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@ARTICLE{sunpy_community2020,
doi = {10.3847/1538-4357/ab4f7a},
url = {https://iopscience.iop.org/article/10.3847/1538-4357/ab4f7a},
author = {{The SunPy Community} and Barnes, Will T. and Bobra, Monica G. and Christe, Steven D. and Freij, Nabil and Hayes, Laura A. and Ireland, Jack and Mumford, Stuart and Perez-Suarez, David and Ryan, Daniel F. and Shih, Albert Y. and Chanda, Prateek and Glogowski, Kolja and Hewett, Russell and Hughitt, V. Keith and Hill, Andrew and Hiware, Kaustubh and Inglis, Andrew and Kirk, Michael S. F. and Konge, Sudarshan and Mason, James Paul and Maloney, Shane Anthony and Murray, Sophie A. and Panda, Asish and Park, Jongyeob and Pereira, Tiago M. D. and Reardon, Kevin and Savage, Sabrina and Sipőcz, Brigitta M. and Stansby, David and Jain, Yash and Taylor, Garrison and Yadav, Tannmay and Rajul and Dang, Trung Kien},
title = {The SunPy Project: Open Source Development and Status of the Version 1.0 Core Package},
journal = {The Astrophysical Journal},
volume = {890},
issue = {1},
pages = {68-},
publisher = {American Astronomical Society},
year = {2020}
}
@article{Glogowski2019drms,
title = {drms: A Python package for accessing HMI and AIA data},
author = {Glogowski, Kolja and Bobra, Monica and Choudhary, Nitin and Amezcua, Arthur and Mumford, Stuart},
year = 2019,
month = 8,
day = 20,
journal = {Journal of Open Source Software},
publisher = {The Open Journal},
volume = 4,
number = 40,
pages = 1614,
doi = {10.21105/joss.01614},
issn = {2475-9066},
date = {2019-08-20}
}
@article{2009EM&P..104..315H,
title = {{The Virtual Solar Observatory{\textemdash}A Resource for International Heliophysics Research}},
author = {{Hill}, Frank and {Martens}, Piet and {Yoshimura}, Keji and {Gurman}, Joseph and {Hourcl{\'e}}, Joseph and {Dimitoglou}, George and {Su{\'a}rez-Sol{\'a}}, Igor and {Wampler}, Steve and {Reardon}, Kevin and {Davey}, Alisdair and {Bogart}, Richard S. and {Tian}, Karen Q.},
year = 2009,
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pages = {315--330},
doi = {10.1007/s11038-008-9274-7},
keywords = {Data management, Virtual observatories, Solar physics, Distributed archives}
}
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title = {Definition of the Flexible Image Transport System (FITS), version 3.0},
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year = 2010,
month = {},
journal = {Astronomy \& Astrophysics},
volume = 524,
pages = {A42},
doi = {10.1051/0004-6361/201015362}
}
@article{sep-0001,
title = {{SunPy Proposal for Enhancement 1: SEP Purpose and Guidelines (SEP 0001)}},
author = {Christe, Steven},
year = 2014,
month = mar,
doi = {10.5281/zenodo.3261403},
url = {https://doi.org/10.5281/zenodo.3261403}
}
@article{sep-0002,
title = {{SunPy Proposal for Enhancement 2: SunPy Organization Definition (SEP 0002)}},
author = {Christe, Steven},
year = 2018,
month = dec,
doi = {10.5281/zenodo.3261663},
url = {https://doi.org/10.5281/zenodo.3261663}
}
@article{sep-0003,
title = {{SunPy Proposal for Enhancement 3: Physical Units in SunPy (SEP 0003)}},
author = {Christe, Steven},
year = 2014,
month = jul,
doi = {10.5281/zenodo.3261707},
url = {https://doi.org/10.5281/zenodo.3261707}
}
@article{sep-0004,
title = {{SunPy Proposal for Enhancement 4: Packages Affiliated with the SunPy Project (SEP 0004)}},
author = {Mumford, Stuart and Christe, Steven},
year = 2014,
month = oct,
doi = {10.5281/zenodo.3261752},
url = {https://doi.org/10.5281/zenodo.3261752}
}
@article{sep-0005,
title = {{SunPy Proposal for Enhancement 5: Coordinates Module (SEP 0005)}},
author = {Chakraborty, Pritish and Mumford, Stuart},
year = 2019,
month = jun,
doi = {10.5281/zenodo.3261768},
url = {https://doi.org/10.5281/zenodo.3261768}
}
@article{sep-0006,
title = {{SunPy Proposal for Enhancement 6: SunPy Board Membership List (SEP 0006)}},
author = {Christe, Steven},
year = 2019,
month = apr,
doi = {10.5281/zenodo.3261786},
url = {https://doi.org/10.5281/zenodo.3261786}
}
@article{sep-0007,
title = {{SunPy Proposal for Enhancement 7: Lightcurve Factory Refactor (SEP 0007)}},
author = {Mumford, Stuart},
year = 2015,
month = dec,
doi = {10.5281/zenodo.3261788},
url = {https://doi.org/10.5281/zenodo.3261788}
}
@article{sep-0008,
title = {{SunPy Proposal for Enhancement 8: Astropy Time (SEP 0008)}},
author = {Mumford, Stuart},
year = 2018,
month = sep,
doi = {10.5281/zenodo.3261794},
url = {https://doi.org/10.5281/zenodo.3261794}
}
@article{sep-0009,
title = {{SunPy Proposal for Enhancement 9: Release Pattern for SunPy Core (SEP 0009)}},
author = {Mumford, Stuart and Hewett, Russell},
year = 2019,
month = jun,
doi = {10.5281/zenodo.3261800},
url = {https://doi.org/10.5281/zenodo.3261800}
}
@article{pyhcStandards,
title = {Python in Heliophysics Community (PyHC) Standards},
author = {Annex, A. and Alterman, B. L. and Azari, A. and Barnes, W. and Bobra, M. and Cecconi, B. and Christe, Steven and Coxon, J. and DeWolfe, A. and Halford, A. and et al.},
year = 2018,
month = dec,
publisher = {Zenodo},
doi = {10.5281/zenodo.2529131},
}
@article{2002A&A...395.1061G,
title = {{Representations of world coordinates in FITS}},
author = {{Greisen}, E.~W. and {Calabretta}, M.~R.},
year = 2002,
month = dec,
journal = {Astronomy \& Astrophysics},
volume = 395,
pages = {1061--1075},
doi = {10.1051/0004-6361:20021326},
keywords = {methods: data analysis, techniques: image processing, astronomical data bases: miscellaneous, Astrophysics},
archiveprefix = {arXiv},
eprint = {astro-ph/0207407},
