Computer Science
Scientific paper
Jul 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spie.6266e..15m&link_type=abstract
Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray. Edited by Turner, Martin J. L.; Hasinger, Günther. Proceedi
Computer Science
1
Scientific paper
SMESE (SMall Explorer For the study of Solar Eruptions) is a Franco-Chinese microsatellite mission. The scientific objectives of SMESE are the study of coronal mass ejections and flares. Its payload consists of three instrument packages : LYOT, DESIR and HEBS. LYOT is composed of a Lyman α (121.6 nm) coronagraph, a Lyman α disk imager and a far UV disk imager. DESIR is an infrared telescope working at 35 μm and 150 μm. HEBS is a high energy burst spectrometer working in X rays and γ rays covering the 10 keV to 600 MeV range. SMESE will be launched around 2011, providing a unique opportunity of detecting and understanding eruptions at the maximum activity phase of the solar cycle in a wide range of energies. The instrumentation on board SMESE is described in this paper.
Auchere Frédéric
Fang Cheng
Gan Weiqun
Millard Anne A.
Molodij Guillaume
No associations
LandOfFree
SMESE: a combined UV-IR-X-gamma solar mission does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with SMESE: a combined UV-IR-X-gamma solar mission, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and SMESE: a combined UV-IR-X-gamma solar mission will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1620282