S
Shane A. Maloney
Researcher at Trinity College, Dublin
Publications - 35
Citations - 1098
Shane A. Maloney is an academic researcher from Trinity College, Dublin. The author has contributed to research in topics: Coronal mass ejection & Solar wind. The author has an hindex of 15, co-authored 29 publications receiving 787 citations. Previous affiliations of Shane A. Maloney include Dublin Institute for Advanced Studies.
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Journal ArticleDOI
The SunPy Project: Open Source Development and Status of the Version 1.0 Core Package
W. T. Barnes,Monica G. Bobra,Steven Christe,N. Freij,Laura A. Hayes,Jack Ireland,Stuart Mumford,David Pérez-Suárez,Daniel F. Ryan,Daniel F. Ryan,Albert Y. Shih,Prateek Chanda,Kolja Glogowski,Kolja Glogowski,Russell J. Hewett,V. Keith Hughitt,Andrew Hill,Kaustubh Hiware,Andrew Inglis,Michael S. Kirk,Michael S. Kirk,Sudarshan Konge,James Mason,Shane A. Maloney,Shane A. Maloney,Sophie A. Murray,Sophie A. Murray,Asish Panda,Jongyeob Park,Tiago M. D. Pereira,Kevin Reardon,Sabrina Savage,Brigitta Sipocz,David Stansby,Yash Jain,Garrison Taylor,Tannmay Yadav,Rajul,Trung Kien Dang +38 more
TL;DR: In this paper, the authors proposed a solar physics division of the American Astronomical Society (AAS) Division of Astronomy Division of the University of Washington (U.W.
Journal ArticleDOI
Propagation of an Earth-directed coronal mass ejection in three dimensions
Jason P. Byrne,Shane A. Maloney,R. T. James McAteer,R. T. James McAteer,Jose Refojo,Peter T. Gallagher +5 more
TL;DR: A new elliptical tie-pointing technique is used to reconstruct a full CME front in 3D, enabling to quantify its deflected trajectory from high latitudes along the ecliptic, and measure its increasing angular width and propagation from 2 to 46 (∼0.2 AU).
Journal ArticleDOI
On the 3-D reconstruction of Coronal Mass Ejections using coronagraph data
Marilena Mierla,Bernd Inhester,A. Antunes,Yannick Boursier,Jason P. Byrne,Robin C. Colaninno,Joseph M. Davila,C. A. de Koning,Peter T. Gallagher,S. Gissot,Russell A. Howard,Timothy A. Howard,M. Kramar,P. L. Lamy,P. C. Liewer,Shane A. Maloney,Christophe Marqué,T. J. McAteer,T. Moran,Luciano Rodriguez,Nandita Srivastava,O. C. Cyr,Guillermo Stenborg,Manuela Temmer,A. Thernisien,Angelos Vourlidas,Matthew J. West,Brian E. Wood,Andrei Zhukov +28 more
TL;DR: In this article, different techniques were used to model the 3D configuration of CMEs in the coronagraph field of view ( up to 15 R-circle dot) and applied these techniques to different CME observed by various coronagraphs.
