Magnetosheath

Results: 75



#Item
21Heliophysics Summer School 2013!  Boulder, CO Lab 4: Magnetosphere 2: A Magnetosphere in Different Places

Heliophysics Summer School 2013! Boulder, CO Lab 4: Magnetosphere 2: A Magnetosphere in Different Places

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Source URL: www.heliophysics.ucar.edu

Language: English - Date: 2013-07-16 13:12:20
22Heliophysics Summer School 2013!  Boulder, CO Lab 4: Magnetosphere 2: A Magnetosphere in Different Places

Heliophysics Summer School 2013! Boulder, CO Lab 4: Magnetosphere 2: A Magnetosphere in Different Places

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Source URL: www.vsp.ucar.edu

Language: English - Date: 2013-07-16 13:12:20
23Shocks: Homework 1. Solar wind with Mach number Msw ≫ 1 hits the Earth’s magnetosphere. Assume the magnetic field in the wind is small enough to be neglected. A simplified of the day-side magnetosphere. Flow streamli

Shocks: Homework 1. Solar wind with Mach number Msw ≫ 1 hits the Earth’s magnetosphere. Assume the magnetic field in the wind is small enough to be neglected. A simplified of the day-side magnetosphere. Flow streamli

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Source URL: www.heliophysics.ucar.edu

Language: English - Date: 2012-06-04 12:37:41
241. The magnetic moment of Earth is approximately 31,000 nT- RE3 . The solar wind has a bulk velocity of 400 km/sec and a density of 5 cm-3 at 1 AU. Assume a very simple model of Earth’s magnetopause in which it is a pl

1. The magnetic moment of Earth is approximately 31,000 nT- RE3 . The solar wind has a bulk velocity of 400 km/sec and a density of 5 cm-3 at 1 AU. Assume a very simple model of Earth’s magnetopause in which it is a pl

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Source URL: www.heliophysics.ucar.edu

Language: English - Date: 2012-06-04 12:42:45
25Structure of the Magnetosphere By J. De Keyser The complex structure of the magnetosphere is the result of the interplay between the charged particles originating in the upper layers of the terrestrial atmosphere, whose

Structure of the Magnetosphere By J. De Keyser The complex structure of the magnetosphere is the result of the interplay between the charged particles originating in the upper layers of the terrestrial atmosphere, whose

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Source URL: www.aeronomy.be

Language: English - Date: 2011-04-18 04:38:40
26Annales Geophysicae: 3009–3019 SRef-ID: ag © European Geosciences Union 2004 Annales Geophysicae

Annales Geophysicae: 3009–3019 SRef-ID: ag © European Geosciences Union 2004 Annales Geophysicae

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Source URL: www.ann-geophys.net

Language: English - Date: 2014-12-04 13:03:58
27Lab 3- Different Magnetosphere

Lab 3- Different Magnetosphere

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Source URL: www.heliophysics.ucar.edu

Language: English - Date: 2013-07-16 12:10:20
28Lab 3- Different Magnetosphere

Lab 3- Different Magnetosphere

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Source URL: www.vsp.ucar.edu

Language: English - Date: 2013-07-16 12:10:20
29Ann. Geophys., 29, 1849–1860, 2011 www.ann-geophys.netdoi:angeo © Author(sCC Attribution 3.0 License.  Annales

Ann. Geophys., 29, 1849–1860, 2011 www.ann-geophys.netdoi:angeo © Author(sCC Attribution 3.0 License. Annales

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Source URL: www.ann-geophys.net

Language: English - Date: 2014-12-04 16:49:28
30Shocks: Homework 1. Solar wind with Mach number Msw ≫ 1 hits the Earth’s magnetosphere. Assume the magnetic field in the wind is small enough to be neglected. A simplified of the day-side magnetosphere. Flow streamli

Shocks: Homework 1. Solar wind with Mach number Msw ≫ 1 hits the Earth’s magnetosphere. Assume the magnetic field in the wind is small enough to be neglected. A simplified of the day-side magnetosphere. Flow streamli

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Source URL: www.vsp.ucar.edu

Language: English - Date: 2012-06-04 12:37:41