派博傳思國際中心

標(biāo)題: Titlebook: Radio Continua During Solar Flares; Selected Contributio Arnold O. Benz Book 1986 Springer Science+Business Media Dordrecht 1986 Corona.Pla [打印本頁]

作者: 離開浮于空中 時(shí)間: 2025-3-21 18:41
書目名稱Radio Continua During Solar Flares影響因子(影響力)

書目名稱Radio Continua During Solar Flares影響因子(影響力)學(xué)科排名

書目名稱Radio Continua During Solar Flares網(wǎng)絡(luò)公開度

書目名稱Radio Continua During Solar Flares網(wǎng)絡(luò)公開度學(xué)科排名

書目名稱Radio Continua During Solar Flares被引頻次

書目名稱Radio Continua During Solar Flares被引頻次學(xué)科排名

書目名稱Radio Continua During Solar Flares年度引用

書目名稱Radio Continua During Solar Flares年度引用學(xué)科排名

書目名稱Radio Continua During Solar Flares讀者反饋

書目名稱Radio Continua During Solar Flares讀者反饋學(xué)科排名

作者: 微粒 時(shí)間: 2025-3-21 20:58

作者: 諷刺 時(shí)間: 2025-3-22 02:02
Book 1986n of energy release and particle acceleration in flares. In the circles of the European solar radio astronomers, loosely organized in CESRA, the idea of a workshop came up intended for active observers of the impulsive phase of flares in radio and associated emissions. The scientific organizing comm

作者: Sciatica 時(shí)間: 2025-3-22 06:10
Interplanetary Phenomena and Solar Radio Burstsrelations with radio emissions. The exceptions suggest that such correlations may be incidental. Therefore, it is concluded that attention should also be given to events with a positive absence of radio emission in order to make progress in understanding solar processes.

作者: fringe 時(shí)間: 2025-3-22 09:18

作者: 時(shí)代 時(shí)間: 2025-3-22 16:27
Magnetohydrodynamic Theories of Solar Flaresof the eruptive instability thought to initiate a large flare and of the reconnection process of energy release. Finally, the role of emerging flux and horizontally moving satellite sunspots is discussed briefly.

作者: lipoatrophy 時(shí)間: 2025-3-22 17:05

作者: AVOID 時(shí)間: 2025-3-22 22:34
The Polarization of Decimetric Pulsationseading spot hypothesis, the magneto-ionic mode of the emission was found to be extraordinary. The high circular polarization of the pulsations was interpreted to be determined by the emission mechanism itself, not by propagation effects or cut-offs (contrary to the metric type I noise storms). Implications for pulsation models are discussed.

作者: carbohydrate 時(shí)間: 2025-3-23 03:59

作者: jungle 時(shí)間: 2025-3-23 09:17

作者: Scintillations 時(shí)間: 2025-3-23 12:57

作者: EXPEL 時(shí)間: 2025-3-23 17:03
On Fast Pulsations in Flare Continuaed, simultaneously or in time succession. Pulsations occur both in classical type IV events and in short-lasting continuum events. The power spectrum shows no large variation during one or two hours. Some implications of fast pulsations for the generation mechanism are discussed.

作者: 滲入 時(shí)間: 2025-3-23 19:59
Exponential Decay and Exciter Profile of Fast Pulses in Type IV Eventsfficiently isolated from the adjacent pulsating activity, appear to have an exponential decay phase similar to that of fast type III bursts..A computational procedure, based on Fourier transform techniques, has been applied; it allows the computation, for every observed point in the time profile, of

作者: syring 時(shí)間: 2025-3-23 22:28
The Polarization of Decimetric Pulsationslarized, the other half showed a mild polarization of 15–55%. The polarization is constant in time and frequency for the strongly polarized group. All the mildly polarized bursts originate from near the limb; the lower degree of circular polarization is likely to be caused by depolarization due to p

