{"id":494796,"date":"2026-05-20T21:55:19","date_gmt":"2026-05-20T21:55:19","guid":{"rendered":"https:\/\/www.europesays.com\/ie\/494796\/"},"modified":"2026-05-20T21:55:19","modified_gmt":"2026-05-20T21:55:19","slug":"multi-viewpoint-observation-of-a-failed-prominence-eruption-on-the-sun","status":"publish","type":"post","link":"https:\/\/www.europesays.com\/ie\/494796\/","title":{"rendered":"Multi-viewpoint observation of a failed prominence eruption on the Sun"},"content":{"rendered":"
  • \n

    Priest, E. R. & Forbes, T. G. The magnetic nature of solar flares. Astron. Astrophys. Rev. 10<\/b>, 313\u2013377 (2002).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Chen, P. F. Coronal mass ejections: models and their observational basis. Living Rev. Sol. Phys. 8<\/b>, 1 (2011).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Webb, D. F. & Howard, T. A. Coronal mass ejections: observations. Living Rev. Sol. Phys. 9<\/b>, 3 (2012).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Airapetian, V. S. et al. Impact of space weather on climate and habitability of terrestrial-type exoplanets. Int. J. Astrobiol. 19<\/b>, 136\u2013194 (2020).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Lugaz, N. et al. Earth\u2019s magnetosphere and outer radiation belt under sub-Alfv\u00e9nic solar wind. Nat. Commun. 7<\/b>, 13001 (2016).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Davenport, J. R. A. The Kepler Catalog of stellar flares. Astrophys. J. 829<\/b>, 23 (2016).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Vida, K. et al. The quest for stellar coronal mass ejections in late-type stars. I. Investigating Balmer-line asymmetries of single stars in Virtual Observatory data. Astron. Astrophys. 623<\/b>, A49 (2019).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Veronig, A. M. et al. Indications of stellar coronal mass ejections through coronal dimmings. Nat. Astron. 5<\/b>, 697\u2013706 (2021).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Odert, P., Leitzinger, M., Hanslmeier, A. & Lammer, H. Stellar coronal mass ejections. I. Estimating occurrence frequencies and mass-loss rates. Mon. Not. R. Astron. Soc. 472<\/b>, 876\u2013890 (2017).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Green, L. M., T\u00f6r\u00f6k, T., Vr\u0161nak, B., Manchester, W. & Veronig, A. The origin, early evolution and predictability of solar eruptions. Space Sci. Rev. 214<\/b>, 46 (2018).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Moore, R. L., Sterling, A. C., Hudson, H. S. & Lemen, J. R. Onset of the magnetic explosion in solar flares and coronal mass ejections. Astrophys. J. 552<\/b>, 833\u2013848 (2001).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Antiochos, S. K., DeVore, C. R. & Klimchuk, J. A. A model for solar coronal mass ejections. Astrophys. J. 510<\/b>, 485\u2013493 (1999).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    T\u00f6r\u00f6k, T., Kliem, B. & Titov, V. S. Ideal kink instability of a magnetic loop equilibrium. Astron. Astrophys. 413<\/b>, L27\u2013L30 (2004).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Gou, T., Liu, R., Kliem, B., Wang, Y. & Veronig, A. M. The birth of a coronal mass ejection. Sci. Adv. 5<\/b>, 7004 (2019).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Liu, R. Magnetic flux ropes in the solar corona: structure and evolution toward eruption. Res. Astron. Astrophys. 20<\/b>, 165 (2020).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Lin, J. & Forbes, T. G. Effects of reconnection on the coronal mass ejection process. J. Geophys. Res. 105<\/b>, 2375\u20132392 (2000).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Gou, T. et al. Solar flare-CME coupling throughout two acceleration phases of a fast CME. Astrophys. J. Lett. 897<\/b>, L36 (2020).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Bateman, G. MHD Instabilities (MIT, 1978).<\/p>\n<\/li>\n

