Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Harvard-Smithsonian Center for Astrophysics
THEMIS S.L., via Lactea s / n, 38200 La Laguna, Tenerife, Islas Canarias, Spain
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138; Instituto de Astrofísica de Canarias, vía Láctea, s / n, La Laguna, Tenerife, Canary Islands, E-38205, Spai; Department of Soil Sciences and Geology, University of La Laguna, Tenerife, Canary Islands E-38205, Spain.
Dept. Edafología y Geología, Universidad de La Laguna, C / Astrofísico Francisco Sánchez, E-38205 Tenerife, Spain
Department Edafología y Geología, Universidad de La Laguna, E-38205 Tenerife, Spain Edafología y Geología, Universidad de La Laguna, C / Astrofísico Francisco Sánchez, E-38205 Tenerife, Spain
CfA
Instituto de Astrophysica de Canarias, Universidad de La Laguna, Tenerife, Spain
Instituto de Astrofisica de Canarias, C / Via Lactea, s / n, La Laguna, E38200 Spain; Department of Soil Sciences and Geology, Universidad de La Laguna, La Laguna, E3820 Spain
Harvard-Smithsonian Center for Astrophysics 60 Garden St., Cambridge, MA, 02139, USA
Departmento de Edafologa y Geologa, Universidad de La Laguna, Tenerife, 38205, Spain; Instituto de Astrofísica de Canarias, C / Vía Láctea s / n, Tenerife, 38205, Spain
HEPL, Stanford University, Stanford, CA 94305-4085, USA
Instituto de Astrofísica de Canarias, C. Vía Láctea s / n, La Laguna, Tenerife, 38200, Spain; Dpto. Edafología y Geología, Universidad de La Laguna, Tenerife, 38200, Spain
ULL
Instituto de Astrofísica de Canarias La Laguna, Tenerife, Spain
Departamento de Edafologia y Geologia, Universidad de La Laguna, La Laguna, Spain
IAC, Spain
Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, Spain
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA
A devil in the detail: parameter cross-talk from the solar cycle and estimation of solar p-mode frequencies
A Doppler Spectro-Imager dedicated to Jovian seismology and aeronomy onboard on Laplace/EJSM Jupiter Ganymede Orbiter
A new strategy for helioseismic inversions
A new upper limit to the temporal variation of the rotation rate of the tachocline between 1994 and 2002
A self-consistent procedure to detect low-l low-n solar p-modes
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