'53 cr' diaporamas de présentation

Collaborations: L. Santos (Hannover) Students : Antoine Reigue, Ariane

509 views • 36 slides

Collaborations: L. Santos (Hannover) Students : Antoine Reigue, Ariane

369 views • 36 slides

Sample return from C-type asteroids: What will we bring back?

Sample return from C-type asteroids: What will we bring back? . Paula Lindgren School of Geographical and Earth Sciences University of Glasgow SPACE Glasgow Research C onference University of Glasgow 2 8 th Oct 2014. Asteroids. Leftovers from the building blocks of our solar system

301 views • 20 slides

Sample return from C-type asteroids: What will we bring back?

Sample return from C-type asteroids: What will we bring back? . Paula Lindgren School of Geographical and Earth Sciences University of Glasgow SPACE Glasgow Research C onference University of Glasgow 2 8 th Oct 2014. Asteroids. Leftovers from the building blocks of our solar system

206 views • 20 slides

50,52,53,54 Cr Resonance Evaluation at ORNL

50,52,53,54 Cr Resonance Evaluation at ORNL. L. Leal, H. Derrien, K. Guber, G. Arbanas and D. Wiarda Nuclear Data Group Oak Ridge National Laboratory. IAEA, March 23-26, 2010. Computer Code SAMMY. Used for analysis of neutron, charged-particle cross- section data.

317 views • 19 slides