002 Dec. 31, NM-64 validated data (*) Real-time data (*) Jan. 1, 2005 Dec. 31, NM-64 (*) validated data(*) Real-time data (*) ^ Normalized data to Jan.-Feb. 1997: 100% = counts/h (*) Dr. M. Storini project (IFSI-Roma) SVIRCO Data Reports In the following we list the Data Reports published and distributed over the years to the scientific community. These reports can be obtained also in an electronic format (pdf files). SVIRCO SERIES OF DATA REPORTS LPS-CNR/IFU-Roma Collaboration N. Iucci, G. Villoresi, N.L. Zangrilli, V. Ianni, F. Signoretti: Cosmic ray NM -64 neutron monitor data I - Rome, Italy, Jan.- Dec.1972, Laboratorio di Ricerca e Tecnologia per lo Studio del Plasma nello Spazio - CNR, Report LPS-74-13, Aprile 1974 G. Villoresi, N.L. Zangrilli, M. Parisi, M. Storini, A. Felici, F. Signoretti: Cosmic ray NM -64 neutron monitor data II - Rome, Italy, Jan.- Dec.1973, Laboratorio di Ricerca e Tecnologia per lo Studio del Plasma nello Spazio - CNR, Report LPS-75-09, April 1975

4 G. Villoresi, N.L. Zangrilli, M. Parisi, M. Storini, A. Felici, F. Signoretti: Cosmic ray NM -64 neutron monitor data III - Rome, Italy, Jan.- Dec.1974, Laboratorio di Ricerca e Tecnologia per lo Studio del Plasma nello Spazio - CNR, Report LPS-75-34, October 1975 G. Villoresi, N.L. Zangrilli, M. Parisi, M. Storini, A. Felici, F. Re, F. Signoretti: Cosmic ray NM -64 neutron monitor data IV - Rome, Italy, Jan.- Dec.1975, Laboratorio di Ricerca e Tecnologia per lo Studio del Plasma nello Spazio - CNR, Report LPS-76-30, November 1976 G. Villoresi, N.L. Zangrilli, M. Parisi, M. Storini, A. Felici, F. Re, F. Signoretti: Cosmic ray NM -64 neutron monitor data V - Rome, Italy, Jan.- Dec.1976, Laboratorio di Ricerca e Tecnologia per lo Studio del Plasma nello Spazio - CNR, Report LPS-78-08, September 1978 G. Villoresi, N.L. Zangrilli, A. Felici, F. Re, F. Signoretti: Cosmic ray NM -64 neutron monitor data VI - Rome, Italy, Jan.- Dec.1977, Laboratorio di Ricerca e Tecnologia per lo Studio del Plasma nello Spazio - CNR, Report LPS-79-2, January 1979 G. Villoresi, N.L. Zangrilli, A. Felici, F. Re, F. Signoretti: Cosmic ray NM -64 neutron monitor data VII - Rome, Italy, Jan.- Dec.1978, Laboratorio di Ricerca e Tecnologia per lo Studio del Plasma nello Spazio - CNR, Report LPS-79-4, March 1979 G. Villoresi, N.L. Zangrilli, A. Felici, F. Re, F. Signoretti: Cosmic ray NM-64 neutron monitor data VIII - Rome, Italy, Jan.- Dec.1979, Istituto di Ricerca e Tecnologia per lo Studio del Plasma nello Spazio - CNR, Report LPS-81-9, June 1981 IFSI-CNR/DFU-La Sapienza Collaboration N. Iucci, F. Re, F. Signoretti, C. Signorini, G. Villoresi, N.L. Zangrilli: Cosmic ray NM -64 neutron monitor data IX - Rome, Italy, Jan.- Dec.1980, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI-83-11, Novemer 1983 N. Iucci, F. Re, F. Signoretti, C. Signorini, G. Villoresi, N.L. Zangrilli: Cosmic ray NM -64 neutron monitor data X - Rome, Italy, Jan.- Dec.1981, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI-83-12, November 1983 N. Iucci, F. Re, F. Signoretti, C. Signorini, G. Villoresi, N.L. Zangrilli: Cosmic ray NM-64 neutron monitor data XI - Rome, Italy, Jan.- Dec.1982, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI-83-13, November1983 N. Iucci, F. Re, F. Signoretti, C. Signorini, G. Villoresi, N.L. Zangrilli: Cosmic ray NM -64 neutron monitor data XII - Rome, Italy, Jan.- Dec.1983, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI-85-6, May1985 N. Iucci, R. Buccellato, F. Re, F. Signoretti, C. Signorini, G. Villoresi, N.L. Zangrilli: Cosmic ray NM -64 neutron monitor data XIII - Rome, Italy, Jan.- Dec.1984, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI-85-13, October 1985 N. Iucci, R. Buccellato, F. Re, F. Signoretti, C. Signorini, G. Villoresi, N.L. Zangrilli: Cosmic ray NM -64 neutron monitor data XIV - Rome, Italy, Jan.- Dec.1985, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI-87-8, July 1987 N. Iucci, R. Buccellato, F. Re, F. Signoretti, C. Signorini, G. Villoresi, N.L. Zangrilli: Cosmic ray NM -64 neutron monitor data XV - Rome, Italy, Jan.- Dec.1986, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI-87-19, December 1987 N. Iucci, F. Re, F. Signoretti, C. Signorini, G. Villoresi, N.L. Zangrilli: Cosmic ray NM -64 neutron monitor data XVI - Rome, Italy, Jan.- Dec.1987, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI-88-21, December 1988 N. Iucci, F. Re, F. Signoretti, C. Signorini, G. Villoresi, N.L. Zangrilli: Cosmic ray NM -64 neutron monitor data XVII - Rome, Italy, Jan.- Dec.1988, Dipartimento di Fisica Università di Roma La Sapienza, Report n. 945, 19 December 1989 N. Iucci, F. Re, F. Signoretti, C. Signorini, G. Villoresi, N.L. Zangrilli: Cosmic ray NM -64 neutron monitor data XVIII - Rome, Italy, Jan.- Dec.1989, Dipartimento di Fisica Università di Roma La Sapienza, Report n. 972, 26 December 1991 N. Iucci, F. Re, F. Signoretti, C. Signorini, G. Villoresi, N.L. Zangrilli: Cosmic ray NM -64 neutron monitor data XIX - Rome, Italy, Jan.- Dec.1990, Dipartimento di Fisica Università di Roma La Sapienza, Report n. 989, 3 December 1991 N. Iucci, F. Re, F. Signoretti, G. Villoresi, N.L. Zangrilli: Cosmic ray NM -64 neutron monitor data XX - Rome, Italy, Jan.- Dec.1991, Dipartimento di Fisica Università di Roma La Sapienza, Report n. 1004, 26 November 1992 N. Iucci, F. Re, F. Signoretti, G. Villoresi, N.L. Zangrilli: Cosmic ray NM -64 neutron monitor data XXI - Rome, Italy, Jan.- Dec.1992, Dipartimento di Fisica Università di Roma La Sapienza, Report n. 1020, 27 September 1993 N. Iucci, F. Re, F. Signoretti, G. Villoresi, N.L. Zangrilli: Cosmic ray NM -64 neutron monitor data XXII - Rome, Italy, Jan.- Dec.1993, Dipartimento di Fisica Università di Roma La Sapienza, Report n. 1044, 14 December 1994

