Building a Time Dependent Code to Simulate Oscillations of Line-Tied Coronal Loops
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van Doorsselaere, T. et al.
Advertised on:
12
2005
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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Ca II 8542 Å brightenings induced by a solar microflareAims: We study small-scale brightenings in Ca II 8542 Å line-core images to determine their nature and effect on localized heating and mass transfer in active regions. Methods: High-resolution two-dimensional spectroscopic observations of a solar active region in the near-infrared Ca II 8542 Å line were acquired with the GREGOR Fabry-PérotKuckein, C. et al.
Advertised on:
122017 -
Calibration for Large Telescopes: Status and ProspectsWe discuss the status of the calibration programme for CanariCam and related initiatives that aim to provide quality calibration facilities for users of the GTC and other telescopes. We have Visible and IR photometry of >300 stars apt for the calibration of CanariCam giving an initial density of ~ 1 star per 100 square degrees of sky. TheMartín-Luis, F. et al.
Advertised on:
122005 -
Calibration of the SDSS/SEGUE Spectroscopic PipelineWe describe an ongoing effort to validate the estimated atmospheric parameters (Teff, log g, [Fe/H]) obtained from SDSS spectroscopy (R = 2000) and ugriz photometry, which are being employed for both the previous SDSS-I and the ongoing SEGUE surveys. The spectroscopic pipeline makes use of a number of methods for the estimation of each parameterSivarani, T. et al.
Advertised on:
122005 -
Can solar g-modes be identified from ground-based velocity measurementsThe question of whether or not solar g-modes can be detected and identified from ground observations is addressed. The limitation imposed by the Earth's atmosphere, the background solar noise spectrum at low frequencies, and a poor theoretical knowledge of these modes are mentioned. Using the best uninterrupted full disk velocity measurementsGarcia, C. et al.
Advertised on:
121988