Solar surveillance with CLIMSO: instrumentation, database and on-going developments | Journal of Space Weather and Space Climate

Topical Issue - Space Weather Instrumentation

Open Access

Issue		J. Space Weather Space Clim. Volume 10, 2020 Topical Issue - Space Weather Instrumentation


Article Number		47
Number of page(s)		12
DOI		https://doi.org/10.1051/swsc/2020039
Published online		07 October 2020

Arge CN, Pizzo VJ. 2000. Improvement in the prediction of SW conditions using near-real-time solar magnetic field updates. J Geophys Res 105: 10465–10479. [CrossRef] [Google Scholar]
Burt J, Smith B. 2012. Deep space climate observatory: The DSCOVR mission. In: 2012 IEEE Aerospace Conference, Big Sky, MT, pp. 1–13. https://doi.org/10.1109/AERO.2012.6187025. [Google Scholar]
Chen P, Ding M, Fang C. 2005. Synthesis of CME-associated moreton and EIT wave features from MHD simulations. Space Sci Rev 121: 201–211. https://doi.org/10.1007/s11214-006-3911-0. [NASA ADS] [CrossRef] [Google Scholar]
Chen PF. 2011. Coronal mass ejections: Models and their observational basis. Living Rev Sol Phys 8: 1. https://doi.org/10.12942/lrsp-2011-1. [Google Scholar]
Cliver EW, Webb DF, Howard RA. 1999. On the origin of solar metric type II bursts. Sol Phys 187: 89. [Google Scholar]
Demarcq J, Hugon M, Rösch J, Trellis M. 1965. Un coronographe achromatique amélioré pour la spectrographie de la couronne solaire. C.R. Acad Sci Paris 261: 4629. [Google Scholar]
Dettwiller L, Noëns J-C. 2008. Les nouveaux coronographes du Pic du Midi: Schémas optiques et buts scientifiques. BUP 102: 1227–1248. [Google Scholar]
Erard S, Cecconi B, Le Sidaner P, Berthier J, Henry F, et al. 2014. The EPN-TAP protocol for the Planetary Science Virtual Observatory. Astron Comput 7–8: 52–61. ISSN 2213-1337. https://doi.org/10.1016/j.ascom.2014.07.008. [CrossRef] [Google Scholar]
Erard S, Cecconi B, Le Sidaner P, Rossi AP, Capria MT, et al. 2018. VESPA: A community-driven Virtual Observatory in Planetary Science. Planet Space Sci 150: 65–85. https://doi.org/10.1016/j.pss.2017.05.013. [NASA ADS] [CrossRef] [Google Scholar]
Génot V, Budnik E, Jacquey C, Bouchemit M, Renard B, et al. 2020. Automated Multi-Dataset Analysis (AMDA): an on-line database and analysis tool for heliospheric and planetary plasma data. Submitted to Planetary Space Science. [Google Scholar]
Hill F, Martens P, Yoshimura K, Gurman J, Hourclé J, et al. 2009. The virtual solar observatory – A resource for International Heliophysics Research. Earth Moon Planet 104: 315–330. https://doi.org/10.1007/s11038-008-9274-7. [CrossRef] [Google Scholar]
Jacquey C, Génot V, Budnik H, Hitier R, Bouchemit M, et al. 2010. AMDA, automated multi-dataset analysis: A web-based service provided by the CDPP. In: The Cluster Active Archive. Astrophysics and Space Science Proceedings, Laakso H, Taylor M, Escoubet C (Eds.), Springer, Dordrecht. https://doi.org/10.1007/978-90-481-3499-1_16. [Google Scholar]
Koechlin L, Dettwiller L, Audejean M, Valais M, López Ariste A. 2019. Solar survey at Pic du Midi: Calibrated data and improved images. A&A 631: A55. https://doi.org/10.1051/0004-6361/201732504. [CrossRef] [EDP Sciences] [Google Scholar]
López Ariste A, Facchin M. 2018. Superoscillations in solar MHD waves and their possible role in heating coronal loops. A&A 615: A145. https://doi.org/10.1051/0004-6361/201731401. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
Lyot B. 1930. La couronne solaire étudiée en dehors des éclipses. Bull Astron 6: 305–316. [Google Scholar]
Lyot B. 1935. Quelques observations de la couronne solaire et des protubérances en 1935. L’Astronomie 51: 203–218. [Google Scholar]
