Theoretical modeling for the stereo mission

Markus J. Aschwanden, L. F. Burlaga, M. L. Kaiser, C. K. Ng, D. V. Reames, M. J. Reiner, T. I. Gombosi, N. Lugaz, W. Manchester IV, I. I. Roussev, T. H. Zurbuchen, C. J. Farrugia, A. B. Galvin, M. A. Lee, J. A. Linker, Z. Mikić, P. Riley, D. Alexander, A. W. Sandman, J. W. Cook & 21 others R. A. Howard, D. Odstrčil, V. J. Pizzo, J. Kóta, P. C. Liewer, J. G. Luhmann, B. Inhester, R. W. Schwenn, S. K. Solanki, V. M. Vasyliunas, T. Wiegelmann, L. Blush, P. Bochsler, I. H. Cairns, P. A. Robinson, V. Bothmer, K. Kecskeméty, A. Llebaria, M. Maksimovic, M. Scholer, R. F. Wimmer-Schweingruber

Research output: Contribution to journalArticle

25 Citations (Scopus)

Abstract

We summarize the theory and modeling efforts for the STEREO mission, which will be used to interpret the data of both the remote-sensing (SECCHI, SWAVES) and in-situ instruments (IMPACT, PLASTIC). The modeling includes the coronal plasma, in both open and closed magnetic structures, and the solar wind and its expansion outwards from the Sun, which defines the heliosphere. Particular emphasis is given to modeling of dynamic phenomena associated with the initiation and propagation of coronal mass ejections (CMEs). The modeling of the CME initiation includes magnetic shearing, kink instability, filament eruption, and magnetic reconnection in the flaring lower corona. The modeling of CME propagation entails interplanetary shocks, interplanetary particle beams, solar energetic particles (SEPs), geoeffective connections, and space weather. This review describes mostly existing models of groups that have committed their work to the STEREO mission, but is by no means exhaustive or comprehensive regarding alternative theoretical approaches.

Original languageEnglish
Pages (from-to)565-604
Number of pages40
JournalSpace Science Reviews
Volume136
Issue number1-4
DOIs
Publication statusPublished - Apr 2008

Fingerprint

coronal mass ejection
STEREO (observatory)
modeling
interplanetary shock waves
space weather
propagation
heliosphere
particle beams
energetic particles
shearing
volcanic eruptions
coronas
solar wind
remote sensing
filaments
sun
expansion
corona
energetics
volcanic eruption

Keywords

  • Coronal mass ejection (CME)
  • Heliosphere
  • Interplanetary particle beams
  • Interplanetary shocks
  • Solar corona
  • Solar energetic particle events (SEP)
  • Solar filaments
  • Solar flares
  • Solar wind
  • Space weather
  • STEREO mission
  • Stereoscopy

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science
  • Physics and Astronomy (miscellaneous)

Cite this

Aschwanden, M. J., Burlaga, L. F., Kaiser, M. L., Ng, C. K., Reames, D. V., Reiner, M. J., ... Wimmer-Schweingruber, R. F. (2008). Theoretical modeling for the stereo mission. Space Science Reviews, 136(1-4), 565-604. https://doi.org/10.1007/s11214-006-9027-8

Theoretical modeling for the stereo mission. / Aschwanden, Markus J.; Burlaga, L. F.; Kaiser, M. L.; Ng, C. K.; Reames, D. V.; Reiner, M. J.; Gombosi, T. I.; Lugaz, N.; Manchester IV, W.; Roussev, I. I.; Zurbuchen, T. H.; Farrugia, C. J.; Galvin, A. B.; Lee, M. A.; Linker, J. A.; Mikić, Z.; Riley, P.; Alexander, D.; Sandman, A. W.; Cook, J. W.; Howard, R. A.; Odstrčil, D.; Pizzo, V. J.; Kóta, J.; Liewer, P. C.; Luhmann, J. G.; Inhester, B.; Schwenn, R. W.; Solanki, S. K.; Vasyliunas, V. M.; Wiegelmann, T.; Blush, L.; Bochsler, P.; Cairns, I. H.; Robinson, P. A.; Bothmer, V.; Kecskeméty, K.; Llebaria, A.; Maksimovic, M.; Scholer, M.; Wimmer-Schweingruber, R. F.

In: Space Science Reviews, Vol. 136, No. 1-4, 04.2008, p. 565-604.

