Please use this identifier to cite or link to this item:
http://hdl.handle.net/2122/13731
DC Field | Value | Language |
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dc.date.accessioned | 2020-10-02T06:18:52Z | - |
dc.date.available | 2020-10-02T06:18:52Z | - |
dc.date.issued | 2019-04 | - |
dc.identifier.uri | http://hdl.handle.net/2122/13731 | - |
dc.description.abstract | We present a preliminary study of the properties of the magnetic field’s fluctuations during the St. Patrick’s Day geomagnetic storm occurred on 17 March 2015. We analyse the minute values of the geomagnetic field recorded simultaneously by a latitudinal network of 18 geomagnetic observatories located at different latitudes, from the equatorial regions to the northern high-latitude ones. We apply the Empirical Mode Decomposition (EMD) method to the X (North) and Y (East) components of the geomagnetic field recorded during a period (13 - 30 March 2015) covering the whole duration of the storm. This adaptive method, which can be applied to signals originating from nonlinear and non-stationary processes, permits us to separate fast (𝜏<200 min) and slow (𝜏>200 min) magnetic fluctuations, which are related to different magnetospheric processes. Indeed, it has been shown that whilemagneticfluctuationsat long timescales (𝜏>200 min) showa large degree of correlationbetween solar windparameters and magnetosphericdynamicsproxies, at short timescales(𝜏<200 min)theyareessentially related to internal magnetospheric processes andseem to be notdirectlydriven by interplanetarychanges. The differentenergycontribution of the fast and slow fluctuationsisinvestigatedas a function of latitudeduring the development of theselectedgeomagneticstorm.The weight of the signal related to the fluctuations on a short time scale shows a dependence on the latitude and geomagnetic activity level. | en_US |
dc.language.iso | English | en_US |
dc.relation.ispartof | EGU General Assembly 2019 | en_US |
dc.subject | Solar terrestrial relationship | en_US |
dc.title | “Characterization of the geomagnetic field fluctuations during St. Patrick’s Day Storm” | en_US |
dc.type | Oral presentation | en_US |
dc.description.status | Unpublished | en_US |
dc.description.ConferenceLocation | Vienna, Austria | en_US |
dc.description.obiettivoSpecifico | 1A. Geomagnetismo e Paleomagnetismo | en_US |
dc.contributor.author | Santarelli, Lucia | - |
dc.contributor.author | De Michelis, Paola | - |
dc.contributor.author | Consolini, Giuseppe | - |
dc.contributor.department | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia | en_US |
dc.contributor.department | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia | en_US |
dc.contributor.department | INAF | en_US |
item.openairetype | Oral presentation | - |
item.cerifentitytype | Publications | - |
item.languageiso639-1 | en | - |
item.grantfulltext | open | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia | - |
crisitem.author.dept | INAF – Istituto di Astrofisica e Planetologia Spaziali, 00133 Roma, Italy | - |
crisitem.author.orcid | 0000-0002-4134-1560 | - |
crisitem.author.orcid | 0000-0002-2708-0739 | - |
crisitem.author.orcid | 0000-0002-3403-647X | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.department.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.department.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
Appears in Collections: | Conference materials |
Files in This Item:
File | Description | Size | Format | |
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EGU_2019Lucia.pdf | 7.09 MB | Adobe PDF | View/Open |
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