Indirect Dependency

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Reik V Donner - One of the best experts on this subject based on the ideXlab platform.

  • common solar wind drivers behind magnetic storm magnetospheric substorm Dependency
    Scientific Reports, 2018
    Co-Authors: Jakob Runge, Georgios Balasis, I A Daglis, Constantinos Papadimitriou, Reik V Donner
    Abstract:

    The dynamical relationship between magnetic storms and magnetospheric substorms is one of the most controversial issues of contemporary space research. Here, we address this issue through a causal inference approach to two corresponding indices in conjunction with several relevant solar wind variables. We find that the vertical component of the interplanetary magnetic field is the strongest and common driver of both storms and substorms. Further, our results suggest, at least based on the analyzed indices, that there is no statistical evidence for a direct or Indirect Dependency between substorms and storms and their statistical association can be explained by the common solar drivers. Given the powerful statistical tests we performed (by simultaneously taking into account time series of indices and solar wind variables), a physical mechanism through which substorms directly or Indirectly drive storms or vice versa is, therefore, unlikely.

  • Common solar wind drivers behind magnetic storm–magnetospheric substorm Dependency
    Scientific Reports, 2018
    Co-Authors: Jakob Runge, Georgios Balasis, I A Daglis, Constantinos Papadimitriou, Reik V Donner
    Abstract:

    The dynamical relationship between magnetic storms and magnetospheric substorms is one of the most controversial issues of contemporary space research. Here, we address this issue through a causal inference approach to two corresponding indices in conjunction with several relevant solar wind variables. We find that the vertical component of the interplanetary magnetic field is the strongest and common driver of both storms and substorms. Further, our results suggest, at least based on the analyzed indices, that there is no statistical evidence for a direct or Indirect Dependency between substorms and storms and their statistical association can be explained by the common solar drivers. Given the powerful statistical tests we performed (by simultaneously taking into account time series of indices and solar wind variables), a physical mechanism through which substorms directly or Indirectly drive storms or vice versa is, therefore, unlikely.

  • common solar wind drivers behind magnetic storm magnetospheric substorm Dependency
    arXiv: Space Physics, 2018
    Co-Authors: Jakob Runge, Georgios Balasis, I A Daglis, Constantinos Papadimitriou, Reik V Donner
    Abstract:

    The dynamical relationship between magnetic storms and magnetospheric substorms presents one of the most controversial problems of contemporary geospace research. Here, we tackle this issue by applying a causal inference approach to two corresponding indices in conjunction with several relevant solar wind variables. We demonstrate that the vertical component of the interplanetary magnetic field is the strongest and common driver of both, storms and substorms, and explains their the previously reported association. These results hold during both solar maximum and minimum phases and suggest that, at least based on the analyzed indices, there is no statistical evidence for a direct or Indirect Dependency between substorms and storms. A physical mechanism by which substorms drive storms or vice versa is, therefore, unlikely.

Jakob Runge - One of the best experts on this subject based on the ideXlab platform.

  • common solar wind drivers behind magnetic storm magnetospheric substorm Dependency
    Scientific Reports, 2018
    Co-Authors: Jakob Runge, Georgios Balasis, I A Daglis, Constantinos Papadimitriou, Reik V Donner
    Abstract:

    The dynamical relationship between magnetic storms and magnetospheric substorms is one of the most controversial issues of contemporary space research. Here, we address this issue through a causal inference approach to two corresponding indices in conjunction with several relevant solar wind variables. We find that the vertical component of the interplanetary magnetic field is the strongest and common driver of both storms and substorms. Further, our results suggest, at least based on the analyzed indices, that there is no statistical evidence for a direct or Indirect Dependency between substorms and storms and their statistical association can be explained by the common solar drivers. Given the powerful statistical tests we performed (by simultaneously taking into account time series of indices and solar wind variables), a physical mechanism through which substorms directly or Indirectly drive storms or vice versa is, therefore, unlikely.

  • Common solar wind drivers behind magnetic storm–magnetospheric substorm Dependency
    Scientific Reports, 2018
    Co-Authors: Jakob Runge, Georgios Balasis, I A Daglis, Constantinos Papadimitriou, Reik V Donner
    Abstract:

    The dynamical relationship between magnetic storms and magnetospheric substorms is one of the most controversial issues of contemporary space research. Here, we address this issue through a causal inference approach to two corresponding indices in conjunction with several relevant solar wind variables. We find that the vertical component of the interplanetary magnetic field is the strongest and common driver of both storms and substorms. Further, our results suggest, at least based on the analyzed indices, that there is no statistical evidence for a direct or Indirect Dependency between substorms and storms and their statistical association can be explained by the common solar drivers. Given the powerful statistical tests we performed (by simultaneously taking into account time series of indices and solar wind variables), a physical mechanism through which substorms directly or Indirectly drive storms or vice versa is, therefore, unlikely.

