Victor De la Luz - Página Personal

Puesto:

Cátedras CONACYT

Grupo:

Servicio de Clima Espacial México (SCiESMEX) / Laboratorio Nacional de Clima Espacial (LANCE)

Contacto:

Teléfono(s): +52 01 443 322 2777 - ext. 80840

Correo Electrónico: vdelaluz(at)igeofisica.unam.mx

Sitio Web: http://www.astromonos.org

Cursos

 

Semblanza:

El Dr. Victor De la Luz se tituló como Licenciado en Ciencias de la Computación en el departamento de Matemáticas de la Facultad de Ciencias de la Universidad Nacional Autónoma de México (UNAM), cursó sus estudios de maestría en el Instituto Nacional de Astrofísica, Óptica y Electrónica (INAOE) en la especialidad de Astrofísica y obtuvo su Doctorado en Ciencias en el Posgrado de Ciencias de la Tierra en la UNAM. Realizó tres post-doctorados en el Grupo de Atmósferas Planetarias y Estelares (GrAPEs) del INAOE. Posteriormente fué contratado como Astrónomo de Soporte en el Gran Telescopío Milimétrico (GTM), el proyecto científico mas importante de México. En el 2014 fue invitado a trabajar en el Departamento de Física de la Universidad Autónoma Metropolitana (UAM) y finalmente ese mismo año se integro al programa de Cátedras Conacyt en el Proyecto del Servicio de Clima Espacial (SCiESMEX).

Autor de 22 articulos científicos, su trabajo a sido galardonado con el premio del Outstanding Paper Award de la American Geophysical Union por el desarrollo de Pakal, un software para resolver la ecuación de transferencia radiativa. Actualmente, gracias a su amplia experiencia en Supercómputo, Física Solar y Radioastronomía le permiten llevar a cabo las operaciones mas críticas del SCiESMEX, entre ellas la operación del Repositorio Institucional de Clima Espacial (RICE), el Sistema de Alerta Temprana de Clima Espacial (SATCE) y el Centro de Supercómputo de Clima Espacial (CESCOM), todos parte del Laboratorio Nacional de Clima Espacial (LANCE).

Oportunidades de Tesis, Trabajo Social y Practicas Profesionales (2017):

¿Te interesa participar en el Servicio de Clima Espacial México? Escribe a vdelaluz@igeofisica.unam.mx, tenemos oportunidades para realizar trabajo social, tesis de licenciatura o de posgrado en el área de clima espacial. 

Información Curricular

Experiencia Laboral:

Postdoctorados:

Estancias de Investigación:

Formación Académica:

 Publicaciones científicas:

