Earth-prints repository, logo   Istituto Nazionale di Geofisica e Vulcanologia

Istituto Nazionale di Geofisica e Vulcanologia
 
|earth-prints home page | roma library | bologna library | catania library | milano library | napoli library | palermo library

Earth-prints >
Affiliation >
INGV >
Papers Published / Papers in press >

Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/3906

Share this record with your favourite social network:     Del.icio.us     Citeulike     Connotea
Facebook     Stumble it!     reddit    
Title: Historical measurements of the Earth’s magnetic field compared with remanence directions from lava flows in Italy over the last four centuries
Authors: Lanza, R.*
Meloni, A.*
Tema, E.*
Keywords: Secular variation
Historical magnetic measurements
Thermal remanent magnetization
Volcanic rocks
Issue Date: 2005
Publisher: Elsevier
Title of journal: Physics of the Earth and Planetary Interiors
Series/Report no.: 1 / 148 (2005)
Abstract: Direct measurements of the Earth’s magnetic field in Italy since 1640 a.d. have been used to check the remanence directions derived from historically dated volcanic rocks of Etna and Vesuvius. Direct measurements consist of the records of L’Aquila and Pola geomagnetic observatories, the repeat stations of the Italian Magnetic Network and the data base of the Historical Italian Geomagnetic Data Catalogue. All have been relocated to the same reference site (Viterbo — lat. 42.45◦N, long. 12.03◦E) in order to draw a reference secular variation (SV) curve. The direction of the Earth’s field at Viterbo has also been calculated from the historical records (2000–1600) of ref. [Jackson, A., Jonkers, A.R.T., Walker, M.R., 2000. Four centuries of geomagnetic secular variation from historical records. Phil. Trans. R. Soc. London, Ser. A 358, 957–990] database. The remanence directions from Etna show a general agreement with the trend of the SV curve, although their inclination is usually lower than that from the direct measurement. The directions from Vesuvius are more scattered. Large discrepancies occur at both volcanoes and in some cases have been ascribed in the literature to poor geographic information, making it difficult to identify the flows actually emplaced during the eruptions reported in the chronicles. Closer examination shows that the great majority of the best-defined remanence directions (semi-angle of confidence α95 < 2.5◦) deviate significantly from the geomagnetic direction measured at the time of the emplacement, the angle between the two directions being larger than the α95 value. The value of 2.5–3.0◦ can thus be regarded as a conservative evaluation of the error when dealing with dating Etna and Vesuvius lava flows older than 17th century, even when the accuracy attained in remanence measurements is higher. In default of a SV curve for Italy derived from archaeological artefacts, a further error in dating is introduced when reference is made to SV curves of other countries, even if well-established, as these are from regions too far from Italy (>600 km) to confidently relocate magnetic directions.
URI: http://hdl.handle.net/2122/3906
DOI: 10.1016/j.pepi.2004.08.005
Appears in Collections:Papers Published / Papers in press
04.05.06. Paleomagnetism
04.05.02. Geomagnetic field variations and reversals
04.02.04. Magnetic and electrical methods

Files in This Item:

