58 citations · 222 across the 15 of their papers we have counts for
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ALMA's view of the Sun's nearest neighbours: The submm/mm SEDs of the alpha Centauri binary and a new source
R. Liseau, V. De la Luz, E. O'Gorman +3
The precise mechanisms that provide the non-radiative energy for heating the chromosphere and the corona of the Sun and other stars are at the focus of intense contemporary researc…
The Chromospheric Solar Limb Brightening at Radio, Millimeter, Sub-millimeter, and Infrared Wavelengths
Victor De la Luz
Observations of the emission at radio, millimeter, sub-millimeter, and infrared wavelengths in the center of the solar disk validate the auto-consistence of semi-empirical models o…
Solar Limb Theoretical Tomography at Millimeter, Sub-millimeter, and Infrared Wavelengths
Victor De la Luz, J. A. Gonzalez-Esparza, P. Corona-Romero +1
Semi-empirical models of the solar Chromosphere show in their emission spectrum, tomography property at millimeter, sub-millimeter, and infrared wavelengths for the center of the s…
A new submm source within a few arcseconds of Centauri: ALMA discovers the most distant object of the solar system
R. Liseau, W. Vlemmings, E. O'Gorman +3
We recently announced the detection of an unknown submillimeter source in our ALMA observations of alpha Cen AB. The source was detected in two epochs, a strong detection at 445~GH…
Origin of the 30 THz emission detected during the 2012 March 13 solar flare at 17:20 UT
G. Trottet, J. -P. Raulin, A. MacKinnon +6
Solar observations in the infrared domain can bring important clues on the response of the low solar atmosphere to primary energy released during flares. At present the infrared co…
ALMA observations of alpha Centauri: First detection of main-sequence stars at 3mm wavelength
R. Liseau, W. Vlemmings, A. Bayo +19
The precise mechanisms that provide the non-radiative energy for heating the chromosphere and the corona of the Sun and those of other stars constitute an active field of research.…
The Chromospheric Solar Millimeter-wave Cavity; a Common Property in the Semi-empirical Models
Victor De la Luz, Miguel Chavez, Emanuele Bertone
The semi-empirical models of the solar chromosphere are useful in the study of the solar radio emission at millimeter - infrared wavelengths. However, current models do not reprodu…
The Limb Brightening and its Relationship with the Millimeter-wave Cavity
Victor De la Luz, Miguel Chavez, Emanuele Bertone
Through a detailed theoretical analysis of the local emission at millimeter,sub-millimeter and infrared wavelength regimes (from \~ 10 GHz up to \~ 10 THz), we found that, associat…
The Relation between the Radial Temperature Profile in the Chromosphere and the Solar Spectrum at Centimeter, Millimeter, Sub-millimeter, and Infrared Wavelengths
Victor De la Luz, Miguel Chavez, Emanuele Bertone +1
Solar observations from millimeter to ultraviolet wavelengths show that there is a temperature minimum between photosphere and chromosphere. Analysis based on semi-empirical models…
Mg II h+k Flux - Rotational Period Correlation for G-type stars
Manuel Olmedo, Miguel Chávez, Emanuele Bertone +1
We present an analysis of the correlation between the mid-UV Mg II h and k emission lines and measured rotational periods of G-type stars. Based on IUE and HST high resolution spec…
The Chromospheric Solar Millimeter-wave Cavity, as a Result of the Temperature Minimum Region
V. De la Luz, J. -P. Raulin, A. Lara
We present a detailed theoretical analysis of the local radio emission at the lower part of the solar atmosphere. To accomplish this, we have used a numerical code to simulate the…