21![Heliophysics 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](https://www.pdfsearch.io/img/e2cceb0737b30f34715ccb52efda4afb.jpg) | Add to Reading ListSource URL: www.heliophysics.ucar.eduLanguage: English - Date: 2013-07-16 13:12:20
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22![Heliophysics 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](https://www.pdfsearch.io/img/13ce81087d03b9623d580bf1fd255f94.jpg) | Add to Reading ListSource URL: www.vsp.ucar.eduLanguage: English - Date: 2013-07-16 13:12:20
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23![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 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](https://www.pdfsearch.io/img/9ec2d600adab6583e1c4a05651751a5d.jpg) | Add to Reading ListSource URL: www.heliophysics.ucar.eduLanguage: English - Date: 2012-06-04 12:37:41
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24![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 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](https://www.pdfsearch.io/img/b2bcc078a90eef279880733c79dedbf3.jpg) | Add to Reading ListSource URL: www.heliophysics.ucar.eduLanguage: English - Date: 2012-06-04 12:42:45
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25![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 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](https://www.pdfsearch.io/img/660fed6a71f6b86bff4ba9543f0eef16.jpg) | Add to Reading ListSource URL: www.aeronomy.beLanguage: English - Date: 2011-04-18 04:38:40
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26![Annales 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](https://www.pdfsearch.io/img/725300f7a7917048e014ecdd029da4c2.jpg) | Add to Reading ListSource URL: www.ann-geophys.netLanguage: English - Date: 2014-12-04 13:03:58
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27![Lab 3- Different Magnetosphere Lab 3- Different Magnetosphere](https://www.pdfsearch.io/img/bd7afc4c3829214cb01a975e42a9e40f.jpg) | Add to Reading ListSource URL: www.heliophysics.ucar.eduLanguage: English - Date: 2013-07-16 12:10:20
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28![Lab 3- Different Magnetosphere Lab 3- Different Magnetosphere](https://www.pdfsearch.io/img/3c01a9a732af613966d10b6f0150510c.jpg) | Add to Reading ListSource URL: www.vsp.ucar.eduLanguage: English - Date: 2013-07-16 12:10:20
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29![Ann. 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](https://www.pdfsearch.io/img/255c6a68d6f0d8b270f0dce999b7b9c2.jpg) | Add to Reading ListSource URL: www.ann-geophys.netLanguage: English - Date: 2014-12-04 16:49:28
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30![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 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](https://www.pdfsearch.io/img/30de09539ab37e1d347b69a4d90a2182.jpg) | Add to Reading ListSource URL: www.vsp.ucar.eduLanguage: English - Date: 2012-06-04 12:37:41
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