primaryclass = {astro-ph},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{Freeland:1998we,
title = {{Data analysis with the SolarSoft system}},
author = {Freeland, S and Handy, B N},
year = 1998,
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volume = 182,
number = 2,
pages = {497--500}
}
@article{Community:2015cy,
title = {{SunPy{\textemdash}Python for solar physics}},
author = {{The SunPy Community} and Mumford, Stuart J and Christe, Steven D and P{\'e}rez-Su{\'a}rez, David and Ireland, Jack and Shih, Albert and Inglis, Andrew R and Liedtke, Simon and Hewett, Russell J and Mayer, Florian and Hughitt, Keith and Freij, Nabil and Meszaros, Tomas and Bennett, Samuel M and Malocha, Michael and Evans, John and Agrawal, Ankit and Leonard, Andrew J and Robitaille, Thomas P and Mampaey, Benjamin and Campos-Rozo, Jose Iv{\'a}n and Kirk, Michael S},
year = 2015,
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}
@article{Muna2016,
title = {{The Astropy Problem}},
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year = 2016,
month = oct,
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pages = {arXiv:1610.03159},
keywords = {Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Physics and Society},
eid = {arXiv:1610.03159},
archiveprefix = {arXiv},
eprint = {1610.03159},
primaryclass = {astro-ph.IM}
}
@article{thompson_coordinate_2006,
title = {{Coordinate systems for solar image data}},
author = {{Thompson}, W.~T.},
year = 2006,
month = apr,
journal = {Astronomy \& Astrophysics},
volume = 449,
pages = {791--803},
doi = {10.1051/0004-6361:20054262},
keywords = {standards, Sun: general, techniques: image processing, astronomical data bases: miscellaneous, methods: data analysis}
}
@manual{bobra_monica_2020_7020094,
title = {{SunPy Proposal for Enhancement 10: Vision and
Mission Statement (SEP 0010)}},
author = {Bobra, Monica and
Bin, Chen and
Christe, Steven and
Hewett, Russell and
Freij, Nabil and
Mumford, Stuart and
Pereira, Tiago and
Pérez-Suárez, David and
Reardon, Kevin and
Ryan, Daniel F. and
Savage, Sabrina},
month = sep,
year = 2020,
doi = {10.5281/zenodo.7020094},
url = {https://doi.org/10.5281/zenodo.7020094}
}
@article{barnes_aiapy_2020,
title = {Aiapy: {{A Python Package}} for {{Analyzing Solar EUV Image Data}} from {{AIA}}},
shorttitle = {Aiapy},
author = {Barnes, Will and Cheung, Mark and Bobra, Monica and Boerner, Paul and Chintzoglou, Georgios and Leonard, Drew and Mumford, Stuart and Padmanabhan, Nicholas and Shih, Albert and Shirman, Nina and Stansby, David and Wright, Paul},
year = {2020},
month = nov,
journal = {The Journal of Open Source Software},
volume = {5},
pages = {2801},
doi = {10.21105/joss.02801},
abstract = {Not Available},
keywords = {Astronomy,Python,Solar Physics},
}
@article{stansby_pfsspy_2020,
title = {pfsspy: {{A Python}} Package for Potential Field Source Surface Modelling},
shorttitle = {Pfsspy},
author = {Stansby, David and Yeates, Anthony and Badman, Samuel},
year = {2020},
month = oct,
journal = {The Journal of Open Source Software},
volume = {5},
pages = {2732},
doi = {10.21105/joss.02732},
abstract = {Not Available},
keywords = {Astronomy,Python,Solar physics},
}
@article{astropy_collaboration_astropy:_2013,
title = {Astropy: {{A}} Community {{Python}} Package for Astronomy},
shorttitle = {Astropy},
author = {{Astropy Collaboration} and Robitaille, Thomas P. and Tollerud, Erik J. and Greenfield, Perry and Droettboom, Michael and Bray, Erik and Aldcroft, Tom and Davis, Matt and Ginsburg, Adam and {Price-Whelan}, Adrian M. and Kerzendorf, Wolfgang E. and Conley, Alexander and Crighton, Neil and Barbary, Kyle and Muna, Demitri and Ferguson, Henry and Grollier, Fr{\'e}d{\'e}ric and Parikh, Madhura M. and Nair, Prasanth H. and Unther, Hans M. and Deil, Christoph and Woillez, Julien and Conseil, Simon and Kramer, Roban and Turner, James E. H. and Singer, Leo and Fox, Ryan and Weaver, Benjamin A. and Zabalza, Victor and Edwards, Zachary I. and Azalee Bostroem, K. and Burke, D. J. and Casey, Andrew R. and Crawford, Steven M. and Dencheva, Nadia and Ely, Justin and Jenness, Tim and Labrie, Kathleen and Lim, Pey Lian and Pierfederici, Francesco and Pontzen, Andrew and Ptak, Andy and Refsdal, Brian and Servillat, Mathieu and Streicher, Ole},
year = {2013},
month = oct,
journal = {Astronomy and Astrophysics},
volume = {558},
pages = {A33},
issn = {0004-6361},
doi = {10.1051/0004-6361/201322068},
abstract = {We present the first public version (v0.2) of the open-source and community-developed Python package, Astropy. This package provides core astronomy-related functionality to the community, including support for domain-specific file formats such as flexible image transport system (FITS) files, Virtual Observatory (VO) tables, and common ASCII table formats, unit and physical quantity conversions, physical constants specific to astronomy, celestial coordinate and time transformations, world coordinate system (WCS) support, generalized containers for representing gridded as well as tabular data, and a framework for cosmological transformations and conversions. Significant functionality is under activedevelopment, such as a model fitting framework, VO client and server tools, and aperture and point spread function (PSF) photometry tools. The core development team is actively making additions and enhancements to the current code base, and we encourage anyone interested to participate in the development of future Astropy versions.},
