標題: Titlebook: Lectures on Solar Physics; H. M. Antia,Arvind Bhatnagar,Peter Ulmschneider Book 2003 Springer-Verlag Berlin Heidelberg 2003 Chromosphere.C [打印本頁] 作者: 無力向前 時間: 2025-3-21 17:34
書目名稱Lectures on Solar Physics影響因子(影響力)
書目名稱Lectures on Solar Physics影響因子(影響力)學科排名
書目名稱Lectures on Solar Physics網(wǎng)絡(luò)公開度
書目名稱Lectures on Solar Physics網(wǎng)絡(luò)公開度學科排名
書目名稱Lectures on Solar Physics被引頻次
書目名稱Lectures on Solar Physics被引頻次學科排名
書目名稱Lectures on Solar Physics年度引用
書目名稱Lectures on Solar Physics年度引用學科排名
書目名稱Lectures on Solar Physics讀者反饋
書目名稱Lectures on Solar Physics讀者反饋學科排名
作者: 彩色的蠟筆 時間: 2025-3-21 22:45
Instrumentation and Observational Techniques in Solar Astronomy,al kinds of back-end instruments, such as monochromatic filters, spectrographs, spectroheliographs, magnetographs, etc., used for photospheric, chromospheric and coronal observations. Standard techniques for making solar observations, e.g., measurements of sunspot areas, coordinates and position of 作者: Provenance 時間: 2025-3-22 02:19
osed approach has been extensively validated with synthetic and realtrajectory data. In our experiments our approach consistently learned motionmodels that were more compact and accurate than those produce978-3-642-26385-9978-3-642-13642-9Series ISSN 1610-7438 Series E-ISSN 1610-742X 作者: menopause 時間: 2025-3-22 05:43
the future to non-nutritional constraints, we imply that we have some understanding of nutritional constraints. The geographical area covered includes North African countries with a Mediterranean coast and West Asian countries with cool, wet winters and hot, dry summers. Areas with steppe vegetation作者: 鉆孔 時間: 2025-3-22 12:02 作者: chassis 時間: 2025-3-22 16:26 作者: 灌溉 時間: 2025-3-22 20:32 作者: Indelible 時間: 2025-3-23 00:17 作者: nullify 時間: 2025-3-23 03:50 作者: 燕麥 時間: 2025-3-23 06:08
P. Venkatakrishnans the ability tolearn incrementally both the parameters and the structure of the model. Theproposed approach has been extensively validated with synthetic and realtrajectory data. In our experiments our approach consistently learned motionmodels that were more compact and accurate than those produce作者: 致敬 時間: 2025-3-23 10:09 作者: Lime石灰 時間: 2025-3-23 14:31
P. K. Manoharans the ability tolearn incrementally both the parameters and the structure of the model. Theproposed approach has been extensively validated with synthetic and realtrajectory data. In our experiments our approach consistently learned motionmodels that were more compact and accurate than those produce作者: 延期 時間: 2025-3-23 18:05 作者: 火花 時間: 2025-3-23 23:05
and temperature. These variations lead to a marked seasonality of feed supply which is a major constraint to livestock production. As it is generally agreed that a plentiful and balanced nutrient supply is the foundation of efficient livestock production, research at ICARDA during the past 10 years作者: 有其法作用 時間: 2025-3-24 03:25 作者: ambivalence 時間: 2025-3-24 10:07 作者: 完成 時間: 2025-3-24 12:27 作者: Indict 時間: 2025-3-24 17:31 作者: harmony 時間: 2025-3-24 20:15 作者: GUILE 時間: 2025-3-24 23:37 作者: 不能強迫我 時間: 2025-3-25 04:32
on the winning thesis of the EURON Georges Giralt award.Modeling and predicting human and vehicle motion is an active research domain.Owing to the difficulty in modeling the various factors that determine motion(e.g. internal state, perception) this is often tackled by applying machinelearning techn作者: Largess 時間: 2025-3-25 07:47
B. N. Dwivedimotion(e.g. internal state, perception) this is often tackled by applying machinelearning techniques to build a statistical model, using as input a collectionof trajectories gathered through a sensor (e.g. camera, laser scanner), and thenusing that model to predict further motion. Unfortunately, mos作者: 驚惶 時間: 2025-3-25 15:10
P. K. Manoharanmotion(e.g. internal state, perception) this is often tackled by applying machinelearning techniques to build a statistical model, using as input a collectionof trajectories gathered through a sensor (e.g. camera, laser scanner), and thenusing that model to predict further motion. Unfortunately, mos作者: Notify 時間: 2025-3-25 17:47 作者: 雪上輕舟飛過 時間: 2025-3-25 22:47 作者: 千篇一律 時間: 2025-3-26 02:38
