Magnetosphere

Results: 1139



#Item
571Plasma physics / Planetary science / Jets / Light sources / Magnetosphere / Plasma / Aurora / Ionosphere / Solar wind / Physics / Space plasmas / Astronomy

3-5 Development of Instrument for the Resonance Scattering Emission of Oxygen Ion (OⅡ:83.4nm) ― Toward the Imagery of Magnetosphere ― YAMAZAKI Atsushi, MIYAKE Wataru, YOSHIKAWA Ichiro, NAKAMURA Masato, and TAKIZAWA

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Source URL: www.nict.go.jp

Language: English - Date: 2013-11-20 21:30:04
572Planetary science / Astrophysics / Plasma physics / Geomagnetism / Jets / Magnetosphere / Magnetopause / Magnetosheath / Solar wind / Physics / Space plasmas / Astronomy

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.aeronomie.be

Language: English - Date: 2011-04-18 04:38:40
573Astroparticle physics / Particle physics / Cosmic rays / Van Allen radiation belt / Electron / Magnetosphere / Radiation / Ionizing radiation / Particle accelerator / Physics / Space plasmas / Geomagnetism

Energetic particles of the magnetosphere By M. Kruglanski The energetic particles in the magnetosphere have various origins: • cosmic rays emitted in our galaxy by novae and supernovae; • galactic particles accelerat

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Source URL: www.bira-iasb.be

Language: English - Date: 2011-04-18 04:12:33
574Astrophysics / Plasma physics / Sun / Light sources / Jets / Coronal mass ejection / Corona / Solar wind / Magnetosphere / Space plasmas / Physics / Astronomy

Coronal mass ejections and magnetized clouds By J. De Keyser It is known that large structures can exist within the corona, that may catapult plasma into space with a speed of 1000 km/s. Such an event is called a coronal

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Source URL: www.bira-iasb.be

Language: English - Date: 2011-04-18 04:10:25
575Astronomy / Plasma physics / Planetary science / Geomagnetism / Jets / Magnetosphere / Aurora / Birkeland current / Solar wind / Physics / Space plasmas / Astrophysics

Coupling with the ionosphere By J. De Keyser While the motion of the outer regions of the magnetosphere is prescribed by the solar-wind magnetosphere interaction, the motion of the inner regions of the magnetosphere is d

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Source URL: www.aeronomie.be

Language: English - Date: 2011-04-18 04:38:40
576Physics / Planetary science / Plasma physics / Jets / Space science / Space weather / Ionosphere / Magnetosphere / Coronal mass ejection / Space plasmas / Space / Meteorology

1 Research on a System for Monitoring, Analyzing, and Forecasting of the Space Environment KIKUCHI Takashi In the 21st century, an age of widespread space-based endeavors, satellite communication, broadcast, and position

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Source URL: www.nict.go.jp

Language: English - Date: 2013-11-20 21:26:34
577Astrophysics / Planetary science / Plasma physics / Geomagnetism / Space science / Magnetosphere / Birkeland current / Aurora / Geomagnetic storm / Physics / Space plasmas / Astronomy

Ionospheric Plasma Convection Observed by HF Radar Network in the Northern Polar Region HASHIMOTO K. Kumiko, KIKUCHI Takashi, KUNITAKE Manabu, OHTAKA Kazuhiro, and WATARI Shin-ichi The space weather forecast is getting m

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Source URL: www.nict.go.jp

Language: English - Date: 2013-11-21 20:04:49
578Geomagnetism / Planetary science / Space plasmas / Plasma physics / Jets / Substorm / THEMIS / Aurora / Magnetosphere / Electromagnetism / Physics / Magnetism

Major magnetic storm events also lead to spectacular auroral displays even at low geographic latitudes. Substorms were first documented in 1964 by Syun-Ichi Akasofu of the University of Alaska using a network of all-sky

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Source URL: cse.ssl.berkeley.edu

Language: English - Date: 2010-01-11 17:34:45
579Space plasmas / Planetary science / Plasma physics / Geomagnetism / Light sources / Magnetosphere / Aurora / Substorm / Sunspot / Physics / Electromagnetism / Astronomy

Exercise 3. Find the magnetic latitudes for field lines that cross the equatorial plane at L = 3.0, L=10.0, L=20.0 and L = 30.0. If magnetic storms are produced by magnetic reconnection events between L=15 and L = 35, at

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Source URL: cse.ssl.berkeley.edu

Language: English - Date: 2010-01-11 17:34:22
580Electromagnetism / Plasma physics / Planetary science / Geomagnetism / Atmosphere / Ionosphere / Magnetosphere / Space weather / Geomagnetic storm / Physics / Space plasmas / Astrophysics

2-3-6 Ionosphere Simulation SHINAGAWA Hiroyuki Space weather forecasts are about to enter a stage incorporating numerical forecasts based on full-scale numerical simulation, in addition to conventional methods used by fo

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Source URL: www.nict.go.jp

Language: English - Date: 2011-07-11 07:57:43
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