Zobrazeno 1 - 7
of 7
pro vyhledávání: '"G. J. M. Vissers"'
Autor:
G. J. M. Vissers, S. Danilovic, X. Zhu, J. Leenaarts, C. J. Díaz Baso, J. M. da Silva Santos, J. de la Cruz Rodríguez, T. Wiegelmann
Publikováno v:
Astronomy and Astrophysics
Context. A proper estimate of the chromospheric magnetic fields is thought to improve modelling of both active region and coronal mass ejection evolution. However, because the chromospheric field is not regularly obtained for sufficiently large field
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::69c899909053c15a48148d8189ca19d8
https://hdl.handle.net/21.11116/0000-000C-B1B0-4
https://hdl.handle.net/21.11116/0000-000C-B1B0-4
Autor:
J. M. da Silva Santos, S. Danilovic, J. Leenaarts, J. de la Cruz Rodríguez, X. Zhu, S. M. White, G. J. M. Vissers, M. Rempel
Publikováno v:
Astronomy and Astrophysics
The solar chromosphere is heated to temperatures higher than predicted by radiative equilibrium. This excess heating is greater in active regions where the magnetic field is stronger. We aim to investigate the magnetic topology associated with an are
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::230c1c87b81bf05467b29a34f2c046d4
https://hdl.handle.net/21.11116/0000-000C-B202-8
https://hdl.handle.net/21.11116/0000-000C-B202-8
Autor:
C. J. Díaz Baso, Sanja Danilovic, G. J. M. Vissers, R. Morosin, Daniel Price, Aaron Reid, J. de la Cruz Rodríguez, J. Leenaarts, Jens Pomoell, Satoshi Inoue
Publikováno v:
Astronomy & Astrophysics. 645:A1
Obtaining the magnetic field vector accurately in the solar atmosphere is essential for studying changes in field topology during flares and to reliably model space weather. We tackle this problem by applying various inversion methods to a confined X
Autor:
T. Fredvik, T. Hillberg, Göran B. Scharmer, Jaime de la Cruz Rodríguez, Mats G. Löfdahl, Oleksii Andriienko, G. J. M. Vissers, Stein Vidar Hagfors Haugan
Context: Data from ground-based, high-resolution solar telescopes can only be used for science with calibrations and processing, which requires detailed knowledge about the instrumentation. [...] Aims: We aim to provide observers with a user-friendly
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f31473e31d057560c767692169e3712f
Penumbral microjets are short-lived, fine-structured and bright jets that are generally observed in chromospheric imaging of the penumbra of sunspots. Here we investigate their potential transition region signature, by combining observations with the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c937b5f4d9cedcea88c30bba6c358b76
http://hdl.handle.net/10852/56960
http://hdl.handle.net/10852/56960
Small and elongated, cool and dense blob-like structures are being reported with high resolution telescopes in physically different regions throughout the solar atmosphere. Their detection and the understanding of their formation, morphology and ther
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e4fa75b12629abb60ca6a2e2fbbdd4a3
Publikováno v:
Astrophysical Journal; 10/10/2015, Vol. 812 Issue 1, p1-1, 1p