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Please use this identifier to cite or link to this item: http://hdl.handle.net/1942/2515

Title: Recent progresses of the BOLD investigation towards UV detectors for the ESA Solar Orbiter
Authors: Hochedez, JF
Alvarez, J.
Auret, F.D.
Bergonzo, P
Castex, MC
Deneuville, A
Defise, JM
Fleck, B
Gibart, P
Goodman, SA
Hainaut, O
Kleider, JP
Lemaire, P
Monroy, E
Munoz, E
Muret, P
Omnes, F
Pace, E
Pau, JL
Ralchenko, V
Roggen, J
Schuhle, U
Van Hoof, C
MANCA, Jean
NESLADEK, Milos
Issue Date: 2002
Publisher: ELSEVIER SCIENCE SA
Citation: DIAMOND AND RELATED MATERIALS, 11(3-6). p. 427-432
Abstract: BOLD (Blind to the Optical Light Detectors) is an international initiative dedicated to the development of novel imaging detectors for UV solar observations. It relies on the diamond and nitride materials that have lately undergone key advances. The investigation is proposed in view of Solar Orbiter UV instruments, for which the expected properties of the new sensors-visible blindness and radiation hardness-will be highly beneficial. Solar Orbiter is a selected Flexi mission of the European Space Agency (ESA). Despite various improvements over the last few decades, the present UV detectors exhibit limitations inherent to their actual technology. Yet the utmost spatial resolution, temporal cadence, sensitivity, and photometric accuracy will be decisive for the forthcoming space solar missions. The advent of imagers made of a large bandgap semiconductor would surmount many weaknesses, thus opening up new prospects and making the instruments cheaper. As for the ESA Solar Orbiter, the aspiration for wide bandgap semi conductor-based UV detectors is still more sensible, for the spacecraft will approach the Sun where the heat and the radiation fluxes are high. We depict motivations and present activities and programme to achieve revolutionary flight cameras within the Solar Orbiter schedule. (C) 2002 Elsevier Science B.V. All rights reserved.
Notes: Observ Royal Belgique, Solar Phys Dept, B-1180 Brussels, Belgium. Max Planck Inst Aeron, Katlenburg Lindau, Germany. IMEC, Louvain, Belgium. Russian Acad Sci, Inst Gen Phys, Moscow 117942, Russia. Univ Florence, Dept Astron & Space Sci, XUV Lab, I-50125 Florence, Italy. ETSI Telecommun, UPM, Dept Ingn Elect, Madrid 28040, Spain. Inst Mat Res, Diepenbeek, Belgium. Univ Paris 11, Inst Astrophys Spatiale, F-91405 Orsay, France. Ctr Rech Hetero Epitaxie & Applicat, F-06560 Valbonne, France. NASA, Goddard Space Flight Ctr, ESA Space Sci Dept, Greenbelt, MD 20771 USA. Univ Liege, Ctr Spatial Liege, Angleur, Belgium. Etud Proprietes Elect Solides Lab, F-38042 Grenoble 9, France. Univ Paris 13, Phys Lasers Lab, F-93430 Villetaneuse, France. CEA, LETI, DEIN, SPE, F-91191 Gif Sur Yvette, France. Univ Pretoria, Dept Phys, Pretoria, South Africa. Ecole Super Elect, Lab Genie Elect Paris, F-91192 Gif Sur Yvette, France.Hochedez, JF, Observ Royal Belgique, Solar Phys Dept, Circular Av 3, B-1180 Brussels, Belgium.
URI: http://hdl.handle.net/1942/2515
DOI: 10.1016/S0925-9635(02)00034-1
ISI #: 000176046300030
ISSN: 0925-9635
Category: A1
Type: Journal Contribution
Validation: ecoom, 2003
Appears in Collections: Research publications

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