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Title: |
2nd ATST-EAST Workshop in Solar Physics: Magnetic Fields from the Photosphere to the Corona
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Volume: |
463
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Year: |
2012
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View this Volume on ADS
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Editors: |
T. R. Rimmele, A. Tritschler, F. Wöger, M. Collados Vera, H. Socas Navarro, R. Schlichenmaier, M. Carlsson, T. Berger, A. Cadavid, H. Gilbert, P. R. Goode, and M. Knolker
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Synopsis: |
THE SECOND ATST-EAST MEETING
MAGNETIC FIELDS FROM THE
PHOTOSPHERE TO THE CORONA
Washington, DC
9–11 November 2011
Ground-based solar astronomy is currently experiencing a Renaissance. A generation of 1m class solar telescopes, which has served the scientific community well for decades, is being replaced by new, large aperture solar telescopes. Adaptive optics has enabled routine diffraction limited observations of the solar atmosphere from ground based telescopes. The full scientific potential of large aperture optical and infrared telescopes equipped with state-of-the-art instrumentation can thus be realized. The size and complexity of these new telescope systems is immense and affordable and maintainable only as ground-based facilities.
Large aperture solar telescopes are about to open up new windows for scientific advances and discovery. The new 1.6m NST at BBSO and the 1.5m GREGOR on Tenerife have already demonstrated the potential for advancing our knowledge of the physics of the solar atmosphere providing significantly improved resolution. The 4m Advanced Technology Solar Telescope (ATST) located on top of the 3000m Haleakala on Maui, HI, and currently under construction, as well as the 4m EST will enable solar astronomers to resolve solar magnetism on its intrinsic scales and thus make these telescopes the world’s leading ground-based resource for studying solar magnetism that controls the solar wind, ares, coronal mass ejections and variability in the Sun’s output.
In November 2011, about 100 scientists, engineers and students met in Washington, DC for the 2nd ATST-EAST Workshop. They emphasized the connectivity provided by solar magnetic fields of the classical atmospheric layers, photosphere, chromosphere and corona and the new capabilities large aperture solar telescopes will provide for measuring magnetic fields and their dynamic behavior. This volume captures the presentations given at the workshop.
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ISBN: |
978-1-58381-808-4
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978-1-58381-809-1
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Paper Title |
Page |
Authors |
Front Matter |
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Book Cover |
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Front Matter |
1 |
Rimmele, T. R.; Tritschler, A.; Woger, F.; Collados Vera, M.; Socas Navarro, H.; Schlichenmaier, R.; Carlsson, M.; Berger, T.; Cadavid, A.; Gilbert, H.; Goode, P. R.; Knolker, M. |
Conference Photos |
2 |
Rimmele, T. R.; Tritschler, A.; Woger, F.; Collados Vera, M.; Socas Navarro, H.; Schlichenmaier, R.; Carlsson, M.; Berger, T.; Cadavid, A.; Gilbert, H.; Goode, P. R.; Knolker, M. |
Part I. Magnetic Coupling through the Solar Atmosphere |
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Magnetometry with Large Solar Telescopes: Beyond the Photospheric Boundaries |
3 |
Pietarila, A. |
