By Wing-huen Ip

"Advances in Geosciences" is the results of a concerted attempt in bringing the most recent effects and making plans actions on the topic of earth and house technological know-how in Asia and the foreign enviornment. the amount editors are all best scientists of their examine fields overlaying 5 sections: sturdy Earth (SE), sun Terrestrial (ST), Planetary technological know-how (PS), Hydrological technological know-how (HS), and Oceans and Atmospheres (OA). the most goal is to focus on the clinical matters necessary to the research of earthquakes, tsunamis, weather swap, drought, flood, typhoons, house weathers, and planetary exploration.

Show description

Read Online or Download Advanced in Geosciences, V2: Solar Terrestrial(St) (2006)(en)(368s) PDF

Similar scientific-popular books

Advanced in Geosciences, V2: Solar Terrestrial(St) (2006)(en)(368s)

"Advances in Geosciences" is the results of a concerted attempt in bringing the most recent effects and making plans actions relating to earth and area technological know-how in Asia and the overseas area. the amount editors are all top scientists of their learn fields overlaying 5 sections: stable Earth (SE), sunlight Terrestrial (ST), Planetary technological know-how (PS), Hydrological technology (HS), and Oceans and Atmospheres (OA).

30-second Theories: The 50 Most Thought-provoking Theories in Science

By way of massive technology, only a few issues are conclusively identified. From Quantum Mechanics to normal choice, what we've as an alternative are theories - principles clarify why issues ensue the best way they do. we do not recognize for definite those are right - not anyone ever observed the massive Bang - yet with them we will be able to paint attractive, breathtaking images of every little thing from human behaviour to what the long run may perhaps carry.

Extra resources for Advanced in Geosciences, V2: Solar Terrestrial(St) (2006)(en)(368s)

Example text

Vaquero, Solar Phys. 219 (2004) 379. J. M. Vaquero, R. M. Trigo and M. C. Gallego, Astron. Nachr. 326 (2005) 112. May 30, 2006 9:24 WSPC/SPI-B368 Advances in Geosciences Vol. edu In the following, I describe the status of theoretical research on solar coronal plumes. Emphasis is placed on the relevance of slow magnetosonic waves, considering results from 1D, 2D, and analytical magnetohydrodynamic models, in addition to results from empirical models and observations. Theoretical models, taking into account the combined effects of plume spreading, heat conduction, and radiative damping, have shown that the waves nonlinearly steepen as they propagate, resulting in the formation of shocks at relatively low coronal heights.

Roberts, Solar Phys. 69 (1981) 27. 19. T. J. Bogdan, C. S. Rosenthal, M. Carlsson, V. Hansteen, A. McMurry, E. J. Zita, M. Johnson, S. Petty-Powell, S. W. McIntosh, ˚ A. Nordlund, R. F. Stein and S. B. F. Dorch, Astron. Nachrichten 323 (2002) 196. May 30, 2006 9:24 WSPC/SPI-B368 Advances in Geosciences Vol. 2 ch02 Solar Coronal Plumes: Theoretical Concepts and Results 31 20. P. Ulmschneider and Z. E. Musielak, Astron. Astrophys. 338 (1998) 311. 21. U. Narain and P. Ulmschneider, Space Sci. Rev.

In that respect, I will consider results from 1D, 2D, and analytical magnetohydrodynamic models, noting that May 30, 2006 9:24 WSPC/SPI-B368 Advances in Geosciences Vol. 2 ch02 Solar Coronal Plumes: Theoretical Concepts and Results 23 some important features considered in 1D and analytical models have not yet been taken into account in the 2D models. I will also briefly describe studies to identify solar plume geometry, expressed through global and local spreading functions. 2. Solar Plume Geometry The calculation of solar plume models requires the determination of plume geometry, typically expressed by the area function A(r).

Download PDF sample

Rated 4.64 of 5 – based on 9 votes