keywords = {methods: data analysis,methods: miscellaneous,virtual observatory tools}
}
@article{the_astropy_collaboration_astropy_2018,
title = {The {{Astropy Project}}: {{Building}} an {{Open-science Project}} and {{Status}} of the v2.0 {{Core Package}}},
shorttitle = {The {{Astropy Project}}},
author = {{The Astropy Collaboration} and {Price-Whelan}, A. M. and Sip{\H o}cz, B. M. and G{\"u}nther, H. M. and Lim, P. L. and Crawford, S. M. and Conseil, S. and Shupe, D. L. and Craig, M. W. and Dencheva, N. and Ginsburg, A. and VanderPlas, J. T. and Bradley, L. D. and {P{\'e}rez-Su{\'a}rez}, D. and {de Val-Borro}, M. and Aldcroft, T. L. and Cruz, K. L. and Robitaille, T. P. and Tollerud, E. J. and Ardelean, C. and Babej, T. and Bach, Y. P. and Bachetti, M. and Bakanov, A. V. and Bamford, S. P. and Barentsen, G. and Barmby, P. and Baumbach, A. and Berry, K. L. and Biscani, F. and Boquien, M. and Bostroem, K. A. and Bouma, L. G. and Brammer, G. B. and Bray, E. M. and Breytenbach, H. and Buddelmeijer, H. and Burke, D. J. and Calderone, G. and Cano Rodr{\'i}guez, J. L. and Cara, M. and Cardoso, J. V. M. and Cheedella, S. and Copin, Y. and Corrales, L. and Crichton, D. and D'Avella, D. and Deil, C. and Depagne, {\'E}. and Dietrich, J. P. and Donath, A. and Droettboom, M. and Earl, N. and Erben, T. and Fabbro, S. and Ferreira, L. A. and Finethy, T. and Fox, R. T. and Garrison, L. H. and Gibbons, S. L. J. and Goldstein, D. A. and Gommers, R. and Greco, J. P. and Greenfield, P. and Groener, A. M. and Grollier, F. and Hagen, A. and Hirst, P. and Homeier, D. and Horton, A. J. and Hosseinzadeh, G. and Hu, L. and Hunkeler, J. S. and Ivezi{\'c}, {\v Z}. and Jain, A. and Jenness, T. and Kanarek, G. and Kendrew, S. and Kern, N. S. and Kerzendorf, W. E. and Khvalko, A. and King, J. and Kirkby, D. and Kulkarni, A. M. and Kumar, A. and Lee, A. and Lenz, D. and Littlefair, S. P. and Ma, Z. and Macleod, D. M. and Mastropietro, M. and McCully, C. and Montagnac, S. and Morris, B. M. and Mueller, M. and Mumford, S. J. and Muna, D. and Murphy, N. A. and Nelson, S. and Nguyen, G. H. and Ninan, J. P. and N{\"o}the, M. and Ogaz, S. and Oh, S. and Parejko, J. K. and Parley, N. and Pascual, S. and Patil, R. and Patil, A. A. and Plunkett, A. L. and Prochaska, J. X. and Rastogi, T. and Reddy Janga, V. and Sabater, J. and Sakurikar, P. and Seifert, M. and Sherbert, L. E. and {Sherwood-Taylor}, H. and Shih, A. Y. and Sick, J. and Silbiger, M. T. and Singanamalla, S. and Singer, L. P. and Sladen, P. H. and Sooley, K. A. and Sornarajah, S. and Streicher, O. and Teuben, P. and Thomas, S. W. and Tremblay, G. R. and Turner, J. E. H. and Terr{\'o}n, V. and {van Kerkwijk}, M. H. and {de la Vega}, A. and Watkins, L. L. and Weaver, B. A. and Whitmore, J. B. and Woillez, J. and Zabalza, V.},
year = {2018},
month = sep,
journal = {The Astronomical Journal},
volume = {156},
pages = {123},
issn = {0004-6256},
doi = {10.3847/1538-3881/aabc4f},
abstract = {The Astropy Project supports and fosters the development of open-source and openly developed Python packages that provide commonly needed functionality to the astronomical community. A key element of the Astropy Project is the core package astropy, which serves as the foundation for more specialized projects and packages. In this article, we provide an overview of the organization of the Astropy project and summarize key features in the core package, as of the recent major release, version 2.0. We then describe the project infrastructure designed to facilitate and support development for a broader ecosystem of interoperable packages. We conclude with a future outlook of planned new features and directions for the broader Astropy Project. .},
keywords = {methods: data analysis,methods: miscellaneous,methods: statistical,reference systems}
}
@article{astropy_collaboration_astropy_2022,
title = {The {{Astropy Project}}: {{Sustaining}} and {{Growing}} a {{Community-oriented Open-source Project}} and the {{Latest Major Release}} (v5.0) of the {{Core Package}}},
shorttitle = {The {{Astropy Project}}},
author = {{Astropy Collaboration} and {Price-Whelan}, Adrian M. and Lim, Pey Lian and Earl, Nicholas and Starkman, Nathaniel and Bradley, Larry and Shupe, David L. and Patil, Aarya A. and Corrales, Lia and Brasseur, C. E. and N{\"o}the, Maximilian and Donath, Axel and Tollerud, Erik and Morris, Brett M. and Ginsburg, Adam and Vaher, Eero and Weaver, Benjamin A. and Tocknell, James and Jamieson, William and {van Kerkwijk}, Marten H. and Robitaille, Thomas P. and Merry, Bruce and Bachetti, Matteo and G{\"u}nther, H. Moritz and Aldcroft, Thomas L. and {Alvarado-Montes}, Jaime A. and Archibald, Anne M. and B{\'o}di, Attila and Bapat, Shreyas and Barentsen, Geert and Baz{\'a}n, Juanjo and Biswas, Manish and Boquien, M{\'e}d{\'e}ric and Burke, D. J. and Cara, Daria and Cara, Mihai and Conroy, Kyle E. and Conseil, Simon and Craig, Matthew W. and Cross, Robert M. and Cruz, Kelle L. and D'Eugenio, Francesco and Dencheva, Nadia and Devillepoix, Hadrien A. R. and Dietrich, J{\"o}rg P. and Eigenbrot, Arthur Davis and Erben, Thomas and Ferreira, Leonardo and {Foreman-Mackey}, Daniel and Fox, Ryan and Freij, Nabil and Garg, Suyog and Geda, Robel and Glattly, Lauren and Gondhalekar, Yash and Gordon, Karl D. and Grant, David and Greenfield, Perry and Groener, Austen M. and Guest, Steve and Gurovich, Sebastian and Handberg, Rasmus and Hart, Akeem and {Hatfield-Dodds}, Zac and Homeier, Derek and Hosseinzadeh, Griffin and Jenness, Tim and Jones, Craig K. and Joseph, Prajwel and