作者: 概觀 時(shí)間: 2025-3-21 23:25 作者: TOM 時(shí)間: 2025-3-22 04:02
https://doi.org/10.1007/978-3-642-51139-4io spectroscopic and mapping techniques, Stokes parameters, antenna temperature conventions, radio frequency interference, virial analysis, principal component analysis, and statistical analysis of the velocity fluctuations.作者: Innocence 時(shí)間: 2025-3-22 06:37
Atmung und Herzkreislauf in Narkose diagrams, spectroscopic, and photometric techniques. We also discuss the asymmetry in the high-latitude molecular cloud population with respect to the northern and southern Galactic hemispheres and the possibility that some high-latitude molecular clouds may be at the disk/halo interface.作者: Lyme-disease 時(shí)間: 2025-3-22 10:39
0067-0057 tbooks by focussing on the diffuse portion of the ISM.ExplorThis book provides an introduction to the physics of interstellar gas in the Galaxy. It deals with the diffuse interstellar medium which supplies a complex environment for exploring the neutral gas content of a galaxy like the Milky Way and作者: cancellous-bone 時(shí)間: 2025-3-22 15:55
An?sthesie beim ambulanten Patientensing the CO(1-0) line to determine the physically relevant quantity, N(H.). In this chapter we discuss these techniques with particular emphasis on determining the conversion factor (called X.) for diffuse and translucent molecular gas. The chapter closes with some comments on using the CO(1-0) line to trace dark gas.作者: 我不重要 時(shí)間: 2025-3-22 20:48 作者: 挑剔為人 時(shí)間: 2025-3-22 22:09 作者: 破布 時(shí)間: 2025-3-23 02:54 作者: Invertebrate 時(shí)間: 2025-3-23 09:32 作者: GEM 時(shí)間: 2025-3-23 10:23 作者: BLINK 時(shí)間: 2025-3-23 14:38 作者: white-matter 時(shí)間: 2025-3-23 19:11 作者: lipoatrophy 時(shí)間: 2025-3-23 22:51
The Diffuse ISM from the Ground: Chemistry and Tracers,echniques of data evaluation. During the course of a study lasting many years, questions and hypotheses, evaluation, interpretation, and new questions and hypotheses follow each other in a process of continuous development extending, in the end, over the whole study. We will now formulate the basic 作者: Hyperopia 時(shí)間: 2025-3-24 04:04
Observing the Diffuse ISM: Making Sense of the Radio Observations,rtant treatments such as thermal oxidation, long-time annealing, ion implantation and crystal growth. Depending on the temperature various defect types are known to occur in silicon after such treatments: i.e. dislocation-type defects at high temperature (800–1200°C), rod-like and {113} defects at i作者: Mangle 時(shí)間: 2025-3-24 07:35 作者: FIS 時(shí)間: 2025-3-24 12:49 作者: 火車車輪 時(shí)間: 2025-3-24 15:45 作者: 上腭 時(shí)間: 2025-3-24 19:28
The Relationship Between CO and H2,eptually optimized packet scheduling algorithm developed for robust low-delay intervehicle video communication. The algorithm has been tested by transmitting video data captured by on-board cameras to another vehicle in proximity, using ad hoc 802.11 wireless technology and the H.264 video coding st作者: MIRTH 時(shí)間: 2025-3-25 02:38 作者: amenity 時(shí)間: 2025-3-25 06:09 作者: chassis 時(shí)間: 2025-3-25 11:34 作者: 暫時(shí)休息 時(shí)間: 2025-3-25 14:03
Coda,er of austenite once the temperature reaches the inter-critical (α?+?γ) region. It is also observed that a significant amount of austenite (6–7%) was found to be retained at room temperature despite a high cooling rate (>20°C?s.). Even after cooling the samples to room temperature, austenite was fou作者: CRUC 時(shí)間: 2025-3-25 19:16 作者: 下垂 時(shí)間: 2025-3-25 22:03 作者: inhumane 時(shí)間: 2025-3-26 00:38 作者: 敲竹杠 時(shí)間: 2025-3-26 06:32 作者: otic-capsule 時(shí)間: 2025-3-26 08:57
Observing the Diffuse ISM: Making Sense of the Radio Observations,ts in thermal equilibrium is extremely small and below detection limit of most analytical tools, handling and testing properties have so far remained an uphill task. One way to circumvent this problem is the study of point defect reactions at non equilibrium conditions, for instance during intensive作者: intrigue 時(shí)間: 2025-3-26 15:15
Observing the Diffuse ISM: The Space Missions, field strength of 0.07?T under different reaction temperatures for 20?min are shown in Fig. 6.1 and 6.2, respectively. It can be seen from Fig. 6.1 that the morphologies of Al.Zr are mainly granular, bulk-shaped, lath-shaped, and spiculate. It shows that the fabrication process, especially the melt作者: Insensate 時(shí)間: 2025-3-26 20:07 作者: 共同時(shí)代 時(shí)間: 2025-3-26 21:07 作者: 偶然 時(shí)間: 2025-3-27 03:43 作者: 撫育 時(shí)間: 2025-3-27 06:50 作者: Etching 時(shí)間: 2025-3-27 09:47