Instrumentation and Observational Techniques in Solar Astronomy,ur Sun being the nearest star, shows intricate surface details and a wide variety of dynamic phenomena. These range in size from a few kilometres to millions of kilometres and in the temporal domain from a fraction of a second to decades. In addition, the Sun displays a great variety of magnetic and作者: 潰爛 時間: 2025-3-26 06:54
Solar Interior and Seismology,cillations have been measured bythe ground based Global Oscillation Network Group project and the space based Michelson Doppler Imager. Each of these modes is trapped in a different region of the solar interior and hence its frequencyis sensitive to structure and dynamics in the corresponding region作者: Adornment 時間: 2025-3-26 09:33
The Active and Explosive Sun,emporal scales. The most notable among these is the solar activity cycle of 11 years, or magnetic cycle of 22 years. On shorter time scales of a few seconds to several hours, spectacular explosive events occur in the solar atmosphere, such as, solar flares, prominence eruptions, and coronal mass eje作者: 旋轉(zhuǎn)一周 時間: 2025-3-26 13:19
Magnetic Flux Tubes and Activity on the Sun,fundamental aspects of magnetic activity: (a) the generation, storage and emergence of magnetic fields from the solar interior; (b) the nature of the surface magnetic fields, especially in the form of small-scale flux tubes; and (c) dynamical processes in flux tubes and heating of the magnetic chrom作者: 值得贊賞 時間: 2025-3-26 19:33 作者: 行為 時間: 2025-3-26 22:40
The Solar Corona,e surface or photosphere (6000 K) to where it freely expands into the solar system as the solar wind. The exact reasons for its high temperature are still being debated despite more than 50 years of research, but magnetic fields are believed to be responsible for this heating. This article reviews s作者: RAFF 時間: 2025-3-27 01:57
The Solar Wind, of the Sun. The topic is split into two parts on the basis of two types of solar wind flows, (i) quasi-stationary winds and (ii) transient flows. The first part covers the basic ideas of the coronal heating and acceleration of the quasi-stationary wind. It also reviews the large-scale properties an作者: deviate 時間: 2025-3-27 09:22
https://doi.org/10.1007/3-540-36963-5Chromosphere; Corona; Solar wind; astrophysics; helioseismology; solar; solar physics; space science作者: infringe 時間: 2025-3-27 09:45
978-3-642-05686-4Springer-Verlag Berlin Heidelberg 2003作者: eulogize 時間: 2025-3-27 15:58 作者: TEM 時間: 2025-3-27 19:04 作者: 脫落 時間: 2025-3-28 01:01
Lecture Notes in Physicshttp://image.papertrans.cn/l/image/583600.jpg作者: capillaries 時間: 2025-3-28 03:39
Magnetic Flux Tubes and Activity on the Sun,fundamental aspects of magnetic activity: (a) the generation, storage and emergence of magnetic fields from the solar interior; (b) the nature of the surface magnetic fields, especially in the form of small-scale flux tubes; and (c) dynamical processes in flux tubes and heating of the magnetic chromosphere.作者: 現(xiàn)代 時間: 2025-3-28 06:23
Book 2003sciences. All contributions are self-contained and do not require prior in-depth knowledge of solar physics. The result is a unique textbook that fulfills the needs of those wishing to have a pedagogic exposition of solar physics bringing them up-to-date in a field full of vitality and with exciting research. .作者: Irrigate 時間: 2025-3-28 11:14
Solar Magnetic Fields, rudiments of such a dynamo mechanism are discussed. Some recent issues arising out of new theoretical and observational developments are mentioned. The importance of magnetic topology for various solar phenomena is highlighted. Finally, a few methods of measuring solar magnetic fields are described.作者: Thyroid-Gland 時間: 2025-3-28 17:45
The Solar Corona,till being debated despite more than 50 years of research, but magnetic fields are believed to be responsible for this heating. This article reviews some recent progress in our understanding, using data from spacecraft (Yohkoh, SOHO and TRACE) and from ground-based eclipse observations.作者: analogous 時間: 2025-3-28 22:04 作者: 外科醫(yī)生 時間: 2025-3-29 00:19
0075-8450 lated areas in both astrophysics and space sciences. All contributions are self-contained and do not require prior in-depth knowledge of solar physics. The result is a unique textbook that fulfills the needs of those wishing to have a pedagogic exposition of solar physics bringing them up-to-date in
