SWIFF: Space weather integrated forecasting framework

G. Lapenta; V. Pierrard; R. Keppens; S. Markidis; S. Poedts; O. Šebek; P.M. Trávníček; P. Henri; F. Califano; F. Pegoraro; M. Faganello; A.L. Restante; Åke Nordlund; Jacob Trier Frederiksen; D.H. Mackay; C.E. Parnell; A. Bemporad; R. Susino; K. Borremans

doi:10.1051/swsc/2013027

SWIFF: Space weather integrated forecasting framework

G. Lapenta, V. Pierrard, R. Keppens, S. Markidis, S. Poedts, O. Šebek, P.M. Trávníček, P. Henri, F. Califano, F. Pegoraro, M. Faganello, A.L. Restante, Åke Nordlund, Jacob Trier Frederiksen, D.H. Mackay, C.E. Parnell, A. Bemporad, R. Susino, K. Borremans

Astrophysics and Planetary Science

14 Citations (Scopus)

Abstract

SWIFF is a project funded by the Seventh Framework Programme of the European Commission to study the mathematical-physics models that form the basis for space weather forecasting. The phenomena of space weather span a tremendous scale of densities and temperature with scales ranging 10 orders of magnitude in space and time. Additionally even in local regions there are concurrent processes developing at the electron, ion and global scales strongly interacting with each other. The fundamental challenge in modelling space weather is the need to address multiple physics and multiple scales. Here we present our approach to take existing expertise in fluid and kinetic models to produce an integrated mathematical approach and software infrastructure that allows fluid and kinetic processes to be modelled together. SWIFF aims also at using this new infrastructure to model specific coupled processes at the Solar Corona, in the interplanetary space and in the interaction at the Earth magnetosphere.

Original language	English
Article number	A05
Journal	Journal of Space Weather and Space Climate
Volume	3
Number of pages	17
ISSN	2115-7251
DOIs	https://doi.org/10.1051/swsc/2013027
Publication status	Published - 18 Feb 2013

Access to Document

10.1051/swsc/2013027

Cite this

Lapenta, G., Pierrard, V., Keppens, R., Markidis, S., Poedts, S., Šebek, O., Trávníček, P. M., Henri, P., Califano, F., Pegoraro, F., Faganello, M., Restante, A. L., Nordlund, Å., Frederiksen, J. T., Mackay, D. H., Parnell, C. E., Bemporad, A., Susino, R., & Borremans, K. (2013). SWIFF: Space weather integrated forecasting framework. Journal of Space Weather and Space Climate, 3, [A05]. https://doi.org/10.1051/swsc/2013027

Lapenta, G, Pierrard, V, Keppens, R, Markidis, S, Poedts, S, Šebek, O, Trávníček, PM, Henri, P, Califano, F, Pegoraro, F, Faganello, M, Restante, AL, Nordlund, Å, Frederiksen, JT, Mackay, DH, Parnell, CE, Bemporad, A, Susino, R & Borremans, K 2013, 'SWIFF: Space weather integrated forecasting framework', Journal of Space Weather and Space Climate, vol. 3, A05. https://doi.org/10.1051/swsc/2013027

@article{9f7d2b28ed934a2ab263fdd4cb24543a,

title = "SWIFF: Space weather integrated forecasting framework",

abstract = "SWIFF is a project funded by the Seventh Framework Programme of the European Commission to study the mathematical-physics models that form the basis for space weather forecasting. The phenomena of space weather span a tremendous scale of densities and temperature with scales ranging 10 orders of magnitude in space and time. Additionally even in local regions there are concurrent processes developing at the electron, ion and global scales strongly interacting with each other. The fundamental challenge in modelling space weather is the need to address multiple physics and multiple scales. Here we present our approach to take existing expertise in fluid and kinetic models to produce an integrated mathematical approach and software infrastructure that allows fluid and kinetic processes to be modelled together. SWIFF aims also at using this new infrastructure to model specific coupled processes at the Solar Corona, in the interplanetary space and in the interaction at the Earth magnetosphere.",

author = "G. Lapenta and V. Pierrard and R. Keppens and S. Markidis and S. Poedts and O. {\v S}ebek and P.M. Tr{\'a}vn{\'i}{\v c}ek and P. Henri and F. Califano and F. Pegoraro and M. Faganello and A.L. Restante and {\AA}ke Nordlund and Frederiksen, {Jacob Trier} and D.H. Mackay and C.E. Parnell and A. Bemporad and R. Susino and K. Borremans",

year = "2013",

month = feb,

day = "18",

doi = "10.1051/swsc/2013027",

language = "English",

volume = "3",

journal = "Journal of Space Weather and Space Climate",

issn = "2115-7251",

publisher = "E D P Sciences",

}

TY - JOUR

T1 - SWIFF

T2 - Space weather integrated forecasting framework

AU - Lapenta, G.

AU - Pierrard, V.

AU - Keppens, R.

AU - Markidis, S.

AU - Poedts, S.

AU - Šebek, O.

AU - Trávníček, P.M.

AU - Henri, P.

AU - Califano, F.

AU - Pegoraro, F.

AU - Faganello, M.

AU - Restante, A.L.

AU - Nordlund, Åke

AU - Frederiksen, Jacob Trier

AU - Mackay, D.H.

AU - Parnell, C.E.

AU - Bemporad, A.

AU - Susino, R.

AU - Borremans, K.

PY - 2013/2/18

Y1 - 2013/2/18

N2 - SWIFF is a project funded by the Seventh Framework Programme of the European Commission to study the mathematical-physics models that form the basis for space weather forecasting. The phenomena of space weather span a tremendous scale of densities and temperature with scales ranging 10 orders of magnitude in space and time. Additionally even in local regions there are concurrent processes developing at the electron, ion and global scales strongly interacting with each other. The fundamental challenge in modelling space weather is the need to address multiple physics and multiple scales. Here we present our approach to take existing expertise in fluid and kinetic models to produce an integrated mathematical approach and software infrastructure that allows fluid and kinetic processes to be modelled together. SWIFF aims also at using this new infrastructure to model specific coupled processes at the Solar Corona, in the interplanetary space and in the interaction at the Earth magnetosphere.

AB - SWIFF is a project funded by the Seventh Framework Programme of the European Commission to study the mathematical-physics models that form the basis for space weather forecasting. The phenomena of space weather span a tremendous scale of densities and temperature with scales ranging 10 orders of magnitude in space and time. Additionally even in local regions there are concurrent processes developing at the electron, ion and global scales strongly interacting with each other. The fundamental challenge in modelling space weather is the need to address multiple physics and multiple scales. Here we present our approach to take existing expertise in fluid and kinetic models to produce an integrated mathematical approach and software infrastructure that allows fluid and kinetic processes to be modelled together. SWIFF aims also at using this new infrastructure to model specific coupled processes at the Solar Corona, in the interplanetary space and in the interaction at the Earth magnetosphere.

U2 - 10.1051/swsc/2013027

DO - 10.1051/swsc/2013027

M3 - Journal article

SN - 2115-7251

VL - 3

JO - Journal of Space Weather and Space Climate

JF - Journal of Space Weather and Space Climate

M1 - A05

ER -

SWIFF: Space weather integrated forecasting framework

Abstract

Access to Document

Fingerprint

Cite this