標(biāo)題: Titlebook: Coronal Physics from Radio and Space Observations; Proceedings of the C Gérard Trottet Conference proceedings 1997 Springer-Verlag Berlin H [打印本頁] 作者: Affordable 時間: 2025-3-21 19:50
書目名稱Coronal Physics from Radio and Space Observations影響因子(影響力)
書目名稱Coronal Physics from Radio and Space Observations影響因子(影響力)學(xué)科排名
書目名稱Coronal Physics from Radio and Space Observations網(wǎng)絡(luò)公開度
書目名稱Coronal Physics from Radio and Space Observations網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Coronal Physics from Radio and Space Observations被引頻次
書目名稱Coronal Physics from Radio and Space Observations被引頻次學(xué)科排名
書目名稱Coronal Physics from Radio and Space Observations年度引用
書目名稱Coronal Physics from Radio and Space Observations年度引用學(xué)科排名
書目名稱Coronal Physics from Radio and Space Observations讀者反饋
書目名稱Coronal Physics from Radio and Space Observations讀者反饋學(xué)科排名
作者: 橡子 時間: 2025-3-21 23:06
Recent developments of the solar Submm-wave telescope (SST),With the approval of funds for the development and construction of the new Solar Submm-wave Telescope, its design was reviewed, updated and manufacturers for the subsystems were selected. The principal characteristics of the system and the proposed research programs are described in this note.作者: 6Applepolish 時間: 2025-3-22 02:13 作者: 朦朧 時間: 2025-3-22 07:57
The Nature of Liquids and Gases,al electrons is fragmented in both space and time. Observations dealing with the extent in heights and spatial scales of the electron acceleration sites are also reviewed. The knowledge of the electron energy spectra deduced at low and high energies from both hard X-ray and centimeter/millimeter obs作者: 行乞 時間: 2025-3-22 09:25
Molecular Distribution Functions,oblem of coronal heating. Radio observations provide powerful diagnostics of the physical conditions in the transition region and the corona. Recent observational and theoretical results are presented and their implications are discussed. The prospects of further observations, in conjunction with ot作者: 宣傳 時間: 2025-3-22 14:51 作者: 宣傳 時間: 2025-3-22 17:46 作者: GLOOM 時間: 2025-3-22 23:41 作者: Asseverate 時間: 2025-3-23 03:02
Spectral Analysis of Wave Motion,vers of type II burst emitting super-Alfvénic disturbances. The paper focuses on the available experimental evidence for this assumption. For instance, the apparent contradiction is discussed between measured speeds of potential shock drivers and their observed type II burst association. Further, se作者: ferment 時間: 2025-3-23 06:20 作者: Injunction 時間: 2025-3-23 11:20 作者: 自制 時間: 2025-3-23 16:46
Parity Violating Effects in Atoms,rrelator (Stokes I and V, 576 channels). Calibration has also been improved. The multifrequency operation remains almost unchanged. It allows simultaneous observations of up to 10 frequencies in the range 150–450 MHz. Integrated data will be available on the internet, and special observing modes may作者: 不透明 時間: 2025-3-23 21:15
https://doi.org/10.1007/978-1-4684-2193-4orders of magnitude over current facilities operating at frequencies between about 200 MHz and a few GHz. Such a leap in performance is motivated by a wide range of fundamental astrophysical questions which we hope to address in the first decades of the next millenium. Some of the myriad possibiliti作者: 尖 時間: 2025-3-24 01:03 作者: 賞心悅目 時間: 2025-3-24 05:36
https://doi.org/10.1007/BFb0106448astronomy; energy release; interferometer; large-scale disturbances; measurement; particle beams; radio in作者: 獨(dú)裁政府 時間: 2025-3-24 07:52
978-3-662-14120-5Springer-Verlag Berlin Heidelberg 1997作者: 多樣 時間: 2025-3-24 13:12
Coronal Physics from Radio and Space Observations978-3-540-68693-4Series ISSN 0075-8450 Series E-ISSN 1616-6361 作者: 過渡時期 時間: 2025-3-24 16:47
Molecular Distribution Functions,ent results of X-ray bright-points, transient brightenings and jets are reviewed, and diagnostics that result from bulk plasma motions are discussed. Finally, three events are examined in detail and the implications of the observation discussed in relation to flare models.作者: hypnogram 時間: 2025-3-24 22:38
