標題: Titlebook: Basic Mechanisms of Solar Activity; V. Bumba,J. Kleczek Book 1976 International Astronomical Union 1976 Corona.Main sequence.Photosphere.R [打印本頁] 作者: Jackson 時間: 2025-3-21 19:52
書目名稱Basic Mechanisms of Solar Activity影響因子(影響力)
書目名稱Basic Mechanisms of Solar Activity影響因子(影響力)學科排名
書目名稱Basic Mechanisms of Solar Activity網(wǎng)絡公開度
書目名稱Basic Mechanisms of Solar Activity網(wǎng)絡公開度學科排名
書目名稱Basic Mechanisms of Solar Activity被引頻次
書目名稱Basic Mechanisms of Solar Activity被引頻次學科排名
書目名稱Basic Mechanisms of Solar Activity年度引用
書目名稱Basic Mechanisms of Solar Activity年度引用學科排名
書目名稱Basic Mechanisms of Solar Activity讀者反饋
書目名稱Basic Mechanisms of Solar Activity讀者反饋學科排名
作者: MAL 時間: 2025-3-21 22:27 作者: Accommodation 時間: 2025-3-22 03:05 作者: 褲子 時間: 2025-3-22 08:25 作者: inferno 時間: 2025-3-22 10:12
Materialien zu Einem Zerfall der Werte,actly what has been predicted by a numerical solar cycle model driven by the dynamo action of the global convection. Another axisymmetric field is also derived by averaging over longitude the absolute value of the magnetic field after subtracting the poloidal field. This field corresponds to the tor作者: 語源學 時間: 2025-3-22 14:19 作者: Asperity 時間: 2025-3-22 17:55 作者: 縮短 時間: 2025-3-22 22:42
Small-Scale Solar Magnetic Fieldsotosphere, and the life-time of the smallest flux elements is very short. The observations further suggest that most of the magnetic flux in quiet regions is supplied directly from below the solar surface rather than being the result of turbulent diffusion of active-region magnetic fields.作者: 不能平靜 時間: 2025-3-23 04:48
Long Term Evolution of Solar Sector Structurein solar longitude of about 100° and a synodic rotation period of about 28 to 29 days. This 28.5 day structure is usually most prominent during a few years near sunspot maximum. Some preliminary comparisons of these observed solar structures with theoretical considerations are given.作者: 存心 時間: 2025-3-23 08:57 作者: 責怪 時間: 2025-3-23 13:09
1743-9213 problems were stressed and the majority of the Scientific Organizing Committee agreed not to deal with short-lived phenomena of the solar activity or with indiv978-90-277-0681-2978-94-010-1481-6Series ISSN 1743-9213 Series E-ISSN 2352-2186 作者: 豪華 時間: 2025-3-23 15:41 作者: objection 時間: 2025-3-23 21:02
Heritagization of the Camino to Finisterre solar differential rotation and to search for giant cell circulation pattern. Details of the observing method and the results from observations during 1974 have been pub-lished very recently (Schr?ter and W?hl, 1975). Our method consists of measuring the position of 5–15 bright Ca.-mottles with res作者: B-cell 時間: 2025-3-24 01:30 作者: 粘連 時間: 2025-3-24 03:11
Kai Maaz,Marko Neumann,Jürgen Baumertore than 15 years of observations are given. The major part of our information concerns the morphology and only some results deal with the kinematics of the field distribution. Results of averaged solar magnetic field fluxes and polarity reversal studies as well as of preliminary investigation of th作者: 離開 時間: 2025-3-24 09:10 作者: Antioxidant 時間: 2025-3-24 13:08 作者: blithe 時間: 2025-3-24 18:23
Herman Heijermans and His Dramasund between the maximum values of the limb effect of the redshift, the boundaries of polarities of the interplanetary magnetic field, the characteristic large-scale distribution of the background magnetic fields and the complex of solar activity.作者: 碎石 時間: 2025-3-24 22:46
https://doi.org/10.1007/978-3-476-04221-7rray Magnetograph. The observations consist of time sequences of simultaneous velocity, magnetic field, and chromospheric network measurements. From these data it appears that the supergranular velocity cells have lifetimes in excess of 30 h. Magnetic field motions associated with supergranulation w作者: forestry 時間: 2025-3-25 00:49
https://doi.org/10.1007/978-3-476-03267-6 has been investigated using the polarity (toward or away from the Sun) of the interplanetary magnetic field as inferred from polar geomagnetic observations. The polarity of the interplanetary magnetic field has previously been shown to be closely related to the polarity (into or out of the Sun) of 作者: 內(nèi)部 時間: 2025-3-25 03:52
Materialien zu Einem Zerfall der Werte,ield derived simply by averaging over longitude corresponds to the general magnetic field and can be regarded as reflecting the poloidal (radial) field since bipolar magnetic fields which have been regarded as reflecting the toroidal field are cancelled out by the averaging. The evolution of pattern作者: Lice692 時間: 2025-3-25 10:01 作者: 散步 時間: 2025-3-25 14:01
