Solar filaments are prominent cold and dense structures of plasma suspended in the hot corona. They are called prominences when observed above the solar limb. Despite they were probably the first solar features to be observed, the magnetic structure of so

• Listing ID: 2008
• Project Leader: INSTITUTO DE ASTROFISICA DE CANARIAS
• Start date: 1/1/2014
• End Date: 12/31/2015
• Region: Canary Islands
• Programme: FP7-PEOPLE-2012-IIF