Molecular Distribution Functions,oblem of coronal heating. Radio observations provide powerful diagnostics of the physical conditions in the transition region and the corona. Recent observational and theoretical results are presented and their implications are discussed. The prospects of further observations, in conjunction with other wavelength ranges are given.作者: 懶惰民族 時間: 2025-3-25 03:06 作者: ELATE 時間: 2025-3-25 06:58 作者: Immobilize 時間: 2025-3-25 09:19 作者: MAIZE 時間: 2025-3-25 11:45 作者: GRIPE 時間: 2025-3-25 19:19
Lecture Notes in Physicshttp://image.papertrans.cn/c/image/238296.jpg作者: Meditative 時間: 2025-3-25 20:51
Coronal mass ejections and type II radio bursts, the radiation of shock accelerated electrons, constitute a unique access to the structure and the dynamics of the coronal magnetoplasma. This is important for understanding the timing and the sites of energy release processes in the solar corona and for studying the physics of collisionless shock w作者: NICE 時間: 2025-3-26 03:52
An upgrade of nobeyama radioheliograph to a dual-frequency (17 and 34 GHz) system,ing of the new system, such as the calibration and development of image synthesis software tools is still under way. Flare images taken at the dual frequencies are presented and compared with that from the . SXT as an example.作者: 單色 時間: 2025-3-26 08:19
Solar astronomy and the Square Kilometer Array Interferometer,n the quiet solar surface should then be practical over much of the frequency range. “Solar microscopy” may also become possible, in which near-field effects are employed to obtain the range as well as position of high brightness solar emission features.作者: Hormones 時間: 2025-3-26 12:28
Spectral Analysis of Wave Motion, the radiation of shock accelerated electrons, constitute a unique access to the structure and the dynamics of the coronal magnetoplasma. This is important for understanding the timing and the sites of energy release processes in the solar corona and for studying the physics of collisionless shock w作者: OCTO 時間: 2025-3-26 15:34
Phenomenology of Weak Interactions,ing of the new system, such as the calibration and development of image synthesis software tools is still under way. Flare images taken at the dual frequencies are presented and compared with that from the . SXT as an example.作者: 繞著哥哥問 時間: 2025-3-26 18:35 作者: 強(qiáng)制性 時間: 2025-3-27 00:03 作者: 毗鄰 時間: 2025-3-27 02:36 作者: Ligneous 時間: 2025-3-27 07:26
Conference proceedings 1997hock waves and coronal mass ejections; particle beams in the solar corona and in the interplanetary medium; and explosive energy-release phenomena and particle acceleration. The different articles give a well-balanced presentation of relevant observations based upon various techniques, models and th作者: 星星 時間: 2025-3-27 11:10 作者: 不妥協(xié) 時間: 2025-3-27 17:09
The Nature of Liquids and Gases,es are also reviewed. The knowledge of the electron energy spectra deduced at low and high energies from both hard X-ray and centimeter/millimeter observations is discussed. The experimental data is compared with the predictions of the avalanche model for solar flares and further tests of the model proposed.作者: Minatory 時間: 2025-3-27 20:56 作者: Bureaucracy 時間: 2025-3-27 23:19 作者: 占線 時間: 2025-3-28 02:28
High Energy Neutrino Interactions,relation to coronal beams, using recent spacecraft data from . and .. Interplanetary electron beams can often be traced back to coronal type III sources, while there is no such relation for interplanetary ion beams. In the third part, we briefly review acceleration mechanisms for coronal and interplanetary beams, separately for electrons and ions.作者: 菊花 時間: 2025-3-28 07:41 作者: 木訥 時間: 2025-3-28 14:07 作者: 管理員 時間: 2025-3-28 16:22