5 N. Iucci, F. Re, F. Signoretti, G. Villoresi, N.L. Zangrilli: Cosmic ray NM -64 neutron monitor data XXIII - Rome, Italy,Jan.- Dec.1994, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI-96-2, January 1996 N. Iucci, F. Re, F. Signoretti, G. Villoresi, N.L. Zangrilli: Cosmic ray NM -64 neutron monitor data XXIV - Rome, Italy,Jan.- Dec.1995, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI-96-3, January 1996 IFSI-CNR/DFU-Roma Tre Collaboration F. Signoretti, F. Re: SVIRCO 2002: January-April Prompt Report, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , May 2002 F. Signoretti, F. Re, M. Storini, P. Diego, M. Parisi: SVIRCO 2001 DATA: January to June2001, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , June 2002 F. Signoretti, F. Re, M. Storini, P. Diego, M. Parisi: SVIRCO 2001 DATA: July to December 2001, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , June 2002 F. Signoretti, F. Re: SVIRCO 2002: May-August Prompt Report, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , September 2002 F. Signoretti, F. Re: SVIRCO 2002: September-December Prompt Report, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , February 2003 F. Signoretti, F. Re, M. Storini, P. Diego, M. Parisi: SVIRCO 2002 DATA: January to June 2002, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , February 2003 F. Signoretti, F. Re: SVIRCO Prompt Report: January 2003, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , February 2003 F. Signoretti, F. Re, M. Storini, P. Diego, M. Parisi: SVIRCO 2002 DATA: July to December 2002, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , March 2003 F. Signoretti, F. Re: SVIRCO Prompt Report: February 2003, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , March 2003 F. Signoretti, F. Re: SVIRCO Prompt Report: March 2003, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , April 2003 F. Signoretti, F. Re: SVIRCO Prompt Report: April 2003, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , May 2003 F. Signoretti, F. Re: SVIRCO Prompt Report: May 2003, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , June 2003 F. Signoretti, F. Re: SVIRCO Prompt Report: June 2003, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , July 2003 F. Signoretti, F. Re: SVIRCO Prompt Report: July 2003, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , August 2003 F. Signoretti, F. Re: SVIRCO Prompt Report: August 2003, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , September 2003 F. Signoretti, F. Re: SVIRCO Prompt Report: September 2003, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , October 2003 F. Signoretti, F. Re: SVIRCO Prompt Report: October 2003, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , November 2003 F. Signoretti, F. Re: SVIRCO Prompt Report: November 2003, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , December 2003 F. Signoretti, F. Re: SVIRCO Prompt Report: December 2003, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , January 2004 F. Signoretti, F. Re: SVIRCO Prompt Report: January 2004, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , February 2004 F. Signoretti, F. Re: SVIRCO Prompt Report: February 2004, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , March 2003 F. Signoretti, F. Re: SVIRCO Prompt Report: March 2004, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , April 2004 F. Signoretti, F. Re: SVIRCO Prompt Report: April 2004, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , May 2004

