author_facet Lin, Naiguo
Frey, H. U.
Mende, S. B.
Mozer, F. S.
Lysak, R. L.
Song, Y.
Angelopoulos, V.
Lin, Naiguo
Frey, H. U.
Mende, S. B.
Mozer, F. S.
Lysak, R. L.
Song, Y.
Angelopoulos, V.
author Lin, Naiguo
Frey, H. U.
Mende, S. B.
Mozer, F. S.
Lysak, R. L.
Song, Y.
Angelopoulos, V.
spellingShingle Lin, Naiguo
Frey, H. U.
Mende, S. B.
Mozer, F. S.
Lysak, R. L.
Song, Y.
Angelopoulos, V.
Journal of Geophysical Research: Space Physics
Statistical study of substorm timing sequence
Paleontology
Space and Planetary Science
Earth and Planetary Sciences (miscellaneous)
Atmospheric Science
Earth-Surface Processes
Geochemistry and Petrology
Soil Science
Water Science and Technology
Ecology
Aquatic Science
Forestry
Oceanography
Geophysics
author_sort lin, naiguo
spelling Lin, Naiguo Frey, H. U. Mende, S. B. Mozer, F. S. Lysak, R. L. Song, Y. Angelopoulos, V. 0148-0227 American Geophysical Union (AGU) Paleontology Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Atmospheric Science Earth-Surface Processes Geochemistry and Petrology Soil Science Water Science and Technology Ecology Aquatic Science Forestry Oceanography Geophysics http://dx.doi.org/10.1029/2009ja014381 <jats:p>Observations of timing sequences of substorms expected in various onset mechanisms are examined by using a space‐time diagram, which correlates observed space signatures and auroral signatures on the ground during substorm onset. Results from a statistical study of 11 substorms show that signatures in the midtail (<jats:italic>x</jats:italic> ∼ 15–25 <jats:italic>R</jats:italic><jats:sub><jats:italic>E</jats:italic></jats:sub>) typically occur before the ground signatures and those in the near‐Earth tail (<jats:italic>x</jats:italic> ∼ 10 <jats:italic>R</jats:italic><jats:sub><jats:italic>E</jats:italic></jats:sub>) and that signatures in the midtail region observed prior to the substorm onset often occur at a time which was shorter than that expected from MHD wave propagation between the different regions. This suggests that the disturbance onsets in different active regions do not seem to have a simple causal relationship between them as described by the reconnection or current disruption models of substorms. The activation of perturbed fields and plasma flows in space including the signatures of reconnection and current disruption may occur in multiple localized regions throughout the stressed tail current sheet. The activation seems to be continuously observed well after the substorm onset. These results to some extent are consistent with suggested global Alfvénic interaction considerations, in which the substorm onset is the result of Alfvénic interaction in the global current systems.</jats:p> Statistical study of substorm timing sequence Journal of Geophysical Research: Space Physics
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Biologie
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title Statistical study of substorm timing sequence
title_unstemmed Statistical study of substorm timing sequence
title_full Statistical study of substorm timing sequence
title_fullStr Statistical study of substorm timing sequence
title_full_unstemmed Statistical study of substorm timing sequence
title_short Statistical study of substorm timing sequence
title_sort statistical study of substorm timing sequence
topic Paleontology
Space and Planetary Science
Earth and Planetary Sciences (miscellaneous)
Atmospheric Science
Earth-Surface Processes
Geochemistry and Petrology
Soil Science
Water Science and Technology
Ecology
Aquatic Science
Forestry
Oceanography
Geophysics
url http://dx.doi.org/10.1029/2009ja014381
publishDate 2009
physical
description <jats:p>Observations of timing sequences of substorms expected in various onset mechanisms are examined by using a space‐time diagram, which correlates observed space signatures and auroral signatures on the ground during substorm onset. Results from a statistical study of 11 substorms show that signatures in the midtail (<jats:italic>x</jats:italic> ∼ 15–25 <jats:italic>R</jats:italic><jats:sub><jats:italic>E</jats:italic></jats:sub>) typically occur before the ground signatures and those in the near‐Earth tail (<jats:italic>x</jats:italic> ∼ 10 <jats:italic>R</jats:italic><jats:sub><jats:italic>E</jats:italic></jats:sub>) and that signatures in the midtail region observed prior to the substorm onset often occur at a time which was shorter than that expected from MHD wave propagation between the different regions. This suggests that the disturbance onsets in different active regions do not seem to have a simple causal relationship between them as described by the reconnection or current disruption models of substorms. The activation of perturbed fields and plasma flows in space including the signatures of reconnection and current disruption may occur in multiple localized regions throughout the stressed tail current sheet. The activation seems to be continuously observed well after the substorm onset. These results to some extent are consistent with suggested global Alfvénic interaction considerations, in which the substorm onset is the result of Alfvénic interaction in the global current systems.</jats:p>
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author Lin, Naiguo, Frey, H. U., Mende, S. B., Mozer, F. S., Lysak, R. L., Song, Y., Angelopoulos, V.
author_facet Lin, Naiguo, Frey, H. U., Mende, S. B., Mozer, F. S., Lysak, R. L., Song, Y., Angelopoulos, V., Lin, Naiguo, Frey, H. U., Mende, S. B., Mozer, F. S., Lysak, R. L., Song, Y., Angelopoulos, V.