Kalmbach, J. Bryce and Karamehmetoglu, Emir and Ka{\l}uszy{\'n}ski, Miko{\l}aj and Kelley, Michael S. P. and Kern, Nicholas and Kerzendorf, Wolfgang E. and Koch, Eric W. and Kulumani, Shankar and Lee, Antony and Ly, Chun and Ma, Zhiyuan and MacBride, Conor and Maljaars, Jakob M. and Muna, Demitri and Murphy, N. A. and Norman, Henrik and O'Steen, Richard and Oman, Kyle A. and Pacifici, Camilla and Pascual, Sergio and {Pascual-Granado}, J. and Patil, Rohit R. and Perren, Gabriel I. and Pickering, Timothy E. and Rastogi, Tanuj and Roulston, Benjamin R. and Ryan, Daniel F. and Rykoff, Eli S. and Sabater, Jose and Sakurikar, Parikshit and Salgado, Jes{\'u}s and Sanghi, Aniket and Saunders, Nicholas and Savchenko, Volodymyr and Schwardt, Ludwig and {Seifert-Eckert}, Michael and Shih, Albert Y. and Jain, Anany Shrey and Shukla, Gyanendra and Sick, Jonathan and Simpson, Chris and Singanamalla, Sudheesh and Singer, Leo P. and Singhal, Jaladh and Sinha, Manodeep and Sip{\H o}cz, Brigitta M. and Spitler, Lee R. and Stansby, David and Streicher, Ole and {\v S}umak, Jani and Swinbank, John D. and Taranu, Dan S. and Tewary, Nikita and Tremblay, Grant R. and de {Val-Borro}, Miguel and Van Kooten, Samuel J. and Vasovi{\'c}, Zlatan and Verma, Shresth and {de Miranda Cardoso}, Jos{\'e} Vin{\'i}cius and Williams, Peter K. G. and Wilson, Tom J. and Winkel, Benjamin and {Wood-Vasey}, W. M. and Xue, Rui and Yoachim, Peter and Zhang, Chen and Zonca, Andrea and {Astropy Project Contributors}},
year = {2022},
month = aug,
journal = {The Astrophysical Journal},
volume = {935},
pages = {167},
issn = {0004-637X},
doi = {10.3847/1538-4357/ac7c74},
abstract = {The Astropy Project supports and fosters the development of open-source and openly developed Python packages that provide commonly needed functionality to the astronomical community. A key element of the Astropy Project is the core package astropy, which serves as the foundation for more specialized projects and packages. In this article, we summarize key features in the core package as of the recent major release, version 5.0, and provide major updates on the Project. We then discuss supporting a broader ecosystem of interoperable packages, including connections with several astronomical observatories and missions. We also revisit the future outlook of the Astropy Project and the current status of Learn Astropy. We conclude by raising and discussing the current and future challenges facing the Project.},
keywords = {1855,1858,1866,Astronomy data analysis,Astronomy software,Astrophysics - Instrumentation and Methods for Astrophysics,Open source software},
annotation = {ADS Bibcode: 2022ApJ...935..167A},
}
@article{scherrer_helioseismic_2012,
title = {The {{Helioseismic}} and {{Magnetic Imager}} ({{HMI}}) {{Investigation}} for the {{Solar Dynamics Observatory}} ({{SDO}})},
author = {Scherrer, P. H. and Schou, J. and Bush, R. I. and Kosovichev, A. G. and Bogart, R. S. and Hoeksema, J. T. and Liu, Y. and Duvall, T. L. and Zhao, J. and Title, A. M. and Schrijver, C. J. and Tarbell, T. D. and Tomczyk, S.},
year = {2012},
month = jan,
journal = {Solar Physics},
volume = {275},
pages = {207--227},
issn = {0038-0938},
doi = {10.1007/s11207-011-9834-2},
abstract = {The Helioseismic and Magnetic Imager (HMI) instrument and investigation as a part of the NASA Solar Dynamics Observatory (SDO) is designed to study convection-zone dynamics and the solar dynamo, the origin and evolution of sunspots, active regions, and complexes of activity, the sources and drivers of solar magnetic activity and disturbances, links between the internal processes and dynamics of the corona and heliosphere, and precursors of solar disturbances for space-weather forecasts. A brief overview of the instrument, investigation objectives, and standard data products is presented.},
}
@article{pesnell_solar_2012,
title = {The {{Solar Dynamics Observatory}} ({{SDO}})},
author = {Pesnell, W. Dean and Thompson, B. J. and Chamberlin, P. C.},
year = {2012},
month = jan,
journal = {Solar Physics},
volume = {275},
pages = {3--15},
issn = {0038-0938},
doi = {10.1007/s11207-011-9841-3},
abstract = {The Solar Dynamics Observatory (SDO) was launched on 11 February 2010 at 15:23 UT from Kennedy Space Center aboard an Atlas V 401 (AV-021) launch vehicle. A series of apogee-motor firings lifted SDO from an initial geosynchronous transfer orbit into a circular geosynchronous orbit inclined by 28\textdegree{} about the longitude of the SDO-dedicated ground station in New Mexico. SDO began returning science data on 1 May 2010. SDO is the first space-weather mission in NASA's Living With a Star (LWS) Program. SDO's main goal is to understand, driving toward a predictive capability, those solar variations that influence life on Earth and humanity's technological systems. The SDO science investigations will determine how the Sun's magnetic field is generated and structured, how this stored magnetic energy is released into the heliosphere and geospace as the solar wind, energetic particles, and variations in the solar irradiance. Insights gained from SDO investigations will also lead to an increased understanding of the role that solar variability plays in changes in Earth's atmospheric chemistry and climate. The SDO mission includes three scientific investigations (the Atmospheric Imaging Assembly (AIA), Extreme Ultraviolet Variability Experiment (EVE), and Helioseismic and Magnetic Imager (HMI)), a spacecraft bus, and a dedicated ground station to handle the telemetry. The Goddard Space Flight Center built and will operate the spacecraft during its planned five-year mission life; this includes: commanding the spacecraft, receiving the science data, and forwarding that data to the science teams. The science investigations teams at Stanford University, Lockheed Martin Solar Astrophysics Laboratory (LMSAL), and University of Colorado Laboratory for Atmospheric and Space Physics (LASP) will process, analyze, distribute, and archive the science data. We will describe the building of SDO and the science that it will provide to NASA.},
