L. Tamblay
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Research Subjects
L. Tamblay has a total of 5 co-authors. Here are the top co-authors by number of shared publications:
- I. Salfate
Departamento de Física, Universidad de La Serena, La Serena, Chile
1 shared publication - Juan A. Lazzús
Departamento de Física, Universidad de La Serena, Casilla 554, La Serena 1700000, Chile
1 shared publication - Luis Palma-Chilla
Departamento de Física, Universidad de La Serena, Casilla 554, La Serena 1700000, Chile
1 shared publication - Pedro Vega-Jorquera
Universidad de La Serena
1 shared publication - R. Pacheco
Departamento de Física, Universidad de La Serena, La Serena, Chile
1 shared publication
Latest Publications
- 1 March 2021
- Published by Pleiades Publishing Ltd in Geomagnetism and Aeronomy
- Vol. 61 (2) , 287-292
Geomagnetic Field Variations during the Total Solar Eclipse of 2 July 2019 in La Serena, Chile
The total solar eclipse on July 2, 2019, has been studied by using data of the La Serena ground magnetic station in Chile located in the path of the totality (at geographic coordinates: 29.827° S, 71.261° W). The event reached 100% darkness and occurred from 1522:34 hr to 1746:36 hr LT. We monitored the X, Y, Z‑components of the geomagnetic field with a fluxgate magnetometer to investigate their variation caused by the passing of the Moon in front of the Sun. Our results show positive growth up to ∼12 nT for all components in the same time window during the eclipse and in total synchrony with its phases. Having to discard any effect on the observations such as magnetic and solar activities, seasonal and geographical conditions, and instrumental effects, we report a total increase of the geomagnetic field during this phenomenon.
- 1 March 2021
- Published by Pleiades Publishing Ltd in Geomagnetism and Aeronomy
- Vol. 61 (2) , 287-292
Geomagnetic Field Variations during the Total Solar Eclipse of 2 July 2019 in La Serena, Chile
The total solar eclipse on July 2, 2019, has been studied by using data of the La Serena ground magnetic station in Chile located in the path of the totality (at geographic coordinates: 29.827° S, 71.261° W). The event reached 100% darkness and occurred from 1522:34 hr to 1746:36 hr LT. We monitored the X, Y, Z‑components of the geomagnetic field with a fluxgate magnetometer to investigate their variation caused by the passing of the Moon in front of the Sun. Our results show positive growth up to ∼12 nT for all components in the same time window during the eclipse and in total synchrony with its phases. Having to discard any effect on the observations such as magnetic and solar activities, seasonal and geographical conditions, and instrumental effects, we report a total increase of the geomagnetic field during this phenomenon.