Found 7 talks width keyword cosmic rays

Thursday January 19, 2023


I will review the status of the QUIJOTE (Q-U-I JOint TEnerife) experiment, a project led from the IAC with the aim of characterising the polarisation of the Cosmic Microwave Background (CMB) and other galactic or extragalactic physical processes that emit in microwaves in the frequency range 10-42GHz, and at large angular scales (1 degree resolution). QUIJOTE consists of two telescopes and three instruments operating from the Teide Observatory, and started operations about 10 years ago, in November 2012.

I will discuss the status of the project, and I will present the latest scientific results associated with the wide survey carried out with the first QUIJOTE instrument (MFI) at 11, 13, 17 and 19GHz, covering approximately 29000 deg$^2$ with polarisation sensitivities in the range of 35-40 $\mu$K/deg. These MFI maps provide the most accurate description we have of the polarization of the emission of the Milky Way in the microwave range, in a frequency domain previously unexplored by other experiments. These maps provide a unique view of the Galactic
magnetic field as traced by the synchrotron emission. These results have been presented in an initial series of 6 scientific articles published on January 12th, 2023.

Finally, I will describe the prospects for future CMB observations from the Teide Observatory.

Thursday June 19, 2014
Universidad de Alcala de Henares


The Extreme Universe Space Observatory (EUSO) Space Program on the International Space Station (ISS) is the first space-based mission worldwide in the field of Ultra High Energy Cosmic Rays (UHECR) and Extremely High Energy Cosmic Rays (EHECR) and will contribute to consolidate a new window in the astronomical observation at the highest energies never observed neither with ground-based nor space-based experiments. Currently the international groups working on ground-based UHECR experiments are organized in the Pierre Auger Collaboration (Argentina, South Hemisphere) and the
Telescope Array Collaboration (Utah, North Hemisphere). JEM-EUSO will pioneer from Space the observation from ISS (North & South Hemispheres) of the non thermal Universe and will provide a real breakthrough toward the understanding of the Extreme Universe at the highest energies never detected from Space. In this Severo Ochoa Seminar an overview of the JEM-EUSO Space Mission and the pathfinders currently being developed, EUSO-BALLOON of the French Space Agency (CNES) and MINI-EUSO (ISS) of the Russian Space Agency (Roscosmos) will be presented. Moreover the Spanish Contribution to this EUSO Program under a Coordinated Proposal of MINECO, that involves Instituto de Astrofísica de Canarias (IAC), Instituto Nacional de Técnica Aerospacial (INTA), Universidad Politécnica de Madrid (UPM), Univesidad de Leon (ULE) and Universidad de Alcalá (UAH) will be reviewed as well.

Thursday December 13, 2012
Universidad de Granada


Hablaré de tres caprichos. El primero pretende responder a la pregunta: ¿Existen lentes magnéticas en el Cosmos? El segundo trata de un problema de Milagro, viendo cómo el campo magnético de nuestra galaxia puede resolver la anisotropía en la distribución de rayos cósmicos de unos 10 TeV. El tercero considera las curvas de rotación de algunas galaxias espirales que tras haber alcanzado la velocidad asintótica, vuelve a tener pendiente positiva.

Monday October 22, 2012
ERI, University of Tokyo, Japan
INFN, Napoli, Italy


The origin and structure of the Earth's crust is still a major question. Current measurements of the nearby crust are based largely on seismic, gravimetric and electrical  techniques. In this talk, we introduce a novel method based on cosmic-ray muons to create a direct snapshot of the density profile within a volcano (and/or other geological features).  By measuring the muon
absorption along the different paths through an object (volcano, mountain, a fault, ...), one can deduce the density profile within the object. The major feature of this
technique makes possible for us to perform a tomographic measurement by placing two or more cosmic ray detection
systems around the object. Another strong point of this technique is the possibility to carry out fulltime monitoring, since  muons are incessantly arriving, recalling they are
the most numerous energetic charged particles at sea level.

Thursday March 15, 2012
Hvar Observatory (Zagreb)


Global warming has often been portrayed as being connected only to greenhouse gasses in widespread media. However, these are just one of many factors influencing Earth’s climate. Over long timescales the Sun has been the major force driving climate changes. So-called global warming skeptics often use arguments of natural (solar driven) climate changes to argue that anthropogenic influences on the climate over last century have been largely overestimated. These arguments frequently involve hypothesized solar – climate linkages, for which there is a low level of scientific understanding, making the arguments problematic to easily prove or refute. There are three solar parameters proposed which may influence the Earth’s climate: total solar irradiance (TSI), ultraviolet (UV) spectral irradiance, or the galactic cosmic ray (GCR) flux. In recent years there has been a vigorous debate in scientific community regarding the notion of a cosmic rays influence on clouds cover. If true, such a link could have serious implications for our understanding of climate change: consequently, this has become one of the most frequent arguments of global warming skeptics. This talk will give a short overview of different forcing factors in the climate system, give a description of some hypothesized mechanisms linking solar activity to Earth’s climate, and present our current work aiming to resolve the hypothesized link between cosmic rays and clouds.

Friday October 16, 2009
Max Planck Institute for Physics, Munich, Germany and Eidgenössische Technische Hochschule Zürich, Switzerland


The window of very high energy (VHE) gamma-ray astronomy was only opened 20 years ago by the first observation of TeV gamma-rays from the CRAB nebula. Since then the field is rapidly expanding and we are approaching the first 100 VHE sources. In contrast to the many orders of magnitude larger flux of charged VHE Cosmic Rays, gamma-rays can be extrapolated back to their sources, the high energy particle processes mostly in stellar environments and thus allows us to retrieve basic information about the ultra-relativistic universe. In my talk I will shortly describe the gamma-ray production mechanisms related to these ultra relativistic processes, losses during the transport of gamma-rays through the universe and the detection methods. This is followed by a review of classes of gamma ray emitters and the relation to multi-wavelength respectively multi-messenger observations. Because of the very rich findings of the past years some restriction to highlight observations have to be made. The talk concludes with an outlook for the next years including possible prospects to build the so-called North-CTA (Cherenkov Telescope Array) on the Canary Islands.

Thursday September 10, 2009
University of Roma, Italy


New results on the antiproton-to-proton and positron-to-all electron ratios over a wide energy range (1 – 100 GeV) have been obtained by the PAMELA mission. These data are mainly interpreted in terms of dark matter annihilation or pulsar contribution. The instrument PAMELA, in orbit since June 15th, 2006 on board the Russian satellite Resurs DK1, is daily delivering to ground 16 Gigabytes of data. The apparatus is designed to study charged particles in the cosmic radiation, with a particular focus on antiparticles for searching antimatter and signals of dark matter annihilation. A combination of a magnetic spectrometer and different detectors allows antiparticles to be reliably identified from a large background of other charged particles. The talk will illustrate the most important scientific results obtained by PAMELA, together with some of the more recent theoretical interpretations.

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    Thursday March 7, 2024 - 10:30 GMT  (Aula)
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    Prof. Kentaro Nagamine
    Thursday March 21, 2024 - 10:30 GMT  (Aula)

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