https://doi.org/10.1007/978-3-7091-0050-9a lot of information about cyclic and secular variations of solar activity rather than an account of new striking results in order to illustrate a certain concept. I beg your pardon in advance for possible defects in my report and for lack of time to quote all related papers.作者: 感情脆弱 時間: 2025-3-25 19:49
The Enigma of Solar Activitytical knowledge, of solar activity. It seems, therefore, that the most useful role for the introductory lecture would be to review the outstanding puzzles presented to us by the activity of the Sun so that we may have those numerous dilemmas clearly in mind as the speakers review the accumulated facts and theories.作者: 有助于 時間: 2025-3-25 22:23 作者: 厭惡 時間: 2025-3-26 02:30
About the Relation between the Limb Effect of the Redshift on the Sun and the Large-Scale Distributiund between the maximum values of the limb effect of the redshift, the boundaries of polarities of the interplanetary magnetic field, the characteristic large-scale distribution of the background magnetic fields and the complex of solar activity.作者: CHAR 時間: 2025-3-26 08:00
Cyclical and Secular Variations of Solar Activitya lot of information about cyclic and secular variations of solar activity rather than an account of new striking results in order to illustrate a certain concept. I beg your pardon in advance for possible defects in my report and for lack of time to quote all related papers.作者: 變異 時間: 2025-3-26 11:24
Basic Mechanisms of Solar Activity978-94-010-1481-6Series ISSN 1743-9213 Series E-ISSN 2352-2186 作者: DRAFT 時間: 2025-3-26 14:58
https://doi.org/10.1057/9780230360143tical knowledge, of solar activity. It seems, therefore, that the most useful role for the introductory lecture would be to review the outstanding puzzles presented to us by the activity of the Sun so that we may have those numerous dilemmas clearly in mind as the speakers review the accumulated facts and theories.作者: 貪婪性 時間: 2025-3-26 20:10
Heritagization of the Camino to Finisterreonal hole area time series provide synodic rotation periods which indicate an almost rigid rotation by such features for lag lengths as short as one rotation. The rotation periods of coronal holes at high latitudes best compare with inferred interplanetary field rotation periods.作者: 名字 時間: 2025-3-26 23:56 作者: 粘土 時間: 2025-3-27 04:29 作者: podiatrist 時間: 2025-3-27 07:28
https://doi.org/10.1007/978-3-319-20212-9We investigated the reality of the differences in rotation rates found from various features. We only used published observations including almost forgotten work of more than half a century ago.作者: 激怒某人 時間: 2025-3-27 10:57
Herman Heijermans and His DramasThe rotation law of the Sun is often described by the Faye formula:.where . is a heliographic latitude and . and . are constants. For a long time researchers have been studying the problem in what way the constants . and . change in time and in dependence on a phase of 11-year cycles.作者: ornithology 時間: 2025-3-27 15:15
Hermann Abert — eine LebensbeschreibungI am going to show two slides which should clearly prove that sunspots are drifting very regularly in the north-south direction on the solar surface.作者: Living-Will 時間: 2025-3-27 18:25 作者: 過份好問 時間: 2025-3-28 01:43 作者: Abjure 時間: 2025-3-28 03:38
Fast Variations of the Solar RotationThe rotation law of the Sun is often described by the Faye formula:.where . is a heliographic latitude and . and . are constants. For a long time researchers have been studying the problem in what way the constants . and . change in time and in dependence on a phase of 11-year cycles.作者: Flatus 時間: 2025-3-28 08:31 作者: Crater 時間: 2025-3-28 13:11
Some Results of the Space Distribution of the Activation Vector of the Filaments in the 11-Year CyclIn order to obtain new information on the manifestation of basic mechanisms of solar activity with the sunspot cycle development we have studied peculiarities of the latitude-time distribution of activation positions and suddenly disappearing filaments with respect to sunspot groups of cycles 18 to 20.作者: integrated 時間: 2025-3-28 15:45
https://doi.org/10.1007/978-94-010-1481-6Corona; Main sequence; Photosphere; Redshift; Solar; Sun; Sunspot作者: Unsaturated-Fat 時間: 2025-3-28 22:00 作者: Prophylaxis 時間: 2025-3-29 00:40 作者: Hdl348 時間: 2025-3-29 06:27 作者: 無王時期, 時間: 2025-3-29 10:13
