派博傳思國際中心

標(biāo)題: Titlebook: Illustrated Glossary for Solar and Solar-Terrestrial Physics; A. Bruzek,C. J. Durrant Book 1977 D. Reidel Publishing Company, Dordrecht, H [打印本頁]

作者: Precise    時間: 2025-3-21 18:04
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書目名稱Illustrated Glossary for Solar and Solar-Terrestrial Physics讀者反饋




書目名稱Illustrated Glossary for Solar and Solar-Terrestrial Physics讀者反饋學(xué)科排名





作者: 激勵    時間: 2025-3-21 22:59
Solar Cycle, Solar Rotation and Large-Scale Circulation,features or indices that show such variations are: Wolf Number (.), plages, prominences, 2800 MHz radio emission and flares. The period of this cyclic variation is approximately 11 yr (.), although in this century the average period has been closer to 10 yr.
作者: 形狀    時間: 2025-3-22 03:45
Non-Spot Magnetic Fields,uch a field. Today, the term general magnetic field is often used interchangeably with polar field. The problem of determining the existence of a true general magnetic field is that of eliminating the effect of transient magnetic fields which collect near the poles. See polar field and large scale m
作者: aristocracy    時間: 2025-3-22 05:55
Quiet Photosphere and Chromosphere,ontinuously changing, waves and oscillations occur and large-scale patterns (supergranulation, chromospheric network) evolve. The characteristics of the quiet Sun are that the overall pattern of its fine structures is statistically uniform and/or stationary, that there is no (conspicuous) enhancemen
作者: Arrhythmia    時間: 2025-3-22 09:26

作者: 熔巖    時間: 2025-3-22 16:26

作者: 者變    時間: 2025-3-22 17:23

作者: Obsessed    時間: 2025-3-23 00:21
Prominences,eir greater density than their coronal surroundings and by temperatures ranging from about 10. K to coronal values at the interface to the corona. They appear as bright (cool and dense) features (in the corona) above the solar limb; when seen projected against the solar disk nearly all prominences s
作者: 影響深遠(yuǎn)    時間: 2025-3-23 03:36

作者: BALE    時間: 2025-3-23 07:04
General Theoretical Terms,f refractive index. This anomalous dispersion is particularly important in the analysis of lines formed in the presence of a magnetic field. The differently split components of the line have different dispersions which leads to a rotation of the axes of the polarization ellipse as the radiation trav
作者: daredevil    時間: 2025-3-23 12:35
Solar Wind and Interplanetary Medium,uously expanding into interplanetary space. The resulting outflow of coronal plasma is known as the solar wind. Because of the very high electrical conductivity of the coronal plasma the magnetic field in the corona controls both the heat conduction and the basic outflow of material. In regions wher
作者: 高度    時間: 2025-3-23 14:00

作者: 悄悄移動    時間: 2025-3-23 18:42

作者: Pander    時間: 2025-3-23 22:12
Illustrated Glossary for Solar and Solar-Terrestrial Physics978-94-010-1245-4Series ISSN 0067-0057 Series E-ISSN 2214-7985
作者: faddish    時間: 2025-3-24 05:02
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/i/image/461231.jpg
作者: confide    時間: 2025-3-24 09:43

作者: 首創(chuàng)精神    時間: 2025-3-24 12:56

作者: ACME    時間: 2025-3-24 16:32
Solar-Terrestrial Physics,Magnetic observatories monitor continuously the geomagnetic field at various latitudes and longitudes of the Earth. With the advent of rockets and satellites, it has been studied also in space.
作者: creditor    時間: 2025-3-24 23:04

作者: 膽大    時間: 2025-3-24 23:22

作者: 豪華    時間: 2025-3-25 03:34
Non-Spot Magnetic Fields,uch a field. Today, the term general magnetic field is often used interchangeably with polar field. The problem of determining the existence of a true general magnetic field is that of eliminating the effect of transient magnetic fields which collect near the poles. See polar field and large scale magnetic field.
作者: Ceramic    時間: 2025-3-25 07:40
Prominences,eir greater density than their coronal surroundings and by temperatures ranging from about 10. K to coronal values at the interface to the corona. They appear as bright (cool and dense) features (in the corona) above the solar limb; when seen projected against the solar disk nearly all prominences show up in absorption as ..
作者: 含沙射影    時間: 2025-3-25 13:44

作者: 溫順    時間: 2025-3-25 17:58
General Theoretical Terms,f refractive index. This anomalous dispersion is particularly important in the analysis of lines formed in the presence of a magnetic field. The differently split components of the line have different dispersions which leads to a rotation of the axes of the polarization ellipse as the radiation traverses the medium.
作者: 低能兒    時間: 2025-3-25 21:04
0067-0057 Organising Committee to establish a small group to recommend a standard nomenclature for solar features and to prepare an illustrated text which would clear the jungle of terms for the benefit of solar physicists as well as of theoreticians and research workers in related fields. The challenge was t
作者: 柳樹;枯黃    時間: 2025-3-26 00:57