  1. M.A. Sergeeva, O.A. Maltseva, J.A. Gonzalez-Esparza, V. De la Luz, P. Corona-Romero, Features of TEC behaviour over the low-latitude North-American region during the period of medium solar activity, Advances in Space Research, https://doi.org/10.1016/j.asr.2017.06.042
  2. E. Romero-Hernandez, J.A. Gonzalez-Esparza, M. Rodriguez-Martinez, M. Sergeeva, E. Aguilar-Rodriguez, J.C. Mejia-Ambriz, V. De la Luz, Study of Ionospheric Disturbances over Mexico Associated with Transient Space Weather Events, Advances in Space Research, January 2017. https://doi.org/10.1016/j.asr.2017.06.042
  3. J. A. Gonzalez-Esparza, V. De la Luz, P. Corona-Romero, J. C. Mejia-Ambriz, L. X. Gonzalez, M. A. Sergeeva, E. Romero-Hernandez, E. Aguilar-Rodriguez. Mexican Space Weather Service (SCiESMEX). Space Weather. Volume 15, Issue 1 January 2017 Pages 3–11. 10.1002/2016SW001496. http://onlinelibrary.wiley.com/doi/10.1002/2016SW001496/abstract
  4. P. Corona-Romero, J. A. Gonzalez-Esparza, C. A. Perez-Alanis, E. Aguilar-Rodriguez, V. de-la-Luz, J. C. Mejia-Ambriz. Calculating travel times and arrival speeds of CMEs to Earth: an analytic tool for space weather forecasting. Space Weather. 10.1002/2016SW001489.
  5. Chavez-Dagostino, M. et al. "Early science with the Large Millimetre Telescope: Deep LMT/AzTEC millimetre observations of ɛ Eridani and its surroundings". Monthly Notices of the Royal Astronomical Society, Volume 462, Issue 3, p.2285-2294. 10.1093/mnras/stw1363.
  6. Liseau, R. et al. 2016/10 "ALMA's view of the nearest neighbors to the Sun. The submm/mm SEDs of the α Centauri binary and a new source". Astronomy & Astrophysics, Volume 594, id.A109, 9 pp 10.1051/0004-6361/201629135.
  7. De la Luz, V. 2016/05, "The Chromospheric Solar Limb Brightening at Radio, Millimeter, Sub-millimeter, and Infrared Wavelengths",The Astrophysical Journal, Volume 825, Issue 2, article id. 138, 12 pp. (2016). 2016ApJ...825..138D.
  8. De la Luz, V. et al. 2016/11, "Solar Limb Theoretical Tomography at Millimeter, Sub-millimeter, and Infrared Wavelengths", Advances in Space Research, Volume 58, Issue 10, p. 2003-2006, 2016AdSpR..58.2003D.
  9. Harrington, K. C. et al. 2016/06, "Early science with the Large Millimeter Telescope: observations of extremely luminous high-z sources identified by Planck", Monthly Notices of the Royal Astronomical Society, Volume 458, Issue 4, p.4383-4399, DOI: 10.1093/mnras/stw614.
  10. Cybulski, Ryan et al. 2016/07, "Early Science with the Large Millimeter Telescope: COOL BUDHIES I - a pilot study of molecular and atomic gas at z ≃ 0.2", Monthly Notices of the Royal Astronomical Society, Volume 459, Issue 3, p.3287-3306. 10.1093/mnras/stw798
  11. Yun, Min S et al. 2015/12. "Early Science with the Large Millimeter Telescope: CO and [C II] Emission in the z = 4.3 AzTEC J095942.9+022938 (COSMOS AzTEC-1)" . Monthly Notices of the Royal Astronomical Society, Volume 454, Issue 4, p.3485-3499. DOI: 10.1093/mnras/stv1963.
  12. Trottet, G. et al. 2015/10. "Origin of the 30 THz Emission Detected During the Solar Flare on 2012 March 13 at 17:20 UT", Solar Physics, Volume 290, Issue 10, pp.2809-2826. DOI: 10.1007/s11207-015-0782-0.
  13. Corona-Romero, P. et al. 2015/09, "Kinematics of ICMEs/Shocks: Blast Wave Reconstruction Using Type-II Emissions", Solar Physics, Volume 290, Issue 9, pp.2439-2454. DOI: 10.1007/s11207-015-0683-2.
  14. Liseau, R. et al. 2015/01, "ALMA observations of alpha Centauri. First detection of main-sequence stars at 3 mm wavelength", Astronomy & Astrophysics, Volume 573, id.L4, 4 pp. DOI: 10.1051/0004-6361/201425189
  15. De la Luz, V. et al. 2014/08, "The Relation Between the Radial Temperature Profile in the Chromosphere and the Solar Spectrum at Centimeter, Millimeter, Submillimeter, and Infrared Wavelengths", Solar Physics, Volume 289, Issue 8, pp.2879-2889 DOI: 10.1007/s11207-014-0511-0.
  16. De la Luz, V. et al. 2014/07, "Xitris: A Software to Acquire, Display, Compress, and Publish Data in Real Time using Distributed Mode for the Solar Radio Interferometer RIS", Journal of Computational Interdisciplinary Sciences (2013) 4(1): 15-22. DOI: 10.6062/jcis.2013.04.01.0066.
  17. De la Luz, V. et al. 2014/07, "The Chromospheric Solar Millimeter-wave Cavity; a Common Property in the Semi-empirical Models", Geofisica Internacional, Volume 54, Issue 2, April–June 2015, Pages 161–166. DOI: 10.1016/j.gi.2015.04.011.
  18. Olmedo, Manuel et al. 2013/12,  "Mg II h + k Flux - Rotational Period Correlation for G-type Stars", Publications of the Astronomical Society of the Pacific, Volume 125, issue 934, pp.1436-1442. DOI: 10.1086/674332.
  19. De la Luz, V. et al.  2013/01, "The Chromospheric Solar Millimeter-wave Cavity Originates in the Temperature Minimum Region", The Astrophysical Journal, Volume 762, Issue 2, article id. 84, 8 pp. (2013). DOI: 10.1088/0004-637X/762/2/84.
  20. De la Luz, V. et al. 2011/08, "Synthetic Spectra of Radio, Millimeter, Sub-millimeter, and Infrared Regimes with Non-local Thermodynamic Equilibrium Approximation", The Astrophysical Journal, Volume 737, Issue 1, article id. 1, 8 pp. (2011). DOI: 10.1088/0004-637X/737/1/1.
  21. De la Luz V. et al. 2010/06, "Pakal: A Three-dimensional Model to Solve the Radiative Transfer Equation", The Astrophysical Journal Supplement, Volume 188, Issue 2, pp. 437-446 (2010). DOI: 10.1088/0067-0049/188/2/437.
  22. De la Luz, V. et al. 2008/07, "3D Simulations of the Quiet Sun Radio Emission at Millimeter and Submillimeter Wavelengths". Geofísica Internacional, Vol. 47 (3), p. 197-203. ISSN 0016-7169.

Publicaciones como Editor

  1. Chavez, Miguel et al. 2013/04, "New Quests in Stellar Astrophysics III: A Panchromatic View of Solar-like Stars, With and Without Planets", New Quests in Stellar Astrophysics III: A Panchromatic View of Solar-Like Stars, With and Without Planets. Proceedings of an International Conference held at Puerto Vallarta, Jalisco, Mexico 12-16 March, 2012. Edited by M. Chavez, E. Bertone, O. Vega and V. De la Luz. San Francisco: Astronomical Society of the Pacific, 2013. ISBN: 978-1-58381-828-2.

Memorias de Congresos

  1. J. D. Lowenthal, K. Harrington, D. Berman, M. Yun, R. Cybulski, G. W. Wilson, I. Aretxaga, M. Chavez, V. De la Luz, N. Erickson, D. Ferrusca, A. Gallup, D. Hughes, A. Montaña, G. Narayanan, D. Sánchez-Argüelles, F. P. Schloerb, K. Souccar, E. Terlevich, R. Terlevich, M. Zeballos and J. A. Zavala, Gravitationally Lensed CO and Dust at High Redshift: New LMT/GTM Images and Spectra of Sub-Millimeter Galaxies, Volume 11, Issue S321 (Formation and Evolution of Galaxy Outskirts) March 2016, p. 363. DOI: https://doi.org/10.1017/S1743921316011145
  2.  De la Luz, V. et al. 2013/04 "The Limb Brightening and its Relationship with the Millimeter-wave Cavity", New Quests in Stellar Astrophysics III: A Panchromatic View of Solar-Like Stars, With and Without Planets. Proceedings of an International Conference held at Puerto Vallarta, Jalisco, Mexico 12-16 March, 2012. Edited by M. Chavez, E. Bertone, O. Vega and V. De la Luz. San Francisco: Astronomical Society of the Pacific, 2013, p.253. BCODE