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container_issue A12
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container_title Journal of Geophysical Research: Space Physics
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description <jats:p>Observations of timing sequences of substorms expected in various onset mechanisms are examined by using a space‐time diagram, which correlates observed space signatures and auroral signatures on the ground during substorm onset. Results from a statistical study of 11 substorms show that signatures in the midtail (<jats:italic>x</jats:italic> ∼ 15–25 <jats:italic>R</jats:italic><jats:sub><jats:italic>E</jats:italic></jats:sub>) typically occur before the ground signatures and those in the near‐Earth tail (<jats:italic>x</jats:italic> ∼ 10 <jats:italic>R</jats:italic><jats:sub><jats:italic>E</jats:italic></jats:sub>) and that signatures in the midtail region observed prior to the substorm onset often occur at a time which was shorter than that expected from MHD wave propagation between the different regions. This suggests that the disturbance onsets in different active regions do not seem to have a simple causal relationship between them as described by the reconnection or current disruption models of substorms. The activation of perturbed fields and plasma flows in space including the signatures of reconnection and current disruption may occur in multiple localized regions throughout the stressed tail current sheet. The activation seems to be continuously observed well after the substorm onset. These results to some extent are consistent with suggested global Alfvénic interaction considerations, in which the substorm onset is the result of Alfvénic interaction in the global current systems.</jats:p>
doi_str_mv 10.1029/2009ja014381
facet_avail Online, Free
finc_class_facet Allgemeine Naturwissenschaft, Physik, Technik, Geologie und Paläontologie, Geographie, Chemie und Pharmazie, Land- und Forstwirtschaft, Gartenbau, Fischereiwirtschaft, Hauswirtschaft, Biologie
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spelling Lin, Naiguo Frey, H. U. Mende, S. B. Mozer, F. S. Lysak, R. L. Song, Y. Angelopoulos, V. 0148-0227 American Geophysical Union (AGU) Paleontology Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Atmospheric Science Earth-Surface Processes Geochemistry and Petrology Soil Science Water Science and Technology Ecology Aquatic Science Forestry Oceanography Geophysics http://dx.doi.org/10.1029/2009ja014381 <jats:p>Observations of timing sequences of substorms expected in various onset mechanisms are examined by using a space‐time diagram, which correlates observed space signatures and auroral signatures on the ground during substorm onset. Results from a statistical study of 11 substorms show that signatures in the midtail (<jats:italic>x</jats:italic> ∼ 15–25 <jats:italic>R</jats:italic><jats:sub><jats:italic>E</jats:italic></jats:sub>) typically occur before the ground signatures and those in the near‐Earth tail (<jats:italic>x</jats:italic> ∼ 10 <jats:italic>R</jats:italic><jats:sub><jats:italic>E</jats:italic></jats:sub>) and that signatures in the midtail region observed prior to the substorm onset often occur at a time which was shorter than that expected from MHD wave propagation between the different regions. This suggests that the disturbance onsets in different active regions do not seem to have a simple causal relationship between them as described by the reconnection or current disruption models of substorms. The activation of perturbed fields and plasma flows in space including the signatures of reconnection and current disruption may occur in multiple localized regions throughout the stressed tail current sheet. The activation seems to be continuously observed well after the substorm onset. These results to some extent are consistent with suggested global Alfvénic interaction considerations, in which the substorm onset is the result of Alfvénic interaction in the global current systems.</jats:p> Statistical study of substorm timing sequence Journal of Geophysical Research: Space Physics
spellingShingle Lin, Naiguo, Frey, H. U., Mende, S. B., Mozer, F. S., Lysak, R. L., Song, Y., Angelopoulos, V., Journal of Geophysical Research: Space Physics, Statistical study of substorm timing sequence, Paleontology, Space and Planetary Science, Earth and Planetary Sciences (miscellaneous), Atmospheric Science, Earth-Surface Processes, Geochemistry and Petrology, Soil Science, Water Science and Technology, Ecology, Aquatic Science, Forestry, Oceanography, Geophysics
title Statistical study of substorm timing sequence
title_full Statistical study of substorm timing sequence
title_fullStr Statistical study of substorm timing sequence
title_full_unstemmed Statistical study of substorm timing sequence
title_short Statistical study of substorm timing sequence
title_sort statistical study of substorm timing sequence
title_unstemmed Statistical study of substorm timing sequence
topic Paleontology, Space and Planetary Science, Earth and Planetary Sciences (miscellaneous), Atmospheric Science, Earth-Surface Processes, Geochemistry and Petrology, Soil Science, Water Science and Technology, Ecology, Aquatic Science, Forestry, Oceanography, Geophysics
url http://dx.doi.org/10.1029/2009ja014381