keywords = {coronal,Helioseismology,SDO,Solar cycle,Space weather},
}
@article{lemen_atmospheric_2012,
title = {The {{Atmospheric Imaging Assembly}} ({{AIA}}) on the {{Solar Dynamics Observatory}} ({{SDO}})},
author = {Lemen, James R. and Title, Alan M. and Akin, David J. and Boerner, Paul F. and Chou, Catherine and Drake, Jerry F. and Duncan, Dexter W. and Edwards, Christopher G. and Friedlaender, Frank M. and Heyman, Gary F. and Hurlburt, Neal E. and Katz, Noah L. and Kushner, Gary D. and Levay, Michael and Lindgren, Russell W. and Mathur, Dnyanesh P. and McFeaters, Edward L. and Mitchell, Sarah and Rehse, Roger A. and Schrijver, Carolus J. and Springer, Larry A. and Stern, Robert A. and Tarbell, Theodore D. and Wuelser, Jean-Pierre and Wolfson, C. Jacob and Yanari, Carl and Bookbinder, Jay A. and Cheimets, Peter N. and Caldwell, David and Deluca, Edward E. and Gates, Richard and Golub, Leon and Park, Sang and Podgorski, William A. and Bush, Rock I. and Scherrer, Philip H. and Gummin, Mark A. and Smith, Peter and Auker, Gary and Jerram, Paul and Pool, Peter and Soufli, Regina and Windt, David L. and Beardsley, Sarah and Clapp, Matthew and Lang, James and Waltham, Nicholas},
year = {2012},
month = jan,
journal = {Solar Physics},
volume = {275},
number = {1-2},
pages = {17--40},
issn = {0038-0938, 1573-093X},
doi = {10.1007/s11207-011-9776-8},
abstract = {The Atmospheric Imaging Assembly (AIA) provides multiple simultaneous high-resolution full-disk images of the corona and transition region up to 0.5 R {$\odot$} above the solar limb with 1.5-arcsec spatial resolution and 12-second temporal resolution. The AIA consists of four telescopes that employ normal-incidence, multilayer-coated optics to provide narrow-band imaging of seven extreme ultraviolet (EUV) band passes centered on specific lines: Fe xviii (94 \AA ), Fe viii, xxi (131 \AA ), Fe ix (171 \AA ), Fe xii, xxiv (193 \AA ), Fe xiv (211 \AA ), He ii (304 \AA ), and Fe xvi (335 \AA ). One telescope observes C iv (near 1600 \AA ) and the nearby continuum (1700 \AA ) and has a filter that observes in the visible to enable coalignment with images from other telescopes. The temperature diagnostics of the EUV emissions cover the range from 6\texttimes 104 K to 2\texttimes 107 K. The AIA was launched as a part of NASA's Solar Dynamics Observatory (SDO) mission on 11 February 2010. AIA will advance our understanding of the mechanisms of solar variability and of how the Sun's energy is stored and released into the heliosphere and geospace.},
langid = {english},
keywords = {Astrophysics and Astroparticles,Extraterrestrial Physics; Space Sciences,Extreme ultraviolet,Meteorology/Climatology,Solar corona,Solar imaging,Solar instrumentation},
}
@article{danryanirish_2021_5715161,
author = {Daniel Ryan and
Stuart Mumford and
Yash Sharma and
ankit and
Adwait Bhope and
Nabil Freij and
Ricky O'Steen and
Baptiste Pellorce and
Laura Hayes and
Mateo Inchaurrandieta and
Derek Homeier and
David Stansby and
Aoife Maria Ryan and
Drew Leonard and
Roy Smart and
Matthew West and
Kritika Ranjan and
P. L. Lim and
shelbej},
title = {sunpy/ndcube: v2.0.1},
month = nov,
year = 2021,
publisher = {Zenodo},
version = {v2.0.1},
doi = {10.5281/zenodo.5715161},
url = {https://doi.org/10.5281/zenodo.5715161}
}
@article{danryanirish_2022_7190661,
author = {Daniel Ryan and
Stuart Mumford and
Nabil Freij and
Andrew Inglis and
Drew Leonard and
Steven Christe and
Vishnunarayan K I and
Albert Y. Shih and
Brigitta Sipőcz and
Silvan Laube and
Keith Hughitt and
Asish Panda and
Jack Ireland and
David Pérez-Suárez and
Larry Manley and
David Stansby and
Yash Jain and
Alex-Ian-Hamilton and
Nitin Choudhary and
derdon and
Daniel Williams and
Michael Charlton and
Samuel Bennett and
Shane Maloney and
Pritish Chakraborty and
Carlos Molina and
Md Akramul Haque and
Florian Mayer and
Harsh Mathur},
title = {sunpy/sunkit-instruments: v0.3.1},
month = oct,
year = 2022,
publisher = {Zenodo},
version = {v0.3.1},
doi = {10.5281/zenodo.7190661},
url = {https://doi.org/10.5281/zenodo.7190661}
}
@article{nabil_freij_2022_6578722,
author = {Nabil Freij and
Jack Ireland and
Stuart Mumford and
Will Barnes and
Vatsalya Chaubey and
Jeffrey Aaron Paul and
Laura Hayes and
P. L. Lim and
Michael Kirk},
title = {sunpy/sunkit-image: v0.4.2},
month = may,
year = 2022,
publisher = {Zenodo},
version = {v0.4.2},
doi = {10.5281/zenodo.6578722},
url = {https://doi.org/10.5281/zenodo.6578722}
}
@article{howard_sun_2008,
title = {Sun {{Earth Connection Coronal}} and {{Heliospheric Investigation}} ({{SECCHI}})},
