標(biāo)題: Titlebook: Galactic and Intergalactic Magnetic Fields; Ulrich Klein,Andrew Fletcher Book 2015 Springer International Publishing Switzerland 2015 Astr [打印本頁(yè)] 作者: Abridge 時(shí)間: 2025-3-21 20:08
書(shū)目名稱(chēng)Galactic and Intergalactic Magnetic Fields影響因子(影響力)
書(shū)目名稱(chēng)Galactic and Intergalactic Magnetic Fields影響因子(影響力)學(xué)科排名
書(shū)目名稱(chēng)Galactic and Intergalactic Magnetic Fields網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱(chēng)Galactic and Intergalactic Magnetic Fields網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱(chēng)Galactic and Intergalactic Magnetic Fields被引頻次
書(shū)目名稱(chēng)Galactic and Intergalactic Magnetic Fields被引頻次學(xué)科排名
書(shū)目名稱(chēng)Galactic and Intergalactic Magnetic Fields年度引用
書(shū)目名稱(chēng)Galactic and Intergalactic Magnetic Fields年度引用學(xué)科排名
書(shū)目名稱(chēng)Galactic and Intergalactic Magnetic Fields讀者反饋
書(shū)目名稱(chēng)Galactic and Intergalactic Magnetic Fields讀者反饋學(xué)科排名
作者: 磨碎 時(shí)間: 2025-3-21 22:19
978-3-319-34671-7Springer International Publishing Switzerland 2015作者: Modicum 時(shí)間: 2025-3-22 01:44 作者: 饒舌的人 時(shí)間: 2025-3-22 07:07
Gerald C. Cupchik,R. Walter Heinrichsthat the nonthermal component with its power-law spectrum is synchrotron radiation (free-free emission preponderates in the Galatic plane and in HII regions), and that a magnetic field must be ubiquitously present in the Milky Way.作者: 閑蕩 時(shí)間: 2025-3-22 10:13
Erwan Josse,Pascal Bach,Laurent Dagornential made up by stars and dark matter. In spiral galaxies, the gas has a neutral and an ionised phase. The neutral phase is made up by (in order of decreasing density) the molecular medium, the cold neutral medium (CNM), and the warm neutral medium (WNM). The ionised phase consists of the warm (WIM) and the hot (HIM) ionised medium (Table 5.1).作者: STELL 時(shí)間: 2025-3-22 15:08
The Evidence Regarding ACL Repair,c field. As pointed out in Sect.?5.5, their synchrotron luminosity is closely associated with the star formation in their disks, this giving rise to the well-known radio-FIR correlation established for star-forming galaxies.作者: STELL 時(shí)間: 2025-3-22 19:51 作者: 遺留之物 時(shí)間: 2025-3-23 00:37 作者: 夸張 時(shí)間: 2025-3-23 02:32
Magnetic Fields in Galaxies,ential made up by stars and dark matter. In spiral galaxies, the gas has a neutral and an ionised phase. The neutral phase is made up by (in order of decreasing density) the molecular medium, the cold neutral medium (CNM), and the warm neutral medium (WNM). The ionised phase consists of the warm (WIM) and the hot (HIM) ionised medium (Table 5.1).作者: 時(shí)間等 時(shí)間: 2025-3-23 08:40 作者: 臭名昭著 時(shí)間: 2025-3-23 09:58 作者: 溫和女孩 時(shí)間: 2025-3-23 15:22
Sander Happaerts,Hans Bruyninckxstic electrons moving in a magnetic field for which there is other independent evidence (Sect.?.), this radiation turns out to be the main diagnostic tool to trace magnetic fields in interstellar and intergalactic space, by virtue of its radiation spectrum and polarisation characteristics.作者: RADE 時(shí)間: 2025-3-23 21:18 作者: flaggy 時(shí)間: 2025-3-23 22:58
Erwan Josse,Pascal Bach,Laurent Dagornential made up by stars and dark matter. In spiral galaxies, the gas has a neutral and an ionised phase. The neutral phase is made up by (in order of decreasing density) the molecular medium, the cold neutral medium (CNM), and the warm neutral medium (WNM). The ionised phase consists of the warm (WI作者: decipher 時(shí)間: 2025-3-24 04:49
C. Bardos,F. Golse,D. Levermoreer a solid understanding of the basic ideas of galactic dynamo theory, which will allow them to engage with current research in this active field. To begin, we use qualitative arguments to derive a very simple mathematical model for a dynamo that includes some of the key elements of dynamo theory. T作者: irreducible 時(shí)間: 2025-3-24 09:23 作者: collagenase 時(shí)間: 2025-3-24 14:42
