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標(biāo)題: Titlebook: Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond; Tetsuya Watanabe,Takeo Kosugi,Alphonse C. Sterling Book 1998 Springer [打印本頁]

作者: 快樂    時間: 2025-3-21 19:30
書目名稱Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond影響因子(影響力)




書目名稱Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond影響因子(影響力)學(xué)科排名




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書目名稱Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond被引頻次




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書目名稱Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond讀者反饋




書目名稱Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond讀者反饋學(xué)科排名





作者: hankering    時間: 2025-3-22 00:14
0067-0057 s book is a collection of papers presented at ameeting held in: Yoyogi, Tokyo, on the occasion of Yohkoh‘s fifthanniversary of operation. The papers constitute a summary ofobservations and results over the five years, including contributionsbased on data from Yohkoh‘s hard and soft X-ray telescopes
作者: resilience    時間: 2025-3-22 03:30
Studies of Coronal Temperaturee is observed to increase with height (Sturrock, Wheatland and Acton, 1996, Foley, Culhane and Acton, 1997). Here we present a full-sun temperature map to illustrate these and other features of the temperature structure of the corona.
作者: acquisition    時間: 2025-3-22 08:16
Deep Survey of Solar Nano-Flares with Yohkoharker 1988) using the soft X-ray position-dependent time profiles. For details, please refer to the full-length paper published in the 1997 September issue of the . with the same title (Shimizu and Tsuneta 1997).
作者: CLOT    時間: 2025-3-22 10:47
Book 1998a collection of papers presented at ameeting held in: Yoyogi, Tokyo, on the occasion of Yohkoh‘s fifthanniversary of operation. The papers constitute a summary ofobservations and results over the five years, including contributionsbased on data from Yohkoh‘s hard and soft X-ray telescopes and itsspe
作者: sterilization    時間: 2025-3-22 14:03
The Behavior of Coronal Holes the minimum of the cycle. In this paper we discuss the role of fine structures in the solar corona with densities comparable to CHs, their relations with photospheric fields, and the connection with the global behavior of CHs through the solar cycle.
作者: Outspoken    時間: 2025-3-22 21:02
Coronal and Interplanetary Disturbances Associated with an Eruptive Prominence of 28 August 1992rmation of the CME (and its interplanetary manifestation). An interplanetary disturbance was observed via interplanetary scintillation technique in the region to the east of the sun-Earth line on 29–30 August 1992.
作者: Orgasm    時間: 2025-3-23 01:12

作者: Coordinate    時間: 2025-3-23 02:49

作者: Morphine    時間: 2025-3-23 06:29

作者: Adj異類的    時間: 2025-3-23 10:40

作者: 骨    時間: 2025-3-23 15:45

作者: 一個攪動不安    時間: 2025-3-23 20:53
Studies of Coronal Temperatureorly known. There are few, if any, full sun temperature maps of the solar corona in the literature. The soft x-ray telescope (SXT) on . is able to provide useful temperature maps for regions where the x-ray signal is sufficiently strong. Previous SXT studies have shown that the coronal temperature d
作者: Abrade    時間: 2025-3-23 22:34

作者: 效果    時間: 2025-3-24 05:19

作者: 收養(yǎng)    時間: 2025-3-24 07:12

作者: gonioscopy    時間: 2025-3-24 14:37

作者: Sleep-Paralysis    時間: 2025-3-24 16:04
Comparison between Statistical Features of X-ray Fluctuations from the Solar Corona and Accretion Dith ranges, including radio, H-alpha, soft X-ray, hard X-ray, and gamma-ray, mainly in order to explain coronal heating and periodicities of flares (e.g., Drake 1971; Datlowe, Elcan, & Hudson 1974; Lin et al. 1984; Dennis 1985; Rieger et al. 1984; Kile & Cliver 1991; Bai & Sturrock 1993). Also, follo
作者: Cumbersome    時間: 2025-3-24 20:16
From the Sun to the Galaxy Clusterst has unprecedented angular resolution of ~ 5. over a wide energy range of 15–95 keV. With HXT, clear evidence of particle acceleration due to magnetic reconnection was obtained (Sakao et al. 1992; Saka 1994; Masuda 1994; Masuda et al. 1994), and the flare morphology was mathematically quantified (I
作者: 圣人    時間: 2025-3-25 01:49

