Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/13379
Authors: Regi, Mauro* 
Bagiacchi, Paolo* 
Di Mauro, Domenico* 
Lepidi, Stefania* 
Cafarella, Lili* 
Title: On the validation of K index values at Italian geomagnetic observatories
Journal: Geoscientific Instrumentation, Methods and Data Systems (GI) 
Series/Report no.: /9 (2020)
Publisher: EGU - Copernicus
Issue Date: 2020
DOI: 10.5194/gi-9-105-2020
URL: https://www.geosci-instrum-method-data-syst-discuss.net/gi-2019-31/
Subject Classification04.05. Geomagnetism 
Abstract: Local K index and the consequent global Kp index are well established three-hour range indices used to characterize the geomagnetic activity. K index is one of the parameters which INTERMAGNET observatories can provide and it’s widely used since several decades, although many other activity indices have been proposed in the meanwhile. The method for determining the K values has to be the same for all observatories. INTERMAGNET consortium recommends the use of one of the 4 methods endorsed by the International Service of Geomagnetic Indices ( ISGI) in close cooperation and agreement with the ad-hoc working group of International Association of Geomagnetism and Aeronomy (IAGA). INTERMAGNET provides the software code KASM, designed for an automatic calculation of K index according to the Adaptive Smoothed method. K values should be independent on the local dynamic response, therefore for their determination each observatory has its own specific scale regulated by the L9 lower limit, which represents the main input parameter for KASM. The determination of an appropriate L9 value for any geomagnetic observatory is then fundamental. In this work we statistically analyze the K values estimated by means of KASM code for the Italian geomagnetic observatories of Duronia (corrected geomagnetic latitude λ~36° N) and Lampedusa (λ~28° N) comparing them with the German observatories of Wingst and Niemegk. Our comparative analysis is finalized to establish the best estimation of the L9 lower limit for these two stations. A comparison of L9 lower limits found for the Italian observatories with results from a previous empirical method was also applied and used to verify the consistency and reliability of our outcomes.
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