author = {Howard, R. A. and Moses, J. D. and Vourlidas, A. and Newmark, J. S. and Socker, D. G. and Plunkett, S. P. and Korendyke, C. M. and Cook, J. W. and Hurley, A. and Davila, J. M. and Thompson, W. T. and St Cyr, O. C. and Mentzell, E. and Mehalick, K. and Lemen, J. R. and Wuelser, J. P. and Duncan, D. W. and Tarbell, T. D. and Wolfson, C. J. and Moore, A. and Harrison, R. A. and Waltham, N. R. and Lang, J. and Davis, C. J. and Eyles, C. J. and {Mapson-Menard}, H. and Simnett, G. M. and Halain, J. P. and Defise, J. M. and Mazy, E. and Rochus, P. and Mercier, R. and Ravet, M. F. and Delmotte, F. and Auchere, F. and Delaboudiniere, J. P. and Bothmer, V. and Deutsch, W. and Wang, D. and Rich, N. and Cooper, S. and Stephens, V. and Maahs, G. and Baugh, R. and McMullin, D. and Carter, T.},
year = {2008},
month = apr,
journal = {Space Science Reviews},
volume = {136},
pages = {67--115},
issn = {0038-6308},
doi = {10.1007/s11214-008-9341-4},
abstract = {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 by the Naval Research Laboratory (USA), the Lockheed Solar and Astrophysics Laboratory (USA), the Goddard Space Flight Center (USA), the University of Birmingham (UK), the Rutherford Appleton Laboratory (UK), the Max Planck Institute for Solar System Research (Germany), the Centre Spatiale de Leige (Belgium), the Institut d'Optique (France) and the Institut d'Astrophysique Spatiale (France). SECCHI comprises five telescopes, which together image the solar corona from the solar disk to beyond 1 AU. These telescopes are: an extreme ultraviolet imager (EUVI: 1 1.7 R{$\odot$}), two traditional Lyot coronagraphs (COR1: 1.5 4 R{$\odot$} and COR2: 2.5 15 R{$\odot$}) and two new designs of heliospheric imagers (HI-1: 15 84 R{$\odot$} and HI-2: 66 318 R{$\odot$}). All the instruments use 2048\texttimes 2048 pixel CCD arrays in a backside-in mode. The EUVI backside surface has been specially processed for EUV sensitivity, while the others have an anti-reflection coating applied. A multi-tasking operating system, running on a PowerPC CPU, receives commands from the spacecraft, controls the instrument operations, acquires the images and compresses them for downlink through the main science channel (at compression factors typically up to 20\texttimes ) and also through a low bandwidth channel to be used for space weather forecasting (at compression factors up to 200\texttimes ). An image compression factor of about 10\texttimes{} enable the collection of images at the rate of about one every 2 3 minutes. Identical instruments, except for different sizes of occulters, are included on the STEREO-A and STEREO-B spacecraft.},
keywords = {Coronal loops,Coronal mass ejections,Heliosphere,Heliospheric imager,Lyot coronagraph,Solar corona,Stereo,XUV heliograph},
annotation = {ADS Bibcode: 2008SSRv..136...67H},
}
@article{muller_solar_2020,
title = {The {{Solar Orbiter}} Mission - {{Science}} Overview},
author = {M{\"u}ller, D. and Cyr, O. C. St and Zouganelis, I. and Gilbert, H. R. and Marsden, R. and {Nieves-Chinchilla}, T. and Antonucci, E. and Auch{\`e}re, F. and Berghmans, D. and Horbury, T. S. and Howard, R. A. and Krucker, S. and Maksimovic, M. and Owen, C. J. and Rochus, P. and {Rodriguez-Pacheco}, J. and Romoli, M. and Solanki, S. K. and Bruno, R. and Carlsson, M. and Fludra, A. and Harra, L. and Hassler, D. M. and Livi, S. and Louarn, P. and Peter, H. and Sch{\"u}hle, U. and Teriaca, L. and Iniesta, J. C. del Toro and {Wimmer-Schweingruber}, R. F. and Marsch, E. and Velli, M. and Groof, A. De and Walsh, A. and Williams, D.},
year = {2020},
month = oct,
journal = {Astronomy \& Astrophysics},
volume = {642},
pages = {A1},
publisher = {{EDP Sciences}},
issn = {0004-6361, 1432-0746},
doi = {10.1051/0004-6361/202038467},
abstract = {\emph{Aims.{$<$}i/{$>$} Solar Orbiter, the first mission of ESA's Cosmic Vision 2015\textendash 2025 programme and a mission of international collaboration between ESA and NASA, will explore the Sun and heliosphere from close up and out of the ecliptic plane. It was launched on 10 February 2020 04:03 UTC from Cape Canaveral and aims to address key questions of solar and heliospheric physics pertaining to how the Sun creates and controls the Heliosphere, and why solar activity changes with time. To answer these, the mission carries six remote-sensing instruments to observe the Sun and the solar corona, and four in-situ instruments to measure the solar wind, energetic particles, and electromagnetic fields. In this paper, we describe the science objectives of the mission, and how these will be addressed by the joint observations of the instruments onboard.\emph{Methods.{$<$}i/{$>$} The paper first summarises the mission-level science objectives, followed by an overview of the spacecraft and payload. We report the observables and performance figures of each instrument, as well as the trajectory design. This is followed by a summary of the science operations concept. The paper concludes with a more detailed description of the science objectives.\emph{Results.{$<$}i/{$>$} Solar Orbiter will combine in-situ measurements in the heliosphere with high-resolution remote-sensing observations of the Sun to address fundamental questions of solar and heliospheric physics. The performance of the Solar Orbiter payload meets the requirements derived from the mission's science objectives. Its science return will be augmented further by coordinated observations with other space missions and ground-based observatories.}}}},
copyright = {\textcopyright{} ESO 2020},
langid = {english},
}
@article{rochus_solar_2020,
title = {The {{Solar Orbiter EUI}} Instrument: {{The Extreme Ultraviolet Imager}}},
shorttitle = {The {{Solar Orbiter EUI}} Instrument},