作者: Jogging    時間: 2025-3-25 05:43
Magnetic Reconnection and Dynamos in Laboratory Plasmas and in many other contexts. One of the achievements of YOHKOH has been to provide observational evidence for magnetic reconnection in the solar corona (e.g. Tsuneta et al, 1992). As well as large scale reconnections which may reconfigure the global field, many theories of coronal heating propose th
作者: Defraud    時間: 2025-3-25 09:38
A Mechanism Driving Solar Flaresfor reconnection is practically missing, indicating a basic deficiency of the flare models and theories. Here I classify the reconnection configurations according to their possible topologies. Considering the physical mechanisms, which would be able to generate these different topologies, I present
作者: 秘傳    時間: 2025-3-25 15:38
On the Origin of Helicity in Active Region Magnetic Fieldsugh the convection zone (Babcock 1961), it acquires writhe through the Coriolis force on internal longitudinal flows (Fan, Fisher, & DeLuca 1993). The tilt . of active regions with respect to the equator is an observable manifestation of such writhe, at photospheric levels. If . is conserved, as we
作者: Obloquy    時間: 2025-3-25 18:32

作者: 愛管閑事    時間: 2025-3-25 23:42
The Filament Disappearance of May 7, 1992] event). It was studied by Khan et al. (1993) from X-ray data obtained with SXT onboard the . satellite. Recently Meudon observers recognised that they had H. observations for the period of the EBI event. We report here our further research on the EBI event, based mainly on H.- and radio-observatio
作者: Malleable    時間: 2025-3-26 03:11

作者: 遷移    時間: 2025-3-26 07:45
Observations of Superhot Plasma in Solar Flaresers and to calculate temperature (..) and emission measure (EM.) of the hotter component assuming a two temperature model. The calculated distributions of .. and EM. are compared with temperatures obtained from the Fe XXV and Ca . diagnostics. In one flare, we find .. of ~30 MK in a loop structure a
作者: Camouflage    時間: 2025-3-26 11:34
dimensional environments extending over many wavelengths. This is particularly so for environments characterized by a refractive index field with a compact region of arbitrary (.-dimensional) variability superimposed upon a transversely inhomogeneous ((.-1)-dimensional) background profile. For such
作者: –DOX    時間: 2025-3-26 12:44
H. Haradimensional environments extending over many wavelengths. This is particularly so for environments characterized by a refractive index field with a compact region of arbitrary (.-dimensional) variability superimposed upon a transversely inhomogeneous ((.-1)-dimensional) background profile. For such
作者: 機(jī)制    時間: 2025-3-26 16:56
Madhulika Guhathakurta,Richard Fisher,Keith Strongin [1]–[7]. Recently, some numerical methods associated with this problem have appeared [4]–[7]. When the wave climbs up the inclined sea shore, there are moving boundaries which are unknown in advance. Under the potential flow assumption, Kim [5] calculated the climbing of a soliton on an inclined
作者: 一條卷發(fā)    時間: 2025-3-27 00:14
L. W. Acton,J. R. Lemendimensional environments extending over many wavelengths. This is particularly so for environments characterized by a refractive index field with a compact region of arbitrary (.-dimensional) variability superimposed upon a transversely inhomogeneous ((.-1)-dimensional) background profile. For such
作者: 橫截,橫斷    時間: 2025-3-27 02:06
A. Sanchez-Ibarra,M. Barraza-Paredesin [1]–[7]. Recently, some numerical methods associated with this problem have appeared [4]–[7]. When the wave climbs up the inclined sea shore, there are moving boundaries which are unknown in advance. Under the potential flow assumption, Kim [5] calculated the climbing of a soliton on an inclined
作者: 令人悲傷    時間: 2025-3-27 06:15