6 F. Signoretti, F. Re: SVIRCO Prompt Report: May 2004, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , June 2004 F. Signoretti, F. Re: SVIRCO Prompt Report: June 2004, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , July 2004 F. Signoretti, F. Re: SVIRCO Prompt Report: July 2004, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , August 2004 F. Signoretti, F. Re: SVIRCO Prompt Report: August 2004, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , September 2004 F. Signoretti, F. Re: SVIRCO Prompt Report: September 2004, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , November 2004 F. Signoretti, F. Re: SVIRCO Prompt Report: October 2004, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , November 2004 F. Signoretti, F. Re: SVIRCO Prompt Report: November 2004, Istituto di Fisica dello Spazio Interplanetario - CNR, Report IFSI , December 2004 F. Signoretti, F. Re: SVIRCO Prompt Report: December 2004, Istituto di Fis ica dello Spazio Interplanetario - CNR, Report IFSI , January 2005 IFSI-INAF/DFU-Roma Tre Collaboration F. Signoretti, M. Storini: SVIRCO Prompt Report: January 2005, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , February 2005 F. Signoretti, F. Re: SVIRCO Prompt Report: February 2005, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , March 2005 F. Signoretti, F. Re: SVIRCO Prompt Report: March 2005, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , April 2005 F. Signoretti, F. Re: SVIRCO Prompt Report: April 2005, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , May 2005 F. Signoretti, F. Re, M. Storini, M. Parisi: SVIRCO DATA: January to December 2003, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , May 2005 F. Signoretti, F. Re, M. Storini, M. Parisi: SVIRCO DATA: January to December 2004, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , May 2005 F. Signoretti, F. Re: SVIRCO Prompt Report: May 2005, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , June 2005 F. Signoretti, F. Re: SVIRCO Prompt Report: June 2005, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , July 2005 F. Signoretti, F. Re: SVIRCO Prompt Report: July 2005, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , August 2005 F. Signoretti, F. Re: SVIRCO Prompt Report: August 2005, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , September 2005 F. Signoretti, F. Re, M. Storini, M. Parisi: SVIRCO DATA: January to December 2000, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , September 2005 F. Signoretti, F. Re, M. Storini, M. Parisi: SVIRCO DATA: January to December 1999, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , October 2005 F. Signoretti, F. Re: SVIRCO Prompt Report: September 2005, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , October 2005 F. Signoretti, F. Re: SVIRCO Prompt Report: October 2005, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , November 2005 F. Signoretti, F. Re: SVIRCO Prompt Report: November 2005, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , December 2005 F. Signoretti, F. Re, M. Storini, M. Parisi: SVIRCO DATA: January to December 1998, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , December 2005 F. Signoretti, F. Re: SVIRCO Prompt Report: December 2005, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , January 2006

7 F. Signoretti, F. Re, M. Storini, M. Parisi: SVIRCO DATA: January to December 2005, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , February 2006 F. Signoretti, F. Re: SVIRCO Prompt Report: January 2006, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , March 2006 F. Signoretti, F. Re: SVIRCO Prompt Report: February 2006, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , March 2006 F. Signoretti, F. Re: SVIRCO Prompt Report: March 2006, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , May 2006 F. Signoretti, F. Re: SVIRCO Prompt Report: April 2006, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , May 2006 F. Signoretti, F. Re: SVIRCO Prompt Report: May 2006, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , June 2006 F. Signoretti, F. Re: SVIRCO Prompt Report: June 2006, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , July 2006 F. Signoretti, F. Re: SVIRCO Prompt Report: July 2006, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , August 2006 F. Signoretti, F. Re: SVIRCO Prompt Report: August 2006, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , September 2006 F. Signoretti, F. Re: SVIRCO Prompt Report: September 2006, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , October 2006 F. Signoretti, F. Re: SVIRCO Prompt Report: October 2006, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , November 2006 F. Signoretti, F. Re: SVIRCO Prompt Report: November 2006, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , December 2006 F. Signoretti, F. Re, M. Storini: SVIRCO Prompt Report: December 2006, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , January 2007 F. Signoretti, F. Re: SVIRCO Prompt Report: January 2007, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , February 2007 F. Signoretti, F. Re, M. Storini, M. Parisi: SVIRCO DATA: 21 May - 31 December 1997, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , February 2007 F. Signoretti, F. Re: SVIRCO Prompt Report: February 2007, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , March 2007 F. Signoretti, F. Re, M. Storini, M. Parisi: SVIRCO DATA: January to December 2006, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , March 2007 F. Signoretti, F. Re: SVIRCO Prompt Report: March 2007, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , April 2007 F. Signoretti, F. Re: SVIRCO Prompt Report: April 2007, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , May 2007 F. Signoretti, F. Re: SVIRCO Prompt Report: May 2007, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , June 2007 F. Signoretti, F. Re: SVIRCO Prompt Report: June 2007, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , July 2007 F. Signoretti, F. Re: SVIRCO Prompt Report: July 2007, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , August 2007 F. Signoretti, F. Re: SVIRCO Prompt Report: August 2007, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , September 2007 F. Signoretti, F. Re: SVIRCO Prompt Report: September 2007, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , October 2007 F. Signoretti, F. Re: SVIRCO Prompt Report: October 2007, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , November 2007 F. Signoretti, F. Re: SVIRCO Prompt Report: November 2007, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , December 2007

