H. Mapson-Menard
University of Birmingham
3 Papers
H. Mapson-Menard is an academic researcher from University of Birmingham. The author has contributed to research in topics: Telescope & Coronal loop. The author has an hindex of 2, co-authored 3 publications.
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Papers
Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI)
Russell A. Howard,John D. Moses,Angelos Vourlidas,Jeffrey S. Newmark,Dennis G. Socker,Simon Plunkett,Clarence M. Korendyke,J. W. Cook,A. Hurley,Joseph M. Davila,William T. Thompson,O. C. St. Cyr,E. Mentzell,Kimberly I. Mehalick,James R. Lemen,Jean-Pierre Wuelser,Dexter W. Duncan,T. D. Tarbell,C. J. Wolfson,A. Moore,Richard A. Harrison,Nicholas R. Waltham,J. Lang,Christopher J. Davis,C. J. Eyles,H. Mapson-Menard,G. M. Simnett,Jean-Philippe Halain,Jean-Marc Defise,Emmanuel Mazy,Pierre Rochus,Raymond Mercier,Marie-Françoise Ravet,Franck Delmotte,F. Auchère,Jean-Pierre Delaboudiniere,Volker Bothmer,W. Deutsch,Dennis Wang,N. Rich,S. Cooper,V. Stephens,G. Maahs,R. Baugh,D. R. McMullin,T. Carter +45 more
TL;DR: The Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) is a five telescope package, which has been developed for the Solar Terrestrial Relation Observatory (STEREO) mission.
The EUV Imaging Spectrometer for Hinode
J. L. Culhane,Louise K. Harra,A. M. James,K. Al-Janabi,L. Bradley,Rifat A Chaudry,Kerrin Rees,J. Tandy,P. D. Thomas,M. C. R. Whillock,Berend Winter,George A. Doschek,Clarence M. Korendyke,Charles M. Brown,S. H. Myers,J. T. Mariska,John F. Seely,J. Lang,B. J. Kent,B. M. Shaughnessy,Peter R. Young,G. M. Simnett,C. M. Castelli,S. Mahmoud,H. Mapson-Menard,Brian J. Probyn,Roger J. Thomas,Joseph M. Davila,Kenneth P. Dere,David L. Windt,John Shea,R. Hagood,Robert W. Moye,Hirohisa Hara,Takashi Watanabe,K. Matsuzaki,Takeo Kosugi,Viggo Hansteen,Ø. Wikstol +38 more
TL;DR: The EUV Imaging Spectrometer (EIS) as mentioned in this paper is a two-element, normal incidence design with a backside-illuminated, thinned CCD, which has a significantly greater effective area than previous orbiting EUV spectrographs with typical active region 2 -5 s exposure times in the brightest lines.
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The Carbon Fibre Structure for the Extreme Ultraviolet Imaging Spectrometer on the Solar-B Satellite
C Castelli,R Hagood,H. Mapson-Menard,Berend Winter +3 more
- 01 Jul 2005
TL;DR: The Extreme Ultraviolet Imaging Spectrometer (EIS) is a core instrument on the Japanese Solar-B mission and is due for launch in the summer of 2006 as discussed by the authors, which is a 3.2 m long telescope employing grating optics and a pair of charge coupled device imaging cameras working in the extreme ultraviolet (EUV) region in two separate wavelength bands between 170-210 and 240-290 A.