作者: Customary    時間: 2025-3-27 12:21

作者: Nomogram    時間: 2025-3-27 16:55

作者: 肉體    時間: 2025-3-27 21:43
Satoru Uenosorder. This raises a philosophical and semantic issue, namely, what is the purpose of defining such concepts as schizophrenia, and what are the tests of its value. The possible options open to us are answers to the following questions: (1) does such a definition exist; (2) is it a true definition;
作者: biosphere    時間: 2025-3-28 00:40
K. Makishimaes of psychosocial actions are tc be understood, described, and explained. In this tradition, behaviors that are deemed unacceptable or disruptive for a socio-cultural group are said to be explained by, caused by, or attributable to some defect, deficiency, disruption, or disorganization of some age
作者: 藥物    時間: 2025-3-28 04:12

作者: PACK    時間: 2025-3-28 07:34

作者: languid    時間: 2025-3-28 10:32

作者: 鞏固    時間: 2025-3-28 15:03
S. Koutchmy,H. Hara,K. Shibata,Y. Suematsu,K. Reardon countries, to help solve shortages in its health care system, particularly in underserviced rural and remote areas. Throughout the 1970s, roughly a third of Canada’s physicians were IMGs. Although this proportion has dropped to 23?% more recently, Canada still has a sizeable dependence on physician
作者: 縫紉    時間: 2025-3-28 22:23

作者: 完整    時間: 2025-3-28 23:13
T. Watanabe,M. Yamamoto,H. Hudson,M. Irie,K. Ichimoto,H. Kurokawa,H. Yatagaiexpansion of humanitarian and family reunion programs and the introduction of multiculturalism. The reasons for the shift to a universal admissions scheme were varied, encompassing changing ideas about race, ethnicity and human rights, the labour and social imperatives of post-war modernisation, and
作者: embolus    時間: 2025-3-29 05:24
Nariaki Nitta countries, to help solve shortages in its health care system, particularly in underserviced rural and remote areas. Throughout the 1970s, roughly a third of Canada’s physicians were IMGs. Although this proportion has dropped to 23?% more recently, Canada still has a sizeable dependence on physician
作者: 顛簸下上    時間: 2025-3-29 09:46
Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond
作者: ingestion    時間: 2025-3-29 11:25

作者: 骯臟    時間: 2025-3-29 17:09

作者: PRISE    時間: 2025-3-29 22:42
Book 1998e solar minimum period. .This wide-ranging volume will be of interest to workers in solarphysics and X-ray astronomy. It also contains material appropriate forsupplemental reading for graduate students in solar physics.
作者: antidote    時間: 2025-3-30 00:02
0067-0057 during the solar minimum period. .This wide-ranging volume will be of interest to workers in solarphysics and X-ray astronomy. It also contains material appropriate forsupplemental reading for graduate students in solar physics.978-94-010-6198-8978-94-011-5220-4Series ISSN 0067-0057 Series E-ISSN 2214-7985
作者: 磨坊    時間: 2025-3-30 05:30
pseudo-differential and Fourier integral operators. In conjunction with the global functional integral techniques pioneered by Wiener (Brownian motion) and Feynman (quantum mechanics), and so successfully applied today in quantum field theory and statistical physics, the .-dimensional classical phy
作者: HACK    時間: 2025-3-30 10:30
H. Hara pseudo-differential and Fourier integral operators. In conjunction with the global functional integral techniques pioneered by Wiener (Brownian motion) and Feynman (quantum mechanics), and so successfully applied today in quantum field theory and statistical physics, the .-dimensional classical phy
作者: 潔凈    時間: 2025-3-30 13:54

作者: 沒血色    時間: 2025-3-30 17:02

作者: 粗鄙的人    時間: 2025-3-30 21:01

作者: Classify    時間: 2025-3-31 04:17

作者: TRAWL    時間: 2025-3-31 09:00

作者: 不透氣    時間: 2025-3-31 10:34
T. Hirayamaons. Three interrelated issues are quickly apparent. There are questions about the coherence of the underlying metaphor in this tradition; about the presumption of distinctive differences between the behaviors considered abnormal and those behaviors considered normative; and about many contradiction
作者: Hypopnea    時間: 2025-3-31 14:02





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