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Universal properties of mirror mode turbulence in the Earth's magnetosheath
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| Zeitschriftentitel: | Geophysical Research Letters |
|---|---|
| Personen und Körperschaften: | , , |
| In: | Geophysical Research Letters, 42, 2015, 9, S. 3085-3092 |
| Format: | E-Article |
| Sprache: | Englisch |
| veröffentlicht: |
American Geophysical Union (AGU)
|
| Schlagwörter: |
| author_facet |
Osmane, A. Dimmock, A. P. Pulkkinen, T. I. Osmane, A. Dimmock, A. P. Pulkkinen, T. I. |
|---|---|
| author |
Osmane, A. Dimmock, A. P. Pulkkinen, T. I. |
| spellingShingle |
Osmane, A. Dimmock, A. P. Pulkkinen, T. I. Geophysical Research Letters Universal properties of mirror mode turbulence in the Earth's magnetosheath General Earth and Planetary Sciences Geophysics |
| author_sort |
osmane, a. |
| spelling |
Osmane, A. Dimmock, A. P. Pulkkinen, T. I. 0094-8276 1944-8007 American Geophysical Union (AGU) General Earth and Planetary Sciences Geophysics http://dx.doi.org/10.1002/2015gl063771 <jats:title>Abstract</jats:title><jats:p>We use more than 7 years of Time History of Events and Macroscale Interactions during Substorms observations to quantify the non‐Gaussian properties associated with mirror mode turbulence in the Earth's magnetosheath. We find that non‐Gaussian statistics of mirror modes lead to the parabolic collapse of kurtosis as the square of the skewness (<jats:italic>K</jats:italic> = <jats:italic>a</jats:italic><jats:italic>S</jats:italic><jats:sup>2</jats:sup>+<jats:italic>B</jats:italic> with <jats:italic>a</jats:italic> ∼ 1.3 and <jats:italic>b</jats:italic> ∼− 1). The parabolic scaling is a global constraint for the magnetosheath and is dictated by kinetic processes. This parabolic scaling is qualitatively independent of the distance to the magnetopause or bow shock, which implies that, even though the bow shock is driving the mirror mode instability, the dynamical evolution of mirror structures is independent of the source region and due to local processes. The parabolic relationship and coefficients between kurtosis and skewness for mirror modes in the Earth's magnetosheath are also similar to those found in a wide range of geophysical and laboratory turbulent environments, providing further evidence that turbulent systems dominated by non‐Gaussian fluctuations hold universal statistical properties.</jats:p> Universal properties of mirror mode turbulence in the Earth's magnetosheath Geophysical Research Letters |
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10.1002/2015gl063771 |
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American Geophysical Union (AGU), 2015 |
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American Geophysical Union (AGU), 2015 |
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0094-8276 1944-8007 |
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| title |
Universal properties of mirror mode turbulence in the Earth's magnetosheath |
| title_unstemmed |
Universal properties of mirror mode turbulence in the Earth's magnetosheath |
| title_full |
Universal properties of mirror mode turbulence in the Earth's magnetosheath |
| title_fullStr |
Universal properties of mirror mode turbulence in the Earth's magnetosheath |
| title_full_unstemmed |
Universal properties of mirror mode turbulence in the Earth's magnetosheath |
| title_short |
Universal properties of mirror mode turbulence in the Earth's magnetosheath |
| title_sort |
universal properties of mirror mode turbulence in the earth's magnetosheath |
| topic |
General Earth and Planetary Sciences Geophysics |
| url |
http://dx.doi.org/10.1002/2015gl063771 |
| publishDate |
2015 |
| physical |
3085-3092 |
| description |
<jats:title>Abstract</jats:title><jats:p>We use more than 7 years of Time History of Events and Macroscale Interactions during Substorms observations to quantify the non‐Gaussian properties associated with mirror mode turbulence in the Earth's magnetosheath. We find that non‐Gaussian statistics of mirror modes lead to the parabolic collapse of kurtosis as the square of the skewness (<jats:italic>K</jats:italic> = <jats:italic>a</jats:italic><jats:italic>S</jats:italic><jats:sup>2</jats:sup>+<jats:italic>B</jats:italic> with <jats:italic>a</jats:italic> ∼ 1.3 and <jats:italic>b</jats:italic> ∼− 1). The parabolic scaling is a global constraint for the magnetosheath and is dictated by kinetic processes. This parabolic scaling is qualitatively independent of the distance to the magnetopause or bow shock, which implies that, even though the bow shock is driving the mirror mode instability, the dynamical evolution of mirror structures is independent of the source region and due to local processes. The parabolic relationship and coefficients between kurtosis and skewness for mirror modes in the Earth's magnetosheath are also similar to those found in a wide range of geophysical and laboratory turbulent environments, providing further evidence that turbulent systems dominated by non‐Gaussian fluctuations hold universal statistical properties.</jats:p> |