Chromospheric Magnetic Fields: Observations, Simulations and their Interpretation |
15 |
de la Cruz Rodríguez, J.; Socas-Navarro, H.; Carlsson, M.; Leenaarts, J. |
He I Spectropolarimetry with FIRS: Towards Vector Magnetometry of Chromospheric Fibrils Plus New Diagnostics of Coronal Rain |
25 |
Schad, T. A.; Penn, M. J.; Lin, H.; Tritschler, A. |
IBIS: High-Resolution Multi-Height Observations and Magnetic Field Retrieval |
33 |
Del Moro, D..; Berrilli, F.; Stangalini, M.; Giannattasio, F.; Piazzesi, R.; Giovannelli, L.; Viticchiè, B.; Vantaggiato, M.; Sobotka, M.; Jurčák, J.; Criscuoli, S.; Giorgi, F.; Zuccarello, F. |
Photospheric and Chromospheric Measurements of a High-Speed Flow near the Light Bridge of a δ-Spot |
43 |
Choudhary, D. P.; Deng, N. |
Spectro-polarimetric Observations of Moving Magnetic Features around a Pore |
51 |
Zuccarello, F.; Berrilli, F.; Criscuoli, S.; Del Moro, D.; Ermolli, I.; Giannattasio, F.; Giorgi, F.; Romano, P.; Viticchiè, B. |
Requirements for the Analysis of Quiet-Sun Internetwork Magnetic Elements with EST and ATST |
57 |
Orozco Suárez, D.; Bellot Rubio, L. R.; Katsukawa, Y. |
Understanding the Role of Small-Scale Flux in Solar Spectral Irradiance Variation |
65 |
Rast, M. P.; Harder, J. W. |
Turbulent Fluctuations in G-band and K-line Intensities Observed with
the Rapid Oscillations in the Solar Atmosphere (ROSA) Instrument |
75 |
Cadavid, A. C.; Lawrence, J. K.; Christian, D. J.; Jess, D. B.; Mathioudakis, M. |
Flux Emergence and Pore Formation: What ATST can See |
83 |
Stein, R. F.; Nordlund, Å. |
The Sunspot Penumbra in the Photosphere: Results from Forward Synthesized Spectroscopy |
89 |
Tritschler, A.; Uitenbroek, H.; Rempel, M. |
The Influence of Molecular Lines on the Measurement of Photospheric Velocities |
99 |
Uitenbroek, H.; Dumont, N.; Tritschler, A. |
Vortices in the Solar Photosphere |
107 |
Shelyag, S.; Fedun, V.; Erdélyi, R.; Keenan, F. P.; Mathioudakis, M. |
The Solar Convection over a Solar Cycle |
115 |
Hanslmeier, A.; Muller, R.; Utz, D. |
Magnetism of Solar Flares and Prominences |
121 |
Heinzel, P.; Hudson, H. S. |
Coronal Seismology with ATST |
133 |
Aschwanden, M. J. |
The Prominence/Coronal Cavity System: A Unified View of Magnetic Structures in the Solar Corona |
147 |
Berger, T. |
The Build-Up to Eruptive Solar Events Viewed as the Development of Chiral Systems |
157 |
Martin, S. F.; Panasenco, O.; Berger, M. A.; Engvold, O.; Lin, Y.; Pevtsov, A. A.; Srivastava, N. |
Alfvén Wave Dynamics in the Expanding Solar Corona |
175 |
Kaghashvili, E. Kh. |
The Distributions of UV Solar Explosive Events |
181 |
Mendoza-Torres, J. E.; Niembro-Hernandez, T. |
Part II. Tools and Techniques |
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Tools for 3D Solar Magnetic Field Measurement |
193 |
Casini, R. |
Solar Dark Matter and Dark Energy: How can CryoNIRSP Help? |
207 |
Kuhn, J. R.; Scholl, I. F.; Mickey, D. L. |
Extracting Information from the Data Flood of New Solar Telescopes: Brainstorming |
215 |
Asensio Ramos, A. |
Interpreting Coronal Polarization Observations |
227 |
Rachmeler, L. A.; Casini, R.; Gibson, S. E. |
Beyond Standard Coronal Seismology Tools |
235 |
Kaghashvili, E. Kh. |
Towards Measuring the Magnetic Energy Spectrum at Sub-Resolution Scales |
243 |
López Ariste, A.; Sainz Dalda, A. |
Comparing Simultaneous Measurements of two High-Resolution Imaging Spectropolarimeters: The ‘Göttingen’ FPI@VTT and CRISP@SST |
251 |
Bello González, N.; Bellot Rubio, L. R.; Ortiz, A.; Rezaei, R.; Rouppe van der Voort, L.; Schlichenmaier, R. |
Chromospheric Multi-Wavelength Observations near the Solar Limb: Techniques and Prospects |
