Archiving project of Specola Solare Ticinese sunspot drawings in collaboration with ETH-Zurich University Archives and GCOS

Thanks to its high correlation with the total solar irradiance, the Sunspot Number (SSN), which represents a 400 years long observational data series, was recently recognized in the latest implementation plan of the Global Climate Observing System (GCOS) as valuable information for climate studies. In Switzerland systematic observations of sunspots started in 1847 by Rudolf Wolf, first in Bern and then at the Federal Observatory in Zurich. Its former external observing station Specola Solare in Locarno, built in 1957, became in 1981 the reference station of the SSN, at the same time when the world data center was transferred from Zurich to the Royal Observatory in Brussels at SILSO.

To ensure that the historical sunspot drawings and data of Specola Solare are archived in the long run, MeteoSwiss in the framework of GCOS Switzerland has decided to support the archiving and digitization of these drawings and data at the ETH Library in Zurich. The project is a joint effort by the Associazione Specola Solare Ticinese (ASST) in Locarno and the ETH Zurich and runs for 5 years.

SNSF Sinergia project involving IRSOL, USI, and IAC approved

The Swiss National Science Foundation (SNSF), within the framework of the “Sinergia” financing programme, has approved a cooperation project involving IRSOL, the Institute of Computational Sciences of Università della Svizzera italiana (USI), and the Instituto de Astrofisica de Canarias (IAC) in Tenerife (Spain).
The project, with title “HPC-techniques for 3D modeling of resonance line polarization with PRD”, aims at developing new numerical methods necessary for modeling the intensity and polarization of the solar radiation from three-dimensional (3D) models of the atmosphere of the Sun, taking partial frequency redistribution (PRD) phenomena into account.
The possibility to carry out such theoretical modeling represents a key step towards the development of new reliable diagnostic techniques for investigating the magnetism of the chromosphere and transition region. This problem is far from trivial, especially from the computational point of view, and indeed it requires merging competences in solar physics, in the theory of the generation and transfer of polarized radiation, and in computational sciences.
The project will allow us to offer a post-doctoral position of four years in each one of the institutes involved, plus a PhD position at the Università della Svizzera italiana (USI).
The contracts will start between the end of 2018 and the first months of 2019.