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| author | Osmane, A., Dimmock, A. P., Pulkkinen, T. I. |
| author_facet | Osmane, A., Dimmock, A. P., Pulkkinen, T. I., Osmane, A., Dimmock, A. P., Pulkkinen, T. I. |
| author_sort | osmane, a. |
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| container_title | Geophysical Research Letters |
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| description | <jats:title>Abstract</jats:title><jats:p>We use more than 7 years of Time History of Events and Macroscale Interactions during Substorms observations to quantify the non‐Gaussian properties associated with mirror mode turbulence in the Earth's magnetosheath. We find that non‐Gaussian statistics of mirror modes lead to the parabolic collapse of kurtosis as the square of the skewness (<jats:italic>K</jats:italic> = <jats:italic>a</jats:italic><jats:italic>S</jats:italic><jats:sup>2</jats:sup>+<jats:italic>B</jats:italic> with <jats:italic>a</jats:italic> ∼ 1.3 and <jats:italic>b</jats:italic> ∼− 1). The parabolic scaling is a global constraint for the magnetosheath and is dictated by kinetic processes. This parabolic scaling is qualitatively independent of the distance to the magnetopause or bow shock, which implies that, even though the bow shock is driving the mirror mode instability, the dynamical evolution of mirror structures is independent of the source region and due to local processes. The parabolic relationship and coefficients between kurtosis and skewness for mirror modes in the Earth's magnetosheath are also similar to those found in a wide range of geophysical and laboratory turbulent environments, providing further evidence that turbulent systems dominated by non‐Gaussian fluctuations hold universal statistical properties.</jats:p> |
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| imprint | American Geophysical Union (AGU), 2015 |
| imprint_str_mv | American Geophysical Union (AGU), 2015 |
| institution | DE-D275, DE-Bn3, DE-Brt1, DE-D161, DE-Zwi2, DE-Gla1, DE-Zi4, DE-15, DE-Pl11, DE-Rs1, DE-105, DE-14, DE-Ch1, DE-L229 |
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| physical | 3085-3092 |
| publishDate | 2015 |
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| publisher | American Geophysical Union (AGU) |
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| series | Geophysical Research Letters |
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| spelling | Osmane, A. Dimmock, A. P. Pulkkinen, T. I. 0094-8276 1944-8007 American Geophysical Union (AGU) General Earth and Planetary Sciences Geophysics http://dx.doi.org/10.1002/2015gl063771 <jats:title>Abstract</jats:title><jats:p>We use more than 7 years of Time History of Events and Macroscale Interactions during Substorms observations to quantify the non‐Gaussian properties associated with mirror mode turbulence in the Earth's magnetosheath. We find that non‐Gaussian statistics of mirror modes lead to the parabolic collapse of kurtosis as the square of the skewness (<jats:italic>K</jats:italic> = <jats:italic>a</jats:italic><jats:italic>S</jats:italic><jats:sup>2</jats:sup>+<jats:italic>B</jats:italic> with <jats:italic>a</jats:italic> ∼ 1.3 and <jats:italic>b</jats:italic> ∼− 1). The parabolic scaling is a global constraint for the magnetosheath and is dictated by kinetic processes. This parabolic scaling is qualitatively independent of the distance to the magnetopause or bow shock, which implies that, even though the bow shock is driving the mirror mode instability, the dynamical evolution of mirror structures is independent of the source region and due to local processes. The parabolic relationship and coefficients between kurtosis and skewness for mirror modes in the Earth's magnetosheath are also similar to those found in a wide range of geophysical and laboratory turbulent environments, providing further evidence that turbulent systems dominated by non‐Gaussian fluctuations hold universal statistical properties.</jats:p> Universal properties of mirror mode turbulence in the Earth's magnetosheath Geophysical Research Letters |
| spellingShingle | Osmane, A., Dimmock, A. P., Pulkkinen, T. I., Geophysical Research Letters, Universal properties of mirror mode turbulence in the Earth's magnetosheath, General Earth and Planetary Sciences, Geophysics |
| title | Universal properties of mirror mode turbulence in the Earth's magnetosheath |
| title_full | Universal properties of mirror mode turbulence in the Earth's magnetosheath |
| title_fullStr | Universal properties of mirror mode turbulence in the Earth's magnetosheath |
| title_full_unstemmed | Universal properties of mirror mode turbulence in the Earth's magnetosheath |
| title_short | Universal properties of mirror mode turbulence in the Earth's magnetosheath |
| title_sort | universal properties of mirror mode turbulence in the earth's magnetosheath |
| title_unstemmed | Universal properties of mirror mode turbulence in the Earth's magnetosheath |
| topic | General Earth and Planetary Sciences, Geophysics |
| url | http://dx.doi.org/10.1002/2015gl063771 |