Marchand E. 1904. La perturbation magnétique du 31 octobre 1903, Bulletin de la Société Astronomique de France et Revue Mensuelle d’Astronomie, de Météorologie et de Physique du. Bulletin de la Société Astronomique de France et Revue Mensuelle d’Astronomie, de Météorologie et de Physique du Globe 18: 34–36. [Google Scholar]
Meunier N, Noëns J-C, Romeuf D, Koutchmy S, Jimenez R., Wurmser O., Rochain S., The OA Team. 2007. Coronagraphic Broad-Band Hα Observations 1998 – 2000. In: The Physics of Chromospheric Plasmas, ASP Conference Series, Vol. 368. [Google Scholar]
Moreton GE. 1960. Hα observations of flare-initiated disturbances with velocities ~1000 km/sec. Astron J 65: 494. [NASA ADS] [CrossRef] [Google Scholar]
Noëns J, Wurmser O. 2000. Ground based limb survey of the sun polar regions in the Hα line. Astrophys Space Sci 273: 17–23. https://doi.org/10.1023/A:1002687606153. [NASA ADS] [CrossRef] [Google Scholar]
Odstrcil D, Pizzo VJ. 1999. Distortion of the interplanetary magnetic field by three-dimensional propagation of coronal mass ejections in a structured solar wind. J Geophys Res 104(A12): 28225–28240. https://doi.org/10.1029/1999JA900319. [NASA ADS] [CrossRef] [Google Scholar]
Oranje BJ. 1983. The CaII K emission from the Sun as a star, I. observational parameters. A&A 122: 88–94. [Google Scholar]
Pariat E, Schmieder B, Berlicki A, Deng Y, Mein N, López Ariste A, Wang S. 2007. Spectrophotometric analysis of Ellerman bombs in the Ca II, Hα, and UV range. A&A 473: 279–289. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
Pomoell J, Poedts S. 2018. EUHFORIA: European heliospheric forecasting information asset. J Space Weather Space Clim 8: A35. https://doi.org/10.1051/swsc/2018020. [CrossRef] [Google Scholar]
Romeuf D, Meunier N, Noëns J-C, Koutchmy S, Jimenez R, Wurmser O, Rochain S, “Observateurs Associés” Team. 2007. Analysis of broad-band Hα coronagraphic observations. A&A 462(2): 731–741. https://doi.org/10.1051/0004-6361:20054159. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
Roudier T, Schmieder B, Filippov B, Chandra R, Malherbe J-M. 2018. Photospheric flows trigger a filament eruption. A&A 618: A43. https://doi.org/10.1051/0004-6361/201832937. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
Rouillard AP, Lavraud B, Génot V, Bouchemit M, Dufourg N, et al. 2017. A propagation tool to connect remote-sensing observations with in-situ measurements of heliospheric structures. Planet Space Sci 147: 61–77. https://doi.org/10.1016/j.pss.2017.07.001. [CrossRef] [Google Scholar]
Sanguillon M, Glorian J-M, Vastel C. 2019. The OV-GSO data center. Astron Data Anal Softw Syst XXVIII 523: 449. [Google Scholar]
Stone EC, Frandsen AM, Mewaldt RA, Christian ER, Margolies D, Ormes JF, Snow F. 1998. The advanced composition explorer. Space Sci Rev 86: 1–22. https://doi.org/10.1023/A:1005082526237. [NASA ADS] [CrossRef] [Google Scholar]
Taylor MB. 2005. TOPCAT & STIL: Starlink Table/VOTable Processing Software. Astron Data Anal Softw Syst XIV 347: 9. [Google Scholar]
Vernazza JE, Avrett EH, Loeser R. 1981. Structure of the solar chromosphere. III. Models of the EUV brightness components of the quiet sun. Astrophys J Suppl Ser 45: 635–725. [Google Scholar]
Wang H, Liu C, Wang S, Deng N, Xu Y, Jing J, Cao W. 2013. Study of rapid formation of a δ sunspot associated with the 2012 July 2 C7.4 flare using high-resolution observations of the New Solar Telescope. Astrophys J L24: 774. [Google Scholar]
Yurchyshyn V, Wang H, Abramenko V. 2003. How directions and helicity of erupted solar magnetic fields define geoeffectiveness of coronal mass ejections. Adv Space Res 32(10): 1965–1970. https://doi.org/10.1016/S0273-1177(03)90634-X. [CrossRef] [Google Scholar]

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.