  • \n

    Kliem, B. & T\u00f6r\u00f6k, T. Torus instability. Phys. Rev. Lett. 96<\/b>, 255002 (2006).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Falconer, D. A., Moore, R. L. & Gary, G. A. Correlation of the coronal mass ejection productivity of solar active regions with measures of their global nonpotentiality from vector magnetograms: baseline results. Astrophys. J. 569<\/b>, 1016\u20131025 (2002).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Wang, Y. & Zhang, J. A comparative study between eruptive X-class flares associated with coronal mass ejections and confined X-class flares. Astrophys. J. 665<\/b>, 1428\u20131438 (2007).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Sun, X. et al. Why Is the great solar active region 12192 flare-rich but CME-poor? Astrophys. J. Lett. 804<\/b>, L28 (2015).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    T\u00f6r\u00f6k, T. & Kliem, B. Confined and ejective eruptions of kink-unstable flux ropes. Astrophys. J. Lett. 630<\/b>, L97\u2013L100 (2005).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Fan, Y. & Gibson, S. E. Onset of coronal mass ejections due to loss of confinement of coronal flux ropes. Astrophys. J. 668<\/b>, 1232\u20131245 (2007).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Ji, H., Wang, H., Schmahl, E. J., Moon, Y. J. & Jiang, Y. Observations of the failed eruption of a filament. Astrophys. J. Lett. 595<\/b>, L135\u2013L138 (2003).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Liu, Y. et al. New observation of failed filament eruptions: the influence of asymmetric coronal background fields on solar eruptions. Astrophys. J. Lett. 696<\/b>, L70\u2013L73 (2009).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Chen, Y., Cheng, X., Chen, J., Dai, Y. & Ding, M. Observations of a failed solar filament eruption involving external reconnection. Astrophys. J. 959<\/b>, 67 (2023).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Karpen, J. T., Kumar, P., Wyper, P. F., DeVore, C. R. & Antiochos, S. K. Solar eruptions in nested magnetic flux systems. Astrophys. J. 966<\/b>, 27 (2024).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Gibson, S. E. & Fan, Y. Coronal prominence structure and dynamics: a magnetic flux rope interpretation. J. Geophys. Res. 111<\/b>, A12103 (2006).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Zhang, J., Cheng, X. & Ding, M.-D. Observation of an evolving magnetic flux rope before and during a solar eruption. Nat. Commun. 3<\/b>, 747 (2012).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Lynch, B. J., Antiochos, S. K., DeVore, C. R., Luhmann, J. G. & Zurbuchen, T. H. Topological evolution of a fast magnetic breakout CME in three dimensions. Astrophys. J. 683<\/b>, 1192\u20131206 (2008).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Shibata, K. & Magara, T. Solar flares: magnetohydrodynamic processes. Living Rev. Sol. Phys. 8<\/b>, 6 (2011).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Karpen, J. T., Antiochos, S. K. & DeVore, C. R. The mechanisms for the onset and explosive eruption of coronal mass ejections and eruptive flares. Astrophys. J. 760<\/b>, 81 (2012).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Petschek, H. E. Magnetic field annihilation. NASA Spec. Publ. 50<\/b>, 425 (1964).<\/p>\n<\/li>\n

