Simultaneous observation of solar neutrons and effects on terrestrial magnetic field in association with a solar flare

Wara Chamani; Rolando Ticona Peralta; Edgar Ricaldi

doi:10.1063/1.3141371

Simultaneous observation of solar neutrons and effects on terrestrial magnetic field in association with a solar flare

Wara Chamani, Rolando Ticona Peralta, Edgar Ricaldi

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Abstract

On November 2,2003 at 17:03:00 UT a solar flare, registered by the GOES satellite, was also recorded by the Neutron Monitor (NM64) of Cosmic Ray Laboratory at Mount Chacaltaya. This flare affected the local geomagnetic field (F): there were variations in the intensity of the horizontal component (H), declination component (D) and vertical component (Z). Variations on these components, estimated as 71 nT, 10 deg. and 19 nT, respectively, have been observed with the Patacamaya's Geomagnetic Observatory; as well as a net increased field (F), estimated as 66 nT, recorded by the Villa Remedios Geomagnetic Observatory. The duration of the magnetic and neutron signals was approximately 40 and 54 minutes, respectively, which shows that the flare was intense and with large emission of neutrons.

Original language	English
Title of host publication	Cosmic Rays and Astrophysics - Proceedings of the 3rd School on Cosmic Rays and Astrophysics
Pages	259-261
Number of pages	3
DOIs	https://doi.org/10.1063/1.3141371
State	Published - 2009
Event	3rd School on Cosmic Rays and Astrophysics - Arequipa, Peru Duration: 25 Aug 2008 → 5 Sep 2008

Publication series

Name	AIP Conference Proceedings
Volume	1123
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Conference

Conference	3rd School on Cosmic Rays and Astrophysics
Country/Territory	Peru
City	Arequipa
Period	25/08/08 → 5/09/08

Keywords

Magnetic Crochet
Solar Flare
Solar Neutron

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10.1063/1.3141371

Cite this

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title = "Simultaneous observation of solar neutrons and effects on terrestrial magnetic field in association with a solar flare",

abstract = "On November 2,2003 at 17:03:00 UT a solar flare, registered by the GOES satellite, was also recorded by the Neutron Monitor (NM64) of Cosmic Ray Laboratory at Mount Chacaltaya. This flare affected the local geomagnetic field (F): there were variations in the intensity of the horizontal component (H), declination component (D) and vertical component (Z). Variations on these components, estimated as 71 nT, 10 deg. and 19 nT, respectively, have been observed with the Patacamaya's Geomagnetic Observatory; as well as a net increased field (F), estimated as 66 nT, recorded by the Villa Remedios Geomagnetic Observatory. The duration of the magnetic and neutron signals was approximately 40 and 54 minutes, respectively, which shows that the flare was intense and with large emission of neutrons.",

keywords = "Magnetic Crochet, Solar Flare, Solar Neutron",

author = "Wara Chamani and {Ticona Peralta}, Rolando and Edgar Ricaldi",

year = "2009",

doi = "10.1063/1.3141371",

language = "Ingl{\'e}s",

isbn = "9780735406599",

series = "AIP Conference Proceedings",

pages = "259--261",

booktitle = "Cosmic Rays and Astrophysics - Proceedings of the 3rd School on Cosmic Rays and Astrophysics",

note = "null ; Conference date: 25-08-2008 Through 05-09-2008",

}

Chamani, W, Ticona Peralta, R & Ricaldi, E 2009, Simultaneous observation of solar neutrons and effects on terrestrial magnetic field in association with a solar flare. in Cosmic Rays and Astrophysics - Proceedings of the 3rd School on Cosmic Rays and Astrophysics. AIP Conference Proceedings, vol. 1123, pp. 259-261, 3rd School on Cosmic Rays and Astrophysics, Arequipa, Peru, 25/08/08. https://doi.org/10.1063/1.3141371

Simultaneous observation of solar neutrons and effects on terrestrial magnetic field in association with a solar flare. / Chamani, Wara; Ticona Peralta, Rolando; Ricaldi, Edgar.

Cosmic Rays and Astrophysics - Proceedings of the 3rd School on Cosmic Rays and Astrophysics. 2009. p. 259-261 (AIP Conference Proceedings; Vol. 1123).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

TY - GEN

T1 - Simultaneous observation of solar neutrons and effects on terrestrial magnetic field in association with a solar flare

AU - Chamani, Wara

AU - Ticona Peralta, Rolando

AU - Ricaldi, Edgar

PY - 2009

Y1 - 2009

N2 - On November 2,2003 at 17:03:00 UT a solar flare, registered by the GOES satellite, was also recorded by the Neutron Monitor (NM64) of Cosmic Ray Laboratory at Mount Chacaltaya. This flare affected the local geomagnetic field (F): there were variations in the intensity of the horizontal component (H), declination component (D) and vertical component (Z). Variations on these components, estimated as 71 nT, 10 deg. and 19 nT, respectively, have been observed with the Patacamaya's Geomagnetic Observatory; as well as a net increased field (F), estimated as 66 nT, recorded by the Villa Remedios Geomagnetic Observatory. The duration of the magnetic and neutron signals was approximately 40 and 54 minutes, respectively, which shows that the flare was intense and with large emission of neutrons.

AB - On November 2,2003 at 17:03:00 UT a solar flare, registered by the GOES satellite, was also recorded by the Neutron Monitor (NM64) of Cosmic Ray Laboratory at Mount Chacaltaya. This flare affected the local geomagnetic field (F): there were variations in the intensity of the horizontal component (H), declination component (D) and vertical component (Z). Variations on these components, estimated as 71 nT, 10 deg. and 19 nT, respectively, have been observed with the Patacamaya's Geomagnetic Observatory; as well as a net increased field (F), estimated as 66 nT, recorded by the Villa Remedios Geomagnetic Observatory. The duration of the magnetic and neutron signals was approximately 40 and 54 minutes, respectively, which shows that the flare was intense and with large emission of neutrons.

KW - Magnetic Crochet

KW - Solar Flare

KW - Solar Neutron

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U2 - 10.1063/1.3141371

DO - 10.1063/1.3141371

M3 - Contribución a la conferencia

AN - SCOPUS:69849100497

SN - 9780735406599

T3 - AIP Conference Proceedings

SP - 259

EP - 261

BT - Cosmic Rays and Astrophysics - Proceedings of the 3rd School on Cosmic Rays and Astrophysics

Y2 - 25 August 2008 through 5 September 2008

ER -

Simultaneous observation of solar neutrons and effects on terrestrial magnetic field in association with a solar flare

Abstract

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Conference

Keywords

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