8 F. Signoretti, F. Re: SVIRCO Prompt Report: December 2007, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , January 2008 F. Signoretti, F. Re: SVIRCO Prompt Report: January 2008, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , February 2008 F. Signoretti, F. Re, M. Storini, M. Parisi: SVIRCO DATA: January to December 2007, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , February 2008 F. Signoretti, F. Re: SVIRCO Prompt Report: February 2008, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , March 2008 F. Signoretti, F. Re: SVIRCO Prompt Report: March 2008, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , April 2008 F. Signoretti, F. Re: SVIRCO Prompt Report: April 2008, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , May 2008 F. Signoretti, F. Re: SVIRCO Prompt Report: May 2008, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , June 2008 F. Signoretti, F. Re: SVIRCO 5-minute Data Report: 21 May - 31 December 1997, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , June 2008 F. Signoretti, F. Re: SVIRCO 5-minute Data Report: January December 1998, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , June 2008 F. Signoretti, F. Re: SVIRCO 5-minute Data Report: January December 1999, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , June 2008 F. Signoretti, F. Re: SVIRCO 5-minute Data Report: January December 2000, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , June 2008 F. Signoretti, F. Re: SVIRCO 5-minute Data Report: January December 2001, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , June 2008 F. Signoretti, F. Re: SVIRCO 5-minute Data Report: January December 2002, Istituto di Fisica dello Spazio Interplanetario - INAF, Report IFSI , June min Data Recovery Pressure uncorrected neutron monitor data and pressure values recorded every 5 minutes from January 1, 1988 to May 20, 1997 can be recovered to produce validated pressurecorrected data with a 2-month person work. This task will be performed during September- October NOTE: 5-min data used for the same period in the past were not validated because the final 5-min data from May 21, 1997 to the present were produced only recently (see data report list).

9 2 - Work for SVIRCO Data Delivery Preparation of the SVIRCO questionnaire for WP3 As required by WP3 the online questionnaire prepared by NKUA was filled. As can be seen in the SVIRCO NM DATA INVENTORY, Rome produces 1 min data (updated every 1 min) since January 2002 (real time data). Moreover, pressure corrected 5-min data (updated every 5 min) are displayed in the SVIRCO server for the prompt check of the scientific community. Here the filled questionnaire: 1 Name of the station : Full ROME/SVIRCO 2 Short SVIRCO 3 Address 4 Head organization 5 Address Università degli Studi Roma Tre Dipartimento di Fisica Via della Vasca Navale Rome, Italy Università degli Studi Roma Tre Dipartimento di Fisica + INAF/IFSI-Roma 6 Principal Investigator Mario Parisi (for NMDB) 7 - address parisi@fis.uniroma3.it 8 Contact Person Mario Parisi 9 address parisi@fis.uniroma3.it 10 Responsible for technical support Fabrizio Signoretti Dip. Fisica-Univ. Roma Tre: Via della Vasca Navale, Rome, Italy + IFSI-Roma: Via del Fosso del Cavaliere, Roma, Italy 11 address fabrizio.signoretti@ifsi-roma.inaf.it 12 Start Date (For this station version) 21 May End Date (For this station version) Running at the present time 14 Time Period of station Operation, if multiple exist (first (1), second (2) etc 15 Other General Information of the Station 16 Geographic Coordinates of the station (lat) 3rd From July 1957 to April 1966 (IGY) and from May 1966 to 20 May 1997, the ROME/SVIRCO Station (now Observatory) performed uninterrupted measurements at the Physics Department G.Marconi of La Sapienza University N 17 Geographic Coordinates of the station E

