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linkages between the atmosphere on the Earth and sun Phần 7 pps

linkages between the atmosphere on the Earth and sun Phần 7 pps

linkages between the atmosphere on the Earth and sun Phần 7 pps

... 3:9  1 Ä  Ä 3:9 The Solar-Stellar Connection 3 37 4 The Ca II H & K Sun The variation of the solar emission in the cores of the calcium resonance lines and their association with magnetic ... of the Sun s interior. The radialvariations of the sound speed and the superadiabatic gradient are now well estab-lished and we know the depth of the convection zone with remarkable precision.Even ... insights on the core rotation and magnetic field, the variability of the tachocline through gravity-mode characteristics, and the interplay of convection,rotation, and magnetic field throughout and...
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linkages between the atmosphere on the Earth and sun Phần 2 ppsx

linkages between the atmosphere on the Earth and sun Phần 2 ppsx

... missing is the almost horizontal passage through the verythin annulus occupying the space between its deepest penetration level and that of the second wave: the space between the second and third ... reflectedbeneath, rather than at, the surface of the Sun, one cannot know the structure of the Sun all the way to the surface. So how can one proceed? And how can the trapped80 D.O. Goughat low and high ... Zahn and I have initiated a simple calculation to assess the effect of the convection-zoneshear on the Maxwell stresses and to estimate the outcome for a Forg´acs-Dajka and Petrovay model. The...
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linkages between the atmosphere on the Earth and sun Phần 3 pps

linkages between the atmosphere on the Earth and sun Phần 3 pps

... sign, depending on the sense of rotation (orientation of the field vector). The magnitudes of thesetwo effects depend on the competition between the Larmor precession rate and the damping rate, ... curved. The conclusion by Solanki et al. (2003) that their data demonstrate the presence ofa current sheet in the upper solar atmosphere is based on the assumption that the observed absorption in the ... base of the convection zonefor the various diffusion parameters, making the thermal and viscous spread of the latitudinal shear imposed by the convective envelope slow with respect to the con-vective...
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linkages between the atmosphere on the Earth and sun Phần 6 ppsx

linkages between the atmosphere on the Earth and sun Phần 6 ppsx

... Faraday ro-tation of the plane of polarization between the source and the observer ((Gragnard and McLean 1 973 )).2Observations The radio data reported were obtained at 77 and 109MHz with the recentlycommissioned ... polar-ized emission from the Sun at both 77 and 109 MHz. Similar emission from the Sun was observed on the following days also, up to 18 August 2006. As the 77 MHz fre-quency is also used with the Gauribidanur ... polar coronal hole1http://www.lmsal.com/solarsoft/Coronal Mass Ejections from Sunspot and Non-Sunspot Regions 3034.2 Implications to the Flare: CME Connection The difference in the latitude...
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linkages between the atmosphere on the Earth and sun Phần 8 pps

linkages between the atmosphere on the Earth and sun Phần 8 pps

... sketches and magnetic field strengths of all sunspots and strongpores. These were used to evaluate the magnetic configurations associated with the sunspots.3 Results and Conclusion The classic Wilson ... 19 97 using the SUMERspectrometer onboard SoHO. The observations used the spectra lines N IV 76 5˚A,formed in the transition region, and Ne VIII 77 0˚A, formed in the low corona. The spectra ... following correlation coefficients and significancelevels for the four data sets: (1) 0:63 and 97: 28%; (2) 0:60 and 96:13;(3)0:36 and 75 :38%; and (4) 0: 67 and 78 :34. If we calculate the rise time...
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linkages between the atmosphere on the Earth and sun Phần 1 docx

linkages between the atmosphere on the Earth and sun Phần 1 docx

... light on the constitution of the Sun. In 1885, the Royal Society, London, constituted the Indian ObservatoriesCommittee comprised of the Astronomer Royal, and a few Fellows of the Royal and Royal ... showed the CN bands and the C2 Swan bands in the head, while the tail showed bands dueto CO. He was ably assisted in the observations by his wife Mary.Contents ixCoronal Mass Ejections from Sunspot ... administration of these observatories. The suggestions of SPC regardingregular observations of the Sun and the thinking of the Indian Observatories Com-mittee on the future orientation of activities...
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linkages between the atmosphere on the Earth and sun Phần 4 potx

linkages between the atmosphere on the Earth and sun Phần 4 potx

... refracted and reflected by interaction with the magnetic field. The perturbation of the wave front in the convection zone in Fig. 5 is not due to the presence of a magnetic field, but rather to the vigorous ... valid on scales smaller than 0.300. In fact,simulations suggest constant angular distribution within ˙50ıfrom the horizon-tal direction on a scale of 0:0500. On the other hand, should the ... through the inversion as a function of optical depth (lower panels)(strength, inclination, and azimut), LOS velocity, and temperature among others.We apply the inversion to both the Fe I 6301.5 and...
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linkages between the atmosphere on the Earth and sun Phần 5 doc

linkages between the atmosphere on the Earth and sun Phần 5 doc

... the sunspot (item 9), and it is conceivable that it continues within the sunspot. The existence of small scale convective upflows and downflows does not contra-dict the systematic upward motions ... for the two magnetic components of the model MISMA. They are identical for the dark core and the bright sides. (f) Velocities along the magnetic field lines for the two magnetic components of the ... time-averaged intensity as a function of wave-length and position along the slit. The bright and fainter vertical strips correspondto the red and blue components of the He multiplet, respectively....
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linkages between the atmosphere on the Earth and sun Phần 9 potx

linkages between the atmosphere on the Earth and sun Phần 9 potx

... destabilization. The cusp-shaped magneticfield in the main phase of the second flare and its evolution in correlation with ribbonseparation provide evidence for the cause of the CME eruption. The propagation ... Te, the effec-tive ion temperatures and non-thermal motions, the plume cross-section relative to the size of the coronal hole, and the plasma bulk speeds.In this paper, we briefly discuss the ... tail of the lithium-like Ne7C. The contributionfunctions of NeVIII and Mg VIII overlap considerably in the temperature range justbelow 1 MK. The contribution functions of NeVIII and Mg IX...
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linkages between the atmosphere on the Earth and sun Phần 10 potx

linkages between the atmosphere on the Earth and sun Phần 10 potx

... reactions in the proto -Sun. Such resonances may expedite the onset of nuclear ignition in the proto -Sun and the redistribution and loss of the proto -Sun s angular momentum.1 IntroductionTo ... 1,2 07 s for the thermal mode and 26 sfor the slow mode, and damping per wave period of 0.06 for the thermal mode and 7. 64 for the slow mode. The thermal wave becomes a propagating wave in the ... values are related to the magnetic environment and the loop geom-etry and can be used to infer the magnetic condition at the onset of the eruption. Weintend to submit the full analysis to A&A.Acknowledgment...
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