Paper Title |
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Authors |
Cover |
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Volume 346 Cover |
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National Solar Observatory; Big Bear Observatory; Sankarasubramanian, K.; Penn, M.; Pevtsov, A. |
Front Matter |
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Volume 346 Front Matter |
1 |
Sankarasubramanian, K.; Penn, M.; Pevtsov, A. |
Conference Photograph |
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Volume 346 Conference Photograph |
2 |
Sankarasubramanian, K.; Penn, M.; Pevtsov, A. |
Part 1. Large-scale Circulation in the Convection Zone and Photosphere |
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Large-scale Transport of Magnetic Flux and Flows in Solar Convection Zone |
3 |
Ambroz, P. |
How Large-scale Flows may Influence Solar Activity? |
19 |
Hathaway, D. |
Large-scale Flows in Subsurface Layers |
33 |
Komm, R.; Howe, R.; Hernandez, I.G.; Hill, F.; Toner, C. |
Photospheric Surface Flows and Sunspot Moats |
41 |
Hagenaar, M. |
On the Characteristic Scales of Solar Convection |
47 |
Sridharan, R. |
CALAS, A Camera for the Large-scale of the Solar Surface |
53 |
Meunier, N.; Rondi, S.; Tkaczuk, R.; Rieutord, M.; Beigbeder, F. |
Part 2. Solar Dynamo |
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Large-scale Organization in the Solar Dynamo and its Observational Signature |
61 |
Dikpati, M. |
Fighting the Taylor-Proudman Constraint - How to Get Differential Rotation Solar-like? |
75 |
Rempel, M. |
What does the Solar Differential Rotation tell us about Large-scale Waves? |
83 |
Kaghashvilii, E.; Webb, G.; Zank, G. |
Coherent Structures vs Independent Modes of the Axisymmetric Magnetic Field Fluctuations |
91 |
Cadavid, A.; Lawrence, J.; McDonald, D.; Ruzmaikin, A. |
How Sensitive are Rotation Inversions to Subtle Features of the Dynamo? |
99 |
Howe, R.; Rempel, M.; Christensen-Dalsgaard, J.; Schou, J.; Thompson, M.; Komm, R.; Hill, F. |
Influence of Depth-dependent Diffusivity Profiles in Governing the Evolution of Weak, Large-scale Magnetic Fields of the Sun |
107 |
Zita, E.; Song, N.; McDonald, E.; Dikpati, M. |
Jets in the Solar Tachocline as Diagnostics of Global MHD Processes |
115 |
Christensen-Dalsgaard, J.; Cobard, T.; Dikpati, M.; Gilman, P.; Thompson, M. |
Part 3. Complexes of Activity, Activity Nests, and Connectivity in the Solar Corona |
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The Formation and Evolution of Complexes of Activity, Activity Nests, and the Large-scale Connectivity in the Solar Corona |
129 |
Benevolenskaya, E. |
Coronal Emission Lines Linear Polarization: a Tracer of Coronal Magnetic Fields Topology |
145 |
Arnaud, J. |
Low Frequency (< 100MHz) Thermal Radio Emission from the Solar Corona and the Effect of Radial Magnetic Field |
153 |
Ramesh, R.; Sastry, Ch. |
Large-scale Non-axisymmetric Magnetic Fields on the Sun and Cool Stars |
159 |
Berdyugina, S. |
Interpretation of Solar and Stellar Activity in terms of Dynamo Modes |
167 |
Fluri, D.; Berdyugina, S. |
Part 4. Filaments and Filament Channels |
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Role of Large-scale Magnetic Fields and Material Flows in the Formation of Filaments and Filament Channels |
177 |
Mackay, D. |
Motions and Interactions among Large-scale Solar Structures on H-Alpha Synoptic Charts |
193 |
McIntosh, P. |
Formation of an Extraordinarily Long Filament Channel |
201 |
Anderson, M.; Martin, S. |
The Internal Structures and Dynamics of Solar Quiescent Prominences |
211 |
Petrie, G.; Low, B. |
Accumulation of Filament Material at the Boundaries of Supergranular Cells |
219 |
Pevtsov, A.; Neidig, D. |
Part 5. Magnetic Field and Flows in Open Magnetic Structures |
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Magnetic Fields and Flows in Open Magnetic Structures |
229 |
Jones, H. |
Radio and EUV Measurements of the Equatorial Coronal Hole of February 25, 1999 |
245 |
Subramanian, K.; Sundaram, G.S. |
Multi-wavelength Observations of Coronal Holes |
251 |
de Toma, G.; Arge, C. |
Automated Coronal Hole Detection using He I 1083 nm Spectroheliograms and Photospheric Magnetograms |
261 |
Henney, C.; Harvey, J. |
The Chromospheric Prolateness and its Variations |
269 |
Vilinga, J.; Koutchmy, S. |
Magnetic Field Reversal of the Sun in Polarization of Radio Emission at 17GHz |
281 |
Tlatov, A.; Gelfreikh, G.; Makarov, V. |
Part 6. Eruptive Phenomenon |
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Large-scale Organizations Related to Eruptive Phenomena on the Solar Surface |
289 |
Lin, J. |
On Magnetic Structures of Solar Active Regions and Geomagnetic Storms |
305 |
Liu, Y. |
Multiple Large-scale MHD Shocks Related Radio Emission at Decameter Wavelengths |
313 |
Ebenezer, E. |
Genesis of AR NOAA10314 |
317 |
Morita, S.; McIntosh, S. |
The Solar Flare and CME Induced as a Collision of Two Opposite Polarities on 1997 May 12 |
327 |
Bharti, L.; Jain, R.; Joshi, C.; Jaafferey, S. |
Part 7. Influence of Small-scale Processes in the Formation and Evolution of Large-scale Strutures and Vice Versa |
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Influence of Small-scale Dynamics on Large-scale Solar Activity |
337 |
DeRosa, M. |
Quiet Sun unaffected by Activity Cycle |
353 |
Livingston, W.; Gray, D.; Wallace, L.; White, O. |
Three Dimensional Numerical Simulation of Solar Convection on MultiProcessors Supercomputer Systems |
357 |
Ustyugov, S. |
Large-scale Structures in Distribution of Coronal Bright Points |
363 |
Sattarov, I.; Pevtsov, A.; Karachik, N.; Sattarova, B. |
Part 8. Posters |
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Comparison of the Stream Structure and Coronal Sources of the Solar Wind During the April 7 & May 12, 1997 Halo CMEs |
371 |
Arge, C.; deToma, G.; Luhmann, J. |
Magnetically Preferred Solar Longitudes: Reality? |
381 |
Henney, C.; Durney, B. |
High Spectral Resolution Study of the He 10830 Spectral Region |
389 |
Malanushenko, O.; Livingston, W.; Jones, H.; Malanushenko, V. |
Active Longitudes in Distribution of EIT Bright Points |
395 |
Sattarov, I.; Pevtsov, A.; Karachik, N.; Sattarova, B. |
Sunspot Cycle 24: Smallest Cycle in 100 Years? |
401 |
Svalgaard, L.; Cliver, E.; Kamide, Y. |
22-Year Variations of the Solar Rotation |
409 |
Tlatov, A.; Makarov, V. |
Indices of Solar Activity in Minimum of Sunspot Cycles |
415 |
Tlatov, A.; Makarov, V. |
The Observed MnI 539.47 nm Spectral Line in Three Sunspots of the NOAA 0431 Complex Active Region |
423 |
Vince, O.; Vince, I. |
Back Matter |
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Volume 346 Back Matter |
431 |
Sankarasubramanian, K.; Penn, M.; Pevtsov, A. |