Full Name
Gaya-Piqué, Luis R.
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Results 1-10 of 10 (Search time: 0.01 seconds).

Issue DateTitleAuthor(s)
12013Antarctic geomagnetic reference model updated to 2010 and provisionally to 2012Tozzi, R.* ; De Santis, A.* ; Gaya-Piqué, L.-R.* 
223-Mar-2006Deep seafloor magnetic observations under GEOSTAR projectDe Santis, A.* ; Di Mauro, D.* ; Cafarella, L.* ; D’Anna, R.* ; Gaya-Piqué, L. R.* ; Palangio, P.* ; Romeo, G.* ; Tozzi, R.* 
3Feb-2009An example of operation for a partly manned Antarctic geomagnetic observatory and the development of a radio link for data transmissionTorta, J. M.* ; Marsal, S.* ; Riddick, J. C.* ; Vilella, C.* ; Altadill, D.* ; Blanch, E.* ; Cid, O.* ; Curto, J. J.* ; De Santis, A.* ; Gaya-Piqué, L. R.* ; Mauricio, J.* ; Pijoan, J. L.* ; Solé, J. G.* ; Ugalde, A.* 
42006A GEOMAGNETIC REFERENCE MODEL FOR ALBANIA, SOUTH-EAST ITALY AND THE IONIAN SEA FROM 1990 TO 2005 WITH PREDICTION TO 2008.Qamili, E. ; De Santis, A. ; Duka, B. ; Dominici, G. ; Bushati, S. ; Cafarella, L. ; Miconi, M. ; Gaya-Pique, L. 
52004A geomagnetic reference model for Albania, Southern Italy and the Ionian Sea from 1990 to 2005Duka, B.* ; Gaya-Piqué, L. R.* ; De Santis, A.* ; Bushati, S.* ; Chiappini, M.* ; Dominici, G.* 
62004Information content and K-entropy of the present geomagnetic fieldDe Santis, A.* ; Tozzi, R.* ; Gaya-Piqué, L.* 
72003ITalian Geomagnetic Reference Field (ITGRF): update for 2000 and secular variation model up to 2005 by autoregressive forecastingDe Santis, A.* ; Gaya-Piqué, L.* ; Dominici, G.* ; Meloni, A.* ; Torta, J. M.* ; Tozzi, R.* 
8Apr-1999A new geomagnetic observatory at Livingston Island (South Shetland Islands): Implications for future regional magnetic surveysTorta, J. M.* ; Gaya-Piqué, L. R.* ; Sole, J. G.* ; Bianco, I.* ; Garcia, A.* 
92006New model alternatives for improving the representation of the core magnetic field of AntarcticaGaya-Piqué, L. R.* ; Ravat, D.* ; De Santis, A.* ; Torta, J. M.* 
102010Two geomagnetic regional models for Albania and south-east Italy from 1990 to 2010 with prediction to 2012 and comparison with IGRF-11Qamili, E.* ; De Santis, A.* ; Cianchini, G.* ; Duka, B.* ; Gaya-Piqué, L. R.* ; Dominici, G.* ; Hyka, Niko*