Observations of the 3D distributions of thermal to near-relativistic electrons in the interplanetardistributions . .(. .) often are plateaued or slightly unstable, with ., implying growth rates of . ～0.03 s.. Most of the time, however, the reduced distributions are stable, with negative slopes, suggesting that other competing wave processes such as whistler growth may be stabilizing the beam.作者: 縮影 時間: 2025-3-28 20:19 作者: Carcinogenesis 時間: 2025-3-28 23:39
Prospects for the solar radio telescope,be done with a solar-dedicated radio synthesis telescope, and to discuss the design constraints imposed by the science envisioned. Special attention was also given to nighttime uses for the instrument. We summarize the “strawman” concept for the instrument here.作者: 季雨 時間: 2025-3-29 06:23
0075-8450 nd WIND and spectral and imaging data from SOHO and YOHKOH provide an unprecedented richness of relevant data. For their better understanding, radio observations - also included in this book - play a key role.978-3-662-14120-5978-3-540-68693-4Series ISSN 0075-8450 Series E-ISSN 1616-6361 作者: 流浪者 時間: 2025-3-29 08:54 作者: 一美元 時間: 2025-3-29 13:25
The Nature of Liquids and Gases,al processes creating enhanced plasma wave turbulence and particle acceleration at shock waves. The ULYSSES, WIND, and SOHO missions together with ground based observations and additional theoretical investigations are an exceptional opportunity to achieve progress in answering the many open questions.作者: 燦爛 時間: 2025-3-29 16:00
Diagnostics of energy release in the X-ray corona,ent results of X-ray bright-points, transient brightenings and jets are reviewed, and diagnostics that result from bulk plasma motions are discussed. Finally, three events are examined in detail and the implications of the observation discussed in relation to flare models.作者: 動作謎 時間: 2025-3-29 22:24
Solar flare radio and hard X-ray observations and the avalanche model,al electrons is fragmented in both space and time. Observations dealing with the extent in heights and spatial scales of the electron acceleration sites are also reviewed. The knowledge of the electron energy spectra deduced at low and high energies from both hard X-ray and centimeter/millimeter obs作者: 北極熊 時間: 2025-3-30 01:40
Radio observations of the quiet sun and their implications on coronal heating,oblem of coronal heating. Radio observations provide powerful diagnostics of the physical conditions in the transition region and the corona. Recent observational and theoretical results are presented and their implications are discussed. The prospects of further observations, in conjunction with ot作者: adj憂郁的 時間: 2025-3-30 08:05
Energy release in the solar corona,particle events, as well as coronal heating and the solar wind. The basic physics of these phenomena and their relationship to each other remains a vigorous area of inquiry. The . at Mont Evray directed its attention to recent observational and theoretical developments relevant to flares and coronal作者: trigger 時間: 2025-3-30 09:51
Observations of the 3D distributions of thermal to near-relativistic electrons in the interplanetar observed at 1 AU are found to have power-law spectra often extending down to ?1 keV, implying a source region at 0.2-1. . altitude. At solar quiet times, a nonthermal, “super-halo” component extending from ～2 to ?10. keV is found to be always present. For impulsive events which produce solar type I作者: 不成比例 時間: 2025-3-30 14:48
Coronal and interplanetary particle beams,leration in the solar corona and in interplanetary space. We start our discussion of coronal beams with a standard flare scenario, established on recent X-ray (.) and radio observations, which constitutes a framework for the understanding of upward and downward accelerated electron beams and their s作者: Duodenitis 時間: 2025-3-30 18:12
Coronal mass ejections and type II radio bursts,vers of type II burst emitting super-Alfvénic disturbances. The paper focuses on the available experimental evidence for this assumption. For instance, the apparent contradiction is discussed between measured speeds of potential shock drivers and their observed type II burst association. Further, se作者: MULTI 時間: 2025-3-30 21:21