  • common solar wind drivers behind magnetic storm magnetospheric substorm Dependency
    arXiv: Space Physics, 2018
    Co-Authors: Jakob Runge, Georgios Balasis, I A Daglis, Constantinos Papadimitriou, Reik V Donner
    Abstract:

    The dynamical relationship between magnetic storms and magnetospheric substorms presents one of the most controversial problems of contemporary geospace research. Here, we tackle this issue by applying a causal inference approach to two corresponding indices in conjunction with several relevant solar wind variables. We demonstrate that the vertical component of the interplanetary magnetic field is the strongest and common driver of both, storms and substorms, and explains their the previously reported association. These results hold during both solar maximum and minimum phases and suggest that, at least based on the analyzed indices, there is no statistical evidence for a direct or Indirect Dependency between substorms and storms. A physical mechanism by which substorms drive storms or vice versa is, therefore, unlikely.

Constantinos Papadimitriou - One of the best experts on this subject based on the ideXlab platform.

  • common solar wind drivers behind magnetic storm magnetospheric substorm Dependency
    Scientific Reports, 2018
    Co-Authors: Jakob Runge, Georgios Balasis, I A Daglis, Constantinos Papadimitriou, Reik V Donner
    Abstract:

    The dynamical relationship between magnetic storms and magnetospheric substorms is one of the most controversial issues of contemporary space research. Here, we address this issue through a causal inference approach to two corresponding indices in conjunction with several relevant solar wind variables. We find that the vertical component of the interplanetary magnetic field is the strongest and common driver of both storms and substorms. Further, our results suggest, at least based on the analyzed indices, that there is no statistical evidence for a direct or Indirect Dependency between substorms and storms and their statistical association can be explained by the common solar drivers. Given the powerful statistical tests we performed (by simultaneously taking into account time series of indices and solar wind variables), a physical mechanism through which substorms directly or Indirectly drive storms or vice versa is, therefore, unlikely.

  • Common solar wind drivers behind magnetic storm–magnetospheric substorm Dependency
    Scientific Reports, 2018
    Co-Authors: Jakob Runge, Georgios Balasis, I A Daglis, Constantinos Papadimitriou, Reik V Donner
    Abstract:

    The dynamical relationship between magnetic storms and magnetospheric substorms is one of the most controversial issues of contemporary space research. Here, we address this issue through a causal inference approach to two corresponding indices in conjunction with several relevant solar wind variables. We find that the vertical component of the interplanetary magnetic field is the strongest and common driver of both storms and substorms. Further, our results suggest, at least based on the analyzed indices, that there is no statistical evidence for a direct or Indirect Dependency between substorms and storms and their statistical association can be explained by the common solar drivers. Given the powerful statistical tests we performed (by simultaneously taking into account time series of indices and solar wind variables), a physical mechanism through which substorms directly or Indirectly drive storms or vice versa is, therefore, unlikely.

  • common solar wind drivers behind magnetic storm magnetospheric substorm Dependency
    arXiv: Space Physics, 2018
    Co-Authors: Jakob Runge, Georgios Balasis, I A Daglis, Constantinos Papadimitriou, Reik V Donner
    Abstract:

    The dynamical relationship between magnetic storms and magnetospheric substorms presents one of the most controversial problems of contemporary geospace research. Here, we tackle this issue by applying a causal inference approach to two corresponding indices in conjunction with several relevant solar wind variables. We demonstrate that the vertical component of the interplanetary magnetic field is the strongest and common driver of both, storms and substorms, and explains their the previously reported association. These results hold during both solar maximum and minimum phases and suggest that, at least based on the analyzed indices, there is no statistical evidence for a direct or Indirect Dependency between substorms and storms. A physical mechanism by which substorms drive storms or vice versa is, therefore, unlikely.

I A Daglis - One of the best experts on this subject based on the ideXlab platform.

  • common solar wind drivers behind magnetic storm magnetospheric substorm Dependency
    Scientific Reports, 2018
    Co-Authors: Jakob Runge, Georgios Balasis, I A Daglis, Constantinos Papadimitriou, Reik V Donner
    Abstract:

    The dynamical relationship between magnetic storms and magnetospheric substorms is one of the most controversial issues of contemporary space research. Here, we address this issue through a causal inference approach to two corresponding indices in conjunction with several relevant solar wind variables. We find that the vertical component of the interplanetary magnetic field is the strongest and common driver of both storms and substorms. Further, our results suggest, at least based on the analyzed indices, that there is no statistical evidence for a direct or Indirect Dependency between substorms and storms and their statistical association can be explained by the common solar drivers. Given the powerful statistical tests we performed (by simultaneously taking into account time series of indices and solar wind variables), a physical mechanism through which substorms directly or Indirectly drive storms or vice versa is, therefore, unlikely.