Distances,try, and physics. Electrochemical study of perfect smooth or bulk materials was the usual way to understand the interaction between the surfaces of such materials with their close environment. Therefore, any modification of the surface structure or composition provides change in the material behavio作者: BLAND 時(shí)間: 2025-3-27 14:16
Dynamical Considerations: Instabilities and Turbulence,gins with an introduction to focused ion beam machining for sample preparation. Steps and strategies to fabricate miniature samples using ion beam milling are presented, along with some precautions and limitations that need to be taken into consideration. Thereafter, imaging tools for in-situ observ作者: BARB 時(shí)間: 2025-3-27 19:43
Coda,eld thermal cycles have been studied. Experiments were carried out at ID11 of the European Synchrotron Radiation Facility, Grenoble, France. A specially designed oven was used to simulate the weld thermal cycles. Time–temperature resolved 2D synchrotron diffraction patterns were recorded and used to作者: Gullible 時(shí)間: 2025-3-28 00:21 作者: 排斥 時(shí)間: 2025-3-28 02:34 作者: Abutment 時(shí)間: 2025-3-28 08:54
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/a/image/140690.jpg作者: pulmonary-edema 時(shí)間: 2025-3-28 14:06
An?sthetika und Koronarzirkulationcuss the phase structure of the ISM, with a special emphasis on why the hydrogen takes the different forms it does. We then outline the observational signatures of the Hot Ionized, Warm Ionized, Warm Neutral, and Cold Neutral media, followed by a brief introduction to the molecular component of the 作者: 強(qiáng)壯 時(shí)間: 2025-3-28 16:39
An?sthetika und Koronarzirkulationllar medium. We concentrate on line processes. After a discussion of absorption and emission lines, we use the 21?cm line of hydrogen as an illustrative example. We also briefly discuss the CN transitions that are pumped by the Cosmic Microwave Background radiation. Collisional excitation, complicat作者: 蒙太奇 時(shí)間: 2025-3-28 22:11
https://doi.org/10.1007/978-3-642-51139-4n with a brief history of molecular observations, from the optical detections of CH, CN, and CH. in the late 1930s, to the rise of radio astronomy in the 1950s and 1960s. A brief discussion of astrochemistry and some of the basic reaction networks for oxygen, carbon, and nitrogen chemistry is includ作者: Heresy 時(shí)間: 2025-3-28 23:23
https://doi.org/10.1007/978-3-642-51139-4es are concerned. In this chapter, we discuss some of the practical considerations involved in making and analyzing these observations. Some of the topics discussed here should be useful in preparing observing proposals or reading observational papers on this medium. Topics covered include basic rad作者: 不適當(dāng) 時(shí)間: 2025-3-29 03:11
An?sthesie und kardiovaskul?res Systemm to imaging and spectroscopic study. From the radio to gamma-rays, satellites have contributed substantially heavily to the field. We review some of the more significant missions and describe some of their special capabilities for studying the diffuse ISM since many of these satellites have produce作者: 現(xiàn)任者 時(shí)間: 2025-3-29 11:07 作者: FIN 時(shí)間: 2025-3-29 11:35
Probleme des an?sthesiologischen Alltagsturn our attention to the smaller objects, like dark clouds, but with an emphasis on the flotsam of the ISM, the small diffuse and translucent clouds. We also discuss how recent work on diffuse clouds is revising our ideas of this component of the ISM.作者: Epidural-Space 時(shí)間: 2025-3-29 15:47 作者: COMMA 時(shí)間: 2025-3-29 20:23
Atmung und Herzkreislauf in Narkosehings like interstellar clouds where luminosity distances play no role. In this chapter we describe some of the techniques that have been applied over the years to obtaining the distances to molecular clouds. In particular we focus on high-latitude molecular clouds to illustrate the efficacy of Wolf作者: 翅膀拍動(dòng) 時(shí)間: 2025-3-30 00:56 作者: 通知 時(shí)間: 2025-3-30 04:55
A Dirty Window978-3-662-54350-4Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: incite 時(shí)間: 2025-3-30 11:41 作者: 頌揚(yáng)國(guó)家 時(shí)間: 2025-3-30 15:04