作者: 發(fā)牢騷 時(shí)間: 2025-3-24 04:18

作者: Overthrow 時(shí)間: 2025-3-24 10:19

作者: FUSC 時(shí)間: 2025-3-24 13:30
Millisecond Radio Spikesre fascinated by their high brightness temperature of up to 10. K, their association with hard X-ray bursts, and a possibly very intimate relation to electron acceleration. This review is intended to bridge the gap that presently seems to separate theory and observations. The wide range of spike obs

作者: Abrade 時(shí)間: 2025-3-24 15:34

作者: 淘氣 時(shí)間: 2025-3-24 21:44

作者: Wernickes-area 時(shí)間: 2025-3-25 02:50
Hollow Beam Distribution of Energetic Electrons and Higher Harmonics of Electron Cyclotron Maserelectrons with a parameter ξ = ω./Ω. are presented in this paper. The results show that the second harmonic of ECM in .-mode dominates the instability if ξ < 1, and if 1.2 ? ξ ? 2 or 2.2 ? ξ ? 3 the third or fourth harmonic will dominate. The second and third harmonics of .-mode waves grow faster on

作者: annexation 時(shí)間: 2025-3-25 04:24
A Model of Ultra-Fast Fine Structures of Microwave Bursts electron cyclotron frequency and electron velocity as well as Landau damping and cyclotron damping) to excite the UFFS (Ultra-Fast Fine Structures) of microwave bursts and adopting a nonlinear density wave as a trigger mechanism to explain the millisecond time structure of the UFFS.

作者: 戰(zhàn)勝 時(shí)間: 2025-3-25 09:41

作者: irritation 時(shí)間: 2025-3-25 14:04
Radio Observations of the Solar Neutron Flare of 3 June, 1982re had an impulsive character. A strong shock wave (.. ≥ 2.9) was observed unusually soon after the impulsive phase of the flare. The radio spectrum of this event shows that the primary acceleration process probably occurred in the region with an electron density of .. = 4.4 × 10. m.. The pulsations

作者: 赦免 時(shí)間: 2025-3-25 17:56

作者: 諷刺 時(shí)間: 2025-3-25 21:12

作者: 慢慢啃 時(shí)間: 2025-3-26 01:07
The Relation Between Flare-Related Metric Continuum Bursts and Coronal Mass Ejectionsontinuum (FC II) or a Slow Drift Continuum (SDC). Comparing properties for the events it was found that the continuum radio bursts were preferentially associated with the broader, more rapidly moving CME transients.

作者: 品牌 時(shí)間: 2025-3-26 04:27

作者: 信任 時(shí)間: 2025-3-26 08:31
Millisecond Radio Spikeservations is summarized and brought into the perspective of recent models. It is concluded that spikes yield a considerable potential for the diagnostics of energetic particles, their origin, and history in astrophysical plasmas.

作者: Cervical-Spine 時(shí)間: 2025-3-26 15:18

作者: 彎腰 時(shí)間: 2025-3-26 17:47
Hollow Beam Distribution of Energetic Electrons and Higher Harmonics of Electron Cyclotron Maserly if 2 ? ξ ? 2.2 and 3 ? ξ ? 3.2, respectively, so it would not be a competition in most cases. It is suggested that the ECM emission at these harmonics in .-mode is a possible mechanism to produce solar spike emissions with high brightness temperature at shorter and longer decimetric wavelengths.

作者: Diverticulitis 時(shí)間: 2025-3-26 22:42

作者: 任意 時(shí)間: 2025-3-27 03:50
https://doi.org/10.1007/978-94-009-4710-8Corona; Planet; Population; Solar flare; Variation; solar

作者: heirloom 時(shí)間: 2025-3-27 07:17

作者: disparage 時(shí)間: 2025-3-27 13:01

作者: Customary 時(shí)間: 2025-3-27 14:09
Discussion on the Classification of Fine Structures in ContinuaA short discussion on classification and terminology connected with fine structures in solar continuum emission at radio frequencies was arranged on Monday, 27 May with C. Slottje acting as chairman.