Research output: Contribution to journalArticle

Aschwanden, MJ, Burlaga, LF, Kaiser, ML, Ng, CK, Reames, DV, Reiner, MJ, Gombosi, TI, Lugaz, N, Manchester IV, W, Roussev, II, Zurbuchen, TH, Farrugia, CJ, Galvin, AB, Lee, MA, Linker, JA, Mikić, Z, Riley, P, Alexander, D, Sandman, AW, Cook, JW, Howard, RA, Odstrčil, D, Pizzo, VJ, Kóta, J, Liewer, PC, Luhmann, JG, Inhester, B, Schwenn, RW, Solanki, SK, Vasyliunas, VM, Wiegelmann, T, Blush, L, Bochsler, P, Cairns, IH, Robinson, PA, Bothmer, V, Kecskeméty, K, Llebaria, A, Maksimovic, M, Scholer, M & Wimmer-Schweingruber, RF 2008, 'Theoretical modeling for the stereo mission', Space Science Reviews, vol. 136, no. 1-4, pp. 565-604. https://doi.org/10.1007/s11214-006-9027-8
Aschwanden MJ, Burlaga LF, Kaiser ML, Ng CK, Reames DV, Reiner MJ et al. Theoretical modeling for the stereo mission. Space Science Reviews. 2008 Apr;136(1-4):565-604. https://doi.org/10.1007/s11214-006-9027-8
Aschwanden, Markus J. ; Burlaga, L. F. ; Kaiser, M. L. ; Ng, C. K. ; Reames, D. V. ; Reiner, M. J. ; Gombosi, T. I. ; Lugaz, N. ; Manchester IV, W. ; Roussev, I. I. ; Zurbuchen, T. H. ; Farrugia, C. J. ; Galvin, A. B. ; Lee, M. A. ; Linker, J. A. ; Mikić, Z. ; Riley, P. ; Alexander, D. ; Sandman, A. W. ; Cook, J. W. ; Howard, R. A. ; Odstrčil, D. ; Pizzo, V. J. ; Kóta, J. ; Liewer, P. C. ; Luhmann, J. G. ; Inhester, B. ; Schwenn, R. W. ; Solanki, S. K. ; Vasyliunas, V. M. ; Wiegelmann, T. ; Blush, L. ; Bochsler, P. ; Cairns, I. H. ; Robinson, P. A. ; Bothmer, V. ; Kecskeméty, K. ; Llebaria, A. ; Maksimovic, M. ; Scholer, M. ; Wimmer-Schweingruber, R. F. / Theoretical modeling for the stereo mission. In: Space Science Reviews. 2008 ; Vol. 136, No. 1-4. pp. 565-604.
@article{75905c1e886f44949951ab21806925ee,
title = "Theoretical modeling for the stereo mission",
abstract = "We summarize the theory and modeling efforts for the STEREO mission, which will be used to interpret the data of both the remote-sensing (SECCHI, SWAVES) and in-situ instruments (IMPACT, PLASTIC). The modeling includes the coronal plasma, in both open and closed magnetic structures, and the solar wind and its expansion outwards from the Sun, which defines the heliosphere. Particular emphasis is given to modeling of dynamic phenomena associated with the initiation and propagation of coronal mass ejections (CMEs). The modeling of the CME initiation includes magnetic shearing, kink instability, filament eruption, and magnetic reconnection in the flaring lower corona. The modeling of CME propagation entails interplanetary shocks, interplanetary particle beams, solar energetic particles (SEPs), geoeffective connections, and space weather. This review describes mostly existing models of groups that have committed their work to the STEREO mission, but is by no means exhaustive or comprehensive regarding alternative theoretical approaches.",
keywords = "Coronal mass ejection (CME), Heliosphere, Interplanetary particle beams, Interplanetary shocks, Solar corona, Solar energetic particle events (SEP), Solar filaments, Solar flares, Solar wind, Space weather, STEREO mission, Stereoscopy",
author = "Aschwanden, {Markus J.} and Burlaga, {L. F.} and Kaiser, {M. L.} and Ng, {C. K.} and Reames, {D. V.} and Reiner, {M. J.} and Gombosi, {T. I.} and N. Lugaz and {Manchester IV}, W. and Roussev, {I. I.} and Zurbuchen, {T. H.} and Farrugia, {C. J.} and Galvin, {A. B.} and Lee, {M. A.} and Linker, {J. A.} and Z. Mikić and P. Riley and D. Alexander and Sandman, {A. W.} and Cook, {J. W.} and Howard, {R. A.} and D. Odstrčil and Pizzo, {V. J.} and J. K{\'o}ta and Liewer, {P. C.} and Luhmann, {J. G.} and B. Inhester and Schwenn, {R. W.} and Solanki, {S. K.} and Vasyliunas, {V. M.} and T. Wiegelmann and L. Blush and P. Bochsler and Cairns, {I. H.} and Robinson, {P. A.} and V. Bothmer and K. Kecskem{\'e}ty and A. Llebaria and M. Maksimovic and M. Scholer and Wimmer-Schweingruber, {R. F.}",
year = "2008",
month = "4",
doi = "10.1007/s11214-006-9027-8",
language = "English",
volume = "136",
pages = "565--604",
journal = "Space Science Reviews",
issn = "0038-6308",
publisher = "Springer Netherlands",
number = "1-4",

