The Embrace Magnetometer Network for South America: First Scientific Results
The present work is the second of a two‐part paper on the Embrace Magnetometer Network. In this part, we provide some of the first scientific findings that we have already achieved with this network. We identified the diurnal and the seasonal natural variations of the H component. We provided the pr...
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| Veröffentlicht in: | Radio science 2018-03, Vol.53 (3), p.379-393 |
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| creator | Denardini, C. M. Chen, S. S. Resende, L. C. A. Moro, J. Bilibio, A. V. Fagundes, P. R. Gende, M. A. Cabrera, M. A. Bolzan, M. J. A. Padilha, A. L. Schuch, N. J. Hormaechea, J. L. Alves, L. R. Barbosa Neto, P. F. Nogueira, P. A. B. Picanço, G. A. S. Bertollotto, T. O. |
| description | The present work is the second of a two‐part paper on the Embrace Magnetometer Network. In this part, we provide some of the first scientific findings that we have already achieved with this network. We identified the diurnal and the seasonal natural variations of the H component. We provided the precise determination of sudden storm commencements and sudden impulse. We showed that the ΔH amplitudes derived from the Embrace MagNet during intense magnetic storm are in very good agreement with the Dst index. We showed that it is possible to investigate the effects on the solar quiet ionospheric current systems as a response to the X‐class solar flares occurring during daytime under magnetically quiet conditions.
Key Points
Magnetic measurements in South America ready for space weather
Magnetic station measurement with near‐observatory data quality
New‐real‐time data providing proxy for Dst and the new Ksa magnetic indices
Plain Language Summary
This manuscript is the second of a two‐part paper and provides the reader with the first scientific findings from the new Embrace Magnetometer Network (Embrace MagNet), which is located in South America and is based on fluxgate magnetometer. The main purpose of this network is to fulfill the gap in magnetic measurement, which are suitable for space weather purpose. Details on the network description and its qualification are provided in the first paper. |
| doi_str_mv | 10.1002/2018RS006540 |
| format | Article |
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Key Points
Magnetic measurements in South America ready for space weather
Magnetic station measurement with near‐observatory data quality
New‐real‐time data providing proxy for Dst and the new Ksa magnetic indices
Plain Language Summary
This manuscript is the second of a two‐part paper and provides the reader with the first scientific findings from the new Embrace Magnetometer Network (Embrace MagNet), which is located in South America and is based on fluxgate magnetometer. The main purpose of this network is to fulfill the gap in magnetic measurement, which are suitable for space weather purpose. Details on the network description and its qualification are provided in the first paper.</description><identifier>ISSN: 0048-6604</identifier><identifier>EISSN: 1944-799X</identifier><identifier>DOI: 10.1002/2018RS006540</identifier><language>eng</language><publisher>Washington: Blackwell Publishing Ltd</publisher><subject>Aeronomy ; Fluxgate magnetometers ; instrumentation ; Magnetic measurement ; Magnetic storms ; magnetism ; magnetometer network ; Magnetometers ; Solar flares ; space weather ; Sudden storm commencements</subject><ispartof>Radio science, 2018-03, Vol.53 (3), p.379-393</ispartof><rights>2018. American Geophysical Union. All Rights Reserved.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c3446-f042c6ddc6389ae5da97d4540086def3e2b09d844ebc42932ec2862f33618f6d3</citedby><cites>FETCH-LOGICAL-c3446-f042c6ddc6389ae5da97d4540086def3e2b09d844ebc42932ec2862f33618f6d3</cites><orcidid>0000-0002-3624-2461 ; 0000-0003-2600-4969 ; 0000-0002-6037-5483 ; 0000-0002-3639-9493 ; 0000-0001-6968-6184 ; 0000-0003-4078-2222 ; 0000-0002-5680-7271 ; 0000-0002-7905-9800 ; 0000-0001-8546-6819 ; 0000-0003-3926-396X ; 0000-0002-7720-6491 ; 0000-0003-3764-2202 ; 0000-0001-6307-7484 ; 0000-0003-0810-1044 ; 0000-0002-4653-2307 ; 0000-0001-5733-3541 ; 0000-0003-4533-3282</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1002%2F2018RS006540$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1002%2F2018RS006540$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,776,780,1411,1427,11493,27901,27902,45550,45551,46384,46443,46808,46867</link.rule.ids></links><search><creatorcontrib>Denardini, C. M.</creatorcontrib><creatorcontrib>Chen, S. S.</creatorcontrib><creatorcontrib>Resende, L. C. A.</creatorcontrib><creatorcontrib>Moro, J.</creatorcontrib><creatorcontrib>Bilibio, A. V.</creatorcontrib><creatorcontrib>Fagundes, P. R.</creatorcontrib><creatorcontrib>Gende, M. A.</creatorcontrib><creatorcontrib>Cabrera, M. A.</creatorcontrib><creatorcontrib>Bolzan, M. J. A.</creatorcontrib><creatorcontrib>Padilha, A. L.</creatorcontrib><creatorcontrib>Schuch, N. J.</creatorcontrib><creatorcontrib>Hormaechea, J. L.</creatorcontrib><creatorcontrib>Alves, L. R.</creatorcontrib><creatorcontrib>Barbosa Neto, P. F.</creatorcontrib><creatorcontrib>Nogueira, P. A. B.</creatorcontrib><creatorcontrib>Picanço, G. A. S.</creatorcontrib><creatorcontrib>Bertollotto, T. O.</creatorcontrib><title>The Embrace Magnetometer Network for South America: First Scientific Results</title><title>Radio science</title><description>The present work is the second of a two‐part paper on the Embrace Magnetometer Network. In this part, we provide some of the first scientific findings that we have already achieved with this network. We identified the diurnal and the seasonal natural variations of the H component. We provided the precise determination of sudden storm commencements and sudden impulse. We showed that the ΔH amplitudes derived from the Embrace MagNet during intense magnetic storm are in very good agreement with the Dst index. We showed that it is possible to investigate the effects on the solar quiet ionospheric current systems as a response to the X‐class solar flares occurring during daytime under magnetically quiet conditions.