257 |
Beck, C.; Rezaei, R. |
Sequential Chomospheric Brightening: An Automated Approach to Extracting Physics from Ephemeral Brightening |
267 |
Kirk, M. S.; Balasubramaniam, K. S.; Jackiewicz, J.; McAteer, R. T. J.; McNamara, B. J. |
Beyond the Solar Corona: Mercury's Magnetic Fields seen with Large Solar Telescopes |
275 |
López Ariste, A.; Leblanc, F. |
Simulations of Chromospheric Heating by Ambipolar Diffusion |
281 |
Khomenko, E.; Collados Vera, M. |
NIRIS: The Second Generation Near-Infrared Imaging Spectro-polarimeter for the 1.6 Meter New Solar Telescope |
291 |
Cao, W.; Goode, P. R.; Ahn, K.; Gorceix, N.; Schmidt, W.; Lin, H. |
A New Technique for Solar Imaging Spectro-polarimetry using Shack-Hartmann and Fabry-Pérot |
301 |
Gosain, S.; Sankarasubramanian, K.; Venkatakrishnan, P.; Raja Bayanna, A. |
ATST Telescope Calibration: Summary of Studies and their Conclusions |
307 |
Elmore, D. F. |
Active Optical Control of Quasi-Static Aberrations for ATST |
315 |
Johnson, L. C.; Upton, R.; Rimmele, T. R.; Hubbard, R.; Barden, S. C. |
Solar Limb Adaptive Optics: A Test of Wavefront Sensors and Algorithms |
321 |
Taylor, G. E.; Rimmele, T. R.; Marino, J.; Tritschler, A.; McAteer, R. T. J. |
Expected Performance of Adaptive Optics in Large Aperture Solar Telescopes |
329 |
Marino, J.; Rimmele, T. R. |
On Zeeman Diagnostics with a 4 m Aperture |
337 |
Kim, I. S.; Alexeeva, I. V.; Suyunova, E. Z. |
Near IR Filter Linear Polarimetry in the Corona with a 4 m Aperture |
347 |
Kim, I. S.; Popov, V. V.; Suyunova, E. Z. |
Part III. New Telecope and Instrumentation Efforts |
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The 1.6 m Off-Axis New Solar Telescope (NST) in Big Bear |
357 |
Goode, P. R.; Cao, W. |
The GREGOR Solar Telescope on Tenerife |
365 |
Schmidt, W.; von der Lühe, O.; Volkmer, R.; Denker, C.; Solanki, S. K.; Balthasar, H.; Bello González, N.; Berkefeld, T.; Collados Vera, M.; Hofmann, A.; Kneer, F.; Lagg, A.; Puschmann, K. G.; Schmidt, D.; Sobotka, M.; Soltau, D.; Strassmeier, K. G. |
Construction of the Advanced Technology Solar Telescope |
377 |
Rimmele, T. R.; Keil, S.; McMullin, J.; Knölker, M.; Kuhn, J. R.; Goode, P. R.; Rosner, R.; Casini, R.; Lin, H.; Tritschler, A.; Wöger, F.; ATST Team |
India's National Large Solar Telescope |
395 |
Hasan, S. S. |
The Chinese Giant Solar Telescope (CGST) |
405 |
Deng, Y.; Liu, Z.; CGST Group |
Instrumental Capabilities of the EST |
413 |
Collados Vera, M.; EST Team |
The GREGOR Fabry-Pérot Interferometer: A New Instrument for High-Resolution Spectropolarimetric Solar Observations |
423 |
Puschmann, K. G.; Balthasar, H.; Bauer, S.-M.; Hahn, T.; Popow, E.; Seelemann, T.; Volkmer, R.; Woche, M.; Denker, C. |
The Visible Broadband Imager: The Sun at High Spatial and Temporal Resolution |
431 |
Wöger, F.; McBride, W.; Ferayorni, A.; Gregory, S.; Hegwer, S.; Tritschler, A.; Uitenbroek, H. |
Instrument Design of the Large Aperture Solar UV Visible and
IR Observing Telescope (SUVIT) for the SOLAR-C Mission |
439 |
Suematsu, Y.; Katsukawa, Y.; Shimizu, T.; Ichimoto, K.; Takeyama, N. |
HELLRIDE: A New Multiline Spectrometer for the Vacuum Tower Telescope, Tenerife |
445 |
Staiger, J. |
The Simple Hyperspectral Imaging Polarimeter Concept |
453 |
Barden, S. C. |
Author Index |
459 |
Rimmele, T. R.; Tritschler, A.; Woger, F.; Collados Vera, M.; Socas Navarro, H.; Schlichenmaier, R.; Carlsson, M.; Berger, T.; Cadavid, A.; Gilbert, H.; Goode, P. R.; Knolker, M. |
Back Matter |
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Back Matter |
461 |
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