10 (lon) 18 Altitude (m) Sea level 19 Geomagnetic cut-off Rigidity 6.27 GV (1995) 20 Average Counting Rate Per Minute 9250 cts/min (Jan./Feb. 1997) 21 Standard (Mean) atmospheric pressure hpa 22 Barometric coefficient 0.70 %/hpa 23 Constant barometric coefficient used at your station 24 (If Else, Please Specify) 25 Thickness of the floor above the NM (in gr/cm^3) Yes 26 Material of the roof Tile roof 27 Type of the used proportional counters BP28 28 (If Else, Please Specify) 29 Number of proportional counters 20 (from Jan. 2005) & 17 (before 2005) Are thereobstacles around the detector (house, rock...)? Material of the moderator (type and thickness) Material of the reflector (type and thickness) Arrangement and grouping of the detectors 34 Other Station Information Specifications of pressure sensor.resolution Specifications of pressure sensor.stability Specifications of pressure sensor.temperature coefficient Small buildings Polyethilene 2.0 cm Polyethilene 7.5 cm From Jan. 2005: 5 sections: three 3-counter, one 5- counter and one 6-counter units. The neutron monitor is housed in a reserved building provided with a double air-conditioning system. The inner temperature is permanently restrained in a range of C, meanwhile the relative hum Up to 0.01 hpa see below see below 38 Type of preamplifier Charge amplifier 39 Dead time of the preamplifier 25 µs 40 UPS use on your system (applied on parts or on the whole system) 41 Hours on battery that your UPS supports 42 Special electronic device for supporting the station designed by you 43 Other Station Electronics Information No Amplifier/discriminator equipped with spectrum stabilizer The atmospheric pressure measurements are carried out by means of not less than three barometers

11 44 Type of acquisition system Real-time 45 (If Else - please describe) Operating system of platform of the acquisition system (If Else - please describe - please describe -indicate the version of operating system) 48 Processor 49 Hard Disk 50 RAM 51 Data resolution 1 min Windows Data update rate One minute 53 Data quality checking in real time Yes 54 By which way Ratios of neutron monitor units 55 Clock Type Electronic 56 Programming language used for software development on the acquisition system ELSE 57 (If Else, Please Specify) HP/Agilent VEE Pro plus MatLab Parts of the acquisition system which have been designed and developed by your team (please describe part) Parts of the acquisition system which have been designed and developed by other NM team(please describe part) Parts of the acquisition system which have been bought by companies (please describe part and manufacturer) Registration system connection properties. Description: Bandwidth Registration system connection properties. Description: Type 63 Time availability Time-correction within the acquisition system: In which way Time wasted for time stamp correction taken into account (Yes, No Specify) Definition of the time interval (the start, the end of time interval, something else - specify) Registration of relevant parameters by station acquisition system(temperature, humidity and so on A second whole acquisition system completed with a multiplicity meter VXI Serie B HP Acquisition system 10Mbps Ethernet 67 Restarting periodically the registration Automatic The end of time interval Temperature, humidity High and low voltages

12 system. By which way? Need of an improved restarting system elaborated in Athens center(description is applied)? Are your acquisition system software developed by your team free-provided to other stations Are your acquisition system hardware developed by your team given to other stations(free or pay)? Are your detector temperature controlled? (e.g. By an air-condition) Other Registration System Information or needs Is there any local server for providing data to internet? How do you provide your data to internet: 74 (If Else, Please Specify) yes Free yes Yes Else http server (At present, fine data are available on e- mail or FTP 75 Ty! pe of WEB server: Linux (apache, mysql, PHP) 76 If Else, Please Describe (please indicate the version of operating system) 77 Full access rights to your server No 78 If Else, Please describe Hardware characteristics of the server system:processor Hardware characteristics of the server system:hard Disk Hardware characteristics of the server system:ram Possible compliance of your station to NMDB requirements without help from other teams.if yes, describe your time plan to succeed it. 83 Clock Type 84 Pr ogramming language used for software development on your server system 85 (If Else or more, Please Specify) Server Internet connection properties.description: Bandwidth Server Internet connection properties.description: Kind Yes. At the present, we are working with the responsible of local server of our Department for preparing the best connection for sending the Rome data to the BIRA server. Our time plan should be completed within one-two months.

13 Time availability (frequency of data 88 sending) 89 Are your Server system software free to other stations 90 Is there any firewall policy? 91 Other Local Server Information or needs Meetings at the Roma Tre Computing Center Several meetings were performed to organize the NM data transfer from the SVIRCO Server to the Roma Tre Computing Center, where a dedicated PC will be used for NMDB project. It was decided that the fast delivery of pressure corrected data with 1-min resolution can be done by a FTP transfer command inserted in the routine of the real-time data correction. 3. Cosmic Ray Fluctuations: Status report for WP5 According to the timing of the work package, it has been realized an inventory of recent and past papers on the subject, necessary to understand the state of art and how to improve the accuracy of results by using different types of analyses. Cosmic ray fluctuations will be studied on different time scales by using reliable datasets coming from the NMDB project. During the Kosice Meeting, it will be discussed with the other partners of the topic (Kosice, Almaty) the different steps to be faced to reach the proposed goals in the framework of NMDB project. One of the aims is, for example, to obtain information on short time scale about travelling interplanetary perturbations, their associated IMF inhomogeneities and then their possible effects on the Earth s environment Inventory of recent and past papers A.V. Grigoryev,,S.A. Starodubtsev,,V.G. Grigoryev, I.G. Usoskin, K. Mursula, Fluctuations of cosmic rays and IMF in the vicinity of interplanetary shocks, Advances in Space Research, 41, , S.A. Starodubtsev, I.G. Usoskin, A.V. Grigoryev, K. Mursula, Long-Term Modulation of the Cosmic Ray Fluctuation Spectrum: Spacecraft Measurements, 29th International Cosmic Ray Conference, Pune, 2, , S. Starodubtsev, and I. Usoskin, Galactic Cosmic Ray Fluctuations: Long-term Modulation of Power Spectrum, 28th International Cosmic Ray Conference, pp , A. Wawrzynczak and M.V. Alania, Fluctuations of the interplanetary magnetic field during the Forbush effects of galactic cosmic rays, Vol. 36, ACTA PHYSICA POLONICA B No 5, K. Kudela, M. Storini, M. Hofer, and A. Belov, Cosmic Rays In Relation To Space Weather, Space Science Reviews 93, , 2000., 2000, Kluwer Academic Publishers. Printed in the Netherlands.