1743-9213 Commission 10, we proposed to organize a Symposium which would stress the observational aspects of solar activity. It was our hope that such a Symposium might stimulate studies of those important problems in solar physics which for a long time had been neglected in overall scientific discussion. Alt作者: 群居動物 時間: 2025-3-29 13:47 作者: Emasculate 時間: 2025-3-29 19:18
Investigation of Coronal Rotation by the Spectroscopic Methodr region an intensive stream of coronal gas directed oppositely to the solar rotation was detected during the time interval 1969–1972. In the greater part of the latitude range, on average, the corona rotates more slowly in comparison with the solar atmosphere at the photospheric level.作者: observatory 時間: 2025-3-29 20:41
Kai Maaz,Marko Neumann,Jürgen Baumerterent role or visibilility of structures in both polarities is discussed. The reflection of both main types of the longitudinal distribution of large-scale solar background magnetic fields (the 27-day, the 28–29-day successions, the ‘supergiant’ structures) in the interplanetary magnetic field distribution is also considered.作者: 沉積物 時間: 2025-3-30 03:19
https://doi.org/10.1007/978-3-476-04221-7oints. These observations suggest that surface motions do not exhibit the detailed flux redistribution expected in the random-walk diffusion of magnetic fields. It is suggested that the surface motions are only the reflection of magnetic field-convective motion interactions which occur deeper in the convection zone.作者: 平 時間: 2025-3-30 06:36
https://doi.org/10.1007/978-3-7091-0050-9ntified in X-ray photographs are seen as small (5?10″) emission features in ground-based H. and Ca K spectroheliograms as well as in transition region lines observed in other Skylab instruments. Typical bright point temperatures are 1.5?2×10. K and typical densities are ~ 5×10. cm..作者: 浮夸 時間: 2025-3-30 10:24
Large-Scale Solar Magnetic Fieldserent role or visibilility of structures in both polarities is discussed. The reflection of both main types of the longitudinal distribution of large-scale solar background magnetic fields (the 27-day, the 28–29-day successions, the ‘supergiant’ structures) in the interplanetary magnetic field distribution is also considered.作者: Suggestions 時間: 2025-3-30 13:50
Velocities Observed in Supergranulesoints. These observations suggest that surface motions do not exhibit the detailed flux redistribution expected in the random-walk diffusion of magnetic fields. It is suggested that the surface motions are only the reflection of magnetic field-convective motion interactions which occur deeper in the convection zone.作者: Glaci冰 時間: 2025-3-30 19:07
Coronal Bright Pointsntified in X-ray photographs are seen as small (5?10″) emission features in ground-based H. and Ca K spectroheliograms as well as in transition region lines observed in other Skylab instruments. Typical bright point temperatures are 1.5?2×10. K and typical densities are ~ 5×10. cm..作者: Intuitive 時間: 2025-3-30 23:59 作者: 窩轉脊椎動物 時間: 2025-3-31 01:12
Differential Rotation and Giant Cell Circulation of the Solar Ca+ -Network solar differential rotation and to search for giant cell circulation pattern. Details of the observing method and the results from observations during 1974 have been pub-lished very recently (Schr?ter and W?hl, 1975). Our method consists of measuring the position of 5–15 bright Ca.-mottles with res作者: 愛國者 時間: 2025-3-31 08:50
Rotational Characteristics of Coronal Holesonal hole area time series provide synodic rotation periods which indicate an almost rigid rotation by such features for lag lengths as short as one rotation. The rotation periods of coronal holes at high latitudes best compare with inferred interplanetary field rotation periods.作者: fiction 時間: 2025-3-31 11:34
Large-Scale Solar Magnetic Fieldsore than 15 years of observations are given. The major part of our information concerns the morphology and only some results deal with the kinematics of the field distribution. Results of averaged solar magnetic field fluxes and polarity reversal studies as well as of preliminary investigation of th作者: 打火石 時間: 2025-3-31 15:44 作者: 贊美者 時間: 2025-3-31 17:58
Investigation of Coronal Rotation by the Spectroscopic Methodear velocity by 0.4 km s. on the latitude and its relative constancy in the latitude interval 35° < . < 50° are the most typical..In the southern polar region an intensive stream of coronal gas directed oppositely to the solar rotation was detected during the time interval 1969–1972. In the greater
