S. D. Sidher
Rutherford Appleton Laboratory
8 Papers
37 Citations
S. D. Sidher is an academic researcher from Rutherford Appleton Laboratory. The author has contributed to research in topics: Spectrometer & Mars Exploration Program. The author has an hindex of 4, co-authored 7 publications. Previous affiliations of S. D. Sidher include Queen Mary University of London.
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Papers
The D/H ratio in the atmospheres of Uranus and Neptune from Herschel-PACS observations
H. Feuchtgruber,Emmanuel Lellouch,G. S. Orton,T. de Graauw,Bart Vandenbussche,Bruce Swinyard,Bruce Swinyard,Raphael Moreno,C. Jarchow,F. Billebaud,Thibault Cavalié,S. D. Sidher,Paul Hartogh +12 more
TL;DR: In this article, the rotational R(0) and R(1) HD lines in the atmospheres of Uranus and Neptune were analyzed in order to derive a D/H ratio with improved precision for both planets.
ISO Observations of Mars: An Estimate of the Water Vapor Vertical Distribution and the Surface Emissivity
Martin Burgdorf,Th. Encrenaz,E. Lellouch,Helmut Feuchtgruber,Gary R. Davis,Bruce Swinyard,Th. de Graauw,Patrick W. Morris,S. D. Sidher,S. D. Sidher,Matthew Joseph Griffin,François Forget,T. L. Lim +12 more
TL;DR: In this paper, two complementary spectrometers onboard the European Space Agency's Infrared Space Observatory (ISO) in both moderate and high-resolution mode were used to extract the infrared spectra of Mars.
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A multiple spacecraft detection of the 2 April 2022 M-class flare and filament eruption during the first close Solar Orbiter perihelion
Miho Janvier,Peter C. Young,'Eric Buchlin,Anna Manou,Gabriel Pelouze,David Long,L. Green,Alexander Warmuth,Frederic Schuller,D. Calchetti,Fatima Kahil,L. R. Bellot Rubio,Susanna Parenti,Selima Baccar,Louise K. Harra,Laura A. Hayes,William B. Thompson,D. Muller,D. N. Baker,Stephanie L. Yardley,David Berghmans,Cis Verbeeck,P. J. Smith,H. Peter,R. Aznar Cuadrado,Sophie Musset,David H. Brooks,Luciano Rodriguez,F. Auchère,T Carlsson,Andrzej Fludra,Donald M. Hassler,D. J. Williams,M. Caldwell,T. Fredvik,A. Giunta,T. Grundy,S. Guest,E. Kraaikamp,S. J. Leeks,Joseph Plowman,Werner Schmutz,U. Schuhle,S. D. Sidher,Luca Teriaca,Sami K. Solanki,J. C. del Toro Iniesta,Joachim Woch,Achim Gandorfer,Johann Hirzberger,D. Orozco Suárez,Thierry Appourchaux,Gherardo Valori,J. Sinjan,Kinga Albert,Reiner Volkmer +55 more
TL;DR: In this article , an M-class flare followed by a filament eruption was seen both by the instruments on board the mission and from several observatories in Earth's orbit, including IRIS, SDO, Hinode, as well as several instruments on Solar Orbiter.
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In-flight calibration of the Herschel-SPIRE instrument
B. M. Swinyard,Peter A. R. Ade,Jean-Paul Baluteau,Herve Aussel,M. J. Barlow,George J. Bendo,Dominique Benielli,James J. Bock,Drew Brisbin,A. Conley,L. Conversi,A. Dowell,Darren Dowell,Marc Ferlet,T. Fulton,Jason Glenn,Adrian M. Glauser,Adrian M. Glauser,Douglas Griffin,Matthew Joseph Griffin,S. Guest,P. Imhof,Kate Gudrun Isaak,S. C. Jones,K. J. King,S. J. Leeks,L. R. Levenson,T. L. Lim,Nanyao Y. Lu,Gibion Makiwa,David A. Naylor,Hien Nguyen,Seb Oliver,Pasquale Panuzzo,Andreas Papageorgiou,C. P. Pearson,C. P. Pearson,Michael Pohlen,Edward Polehampton,Edward Polehampton,D. Pouliquen,Dimitra Rigopoulou,Dimitra Rigopoulou,S. Ronayette,Helene Roussel,A. Rykala,Giorgio Savini,Bernhard Schulz,Arnold A. Schwartz,David L. Shupe,Bruce Sibthorpe,S. D. Sidher,Anthony J. Smith,Locke D. Spencer,Markos Trichas,H. Triou,Ivan Valtchanov,Roger Wesson,Adam Woodcraft,C. K. Xu,Michael Zemcov,L. Zhang +61 more
TL;DR: In this paper, the authors present the photometric, spectroscopic and spatial accuracy of the SPIRE system using a combination of the emission from the Herschel telescope itself and the modelled continuum emission from solar system objects and other astronomical targets.
The D/H ratio in the atmospheres of Uranus and Neptune from Herschel PACS observations
H. Feuchtgruber,Emmanuel Lellouch,G. S. Orton,T. de Graauw,Bart Vandenbussche,Bruce Swinyard,Bruce Swinyard,Raphael Moreno,C. Jarchow,F. Billebaud,Thibault Cavalié,S. D. Sidher,Paul Hartogh +12 more
TL;DR: In this article, the rotational R(0) and R(1) HD lines in the atmospheres of Uranus and Neptune were analyzed in order to derive a D/H ratio with improved precision for both planets.
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