Key Points
Magnetic measurements in South America ready for space weather
Magnetic station measurement with near‐observatory data quality
New‐real‐time data providing proxy for Dst and the new Ksa magnetic indices
Plain Language Summary
This manuscript is the second of a two‐part paper and provides the reader with the first scientific findings from the new Embrace Magnetometer Network (Embrace MagNet), which is located in South America and is based on fluxgate magnetometer. The main purpose of this network is to fulfill the gap in magnetic measurement, which are suitable for space weather purpose. 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M.</creator><creator>Chen, S. S.</creator><creator>Resende, L. C. A.</creator><creator>Moro, J.</creator><creator>Bilibio, A. V.</creator><creator>Fagundes, P. R.</creator><creator>Gende, M. A.</creator><creator>Cabrera, M. A.</creator><creator>Bolzan, M. J. A.</creator><creator>Padilha, A. L.</creator><creator>Schuch, N. J.</creator><creator>Hormaechea, J. L.</creator><creator>Alves, L. R.</creator><creator>Barbosa Neto, P. F.</creator><creator>Nogueira, P. A. B.</creator><creator>Picanço, G. A. S.</creator><creator>Bertollotto, T. 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A.</au><au>Moro, J.</au><au>Bilibio, A. V.</au><au>Fagundes, P. R.</au><au>Gende, M. A.</au><au>Cabrera, M. A.</au><au>Bolzan, M. J. A.</au><au>Padilha, A. L.</au><au>Schuch, N. J.</au><au>Hormaechea, J. L.</au><au>Alves, L. R.</au><au>Barbosa Neto, P. F.</au><au>Nogueira, P. A. B.</au><au>Picanço, G. A. S.</au><au>Bertollotto, T. O.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Embrace Magnetometer Network for South America: First Scientific Results</atitle><jtitle>Radio science</jtitle><date>2018-03</date><risdate>2018</risdate><volume>53</volume><issue>3</issue><spage>379</spage><epage>393</epage><pages>379-393</pages><issn>0048-6604</issn><eissn>1944-799X</eissn><abstract>The present work is the second of a two‐part paper on the Embrace Magnetometer Network. In this part, we provide some of the first scientific findings that we have already achieved with this network. We identified the diurnal and the seasonal natural variations of the H component. We provided the precise determination of sudden storm commencements and sudden impulse. We showed that the ΔH amplitudes derived from the Embrace MagNet during intense magnetic storm are in very good agreement with the Dst index. We showed that it is possible to investigate the effects on the solar quiet ionospheric current systems as a response to the X‐class solar flares occurring during daytime under magnetically quiet conditions.
Key Points
Magnetic measurements in South America ready for space weather
Magnetic station measurement with near‐observatory data quality
New‐real‐time data providing proxy for Dst and the new Ksa magnetic indices
Plain Language Summary
This manuscript is the second of a two‐part paper and provides the reader with the first scientific findings from the new Embrace Magnetometer Network (Embrace MagNet), which is located in South America and is based on fluxgate magnetometer. The main purpose of this network is to fulfill the gap in magnetic measurement, which are suitable for space weather purpose. Details on the network description and its qualification are provided in the first paper.</abstract><cop>Washington</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1002/2018RS006540</doi><tpages>15</tpages><orcidid>https://orcid.org/0000-0002-3624-2461</orcidid><orcidid>https://orcid.org/0000-0003-2600-4969</orcidid><orcidid>https://orcid.org/0000-0002-6037-5483</orcidid><orcidid>https://orcid.org/0000-0002-3639-9493</orcidid><orcidid>https://orcid.org/0000-0001-6968-6184</orcidid><orcidid>https://orcid.org/0000-0003-4078-2222</orcidid><orcidid>https://orcid.org/0000-0002-5680-7271</orcidid><orcidid>https://orcid.org/0000-0002-7905-9800</orcidid><orcidid>https://orcid.org/0000-0001-8546-6819</orcidid><orcidid>https://orcid.org/0000-0003-3926-396X</orcidid><orcidid>https://orcid.org/0000-0002-7720-6491</orcidid><orcidid>https://orcid.org/0000-0003-3764-2202</orcidid><orcidid>https://orcid.org/0000-0001-6307-7484</orcidid><orcidid>https://orcid.org/0000-0003-0810-1044</orcidid><orcidid>https://orcid.org/0000-0002-4653-2307</orcidid><orcidid>https://orcid.org/0000-0001-5733-3541</orcidid><orcidid>https://orcid.org/0000-0003-4533-3282</orcidid><oa>free_for_read</oa></addata></record> |
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| source | Wiley Free Content; Wiley-Blackwell AGU Digital Library; Wiley Online Library Journals Frontfile Complete; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals |
| subjects | Aeronomy Fluxgate magnetometers instrumentation Magnetic measurement Magnetic storms magnetism magnetometer network Magnetometers Solar flares space weather Sudden storm commencements |
| title | The Embrace Magnetometer Network for South America: First Scientific Results |
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