Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Bartholomeus van der Holst"'
We use the Space Weather Modeling Framework's Alfvén Wave Solar atmosphere Model to simualte the origin and evolution of solar wind plasma during multiple SO and PSP flybys. Synthetic spectral and narrow band imaging, synthetic spectra and in-situ p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f0ee599576d8de40052afc0bf7e5fb5b
https://doi.org/10.5194/egusphere-egu23-10158
https://doi.org/10.5194/egusphere-egu23-10158
J. Schmidt and Cairns (2019) have recently claimed that they can predict Coronal Mass Ejection (CME) arrival times with an accuracy of 0.9+-1.9 hours for four separate events. They also stated that the accuracy gets better with increased grid resolut
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a0f62c391987d2d6b1e2aeee72f624fa
https://doi.org/10.22541/essoar.167751578.81634844/v1
https://doi.org/10.22541/essoar.167751578.81634844/v1
Autor:
F. A. Nuevo, Nishtha Sachdeva, Cecilia Mac Cormack, Richard A. Frazin, Ward B. Manchester, A. M. Vásquez, Bartholomeus van der Holst, D. G. Lloveras
Publikováno v:
Solar Physics. 295
We carry out a study of the global three-dimensional (3D) structure of the electron density and temperature of the quiescent inner solar corona ( $r