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Fine Structure of Solar Radio Bursts
The study of the fine structure of solar radio emissions is key to understanding plasma processes in the solar corona. It remains a reliable means for both diagnosing the corona and verifying the results of laboratory plasma experiments on wave-wave and wave-particle interactions. This monograph pro...
| Clasificación: | Libro Electrónico |
|---|---|
| Autor principal: | |
| Autor Corporativo: | |
| Formato: | Electrónico eBook |
| Idioma: | Inglés |
| Publicado: |
Berlin, Heidelberg :
Springer Berlin Heidelberg : Imprint: Springer,
2011.
|
| Edición: | 1st ed. 2011. |
| Colección: | Astrophysics and Space Science Library,
375 |
| Temas: | |
| Acceso en línea: | Texto Completo |
MARC
| LEADER | 00000nam a22000005i 4500 | ||
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| 001 | 978-3-642-20015-1 | ||
| 003 | DE-He213 | ||
| 005 | 20220117130757.0 | ||
| 007 | cr nn 008mamaa | ||
| 008 | 110628s2011 gw | s |||| 0|eng d | ||
| 020 | |a 9783642200151 |9 978-3-642-20015-1 | ||
| 024 | 7 | |a 10.1007/978-3-642-20015-1 |2 doi | |
| 050 | 4 | |a QB500.5-785 | |
| 072 | 7 | |a PHV |2 bicssc | |
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| 082 | 0 | 4 | |a 523.2 |2 23 |
| 100 | 1 | |a Chernov, Gennady P. |e author. |4 aut |4 http://id.loc.gov/vocabulary/relators/aut | |
| 245 | 1 | 0 | |a Fine Structure of Solar Radio Bursts |h [electronic resource] / |c by Gennady P. Chernov. |
| 250 | |a 1st ed. 2011. | ||
| 264 | 1 | |a Berlin, Heidelberg : |b Springer Berlin Heidelberg : |b Imprint: Springer, |c 2011. | |
| 300 | |a XVI, 284 p. |b online resource. | ||
| 336 | |a text |b txt |2 rdacontent | ||
| 337 | |a computer |b c |2 rdamedia | ||
| 338 | |a online resource |b cr |2 rdacarrier | ||
| 347 | |a text file |b PDF |2 rda | ||
| 490 | 1 | |a Astrophysics and Space Science Library, |x 2214-7985 ; |v 375 | |
| 505 | 0 | |a Preface -- Acknowledgments -- 1 Introduction -- 2 Pulsations -- 3 Spike bursts -- 4 Zebra pattern and fiber bursts -- 5 Recent results of zebra patterns in solar radio bursts -- References -- Subject Index. | |
| 520 | |a The study of the fine structure of solar radio emissions is key to understanding plasma processes in the solar corona. It remains a reliable means for both diagnosing the corona and verifying the results of laboratory plasma experiments on wave-wave and wave-particle interactions. This monograph provides a comprehensive review of the fine structure of solar radio bursts. Based on the diversity of experimental data resulting from the progress made in observational techniques, the validity of various theoretical models is reexamined. The book serves as an up-to-date reference work for all researchers in this field. | ||
| 650 | 0 | |a Solar system. | |
| 650 | 0 | |a Astronomy-Observations. | |
| 650 | 0 | |a Astrophysics. | |
| 650 | 0 | |a Plasma (Ionized gases). | |
| 650 | 1 | 4 | |a Space Physics. |
| 650 | 2 | 4 | |a Astronomy, Observations and Techniques. |
| 650 | 2 | 4 | |a Astrophysics. |
| 650 | 2 | 4 | |a Plasma Physics. |
| 710 | 2 | |a SpringerLink (Online service) | |
| 773 | 0 | |t Springer Nature eBook | |
| 776 | 0 | 8 | |i Printed edition: |z 9783642200144 |
| 776 | 0 | 8 | |i Printed edition: |z 9783642269035 |
| 776 | 0 | 8 | |i Printed edition: |z 9783642200168 |
| 830 | 0 | |a Astrophysics and Space Science Library, |x 2214-7985 ; |v 375 | |
| 856 | 4 | 0 | |u https://doi.uam.elogim.com/10.1007/978-3-642-20015-1 |z Texto Completo |
| 912 | |a ZDB-2-PHA | ||
| 912 | |a ZDB-2-SXP | ||
| 950 | |a Physics and Astronomy (SpringerNature-11651) | ||
| 950 | |a Physics and Astronomy (R0) (SpringerNature-43715) | ||