File Description SizeFormat
08052012484507834.pdf272.75KbAdobe PDFView/Open
  • Alexandrescu, M., Courtillot, V., Le Mou¨el, J.-L., 1997. Highresolution
  • secular variation of the geomagnetic field in western
  • Europe over the last 4 centuries: comparison and integration of
  • historical data from Paris and London. J. Geophys. Res. 102,
  • 20245–20258.
  • Angelino, A., Incoronato, A., 1996. Stratigrafia magnetica in aree
  • vulcaniche; esperienze al Vesuvio e all’Etna. 15◦ Convegno
  • GNGTS, CNR Roma, pp. 13–18.
  • Baag, C., Helsley, C.E., Xu, S.Z., Lienert, B.R., 1995. Deflection
  • of palaeomagnetic directions due to magnetisation of underlying
  • terrain. J. Geophys. Res. 100, 10013–10027.
  • Bucur, I., 1994. The direction of the terrestrial magnetic field in
  • France during the last 21 centuries. Phys. Earth Planet. Int. 87,
  • 95–109.
  • Cafarella, L., De Santis, A., Meloni, A., 1992a. The Historical Italian
  • Geomagnetic Data Catalogue. ING, Rome, p. 160.
  • Cafarella, L., De Santis, A., Meloni, A., 1992b. Secular variation
  • from historical geomagnetic field measurements. Phys. Earth
  • Planet. Inter. 73, 206–221.
  • Carracedo, J.C., Principe, C., Rosi, M., Soler,V., 1993. Time correlation
  • by palaeomagnetism of the 1631 eruption of MountVesuvius
  • Volcanological and volcanic hazard implications. J. Volcanol.
  • Geotherm. Res. 58, 203–209.
  • Chiari, G., Lanza, R., 1999. Remanent magnetization of mural paintings
  • from the Bibliotheca Apostolica (Vatican Rome). J. Appl.
  • Geophys. 41, 137–143.
  • Cioni, R., Gurioli, L., Lanza, R., Zanella, E., 2004. Temperatures of
  • the A.D. 79 pyroclastic density current deposits (Vesuvius Italy).
  • J. Geophys. Res. 109, B02207, doi: 10.1029/2002JB.002251.
  • Coticchia, A., De Santis, A., Di Ponzio, A., Dominici, G., Meloni,
  • A., Pierozzi, M., Sperti, M., 2000. Italian Magnetic Network and
  • Geomagnetic Field Maps of Italy at year 2000. Boll. Geod. Sci.
  • Aff. LX/4, 262–291.
  • De Santis, A., 1992. Conventional spherical harmonic analysis for
  • regional modelling of the geomagnetic field. Geophys. Res. Lett.
  • 19, 1065–1067.
  • Hoye, G.S., 1981. Archaeomagnetic secular variation record of
  • Mount Vesuvius. Nature 291, 216–218.
  • Iliceto, V., Napoleone, G., Pinna, E., 1973. Geomagnetic changes
  • during the cooling process of the Mount Etna 1971 lava
  • flow: preliminary report. Boll. Assoc. Geof. Ital. 22, 89–
  • 94.
  • Incoronato, A., Angelino, A., Romano, R., Ferrante, A., Sauna, R.,
  • Vanacore, G., Vecchione, C., 2002. Retrieving geomagnetic secular
  • variations from lava flows: evidence from Mounts Arso,
  • Etna and Vesuvius (southern Italy). Geophys. J. Int. 149, 724–
  • 730.
  • INGV, 2003. Risultati delle osservazioni magnetiche, L’Aquila, 55
  • pp.
  • Jackson, A., Jonkers, A.R.T., Walker, M.R., 2000. Four centuries
  • of geomagnetic secular variation from historical records. Phil.
  • Trans. R. Soc. London, Ser. A 358, 957–990.
  • Knudsen, M.F., Jacobsen, B.H., Abrahamsen, N., 2003. Paleomagnetic
  • distortion modelling and possible recovery by inversion.
  • Phys. Earth Planet. Inter. 135, 55–73.
  • Lanza, R., Zanella, E., 2003. Paleomagnetic secular variation at Vulcano
  • (Aeolian Islands) during the last 135 kyr. Earth Planet. Sci.
  • Lett. 213, 321–336.
  • Noel, M., Batt, C.M., 1990. A method for correcting geographically
  • separated remanence directions for the purpose of archeomagnetic
  • dating. Geophys. J. Int. 102, 753–756.
  • Principe, C., Tanguy, J.C., Arrighi, S., Paiotti, A., Le Goff, M., Zoppi,
  • U., in press. Chronology of Vesuvius’ activity from A.D. 79 to
  • 1631 based on archeomagnetism of lavas and historical sources.
  • Bull. Volcanol.
  • Rolph, T.C., 1997. An investigation of the magnetic variation within
  • two recent lava flows. Geophys. J. Int. 130, 125–136.
  • Rolph, T.C., Shaw, J., Guest, J.E., 1987. Geomagnetic field variations
  • as a dating tool: application to Sicilian lavas. J. Archaeological
  • Sci. 14, 215–225.
  • Talamo, R., 1975. Le carte magnetiche d’ Italia delle isodinamiche
  • dellaHe delle isogone dell’ Istituto Geografico Militare e loro aggiornamento
  • al. 1973.0. Boll. Geod. Sci. Aff. XXXIV/1, 73–77.
  • Tanguy, J.C., Le Goff, M., Principe, C., Arrighi, S., Chillemi, V.,
  • Paiotti, A., La Delfa, S., Patan`e, G., 2003. Archeomagnetic dating
  • of Mediterranean volcanics of the last 2100 years: validity and
  • limits. Earth Planet. Sci. Lett. 211, 111–124.
  • Tanguy, J.C., Le Goff, M., 2004. Distortion of the geomagnetic field
  • in volcanic terrains: an experimental study of the Mount Etna
  • stratovolcano. Phys. Earth Planet. Inter. 141, 59–70.
  • Tarling, D., 1988. Secular variation of the geomagnetic field —
  • the archaeomagnetic record. In: Stephenson, F.R., Wolfendale,
  • A.W. (Eds.), Secular Solar and Geomagnetic Variations in
  • the Last 10,000 years, NATO ASI Series, vol. 236, pp. 349–
  • 366.
  • Thellier, E., 1981. Sur la direction du champ magnetique terrestre, en
  • France, durant les deux derniers millenaires. Phys. Earth Planet.
  • Inter. 13, 89–132.
  • von Kesslitz, W., 1911. Ergebnisse aus den Erdmagnetischen
  • Beobachtungen in Pola (1847–1909). HydrographischenAmtder
  • Kaiserlichen und K¨oniglichen Kriegsmarine, Pola.

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.

 

Valid XHTML 1.0! ICT Support, development & maintenance are provided by theAePIC team @CILEA.Powered onDSpace Software. Feedback