14 J. W. Bieber and P. Evenson, CME Geometry in Relation to Cosmic Ray Anisotropy, Geophysical Research Letters, vol. 25, no.15, pages , August 1, A. Chilingarian for the ASEC team, Monitoring and Forecasting of the Geomagnetic and Radiation Storms During the 23rd Solar Cycle. Aragats Regional Space Weather Center, Adv. Space Res., 31, , H. Mavromichalaki,V. Yanke, L. Dorman, N. Iucci, A. Chilingaryan, O. Kryakunova, Neutron Monitor Network in Real Time and Space Weather, 2004 Kluwer Academic Publishers..Printed in the Netherlands, I.A.Daglis (ed.),effects of Space Weather on Technology Infrastructure, K. Kudela 1,J.Rybák 2, A. Antalová 1 And M. Storini, Time Evolution Of Low-Frequency Periodicities in Cosmic Ray Intensity, Solar Physics 205: , K. Kudela, M. Storini, Direct and indirect relations of cosmic rays to Space Weather, Proc. SOLSPA: The Second Solar Cycle and Space Weather Euroconference, Vico Equense, Italy, September 2001 (ESA SP-477, February 2002). Karel Kudela, Bingsen Xue, Guiming Le, Juan Miao, Gabriela Andejkova, Geomagnetic activity onset prediction: Problems with possible signatures in cosmic rays, Proc. ISCS 2003 Symposium, Solar Variability as Input to the Earth s Environment, Tatranska Lomnica, Slovakia, June 2003 (ESA SP-535, September 2003). K. Kudela and R. Langer, On the index of cosmic ray fluctuations at neutron monitor energies, Contrib. Astron. Obs. Skalnaté Pleso, 25, 5-12, L. I. Dorman, Space weather and dangerous phenomena on the Earth: principles of great geomagnetic storms forecasting by online cosmic ray data, Annales Geophysicae, 23: , L. I. Dorman, Cosmic rays and space weather effects: methods of forecasting, Solar Extreme Events of 2007:Fundamental Science and Applied Aspects, September 2007, International Symposium Athens, Greece. l. Dorman, L. Pustil nik, A. Sternlieb, I. Zukerman, Using ground-level cosmic ray observations for automatically generating prediction of hazardous energetic particle levels, Adv. Space Res-, vol. 31, No. 4, pp , A. Belov, L. Baisultanova, E. Eroshenko, H. Mavromichalaki, V. Yanke, V. Pchelkin, C. Plainaki,and G. Mariatos, Magnetospheric effects in cosmic rays during the unique magnetic storm on November 2003, Journal Of Geophysical Research, Vol. 110, A09S20, Doi: /2005ja011067, 2005 N. Gopalswamy, A. Lara, P, K. Manoharan, R.A. Howard, An empirical model to predict the 1 AU arrival of interplanetary shocks, Adv. Space Res-, vol. 36, pp , L. F. Burlaga, N. F Ness, M. H. Acu na, Y.-M. Wang, N. R. Sheeley Jr., C. Wang, and J. D. Richardson, Global structure and dynamics of large-scale fluctuations in the solar wind: Voyager 2 observations during 2005 and 2006, Journal Of Geophysical Research, Vol. 113, A02104, doi: /2007ja012796, 2008 A. H. Luttrell and A. K. Richter, A Study of MHD Fluctuations Upstream and Downstream, of Quasi- Parallel Interplanetary Shocks, Journal Of Geophysical Research, Vol. 92, No. A3, Pages , March 1, 1987

15 J. Owens, Cosmic Ray Scintillations General Theory of Interplanetary Scintillations, Journal of Geophysical Research, Vol. 92, No. A3, Pages , March 1, L.I. Dorman and I.Ya. Libin, Cosmic ray scintillations and dynamic processes in space, Space Science Reviews, , Selection of two events for Kosice Meeting Two events occurred on September and July 2005 were selected for the Kosice Meeting. The calculation is based on the use of the 5 minute pressure-corrected data of NMs from the NMDB network, at high latitude and low latitude with high statistics, as well as IMF and solar wind data (ACE), geomagnetic (Kp, ap, Dst) indices and solar data. The final output of this analysis should be information on the changes of the interplanetary medium conditions before and during the interplanetary disturbances. In particular, for the September 2005 event (preceded by days of low solar activity) the active region AR 10808, rotating from the Eastern limb to the solar central meridian, gave origin to successive coronal mass ejections affecting the interplanetary medium.