author = {Rochus, P. and Auch{\`e}re, F. and Berghmans, D. and Harra, L. and Schmutz, W. and Sch{\"u}hle, U. and Addison, P. and Appourchaux, T. and Cuadrado, R. Aznar and Baker, D. and Barbay, J. and Bates, D. and BenMoussa, A. and Bergmann, M. and Beurthe, C. and Borgo, B. and Bonte, K. and Bouzit, M. and Bradley, L. and B{\"u}chel, V. and Buchlin, E. and B{\"u}chner, J. and Cab{\'e}, F. and Cadiergues, L. and Chaigneau, M. and Chares, B. and Cortez, C. Choque and Coker, P. and Condamin, M. and Coumar, S. and Curdt, W. and Cutler, J. and Davies, D. and Davison, G. and Defise, J.-M. and Zanna, G. Del and Delmotte, F. and Delouille, V. and Dolla, L. and Dumesnil, C. and D{\"u}rig, F. and Enge, R. and Fran{\c c}ois, S. and Fourmond, J.-J. and Gillis, J.-M. and Giordanengo, B. and Gissot, S. and Green, L. M. and Guerreiro, N. and Guilbaud, A. and Gyo, M. and Haberreiter, M. and Hafiz, A. and Hailey, M. and Halain, J.-P. and Hansotte, J. and Hecquet, C. and Heerlein, K. and Hellin, M.-L. and Hemsley, S. and Hermans, A. and Hervier, V. and Hochedez, J.-F. and Houbrechts, Y. and Ihsan, K. and Jacques, L. and J{\'e}r{\^o}me, A. and Jones, J. and Kahle, M. and Kennedy, T. and Klaproth, M. and Kolleck, M. and Koller, S. and Kotsialos, E. and Kraaikamp, E. and Langer, P. and Lawrenson, A. and Clech', J.-C. Le and Lenaerts, C. and Liebecq, S. and Linder, D. and Long, D. M. and Mampaey, B. and {Markiewicz-Innes}, D. and Marquet, B. and Marsch, E. and Matthews, S. and Mazy, E. and Mazzoli, A. and Meining, S. and Meltchakov, E. and Mercier, R. and Meyer, S. and Monecke, M. and Monfort, F. and Morinaud, G. and Moron, F. and Mountney, L. and M{\"u}ller, R. and Nicula, B. and Parenti, S. and Peter, H. and Pfiffner, D. and Philippon, A. and Phillips, I. and Plesseria, J.-Y. and Pylyser, E. and Rabecki, F. and {Ravet-Krill}, M.-F. and Rebellato, J. and Renotte, E. and Rodriguez, L. and Roose, S. and Rosin, J. and Rossi, L. and Roth, P. and Rouesnel, F. and Roulliay, M. and Rousseau, A. and Ruane, K. and Scanlan, J. and Schlatter, P. and Seaton, D. B. and Silliman, K. and Smit, S. and Smith, P. J. and Solanki, S. K. and Spescha, M. and Spencer, A. and Stegen, K. and Stockman, Y. and Szwec, N. and Tamiatto, C. and Tandy, J. and Teriaca, L. and Theobald, C. and Tychon, I. and van {Driel-Gesztelyi}, L. and Verbeeck, C. and Vial, J.-C. and Werner, S. and West, M. J. and Westwood, D. and Wiegelmann, T. and Willis, G. and Winter, B. and Zerr, A. and Zhang, X. and Zhukov, A. N.},
year = {2020},
month = oct,
journal = {Astronomy \& Astrophysics},
volume = {642},
pages = {A8},
publisher = {{EDP Sciences}},
issn = {0004-6361, 1432-0746},
doi = {10.1051/0004-6361/201936663},
abstract = {\emph{Context.{$<$}i/{$>$} The Extreme Ultraviolet Imager (EUI) is part of the remote sensing instrument package of the ESA/NASA Solar Orbiter mission that will explore the inner heliosphere and observe the Sun from vantage points close to the Sun and out of the ecliptic. Solar Orbiter will advance the ``connection science'' between solar activity and the heliosphere.\emph{Aims.{$<$}i/{$>$} With EUI we aim to improve our understanding of the structure and dynamics of the solar atmosphere, globally as well as at high resolution, and from high solar latitude perspectives.\emph{Methods.{$<$}i/{$>$} The EUI consists of three telescopes, the Full Sun Imager and two High Resolution Imagers, which are optimised to image in Lyman-\emph{{$\alpha<$}i/{$>$} and EUV (17.4 nm, 30.4 nm) to provide a coverage from chromosphere up to corona. The EUI is designed to cope with the strong constraints imposed by the Solar Orbiter mission characteristics. Limited telemetry availability is compensated by state-of-the-art image compression, onboard image processing, and event selection. The imposed power limitations and potentially harsh radiation environment necessitate the use of novel CMOS sensors. As the unobstructed field of view of the telescopes needs to protrude through the spacecraft's heat shield, the apertures have been kept as small as possible, without compromising optical performance. This led to a systematic effort to optimise the throughput of every optical element and the reduction of noise levels in the sensor.\emph{Results.{$<$}i/{$>$} In this paper we review the design of the two elements of the EUI instrument: the Optical Bench System and the Common Electronic Box. Particular attention is also given to the onboard software, the intended operations, the ground software, and the foreseen data products.\emph{Conclusions.{$<$}i/{$>$} The EUI will bring unique science opportunities thanks to its specific design, its viewpoint, and to the planned synergies with the other Solar Orbiter instruments. In particular, we highlight science opportunities brought by the out-of-ecliptic vantage point of the solar poles, the high-resolution imaging of the high chromosphere and corona, and the connection to the outer corona as observed by coronagraphs.}}}}}}},
copyright = {\textcopyright{} ESO 2020},
langid = {english},
}
@Article{Hunter:2007,
Author = {Hunter, J. D.},
Title = {Matplotlib: A 2D graphics environment},
Journal = {Computing in Science \& Engineering},
Volume = {9},
Number = {3},
Pages = {90--95},
abstract = {Matplotlib is a 2D graphics package used for Python for
application development, interactive scripting, and publication-quality
image generation across user interfaces and operating systems.},
publisher = {IEEE COMPUTER SOC},
doi = {10.1109/MCSE.2007.55},
year = 2007
}
@Article{ harris2020array,
title = {Array programming with {NumPy}},
author = {Charles R. Harris and K. Jarrod Millman and St{\'{e}}fan J.