Knowledge Database and Inversionich are dwarf galaxies. For example, the Virgo Cluster contains some 250 large galaxies and more than 2000 smaller ones. Small assemblies of galaxies are referred to as groups. For instance, the local group comprises two really massive galaxies, the Milky Way and M?31, and a third one, M?33, being s作者: DUST 時(shí)間: 2025-3-24 15:29 作者: 藥物 時(shí)間: 2025-3-24 19:02
J. Tiago Gon?alves,Ricardo MostanyIn this chapter, we shall treat the main diagnostic tools that we have at hand to investigate interstellar and intergalactic magnetic fields.作者: TRUST 時(shí)間: 2025-3-25 02:34 作者: 共同生活 時(shí)間: 2025-3-25 06:02 作者: Palpitation 時(shí)間: 2025-3-25 08:45 作者: Bone-Scan 時(shí)間: 2025-3-25 12:28 作者: 含鐵 時(shí)間: 2025-3-25 17:04
C. Bardos,F. Golse,D. Levermore and clearly identifying assumptions that are made, we hope that even readers who are not enthusiastic about mathematics can gain an intuative feeling for the theory. The main properties of the derived dynamo equations are illustrated by directly solving some simple cases. In addition we provide sho作者: ALT 時(shí)間: 2025-3-25 23:13 作者: animated 時(shí)間: 2025-3-26 00:56 作者: 詞根詞綴法 時(shí)間: 2025-3-26 05:40 作者: IVORY 時(shí)間: 2025-3-26 11:14
Magnetic Fields in Galaxies,ential made up by stars and dark matter. In spiral galaxies, the gas has a neutral and an ionised phase. The neutral phase is made up by (in order of decreasing density) the molecular medium, the cold neutral medium (CNM), and the warm neutral medium (WNM). The ionised phase consists of the warm (WI作者: gangrene 時(shí)間: 2025-3-26 15:27
Galactic Dynamos,er a solid understanding of the basic ideas of galactic dynamo theory, which will allow them to engage with current research in this active field. To begin, we use qualitative arguments to derive a very simple mathematical model for a dynamo that includes some of the key elements of dynamo theory. T作者: Acumen 時(shí)間: 2025-3-26 18:44
Active Galactic Nuclei,c field. As pointed out in Sect.?5.5, their synchrotron luminosity is closely associated with the star formation in their disks, this giving rise to the well-known radio-FIR correlation established for star-forming galaxies.作者: 全面 時(shí)間: 2025-3-26 21:34
Intergalactic Magnetic Fields,ich are dwarf galaxies. For example, the Virgo Cluster contains some 250 large galaxies and more than 2000 smaller ones. Small assemblies of galaxies are referred to as groups. For instance, the local group comprises two really massive galaxies, the Milky Way and M?31, and a third one, M?33, being s作者: ligature 時(shí)間: 2025-3-27 02:41 作者: Hemoptysis 時(shí)間: 2025-3-27 08:49 作者: MUMP 時(shí)間: 2025-3-27 10:47 作者: ARK 時(shí)間: 2025-3-27 16:37
Introduction,art from iron, magnetism was exhibited in a natural state by cobalt and manganese, and by many of their compounds. The phenomenon was coined “magnetism” (derived from city of Magnesia in Asia Minor, where they say the phenomenon was first recognised).作者: Intend 時(shí)間: 2025-3-27 21:42 作者: 不知疲倦 時(shí)間: 2025-3-28 01:31
y.Discusses the role of magnetic fields in the evolution of This course-tested textbook conveys the fundamentals of magnetic fields and relativistic plasma in diffuse cosmic media, with a primary focus on phenomena that have been observed at different wavelengths. Theoretical concepts are addressed 作者: 無(wú)效 時(shí)間: 2025-3-28 03:18 作者: GLADE 時(shí)間: 2025-3-28 06:33 作者: cravat 時(shí)間: 2025-3-28 13:21
Cosmological Magnetic Fields,ld up the magnetic field. Even worse: strong magnetic fields are already present at large redshifts. Cosmological magnetic fields have been discussed to some extent in the excellent review by Widrow?(2002). One mechanism that has been briefly addressed in the previous chapter is the Biermann battery Biermann?(1950).作者: lobster 時(shí)間: 2025-3-28 14:55 作者: 獨(dú)裁政府 時(shí)間: 2025-3-28 21:49
Measuring Depression in Children and Young Peoplea psychological functioning standpoint. This chapter aims to provide a context to understanding the potential difficulties, how to measure areas of risk including depression and anxiety, and how to use that information in clinical practice. Recommendations are provided in order to screen for psychol作者: 使迷醉 時(shí)間: 2025-3-28 23:37