16 4. Training & dissemination for WP6 4.1 INAF/UNIRomaTre Synergies for NMDB The first local open doors of the SVIRCO Observatory for the current year was performed on February 18, 2008 for students of the Italian high schools. It was organized as a stage of Astronomy and included Cosmic Rays, Space Weather and the Nucleonic component detection by means of neutron monitors. Follows the program: (images of Parisi presentation are in )

17 4.2 Concepts for PO site An high number of Web sites provide, for users with different levels of knownoledge, background information on basic concepts in solar and heliospheric physics, cosmic rays, magnetospheric, terrestrial physics, climate and space wheater. In this contest, the main concepts to organize a PO site in relation to our project, should be based on: - Importance of the neutron monitor measurements and the collaborative efforts among neutron monitor stations; - Underlining of past historical collaboration (IGY, IQSY) and its results obtained in cosmic ray physics; - Identification of key issue for Space Wheater and its effect in the Earth s environment and human activity; - Relevance of know-how transfer from the single cosmic ray station to the NMDB project; - Importance of forecast/prediction work for the maximum phase of the next solar activity cycle N. 24. These topics had to be adapted for students, young researchers, public community involving experts to develop outreach programes, training courses and dissemination activity. It is important that this outreach activity should focus on developing partnership between existing European programmes to broaden its visibility and impact. Proposed organization of the Web site (Items+subitems) (Suggestions and comments are reported for each Item) Home + What is a neutron monitor? - Neutron monitors are ground-based detectors for cosmic ray measurements. Cosmic rays are highly energetic charged particles (predominantly protons, together with heavier nuclei of atoms, but also electrons and gamma rays) originating in the galaxy and traveling through interstellar space. They have to propagate through the interplanetary magnetic field that is frozen into the solar wind, and the Earth s magnetic field before they arrive at the Earth s atmosphere. Due to collisions with nuclei of atmospheric atoms, showers of secondary particles are produced. The nuclear active components of the secondaries are detected by a neutron monitor. -The counting rate of a neutron monitor is, therefore, a measure of the intensity of cosmic rays arriving at a measurement site (it depends on latitude, longitude and elevation). An optimal distribution of neutron monitors across the Earth s surface is required to derive the time-dependent directionality and intensity spectrum of cosmic rays within the energy range of detection on Earth. By using data of the great instrument (the world-wide network of detectors + geomagnetic field measurements), together with those of solar wind, interplanetary magnetic field and solar atmosphere, it is possible to study all aspects of galactic cosmic ray intensity variations and the solar cosmic rays propagation in the heliosphere. - Since IGY (1957), continuous measurements of the cosmic ray secondary component in the terrestrial atmosphere, recorded by neutron monitors, provide a continuous monitoring

18 of cosmic ray primary energy spectrum in an interval of rigidity (~ GV) and in different directions of particle arrival. + History: IGY IQSY IHY, past collaborations since Articles, memories, photographs and all material of historical significance. - Importance of large international collaborations among cosmic ray groups and Institutions. NMDB Project + Objectives An e-infrastructure project fosters a coordinated approach to the deployment of digital resources for the scientific community, supporting data storage, archiving, access, interpretation, interoperability and joint research activity. - The central objective of our project is the deployment of a digital repository with cosmic ray data that will be a useful tool for a broad field of scientific communities to promote cosmic ray research and its applications (space weather). To achieve this objective the existing data archives of continuous neutron monitor measurements over many years have to be pooled and a real-time database has to be developed that collects observational data in the highest time resolution from as many European neutron monitor stations as possible. - Activities of the WP6 work package: The principal objective of the present project, i.e. the establishment of easy access for a broad community to the data of neutron monitors, can only be successful if young researchers and non-specialised users can understand neutron monitor data. This requires training on fundamental aspects of cosmic rays and neutron monitors, on the impact of cosmic rays on the Earth, and on the use of the tools for data access that the present project will develop. We will develop a web-based system of training courses and public outreach activities, including user-expert interaction, in order to enable students, researchers and the general public to learn the basic principles relevant to cosmic rays and their effects on technology and human activity. Simultaneously we need a classical training course for students and young researchers to further a direct communication and interaction with experienced scientists and to intensify scientific cooperation in the field relevant to the database.