  • \n

    Lin, J. et al. Direct observations of the magnetic reconnection site of an eruption on 2003 November 18. Astrophys. J. 622<\/b>, 1251\u20131264 (2005).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Gou, T., Veronig, A. M., Dickson, E. C., Hernandez-Perez, A. & Liu, R. Direct observation of two-step magnetic reconnection in a solar flare. Astrophys. J. Lett. 845<\/b>, L1 (2017).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Vr\u0161nak, B. Processes and mechanisms governing the initiation and propagation of CMEs. Ann. Geophys. 26<\/b>, 3089\u20133101 (2008).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Zhang, J., Dere, K. P., Howard, R. A., Kundu, M. R. & White, S. M. On the temporal relationship between coronal mass ejections and flares. Astrophys. J. 559<\/b>, 452\u2013462 (2001).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Temmer, M., Veronig, A. M., Kontar, E. P., Krucker, S. & Vr\u0161nak, B. Combined STEREO\/RHESSI study of coronal mass ejection acceleration and particle acceleration in solar flares. Astrophys. J. 712<\/b>, 1410\u20131420 (2010).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Aulanier, G. & Dud\u00edk, J. Drifting of the line-tied footpoints of CME flux-ropes. Astron. Astrophys. 621<\/b>, A72 (2019).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Jiang, C. et al. A model of failed solar eruption initiated and destructed by magnetic reconnection. Mon. Not. R. Astron. Soc. 525<\/b>, 5857\u20135867 (2023).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Gou, T. et al. Complete replacement of magnetic flux in a flux rope during a coronal mass ejection. Nat. Astron. 7<\/b>, 815\u2013824 (2023).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Ruffenach, A. et al. Multispacecraft observation of magnetic cloud erosion by magnetic reconnection during propagation. J. Geophys. Res. 117<\/b>, A09101 (2012).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Luo, R. & Liu, R. Where and how does a decay-index profile become saddle-like? Astrophys. J. 929<\/b>, 2 (2022).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    DeVore, C. R. & Antiochos, S. K. Homologous confined filament eruptions via magnetic breakout. Astrophys. J. 680<\/b>, 740\u2013756 (2008).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Demoulin, P., Henoux, J. C., Priest, E. R. & Mandrini, C. H. Quasi-separatrix layers in solar flares. I. Method. Astron. Astrophys. 308<\/b>, 643\u2013655 (1996).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Yashiro, S., Akiyama, S., Gopalswamy, N. & Howard, R. A. Different power-law indices in the frequency distributions of flares with and without coronal mass ejections. Astrophys. J. Lett. 650<\/b>, L143\u2013L146 (2006).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Li, T. et al. Magnetic flux of active regions determining the eruptive character of large solar flares. Astrophys. J. 900<\/b>, 128 (2020).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Donati, J. F. & Landstreet, J. D. Magnetic fields of nondegenerate stars. Annu. Rev. Astron. Astrophys. 47<\/b>, 333\u2013370 (2009).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Alvarado-G\u00f3mez, J. D., Drake, J. J., Cohen, O., Moschou, S. P. & Garraffo, C. Suppression of coronal mass ejections in active stars by an overlying large-scale magnetic field: a numerical study. Astrophys. J. 862<\/b>, 93 (2018).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Lemen, J. R. et al. The atmospheric imaging assembly (AIA) on the Solar Dynamics Observatory (SDO). Sol. Phys. 275<\/b>, 17\u201340 (2012).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Pesnell, W. D., Thompson, B. J. & Chamberlin, P. C. The Solar Dynamics Observatory (SDO). Sol. Phys. 275<\/b>, 3\u201315 (2012).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Cheung, M. C. M. et al. Thermal diagnostics with the atmospheric imaging assembly on board the Solar Dynamics Observatory: a validated method for differential emission measure inversions. Astrophys. J. 807<\/b>, 143 (2015).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Golub, L. et al. The X-ray telescope (XRT) for the Hinode Mission. Sol. Phys. 243<\/b>, 63\u201386 (2007).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    M\u00fcller, D. et al. The Solar Orbiter mission. Science overview. Astron. Astrophys. 642<\/b>, A1 (2020).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Rochus, P. et al. The Solar Orbiter EUI instrument: the extreme ultraviolet imager. Astron. Astrophys. 642<\/b>, A8 (2020).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Veronig, A. M. et al. Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. Living Rev. Sol. Phys. 22<\/b>, 2 (2025).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Brueckner, G. E. et al. The large angle spectroscopic coronagraph (LASCO). Sol. Phys. 162<\/b>, 357\u2013402 (1995).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Cargill, P. J. On the aerodynamic drag force acting on interplanetary coronal mass ejections. Sol. Phys. 221<\/b>, 135\u2013149 (2004).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Vr\u0161nak, B. & \u017dic, T. Transit times of interplanetary coronal mass ejections and the solar wind speed. Astron. Astrophys. 472<\/b>, 937\u2013943 (2007).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Warmuth, A. Large-scale globally propagating coronal waves. Living Rev. Sol. Phys. 12<\/b>, 3 (2015).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Howard, T. A. & Pizzo, V. J. Challenging some contemporary views of coronal mass ejections. I. The case for blast waves. Astrophys. J. 824<\/b>, 92 (2016).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Morosan, D. E., Pomoell, J., Kumari, A., Kilpua, E. K. J. & Vainio, R. A type II solar radio burst without a coronal mass ejection. Astron. Astrophys. 675<\/b>, A98 (2023).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Culhane, J. L. et al. The EUV imaging spectrometer for Hinode. Sol. Phys. 243<\/b>, 19\u201361 (2007).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    De Pontieu, B. et al. The Interface Region Imaging Spectrograph (IRIS). Sol. Phys. 289<\/b>, 2733\u20132779 (2014).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Krucker, S. et al. The spectrometer\/telescope for imaging X-rays (STIX). Astron. Astrophys. 642<\/b>, A15 (2020).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Massa, P. et al. The STIX imaging concept. Sol. Phys. 298<\/b>, 114 (2023).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Gary, D. E. et al. Microwave and hard X-ray observations of the 2017 September 10 solar limb flare. Astrophys. J. 863<\/b>, 83 (2018).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Scherrer, P. H. et al. The helioseismic and magnetic imager (HMI) investigation for the Solar Dynamics Observatory (SDO). Sol. Phys. 275<\/b>, 207\u2013227 (2012).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Solanki, S. K. et al. The polarimetric and helioseismic imager on Solar Orbiter. Astron. Astrophys. 642<\/b>, A11 (2020).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Alissandrakis, C. E. On the computation of constant alpha force-free magnetic field. Astron. Astrophys. 100<\/b>, 197\u2013200 (1981).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Wuelser, J.-P. et al. EUVI: the STEREO-SECCHI extreme ultraviolet imager. In Proc. SPIE Conference Series, Telescopes and Instrumentation for Solar Astrophysics, Vol. 5171 (eds Fineschi, S. & Gummin, M. A.) 111\u2013122 (SPIE, 2004).<\/p>\n<\/li>\n","protected":false},"excerpt":{"rendered":"Priest, E. R. & Forbes, T. G. The magnetic nature of solar flares. Astron. Astrophys. Rev. 10, 313\u2013377…\n","protected":false},"author":2,"featured_media":494797,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":"","_share_on_mastodon":"0"},"categories":[270],"tags":[582,85847,1778,18,910,19,17,452,133,85848,451],"class_list":["post-494796","post","type-post","status-publish","format-standard","has-post-thumbnail","category-space","tag-astronomy","tag-astrophysical-plasmas","tag-astrophysics-and-cosmology","tag-eire","tag-general","tag-ie","tag-ireland","tag-physics","tag-science","tag-solar-physics","tag-space"],"share_on_mastodon":{"url":"https:\/\/pubeurope.com\/@ie\/116609136919789038","error":""},"_links":{"self":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/posts\/494796","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/comments?post=494796"}],"version-history":[{"count":0,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/posts\/494796\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/media\/494797"}],"wp:attachment":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/media?parent=494796"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/categories?post=494796"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/tags?post=494796"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}