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Commit 3f8d0fac authored by Alexander Martinez's avatar Alexander Martinez
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cambios menores de sugerencias

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......@@ -4,7 +4,7 @@ The LAGO (Latin American Giant Observatory) project is an extended Astroparticle
The LAGO detection network consists in single or small arrays of particle [detectors](../activities/detectors.md) at ground level, spanning over different [sites](sites.md) located at significantly different latitudes (currently from Mexico up to the Antarctic region) and different altitudes (from sea level up to more than 5000 meters over sea level), covering a huge range of geomagnetic rigidity cut-offs and atmospheric absorption/reaction levels.
The LAGO Project is operated by the LAGO Collaboration, a non-centralized and distributed collaborative network of more than 80 scientist from more than 25 institutions of 9 latinamerican countries (currently Argentina, Bolivia, Brazil, Colombia, Ecuador, Mexico, Peru and Venezuela. [See the complete list of the collaboration members and their institutions](collaboration.md)).
The LAGO Project is operated by the LAGO Collaboration, a non-centralized and distributed collaborative network of more than 80 scientist from more than 25 institutions of 9 latinamerican countries (currently Argentina, Bolivia, Brasil, Colombia, Ecuador, Mexico, Peru and Venezuela. [See the complete list of the collaboration members and their institutions](collaboration.md)).
Finally, [detectors](../activities/detectors.md) installed in various universities are used as a tool to [teach students](../activities/teaching.md) about particle and astroparticle physics, in particular by leading them to the measurement of the muon decay.
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......@@ -21,7 +21,7 @@ Collaboration Secretary: TBD
- Guatemala: H.E. Pérez-Figueroa
- Mexico: H. Salazar
- Peru: L. Otiniano
- Spain: R. Mayo-García
- España: R. Mayo-García
**Tasks Coordinators**
......@@ -44,7 +44,6 @@ Collaboration Secretary: TBD
1. Audelo, M <sup>8</sup> [M. Audelo]
1. Ballina Escobar, Maynor Giovanni <sup>18</sup> [M.G. Ballina-Escobar]
1. Becerra Villamizar, Daniel Camilo <sup>17</sup> [D. C. Becerra-Villamizar]
1. Bertou, Xavier <sup>2</sup> [X. Bertou]
1. Caballero Mora, Karen Salome <sup>15</sup> [K.S. Caballero-Mora]
1. Caiza, R <sup>7</sup> [R. Caiza]
1. Calderón-Ardila, Rolando <sup>13</sup> [R. Calderón-Ardila]
......@@ -53,7 +52,6 @@ Collaboration Secretary: TBD
1. Carramiñana Alonso, Alberto <sup>14</sup> [A. Carramiñana-Alonso]
1. Carrasco, Esperanza <sup>14</sup> [E. Carrasco]
1. Carrera Jarrín, E <sup>26</sup> [E. Carrera-Jarrín]
1. Castillo Delacroix, Lucas Ezequiel <sup>10</sup> [L. E. Castillo Delacroix]
1. Castromonte, César <sup>25</sup> [C. Castromonte]
1. Cazar, D <sup>26</sup> [D. Cazar]
1. Christian, Gutierrez <sup>5</sup> [C. Gutierrez]
......@@ -61,7 +59,6 @@ Collaboration Secretary: TBD
1. Coloma Borja, D.A. <sup>26</sup> [D. Coloma-Borja]
1. Conde Sanchez, Ruben <sup>1</sup> [R. Conde]
1. Cotzomi Paleta, Jorge <sup>1</sup> [J. Cotzomi]
1. Dall'ara, Dario <sup>10</sup> [D. Dallara]
1. Dasso, Sergio <sup>12, 5</sup> [S. Dasso]
1. de Aguiar, Renan <sup>27</sup> [R. Aguiar]
1. de Albuquerque Silva, Alex <sup>28</sup> [A. Albuquerque]
......@@ -71,7 +68,6 @@ Collaboration Secretary: TBD
1. Durán, Jesús Andrés <sup>23</sup> [J.A. Durán]
1. Echiburu, Mauricio <sup>20</sup> [M. Echiburu]
1. Galindo Tellez, Aline <sup>14</sup> [A. Galindo-Tellez]
1. González, Manuel <sup>2</sup> [M. González]
1. Gómez Berisso, Mariano <sup>2</sup> [M. Gómez Berisso]
1. Grisales Casadiegos, Jenniffer <sup>22</sup> [J. Grisales-Casadiegos]
1. Gulisano, Adriana María <sup>12, 6, 11</sup> [A. M. Gulisano]
......@@ -114,7 +110,6 @@ Collaboration Secretary: TBD
1. Rubio-Montero, Antonio Juan <sup>3</sup> [A.J. Rubio-Montero]
1. Sacahuí Reyes, José Rodrigo <sup>18</sup> [J.R. Sacahui]
1. Salazar Ibarguen, Humberto <sup>1</sup> [H. Salazar]
1. Salomón, Nicolás <sup>10</sup> [N. Salomón]
1. Samanés, Jorge <sup>4</sup> [J. Samanes]
1. Santos, Noelia Ayelén <sup>5</sup> [N.A. Santos]
1. Sarmiento-Cano, Christian <sup>13</sup> [C. Sarmiento-Cano]
......
......@@ -48,7 +48,7 @@ What one would expect is that WCD would see an increase in the photon flux when
[GRB](../blog/posts/grb.md) The most violent events in the Universe.
## Solar Physics
## Space Weather
[Solar Physics](../blog/posts/solar.md) Understanding the solar activity and its impact on Cosmic Rays.
[Space Weather](../blog/posts/solar.md) Understanding the solar activity and its impact on Cosmic Rays.
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# Solar Physics
# Space Weather
In their way to the Earth, the cosmic rays produced in the galaxy by many different sources (called Galactic Cosmic Rays, GCR), find themselves deflected by magnetic fields.
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