van der Walt and Ralf Gommers and Pauli Virtanen and David
Cournapeau and Eric Wieser and Julian Taylor and Sebastian
Berg and Nathaniel J. Smith and Robert Kern and Matti Picus
and Stephan Hoyer and Marten H. van Kerkwijk and Matthew
Brett and Allan Haldane and Jaime Fern{\'{a}}ndez del
R{\'{i}}o and Mark Wiebe and Pearu Peterson and Pierre
G{\'{e}}rard-Marchant and Kevin Sheppard and Tyler Reddy and
Warren Weckesser and Hameer Abbasi and Christoph Gohlke and
Travis E. Oliphant},
year = {2020},
month = sep,
journal = {Nature},
volume = {585},
number = {7825},
pages = {357--362},
doi = {10.1038/s41586-020-2649-2},
publisher = {Springer Science and Business Media {LLC}},
url = {https://doi.org/10.1038/s41586-020-2649-2}
}
@ARTICLE{2020SciPy-NMeth,
author = {Virtanen, Pauli and Gommers, Ralf and Oliphant, Travis E. and
Haberland, Matt and Reddy, Tyler and Cournapeau, David and
Burovski, Evgeni and Peterson, Pearu and Weckesser, Warren and
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Brett, Matthew and Wilson, Joshua and Millman, K. Jarrod and
Mayorov, Nikolay and Nelson, Andrew R. J. and Jones, Eric and
Kern, Robert and Larson, Eric and Carey, C J and
Polat, {\.I}lhan and Feng, Yu and Moore, Eric W. and
{VanderPlas}, Jake and Laxalde, Denis and Perktold, Josef and
Cimrman, Robert and Henriksen, Ian and Quintero, E. A. and
Harris, Charles R. and Archibald, Anne M. and
Ribeiro, Ant{\^o}nio H. and Pedregosa, Fabian and
{van Mulbregt}, Paul and {SciPy 1.0 Contributors}},
title = {{{SciPy} 1.0: Fundamental Algorithms for Scientific
Computing in Python}},
journal = {Nature Methods},
year = {2020},
volume = {17},
pages = {261--272},
adsurl = {https://rdcu.be/b08Wh},
doi = {10.1038/s41592-019-0686-2},
}
@article{https://doi.org/10.1029/2018JA025877,
author = {Burrell, A. G. and Halford, A. and Klenzing, J. and Stoneback, R. A. and Morley, S. K. and Annex, A. M. and Laundal, K. M. and Kellerman, A. C. and Stansby, D. and Ma, J.},
title = {Snakes on a Spaceship—An Overview of Python in Heliophysics},
journal = {Journal of Geophysical Research: Space Physics},
volume = {123},
number = {12},
pages = {10,384-10,402},
keywords = {open source, Python, reproducible science, system science, heliophysics, software},
doi = {https://doi.org/10.1029/2018JA025877},
url = {https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2018JA025877},
eprint = {https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2018JA025877},
abstract = {Abstract Computational analysis has become ubiquitous within the heliophysics community. However, community standards for peer review of codes and analysis have lagged behind these developments. This absence has contributed to the reproducibility crisis, where inadequate analysis descriptions and loss of scientific data have made scientific studies difficult or impossible to replicate. The heliophysics community has responded to this challenge by expressing a desire for a more open, collaborative set of analysis tools. This article summarizes the current state of these efforts and presents an overview of many of the existing Python heliophysics tools. It also outlines the challenges facing community members who are working toward the goal of an open, collaborative, Python heliophysics toolkit and presents guidelines that can ease the transition from individualistic data analysis practices to an accountable, communalistic environment.},
year = {2018}
}
@article{barnum2022python,
title={Python in Heliophysics Community (PyHC): current status and future outlook},
author={Barnum, Julie and Masson, Arnaud and Friedel, Reinhard HW and Roberts, Aaron and Thomas, Brian A},
journal={Advances in Space Research},
year={2022},
publisher={Elsevier}
}
@manual{mumford_stuart_2014_3261752,
title = {{SunPy Proposal for Enhancement 4: Packages
Affiliated with the SunPy Project (SEP 0004)}},
author = {Mumford, Stuart and
Christe, Steven},
month = oct,
year = 2014,
doi = {10.5281/zenodo.3261752},
url = {https://doi.org/10.5281/zenodo.3261752}
}
@manual{annex_a_2018_2529131,
author = {Annex, A. and
Alterman, B. L. and
Azari, A. and
Barnes, W. and
Bobra, M. and
Cecconi, B. and
Christe, Steven and
Coxon, J. and
DeWolfe, A. and
Halford, A. and
Harter, B. and
Ireland, J. and
Jahn, J. and
Klenzing, J. and
Liu, M. and
Mason, J. and
McGranaghan, R. and
Murphy, N. and
Murray, S. and
Niehof, J. and
Nguyen, M. D. and
Panneton, R. and
Pembroke, A. and
Pérez-Suárez, D. and
Piker, C. and
Roberts, A. and
Ryan, D. and
Savage, S. and
Smith, J. and
Stansby, D. and
Vandegriff, J. and
Weigel, R. S.},
title = {Python in Heliophysics Community (PyHC) Standards},
month = dec,
year = 2018,
publisher = {Zenodo},
version = {v1.0},
doi = {10.5281/zenodo.2529131},
url = {https://doi.org/10.5281/zenodo.2529131}
}
@article{greisen_representations_2002,
title = {Representations of World Coordinates in {{FITS}}},
author = {Greisen, E. W. and Calabretta, M. R.},
year = {2002},
month = dec,
journal = {Astronomy and Astrophysics},
volume = {395},
pages = {1061},
doi = {10.1051/0004-6361:20021326},
abstract = {The initial descriptions of the FITS format provided a simplified method for describing the physical coordinate values of the image pixels, but deliberately did not specify any of the detailed conventions required to convey the complexities of actual image coordinates. Building on conventions in wide use within astronomy, this paper proposes general extensions to the original methods for describing the world coordinates of FITS data. In subsequent papers, we apply these general conventions to the methods by which spherical coordinates may be projected onto a two-dimensional plane and to frequency/wavelength/velocity coordinates.},
langid = {english},
}
@manual{christe_steven_2018_3261663,
title = {{SunPy Proposal for Enhancement 2: SunPy
Organization Definition (SEP 0002)}},
author = {Christe, Steven},
month = dec,
year = 2018,
doi = {10.5281/zenodo.3261663},
url = {https://doi.org/10.5281/zenodo.3261663}
}
@article{wells_fits_1981,
title = {{{FITS}} - a {{Flexible Image Transport System}}},
author = {Wells, D. C. and Greisen, E. W. and Harten, R. H.},
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month = jun,
journal = {Astronomy and Astrophysics Supplement Series},
volume = {44},
pages = {363},
issn = {0365-0138}
}