作者: osteoclasts    時間: 2025-3-26 07:40
Quiet Photosphere and Chromosphere,he quiet Sun are that the overall pattern of its fine structures is statistically uniform and/or stationary, that there is no (conspicuous) enhancement or reduction of radiation and that there is no extended magnetic flux concentration (see Figure 3.3). Only at very low resolution (?l0″) does the quiet Sun really appear quiet.
作者: expeditious    時間: 2025-3-26 10:51
Active Regions,ce of a certain (transient) phenomenon (e.g. flare activity, surge activity, X-ray activity) or the occurrence of ‘a(chǎn)ctive regions’ (‘solar activity’ in general). Radio activity, for example, can imply both the occurrence of radio bursts and the longer-lasting enhancement of radio emission.
作者: 修正案    時間: 2025-3-26 15:39
Spots and Faculae, the weak photospheric network. The faculae are cospatial with bright plages observed in chromospheric lines (H Balmer lines, Ca II lines, He II 304 ?) and transition region lines, and with regions of enhanced magnetic fields.
作者: 平    時間: 2025-3-26 19:55
Flares and Associated Phenomena,article or high energy flare). The temperatures attained in the chromosphere are ≈ 10. K (chromospheric or low temperature flare), in the corona ≈ 10. K (high temperature flare). The energies of observed particles range from 20 keV up to ≈ 1 GeV. The total energy released in the largest events is ≈ 10. erg.
作者: 車床    時間: 2025-3-26 23:18
Solar Wind and Interplanetary Medium,nductivity of the coronal plasma the magnetic field in the corona controls both the heat conduction and the basic outflow of material. In regions where the magnetic field lines reach high into the corona (e.g. over coronal holes) the coronal expansion is greatly enhanced.
作者: 意見一致    時間: 2025-3-27 03:12

作者: employor    時間: 2025-3-27 08:49
0067-0057 d be a step on the road to standardisation if these terms were not re-used for new phenomena. New observations and new theories will lead to reappraisals and re978-94-010-1247-8978-94-010-1245-4Series ISSN 0067-0057 Series E-ISSN 2214-7985
作者: 不來    時間: 2025-3-27 11:27

作者: Minutes    時間: 2025-3-27 14:37
DSC and SWAXS Studies on the Effects of Silk Nanocrystals on Crystallization of Poly(,-Lactic Acid)s such as slow crystallization rate and low crystallinity restrict its commercial uses. In order to overcome these limitations, organic nanofillers are incorporated into the PLLA matrix. Herein, we report the use of silk nanocrystal (SNC) as a solid-state nucleation agent, which has been prepared in
作者: 哄騙    時間: 2025-3-27 19:26
Die Feuerprobe auf Silber und Gold,wirkung geeigneter Reagenzien bei h?heren Temperaturen erzielt wird. Grunds?tzlich betrachtet sind die für die verschiedenen Metalle angewendeten Feuerproben eine im kleinsten Ma?stab durchgeführte Nachahmung der technischen Hüttenprozesse.
作者: backdrop    時間: 2025-3-28 00:38

作者: Malaise    時間: 2025-3-28 05:24
,Computational Approaches for Predicting Binding Partners, Interface Residues, and Binding Affinity of Protein–Protein Complexes,nsive experimental techniques suggest the need for computational methods to complement them. Several such state-of-the-art methods have been reported for analyzing diverse aspects such as predicting binding partners, interface residues, and binding affinity for protein–protein complexes with reliabl
作者: HILAR    時間: 2025-3-28 10:05

作者: 講個故事逗他    時間: 2025-3-28 14:23

作者: 搬運工    時間: 2025-3-28 16:58
https://doi.org/10.1007/1-4020-3508-Xn characteristics are examined both experimentally and numerically. In order to explore the possibilities for further finite element research on such vibration analysis, the sub-structural effects on the numerical model is considered in a limited manner.
作者: attenuate    時間: 2025-3-28 22:45
Competitiveness of Industrial Production in the Regional Contextr determines the presence of the process of regional convergence. Our analysis demonstrates that in the period from 1990 to 2015, Russian regions tend to diverge in terms of “industrial production volumes.” The results of the study can be used to develop strategic and program documents.
作者: abolish    時間: 2025-3-29 01:40
Studies in Fuzziness and Soft Computing surfaces area reduction and hence weight reduction, boundary layer ingestion (Friedrichs J, Budziszewski N, Energies 11, Modelling of a boundary layer ingesting propulsor, 2018) and more. In this paper it is the effect of the duct over the propeller efficiency which will be quantified. To do so, a
作者: AMITY    時間: 2025-3-29 06:20
Adam G?ska,Jerzy S?adek,Piotr G?skah respect to the real-world security it provides against particularly powerful adversaries..We approach the setting by formalizing a cryptographic primitive that addresses specifically the secure software updating problem. We define strong, rigorous security models that capture forward security (ste
作者: Erythropoietin    時間: 2025-3-29 10:36
Data Monitoring: Structure for Clinical Trials and Sequential Monitoring Procedures,rder to fulfil the investigators’ ethical responsibilities to participants in a trial provides a rationale for the monitoring committee to be composed of experts independent of the investigators and suggests some basic structure for the committee’s meetings. The nature of statistical assessment of a
作者: overbearing    時間: 2025-3-29 15:27
Das vegetative Nervensystem, auch der Kochsalzgehalt des Blutes und der Gewebss?fte in dem osmotischen Bereich einer physiologischen Kochsalzl?sung gehalten. Sinkt der Wassergehalt des Blutes und der Gewebe unter ein gewisses Ma?, so treten ?sophaguskontraktionen auf, welche das Durstgefühl zum Ausdruck bringen.
作者: browbeat    時間: 2025-3-29 16:54
Gilda Guimar?es,Izabella Oliveiraplores how media productions display issues related to albinism in the African continent. Related points of analysis regard the ways these two documentaries portray “traditional” healing practices and humanitarian activities carried out by international and national NGOs.
作者: 陪審團(tuán)    時間: 2025-3-29 23:35

作者: PLIC    時間: 2025-3-30 03:09





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