作者: 碌碌之人 時(shí)間: 2025-3-27 20:15
Occurrence of Solar Decimetric Spike Bursts over a Period of 4 Years During the 21st CycleA total number of 460 DCIM events, single or groups, were observed during the period of October 1980 to December 1984 with the Weissenau spectrograph as dynamic film spectra. Several parameters describing these data were evaluated statistically and the main features were discussed in context with associated burst types.

作者: 填料 時(shí)間: 2025-3-27 23:08

作者: 聯(lián)合 時(shí)間: 2025-3-28 03:46

作者: 東西 時(shí)間: 2025-3-28 07:17
A Model of Ultra-Fast Fine Structures of Microwave Bursts electron cyclotron frequency and electron velocity as well as Landau damping and cyclotron damping) to excite the UFFS (Ultra-Fast Fine Structures) of microwave bursts and adopting a nonlinear density wave as a trigger mechanism to explain the millisecond time structure of the UFFS.

作者: amorphous 時(shí)間: 2025-3-28 11:23
Alberto Abrami,Mauro Messerotti,Paolo Zlobecfuture. It will appeal to both beginners and seasoned researchers in nonlinear science, numerous areas of physics (optics, quantum physics, biophysics), and applied mathematics (ODEs, PDEs, dynamical systems, machine learning) as well as engineering..978-3-030-44992-6Series ISSN 2195-9994 Series E-ISSN 2196-0003

作者: Flat-Feet 時(shí)間: 2025-3-28 18:36
H. W. Urbarzings together compelling papers from scholars in Brazil, Canada, England, and the United States to illustrate how this inventive potential has been harnessed around the world..978-3-319-82071-2978-3-319-40295-6

作者: Onerous 時(shí)間: 2025-3-28 22:18
Hong Wei Liings together compelling papers from scholars in Brazil, Canada, England, and the United States to illustrate how this inventive potential has been harnessed around the world..978-3-319-82071-2978-3-319-40295-6

作者: 控訴 時(shí)間: 2025-3-29 00:39

作者: 大罵 時(shí)間: 2025-3-29 03:53
Book 1986 next cycle. This volume contains the reviews and a selection of contributions and extended abstracts of papers presented at the workshop. I wish to thank the local organizers, in particular A. Abrami, M. Comari, F. Depolli, L. Fornasari, M. Messerotti (chairman), M. Nonino, and P. Zlobec. Financial

作者: A保存的 時(shí)間: 2025-3-29 08:57

作者: 起波瀾 時(shí)間: 2025-3-29 13:56

作者: OTHER 時(shí)間: 2025-3-29 17:23
M. J. Aschwandenrelatively influential attributes from the MLR based on the absolute values of the coefficients, to find the classification function/expression for predicting the breast cancer using the training data set. As a part of this process, LP model also finds the initial thresholds where . and .?+?1 are th

作者: largesse 時(shí)間: 2025-3-29 23:34

作者: 武器 時(shí)間: 2025-3-30 02:47

作者: 檔案 時(shí)間: 2025-3-30 07:52
A. O. Benzementing renewable energy, risk prevention systems to cover possible environmental accidents, and preventing oil and methane leaks are the top three green practices. The finding helps practitioners and policymakers of the petroleum companies to implement effective green practices to sustain the envi

作者: 陪審團(tuán)每個(gè)人 時(shí)間: 2025-3-30 12:02
M. Nonino,M. Comari,P. Zlobec,A. Abrami,M. Messerottie models present in the literature that require manual parameterization for updating and implementing them. MATLAB is used for the computational implementation of ANN models. From the results of Pearson correlation coefficient, the correlation obtained among the targeted and forecasted performance v

作者: 偉大 時(shí)間: 2025-3-30 14:43
M. St?hli,A. Magunes rebate contracts?in a multi-level SC using fair share mechanism have been devised. In the sales rebate contract, the supplier charges the buyer wholesale price per unit purchased but then gives rebate to the buyer per unit sold above some threshold. The objective of this paper is to determine the

作者: 英寸 時(shí)間: 2025-3-30 19:14