}

TY - JOUR

T1 - Theoretical modeling for the stereo mission

AU - Aschwanden, Markus J.

AU - Burlaga, L. F.

AU - Kaiser, M. L.

AU - Ng, C. K.

AU - Reames, D. V.

AU - Reiner, M. J.

AU - Gombosi, T. I.

AU - Lugaz, N.

AU - Manchester IV, W.

AU - Roussev, I. I.

AU - Zurbuchen, T. H.

AU - Farrugia, C. J.

AU - Galvin, A. B.

AU - Lee, M. A.

AU - Linker, J. A.

AU - Mikić, Z.

AU - Riley, P.

AU - Alexander, D.

AU - Sandman, A. W.

AU - Cook, J. W.

AU - Howard, R. A.

AU - Odstrčil, D.

AU - Pizzo, V. J.

AU - Kóta, J.

AU - Liewer, P. C.

AU - Luhmann, J. G.

AU - Inhester, B.

AU - Schwenn, R. W.

AU - Solanki, S. K.

AU - Vasyliunas, V. M.

AU - Wiegelmann, T.

AU - Blush, L.

AU - Bochsler, P.

AU - Cairns, I. H.

AU - Robinson, P. A.

AU - Bothmer, V.

AU - Kecskeméty, K.

AU - Llebaria, A.

AU - Maksimovic, M.

AU - Scholer, M.

AU - Wimmer-Schweingruber, R. F.

PY - 2008/4

Y1 - 2008/4

N2 - We summarize the theory and modeling efforts for the STEREO mission, which will be used to interpret the data of both the remote-sensing (SECCHI, SWAVES) and in-situ instruments (IMPACT, PLASTIC). The modeling includes the coronal plasma, in both open and closed magnetic structures, and the solar wind and its expansion outwards from the Sun, which defines the heliosphere. Particular emphasis is given to modeling of dynamic phenomena associated with the initiation and propagation of coronal mass ejections (CMEs). The modeling of the CME initiation includes magnetic shearing, kink instability, filament eruption, and magnetic reconnection in the flaring lower corona. The modeling of CME propagation entails interplanetary shocks, interplanetary particle beams, solar energetic particles (SEPs), geoeffective connections, and space weather. This review describes mostly existing models of groups that have committed their work to the STEREO mission, but is by no means exhaustive or comprehensive regarding alternative theoretical approaches.

AB - We summarize the theory and modeling efforts for the STEREO mission, which will be used to interpret the data of both the remote-sensing (SECCHI, SWAVES) and in-situ instruments (IMPACT, PLASTIC). The modeling includes the coronal plasma, in both open and closed magnetic structures, and the solar wind and its expansion outwards from the Sun, which defines the heliosphere. Particular emphasis is given to modeling of dynamic phenomena associated with the initiation and propagation of coronal mass ejections (CMEs). The modeling of the CME initiation includes magnetic shearing, kink instability, filament eruption, and magnetic reconnection in the flaring lower corona. The modeling of CME propagation entails interplanetary shocks, interplanetary particle beams, solar energetic particles (SEPs), geoeffective connections, and space weather. This review describes mostly existing models of groups that have committed their work to the STEREO mission, but is by no means exhaustive or comprehensive regarding alternative theoretical approaches.

KW - Coronal mass ejection (CME)

KW - Heliosphere

KW - Interplanetary particle beams

KW - Interplanetary shocks

KW - Solar corona

KW - Solar energetic particle events (SEP)

KW - Solar filaments

KW - Solar flares

KW - Solar wind

KW - Space weather

KW - STEREO mission

KW - Stereoscopy

UR - http://www.scopus.com/inward/record.url?scp=44649195560&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=44649195560&partnerID=8YFLogxK

U2 - 10.1007/s11214-006-9027-8

DO - 10.1007/s11214-006-9027-8

M3 - Article

VL - 136

SP - 565

EP - 604

JO - Space Science Reviews

JF - Space Science Reviews

SN - 0038-6308

IS - 1-4

ER -