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Tozzi, Roberta
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Results 1-20 of 64 (Search time: 0.057 seconds).

Issue DateTitleAuthor(s)
1201520 March 2015 solar eclipse influence on sporadic E layerPezzopane, M.* ; Pietrella, M.* ; Pignalberi, A.* ; Tozzi, R.* 
22013Antarctic geomagnetic reference model updated to 2010 and provisionally to 2012Tozzi, R.* ; De Santis, A.* ; Gaya-Piqué, L.-R.* 
310-Aug-2015Applying a curl-B technique to Swarm vector data to estimate nighttime F region current intensitiesTozzi, R.* ; Pezzopane, M.* ; De Michelis, P.* ; Piersanti, M.* 
41-Jan-2021Can an impulsive variation of the solar wind plasma pressure trigger a plasma bubble? A case study based on CSES, Swarm and THEMIS dataPiersanti, Mirko* ; Pezzopane, Michael* ; Zhima, Zeren* ; Diego, Piero* ; Xiong, C* ; Tozzi, Roberta* ; Pignalberi, Alessio* ; D'Angelo, Giulia* ; Battiston, Roberto* ; Huang, J* ; Picozza, P.* ; Rui, Y* ; Shen, Xuhui* ; Sparvoli, Roberta* ; Ubertini, Pietro* ; Yang, Y.* ; Zoffoli, Simona* 
52019Characterising the electron density fluctuations in the high-latitude ionosphere at Swarm altitude in response to the geomagnetic activityGiannattasio, Fabio* ; De Michelis, Paola* ; Consolini, Giuseppe* ; Quattrociocchi, Virgilio* ; Coco, Igino* ; Tozzi, Roberta* 
628-May-2016Comparison between IRI and preliminary Swarm Langmuir probe measurements during the St. Patrick storm periodPignalberi, A.* ; Pezzopane, M.* ; Tozzi, R.* ; De Michelis, P.* ; Coco, I.* 
73-Nov-2009Complexity in the sunspot cycleConsolini, G.* ; Tozzi, R.* ; De Michelis, P.* 
82007The contribution of geomagnetic observatories and magnetic models to the study of secular variation and jerks in AntarcticaMeloni, A.* ; Cafarella, L.* ; De Michelis, P.* ; Tozzi, R.* 
923-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.* 
102021Dependence of Parallel Electrical Conductivity in the Topside Ionosphere on Solar and Geomagnetic ActivityGiannattasio, Fabio* ; Pignalberi, Alessio* ; De Michelis, Paola* ; Coco, Igino* ; Consolini, Giuseppe* ; Pezzopane, Michael* ; Tozzi, Roberta* 
112002Detecting geomagnetic field nonlinearities by bispectral analysis and a phase coupling nonlinear techniqueTozzi, R.* ; De Santis, A.* 
122022Dissipation of field-aligned currents in the topside ionosphereGiannattasio, Fabio* ; Consolini, Giuseppe* ; Coco, Igino* ; De Michelis, Paola* ; Pezzopane, Michael* ; Pignalberi, Alessio* ; Tozzi, Roberta* 
132019Features of Magnetic Field Fluctuations in the Ionosphere at Swarm altitudeDe Michelis, Paola* ; Consolini, Giuseppe* ; Tozzi, Roberta* ; Giannattasio, Fabio* ; Quattrociocchi, Virgilio* ; Coco, Igino* 
142021Forecasting SYM‐H Index: A Comparison Between Long Short‐Term Memory and Convolutional Neural NetworksSiciliano, F* ; Consolini, Giuseppe* ; Tozzi, Roberta* ; Gentili, M* ; Giannattasio, Fabio* ; De Michelis, Paola* 
1510-Jun-2020From the Sun to Earth: effects of the 25 August 2018 geomagnetic stormPiersanti, Mirko* ; De Michelis, Paola* ; Del Moro, Dario* ; Tozzi, Roberta* ; Pezzopane, Michael* ; Consolini, Giuseppe* ; Marcucci, Maria Federica* ; Laurenza, Monica* ; Di Matteo, Simone* ; Pignalberi, Alessio* ; Quattrociocchi, Virgilio* ; Diego, Piero* 
168-Aug-2009Geomagnetic jerks in the polar regionsTozzi, R.* ; De Michelis, P.* ; Meloni, A.* 
172005Geomagnetic jerks: observation and theoretical modelingDe Michelis, P.* ; Tozzi, R.* ; Meloni, A.* 
182005Geomagnetic storms, dependence on solar and interplanetary phenomena: a reviewMeloni, A.* ; De Michelis, P.* ; Tozzi, R.* 
197-Jan-2021High-latitude polar pattern of ionospheric electron density: Scaling features and IMF dependenceConsolini, Giuseppe* ; Tozzi, Roberta* ; De Michelis, Paola* ; Coco, Igino* ; Giannattasio, Fabio* ; Pezzopane, Michael* ; Marcucci, Maria Federica* ; Balasis, Georgios* 
202010Impact of the Faraday rotation on the SMOS measurements over the dome C test site: A semi-empirical studyBrogioni, M.* ; Macelloni, G.* ; Romano, Vincenzo* ; Tozzi, Roberta* ; Drinkwater, M.*