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 ... existsthere. From the simulation we measure the separation of the peaks to be approx-imately 4.5Mm behind and 1 68 s after the rise of the jet, deduced from the crosssection of the Vxcomponent ... features on the Sun, the observed umbral and penumbral fine-structures are very dynamic and subject to constant change and transformation on small spatial scales. Ourunderstanding of these processes and...

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

... 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 trapped 80 D.O. Goughat low and high ... 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 ... 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...

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 ... G<B<50 G the Stokes Q and U profiles are only sensitive to the orientation of the magnetic field vector. The 8, 4 98 ˚A line is, however, sensitive to both the orientation and the strength of the magnetic...

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

... 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 distributions of CMEs (no butterfly diagram) and flares ... between the flaring rate and sunspot number during the maxi-mum phase. This result further confirms the close relation between flares and CMEsirrespective of the source region: sunspot regions or ... behind the limbs can produce type II bursts due to the extended nature of the shock and the wide beams of the radio emission, but theseshocks need not reach Earth. On the other hand, there are...

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

... 3:9  1 Ä  Ä 3:9 The Solar-Stellar Connection 3374 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 ... theycan be measured), then sunspots themselves as well as the quiet Sun, before mov-ing upwards into the atmosphere and the corona, with the violence of coronal massejections and of ﬂares. Finally, ... 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...

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

... light on the constitution of the Sun. In 188 5, the Royal Society, London, constituted the Indian ObservatoriesCommittee comprised of the Astronomer Royal, and a few Fellows of the Royal and Royal ... positions of stars, and a principal source of stellar positions for mostof the southern hemisphere stars. John Goldingham (1796– 180 5, 181 2– 183 0), T.G.Taylor ( 183 0– 184 8), W.S. Jacob ( 184 9– 185 8), and ... 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...

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...

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 ... theory and observa-tions of sunspots, see the recent book by Thomas and Weiss (20 08) and the reviewsby Solanki (2003) and Thomas and Weiss (2004).2 Umbral MagnetoconvectionIn a broad sense, there ... physical and thermodynamical information: the damping, the Doppler width, the optical depth, and the macroscopic velocity of the plasma. Combining it with the information carried by Stokes Q and U...

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 ... regions, namely NOAA AR 10 484 , 10 486 , and 10 488 . On 25 October, weobserved two surges between 01:50 UT and 04:15 UT that originated from NOAAAR 10 484 . The first surge was small; the second one ... flare. The five flares yielded tc0values between 1, 088 and 2,016 s and tcvalues between 22 and 1; 02s(Table1). The right-hand panel of Fig. 3 shows convolutions of the time profiles per energyband...

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 ... equal to the respective light-travel times and with amplitudes consistent with PPN expressionsfor the accelerations used in the standard ephemeris. The standard theory of the origin of the solar ... Torsional Oscillation Precede the Sunspot Cycle? 501 The two completely novel aspects of our model are (1) the Nandy–Choudhurihypothesis, which allows the formation of strong toroidal ﬁeld in the...

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