  • Common solar wind drivers behind magnetic storm–magnetospheric substorm Dependency
    Scientific Reports, 2018
    Co-Authors: Jakob Runge, Georgios Balasis, I A Daglis, Constantinos Papadimitriou, Reik V Donner
    Abstract:

    The dynamical relationship between magnetic storms and magnetospheric substorms is one of the most controversial issues of contemporary space research. Here, we address this issue through a causal inference approach to two corresponding indices in conjunction with several relevant solar wind variables. We find that the vertical component of the interplanetary magnetic field is the strongest and common driver of both storms and substorms. Further, our results suggest, at least based on the analyzed indices, that there is no statistical evidence for a direct or Indirect Dependency between substorms and storms and their statistical association can be explained by the common solar drivers. Given the powerful statistical tests we performed (by simultaneously taking into account time series of indices and solar wind variables), a physical mechanism through which substorms directly or Indirectly drive storms or vice versa is, therefore, unlikely.

  • common solar wind drivers behind magnetic storm magnetospheric substorm Dependency
    arXiv: Space Physics, 2018
    Co-Authors: Jakob Runge, Georgios Balasis, I A Daglis, Constantinos Papadimitriou, Reik V Donner
    Abstract:

    The dynamical relationship between magnetic storms and magnetospheric substorms presents one of the most controversial problems of contemporary geospace research. Here, we tackle this issue by applying a causal inference approach to two corresponding indices in conjunction with several relevant solar wind variables. We demonstrate that the vertical component of the interplanetary magnetic field is the strongest and common driver of both, storms and substorms, and explains their the previously reported association. These results hold during both solar maximum and minimum phases and suggest that, at least based on the analyzed indices, there is no statistical evidence for a direct or Indirect Dependency between substorms and storms. A physical mechanism by which substorms drive storms or vice versa is, therefore, unlikely.

Georgios Balasis - One of the best experts on this subject based on the ideXlab platform.

  • common solar wind drivers behind magnetic storm magnetospheric substorm Dependency
    Scientific Reports, 2018
    Co-Authors: Jakob Runge, Georgios Balasis, I A Daglis, Constantinos Papadimitriou, Reik V Donner
    Abstract:

    The dynamical relationship between magnetic storms and magnetospheric substorms is one of the most controversial issues of contemporary space research. Here, we address this issue through a causal inference approach to two corresponding indices in conjunction with several relevant solar wind variables. We find that the vertical component of the interplanetary magnetic field is the strongest and common driver of both storms and substorms. Further, our results suggest, at least based on the analyzed indices, that there is no statistical evidence for a direct or Indirect Dependency between substorms and storms and their statistical association can be explained by the common solar drivers. Given the powerful statistical tests we performed (by simultaneously taking into account time series of indices and solar wind variables), a physical mechanism through which substorms directly or Indirectly drive storms or vice versa is, therefore, unlikely.

  • Common solar wind drivers behind magnetic storm–magnetospheric substorm Dependency
    Scientific Reports, 2018
    Co-Authors: Jakob Runge, Georgios Balasis, I A Daglis, Constantinos Papadimitriou, Reik V Donner
    Abstract:

    The dynamical relationship between magnetic storms and magnetospheric substorms is one of the most controversial issues of contemporary space research. Here, we address this issue through a causal inference approach to two corresponding indices in conjunction with several relevant solar wind variables. We find that the vertical component of the interplanetary magnetic field is the strongest and common driver of both storms and substorms. Further, our results suggest, at least based on the analyzed indices, that there is no statistical evidence for a direct or Indirect Dependency between substorms and storms and their statistical association can be explained by the common solar drivers. Given the powerful statistical tests we performed (by simultaneously taking into account time series of indices and solar wind variables), a physical mechanism through which substorms directly or Indirectly drive storms or vice versa is, therefore, unlikely.

  • common solar wind drivers behind magnetic storm magnetospheric substorm Dependency
    arXiv: Space Physics, 2018
    Co-Authors: Jakob Runge, Georgios Balasis, I A Daglis, Constantinos Papadimitriou, Reik V Donner
    Abstract:

    The dynamical relationship between magnetic storms and magnetospheric substorms presents one of the most controversial problems of contemporary geospace research. Here, we tackle this issue by applying a causal inference approach to two corresponding indices in conjunction with several relevant solar wind variables. We demonstrate that the vertical component of the interplanetary magnetic field is the strongest and common driver of both, storms and substorms, and explains their the previously reported association. These results hold during both solar maximum and minimum phases and suggest that, at least based on the analyzed indices, there is no statistical evidence for a direct or Indirect Dependency between substorms and storms. A physical mechanism by which substorms drive storms or vice versa is, therefore, unlikely.