Journal ArticleDOI
The Spectrometer/Telescope for Imaging X-rays (STIX)
Säm Krucker,Säm Krucker,G. J. Hurford,G. J. Hurford,Oliver Grimm,Oliver Grimm,S. Kögl,H.-P. Gröbelbauer,L. Etesi,Diego Casadei,André Csillaghy,Arnold O. Benz,N. G. Arnold,F. Molendini,Piotr Orleanski,D. Schori,H. Xiao,M. Kuhar,N. Hochmuth,S. Felix,F. Schramka,Simon Marcin,S. Kobler,L. Iseli,M. Dreier,H. J. Wiehl,Lucia Kleint,Marina Battaglia,Erica Lastufka,Erica Lastufka,H. Sathiapal,K. Lapadula,Martin Bednarzik,G. Birrer,St. Stutz,Ch. Wild,F. Marone,Konrad Skup,Andrzej Cichocki,K. Ber,Konrad Rutkowski,Waldemar Bujwan,G. Juchnikowski,M. Winkler,M. Darmetko,M. Michalska,Karol Seweryn,A. Białek,Piotr Osica,Janusz Sylwester,Miroslaw Kowalinski,D. Ścisłowski,Marek Siarkowski,Marek Stęślicki,Tomasz Mrozek,Tomasz Mrozek,Piotr Podgorski,A. Meuris,O. Limousin,O. Gevin,I. Le Mer,S. Brun,Antoine Strugarek,N. Vilmer,Sophie Musset,Sophie Musset,Milan Maksimovic,František Fárník,Z. Kozáček,Jana Kašparová,G. Mann,H. Önel,Alexander Warmuth,J. Rendtel,J. Anderson,Svend-Marian Bauer,Frank Dionies,J. Paschke,D. Plüschke,M. Woche,F. Schuller,Astrid M. Veronig,Ewan C. Dickson,Peter T. Gallagher,Peter T. Gallagher,Shane A. Maloney,Shane A. Maloney,D. S. Bloomfield,D. S. Bloomfield,Michele Piana,Anna Maria Massone,Federico Benvenuto,Paolo Massa,R. A. Schwartz,R. A. Schwartz,R. A. Schwartz,Brian R. Dennis,H. F. van Beek,Javier Rodriguez-Pacheco,Robert P. Lin +99 more
TL;DR: The Spectrometer Telescope for Imaging X-rays (STIX) as mentioned in this paper is a hard X-ray imaging spectrometer, which covers the energy range from 4 to 150 keV and provides diagnostics of the hottest (⪆10 MK) flare plasma while quantifying the location, spectrum, and energy content of flare-accelerated nonthermal electrons.
Journal ArticleDOI
Models and data analysis tools for the Solar Orbiter mission
Alexis P. Rouillard,Rui F. Pinto,Rui F. Pinto,Angelos Vourlidas,A. De Groof,William T. Thompson,Alessandro Bemporad,S. Dolei,Mikel Indurain,Eric Buchlin,Clementina Sasso,Daniele Spadaro,Kévin Dalmasse,Johann Hirzberger,I. Zouganelis,Antoine Strugarek,A. S. Brun,Matthieu Alexandre,David Berghmans,N. E. Raouafi,Thomas Wiegelmann,Paolo Pagano,C. N. Arge,Teresa Nieves-Chinchilla,Teresa Nieves-Chinchilla,Michael Lavarra,Nicolas Poirier,T. Amari,Angels Aran,Vincenzo Andretta,Ester Antonucci,Anastasios Anastasiadis,F. Auchère,L. R. Bellot Rubio,Bogdan Nicula,X. Bonnin,M. Bouchemit,E. Budnik,S. Caminade,Baptiste Cecconi,J. Carlyle,I. Cernuda,Joseph M. Davila,L. Etesi,F. Espinosa Lara,Andrei Fedorov,Silvano Fineschi,Andrzej Fludra,Vincent Génot,Manolis K. Georgoulis,Manolis K. Georgoulis,Holly Gilbert,A. Giunta,Raul Gomez-Herrero,S. Guest,M. Haberreiter,Donald M. Hassler,Carl J. Henney,R. A. Howard,Timothy S. Horbury,Miho Janvier,S. I. Jones,S. I. Jones,Kamen Kozarev,E. Kraaikamp,A. Kouloumvakos,Säm Krucker,Andreas Lagg,Jon A. Linker,Benoit Lavraud,Benoit Lavraud,Philippe Louarn,Milan Maksimovic,Shane A. Maloney,G. Mann,Arnaud Masson,Daniel Müller,H. Önel,Pedro Osuna,D. Orozco Suárez,Christopher J. Owen,Athanasios Papaioannou,David Pérez-Suárez,Javier Rodriguez-Pacheco,S. Parenti,Etienne Pariat,Hardi Peter,Simon Plunkett,Jens Pomoell,Jim M. Raines,Tino L. Riethmüller,N. Rich,Luciano Rodriguez,Marco Romoli,L. Sanchez,Sami K. Solanki,Sami K. Solanki,O. C. St. Cyr,Thomas Straus,Roberto Susino,Luca Teriaca,J. C. del Toro Iniesta,Rita Ventura,Cis Verbeeck,Nicole Vilmer,Alexander Warmuth,Andrew Walsh,C. Watson,David R. Williams,Y. Wu,Y. Wu,Andrei Zhukov,Andrei Zhukov +112 more
TL;DR: In this paper, a review of the current modelling of the Sun and its atmosphere can support Solar Orbiter science is presented. But the focus here is on the large scales and little is described with regards to kinetic processes.