19 This can be realized on-line in the website and also organizing visits and open days in each station, providing dissemination activities, relevant for European Commission, including multimedia material (posters, press release and publications). + Neutron monitor network: importance - The neutron monitor network is one of the first infrastructure created in the IGY period which has continuously registered cosmic ray measurements and disseminated data to the scientific community. Data from neutron monitor network can be used to derive the latitude curves of the nucleonic intensity at different times. By using right coupling functions between cosmic ray component in the atmosphere and primaries of cosmic rays, the cosmic ray rigidity spectrum in the interval 2-15 GV are obtained. - Moreover, an other important aspect of the neutron monitor network is that it is a multidirectional instrument taking into account different asymptotic cone of acceptance of the stations. This allows computation of anisotropies, pitch angle distribution and the possibility to identify precursors of a cosmic ray event. - The NMDB project realize an upgrade of connection of online real data with high time resolution (e-infrastructures) in order to improve an unique structure to study solar cosmic ray modulation and effect on Earth s environment and possible relative effects generated by solar activity. +Workpackages - List, strategy and description Importance of a close cooperation to create an on-line database. Underline the architectural design of database to unify data acquisition and exploitation. +-Metadata General information of all stations as reported in the questionnaire prepared by NKUA- Athens. Link to single station sites. Space physics: Tutorials (online for high school students and young researchers) + Sun, heliosphere + Cosmic rays (solar and galactic) + Solar wind, interplanetary magnetic field and interaction with magnetosphere and Earth s environment +Gallery/Image/movies +Links +Languages +Ask an expert The tutorial lectures have to explain the complex study of Solar-Terrestrial Relationships with the aim to clarify solar origin and propagation into heliosphere of interplanetary perturbations influencing cosmic ray modulation and terrestrial environment and to define possibly model of forecast. In particular: - variations of galactic cosmic rays on different time scale and at different energies; relation with solar activity sources and interplanetary parameters.

20 - characterization of different types of perturbation in interplanetary space (high/low speed streams, shocks, flare ejecta, magnetic clouds) and connection with cosmic ray isotropic variation and anisotropy; - emission and propagation of energetic particles (SEP) recorded by satellite/spacecraft (GOES/ACE) and to the ground (GLE); - interaction of solar wind and magnetosphere. For each type of perturbation, correlation between interplanetary parameters with geomagnetic activity indices for studying different conditions forecasting intense geomagnetic storms and substorms; - available information on characteristics of a CME (speed, size, morphology, central location), recorded by coronograph LASCO on SOHO, also by STEREO spacecrafts and in the UV and soft-x on SOHO and Yohkoh; information on flares (for instance, the flares associated with CMEs are of long duration and also have associated meter wavelength Type II and, particularly, Type IV radio burst). - Space Weather and cosmic rays + Decision of items for tutorial lectures or master classes. + Decision for items to be developed at different levels of knowledge: students of different degrees, young researchers, experts (lessons, exercises, films, electronic books ). It will be useful also a selection of recommended books for users, divided by difficult levels (for high levels, see these examples: - Dorman, Lev I., Cosmic rays in the Earth s Atmosphere and Underground, Series: Astrophysics and Space Science Library, Vol. 303, 2004, XXXII, 862 p., Hardcover, ISBN: Dorman, Lev I., Cosmic ray interactions, Propagation, and Acceleration in Space Plasma, Series: Astrophysics and Space Science Library, Vol. 339, 2006, XXXIII, 847 p., Hardcover, ISBN: Bieber J.W., E. Eroshenko, P. Evenson, E.O. Flueckiger and R. Kallenback (Eds), Cosmic Rays and Earth, Proceedings of an ISSI Workshop, Bern, Swizerland, Kluwer Academic Publisher, SSSI 19, Reprinted from Space Science Reviews, Vol.93,Nos. 1-2, ) Possible topics to be developed: + What is space weather? + What is pace climate? + Hazard + Effects of cosmic rays on biological bodies (e.g. human health, crew hazard, ) + Effects of cosmic rays in the terrestrial atmosphere (e.g. ionization, PCA events, ) + Effects of cosmic rays on technological objects (e.g. PC performance, control system disruption, ) + Need of nowcast systems and their applications. + Need of forecast systems and.their applications. + Organization of images from ground-base and space connected with NMDB service. + A specific glossary for NMDB project + Selection of useful outside links

21 (e.g. other list of website taking into account of the list extensively prepared by NKUA- Athens: (per esperti) of course they are only examples). - Research/services/disseminations + Decision for the web site update with the obtained results during the project; + Preparation of reader files for users of available applications on line (ask users if difficulties were found after the running work: with a command?); + Development of Dissemination Systems for Alerts to the interested users. - Data repositories/archive use + Preparation of web pages for young training (e.g. data display, correlations, parameter evaluations, Stormer cutofff, ). - News & events General and specific information (e.g. events, seminars, conferences, open doors at the cosmic ray stations),

22 Other Web sites: pdf (Cosmic ray: an overview) (Basic, Cosmic rays, Sun, Space Weather)