| Preface | |
| Foreword | |
| Committees and Supporting Organizations | |
| Acknowledgements | |
| Participants | |
| Overview of Infrared Solar Physics | p. 1 |
| The Cold Heart of the Solar Chromosphere | p. 11 |
| Properties of Faculae from Observations Near the Opacity Minimum | p. 23 |
| A Solar Plage Model | p. 29 |
| Formation of the Solar 10830 A Line | p. 35 |
| Interpreting Recent Observations of He I 10830 A | p. 49 |
| Variability of the Solar He I 10830 A Triplet | p. 59 |
| Observations of Solar Oscillations in He I 10830 A | p. 65 |
| Observations of Dynamic Events in He I [lambda] 10830 | p. 71 |
| An Investigation of IR Triplet He I 10830 A Profiles in Active Regions and the Quiet Chromosphere | p. 77 |
| Potential IR Observations of the Solar Corona | p. 81 |
| The Sun in Submillimeter Radiation | p. 85 |
| Far Infrared and Submillimeter Continuum Observations of Solar Flares: Justifications and Prospects for Ground-Based Experiments | p. 93 |
| Submillimeter and Far Infrared Emission from Solar Flares | p. 103 |
| Infrared and Submillimeter Diagnostics of Activity and Flares | p. 113 |
| The Observed Spectrum of Solar Burst Continuum Emission in the Submillimeter Spectral Range | p. 125 |
| Interferometry of Solar Flares at 3-mm Wavelength | p. 131 |
| Eclipse Observations of the Extreme Solar Limb at Submillimeter Wavelengths | p. 139 |
| 12-[mu]m Observations at the 1991 Eclipse | p. 151 |
| 850 [mu]m Observations of the 11 July 1991 Total Solar Eclipse | p. 161 |
| Observations of the 1991 Eclipse at 3.5 mm Wavelength | p. 167 |
| Near IR Observations of the 11 July 1991 Total Solar Eclipse from Mauna Kea, Hawaii | p. 173 |
| Infrared Images of the Sun During the July 11, 1991 Solar Eclipse | p. 179 |
| IR Observations of the K and F Corona During the 1991 Eclipse | p. 185 |
| Infrared Coronal Observations at the 1991 Solar Eclipse | p. 199 |
| On the Coronal and Prominence Structures Observed at the Total Solar Eclipse of 11 July 1991 | p. 205 |
| The White-Light, Far Red (600-700 nm) and Emission Coronae at the July 11, 1991 Eclipse | p. 211 |
| The Structure of the White-Light Corona at the 1991 Eclipse | p. 217 |
| Subphotospheric Convection | p. 225 |
| The Infrared Granulation - Observations | p. 239 |
| Simultaneous IR and Visible Light Measurements of the Solar Granulation | p. 251 |
| Measurements of Horizontal Flows in 1.6[mu]m Granulation | p. 259 |
| On Sunspot and Facular Contrast Variations Near 2 [mu]m and 4 [mu]m | p. 265 |
| Solar 5-minute Oscillations at 2.23 [mu]m | p. 271 |
| Ground-Based Near-Infrared Observations of Global Solar Oscillations | p. 277 |
| Solar Oscillations Instrument at an Infrared Wavelength of 1.6 [mu]m at Yunnan Observatory | p. 283 |
| Magnetic Fields, Oscillations, and Heating in the Quiet Sun Temperature Minimum Region from Ultraviolet Observations at 1600 A | p. 287 |
| Atomic Physics at the 12 [mu]m and Related Lines | p. 297 |
| The Formation of Infrared Rydberg Lines | p. 309 |
| Modeling the Infrared Magnesium and Hydrogen Lines from Quiet and Active Solar Regions | p. 323 |
| Computation of Infrared Hydrogen Lines | p. 341 |
| New Atomic Data for Mg I Lines | p. 347 |
| On the Ion Broadening of the 12 [mu]m lines of Atomic Magnesium | p. 353 |
| High-l Rydberg Lines of Fe I in the ATMOS Spectra: 4f-5g, 5g-6h ... | p. 359 |
| High-n Hydrogen Lines in Solar Infrared Spectra from Balloon-borne, Mauna Kea, and ATMOS Observations | p. 365 |
| Solar Submillimeter and Millimeter Spectroscopy between 7 and 30 cm[superscript -1] from the James Clerk Maxwell Telescope | p. 371 |
| Vector Magnetometry Using the 12-[mu]m Emission Lines | p. 379 |
| Properties of Magnetic Features from the Analysis of Near-Infrared Spectral Lines | p. 393 |
| Theoretical Models of Magnetic Flux Tubes: Structure and Dynamics | p. 407 |
| The Thermal and Magnetic Structure of Sunspots | p. 423 |
| Infrared Measurements of Stellar Magnetic Fields | p. 437 |
| Near Infrared Imaging Magnetometry | p. 449 |
| Flux Tube Shredding and Its Infrared Signature | p. 459 |
| The Structure of Umbral Fluxtubes | p. 465 |
| 1.5 [mu]m Observations and the Depth of Sunspot Penumbrae | p. 471 |
| A Magnetic Field Strength vs. Temperature Relation in Sunspots | p. 477 |
| The IR Contrast of Magnetic Elements Obtained from High Spatial Resolution Observations at 1.6 [mu]m | p. 483 |
| Diagnostic Tools for Sunspots: the Molecules C[subscript 2], MgH and TiO | p. 489 |
| New Infrared Measurements of Magnetic Fields on Cool Stars | p. 493 |
| Atomic Spectroscopy in the Infrared | p. 501 |
| The ATMOS Solar Atlas | p. 511 |
| Synthetic Infrared Spectra | p. 523 |
| Line Shifts and Asymmetries in the IR Solar Spectrum | p. 533 |
| Solar Abundances of C, N, and O | p. 539 |
| Analysis of Very High Excitation Fe I Lines (4f - 5g) in the Solar Infrared Spectrum | p. 543 |
| The Sun as a Laboratory Source for IR Molecular Spectroscopy | p. 549 |
| Prospects in Adaptive Optics for Solar Applications | p. 557 |
| Solar Optical Interferometry | p. 567 |
| The Near-Infrared Capabilities of LEST | p. 579 |
| A 4-meter McMath Telescope for the Infrared | p. 589 |
| The Applicability of a 5-18 [mu]m Array Camera to Solar Imaging | p. 595 |
| Near-IR Solar Coronal Observations with New-Technology Reflecting Coronagraphs | p. 603 |
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