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Developments in Observations and Theory for Solar Cycle 22 Laurel, Maryland, 8-9 June 1989

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Developments in Observations and Theory for Solar Cycle 22 Laurel, Maryland, 8-9 June 1989 MA Workshop #2: Developments in Observations and Theory for Solar Cycle 22 Laurel, Maryland, 8-9 June 1989 {i<?',.., '- i _'-_'? ; ._,/ , _t MAX Workshop #2: Developments in Observations and Theory for Solar Cycle 22 Laurel, Maryland, 8-9 June 1989 Edited by Robert M. Winglee University of Colorado Boulder, Colorado Brian R. Dennis NASA Goddard Space Flight Center Greenbelt, Maryland Cover An eruptive prominence associated with the X1.6 3B flare of June 20, 1989. This event and its coronal mass ejection were well observed during the first Max '91 Campaign. This digital H-alpha image was obtained at 15:04 UT ( 4 minutes before the peak of the event in soft X-rays) by the Holloman Solar Observatory of the USAF SOON system. TABLE OF CONTENTS Preface ......................... vii Group Summaries High Energy Flare Physics Group Summary .......... ld] J. M. Ryan and J. D. Kurfess Magnetograph Group Summary ............... 17d_ H. P. Jones Theory and Modeling Group ................ 27_ G. D. Holman Summary of Observations of AR 5395 • . ° • . , , . ° , . 31c_z?:? j /I D. M. Zarro and R. M. Winglee Invited Reviews Scientific Objectives of Solar Gamma-Ray Observations ..... 33_;_/ R. E. Lingenfelter The Gamma-Ray Observatory: An Overview ......... D. A. Kniffen When and Where to Look to Observe Major Solar Flares .... 46_ T. Bai Access to MAX'91 Information via Computer Networks .... 6_. A. L. Kiplinger -7 High Energy Flare Physics Capabilities of GRO/OSSE for Observing Solar Flares . J. D. Kurfess, W. N. Johnson, G. H. Share, S. M. Matz and R. J. Murphy The Solar Gamma Ray and Neutron Capabilities of COMPTEL on the Gamma Ray Observatory ............. 755_ J. M. Ryan and J. A. Lockwood The BATSE Experiment on the Gamma Ray Observatory: Solar Flare Hard X-ray and Gamma-Ray Capabilities .... G. J. Fishman, C. A Meegan, R. B. Wilson, T. A. Parnell, W. S. Paciesas, G. N. Pendleton, H. S. Hudson, J. L. Matteson, L. E. Peterson, T. L. Cline, B. J. Teegarden and B. E. Schaefer The Solar Flare and Cosmic Gamma-Ray Burst Experiment Aboard the Ulysses Spacecraft .......... 107_t/ M. Boer, M. Sommer and K. Hurley VLA-MAX'91 Tests of High Energy Flare Physics ...... K. R. Lang and R. F. Willson First Interferometric Observations with Arc-See. Resolution of Solar Bursts at Millimeter Wavelengths ......... M. R. Kundu, S. M. White, N. Gopalswamy and J. H. Bieging Observational Goals for MAX'91 to Identify the Causative Agent for Impulsive Bursts .............. D. A. Batchelor Solar Flare Gamma-Ray and Hard X-Ray Imaging with the GRID-on-a Balloon ............... L. E. Orwig, C. J. Crannell, B. R. Dennis, R. Starr, G. J. Hurford, T. A. Prince, H. S. Hudson, F. van Beck, M. E. Greene, W. N. Johnson, J. P. Norris, K. S. Wood and J. M. Davis ii The Soft X-ray Telescope for Solar-A ......... 158 W. A. Brown, L. W. Acton, M. E. Brunet, J. R. Lemen and K. T. Strong Pre-Pulses: Signature of a Trigger Process in Short (< 60 secs) Solar Hard X-Ray Flares ............... 173_7 U. Desai and L. E. Orwig Theory and Modelling Flare Model Sensitivity of the Balmer Spectrum ....... A. Falchi, R. Falciani, L. A. Smaldone and G. P. Tozzi Joule Heating and Runaway Electron Acceleration in a Solar Flare ..................... G. D. Holman, M. R. Kundu and S. R. Kane Heating and Acceleration of Coronal and Chromospheric Ions During Solar Flares .................. M. E. McKean, R. M. Winglee and G. A. Dulk Chromospheric-Coronal Coupling During Solar Flares: Current Systems and Particle Acceleration ....... 2195. _ / R. M. Winglee, M. E. McKean and G. A. Dulk Development of a Numerical Solution to the Time Dependent Kinetic Equation ................... R. J. Hamilton, E. T. Lu and V. Petrosian Observations of AR 5395 Some of the Terrestrial Effects of A R 5395 ......... 233. D. Speich 10.7-cm Microwave Observations of AR 5395 and Related Terrestrial Effects ................ 242 V. Gaizauskas, T. J. Hughes, and K. F. Tapping 111 Interplanetary Energetic Particle Observations of the March 1989 Events ..................... 246_;_ _-. E. T. Sarris and S. M. Krimigis SMM UV Observations of Active Region 5395 ........ 248 _, S. A. Drake and J. B. Gurman XRP Observations of AR 5395 .............. 259 _. , G. Slater Hard X-Ray Highlights of AR 5395 ............ R. A. Schwartz and B. R. Dennis SMM-GRS Observations of AR 5395 ............ D. J. Forrest Observations of AR 5395 in Coronal Emission Lines ..... 281 :j :: R. C. Altrock Ha Imaging Spectroscopy of March 1989 Flares ....... J.-P. Wiilser and R. C. Canfield Optical Observations of A R 5395 ............. 295 D. Neidig Magnetograph Observations from AR 5395 from NSO/Kitt Peak ................... 297 _ H. P. Jones BBSO coverage of AR 5395 ................ 299 H. Zirin Owens Valley Observations of AR 5395 .......... 30!_ G. Hurford RSTN Observations of the 06 and 10 March 1989 Solar Flares ..................... 306., , E. W. Cliver and L. C. Gentile iv Observatory Reports Investigation of Active Regions at High Resolution by Balloon Flights of the Solar Optical Universal Polarimeter (SOUP) 310 5_ T. Tarbell, Z. Frank, C. Gilbreth, R. Shine, A. Title, K. Topka and J. Wolfson The Onset of the Solar Activity Cycle 22 .......... H. S. Ahluwalia An Imaging Vector Magnetograph for the Next Solar Maximum: A Progress Report ............. 324_ D. L. Mickey, B. J. LaBonte and R. C. Canfield The Owens Valley Solar Array .............. G. J. Hurford and D. E. Gary The HAO/NSO Advanced Stokes Polarimeter ........ B. W. Lites and D. F. Elmore Observing Facilities for MAX'91 at NSO/Kitt Peak ..... 342 -_ H. P. Jones New Instrumentation at NSO/Sac Peak ........... 344 R. N. Smartt A High-Speed Digital Camera System for the Observation of Rapid Ha Fluctuations in Solar Flares ......... 346 A. L. Kiplinger Analysis of Video Spectra-Spectroheliograms from the San Fernando Observatory .............. 349:,"_-._.... G. A. Chapman and S. R. Walton Limb-Occulted Microwave and X-ray Flares ........ 353 E. J. Schmahl, M. R. Kundu, J. Tappin and G. Simnett V VLA Capabilities for MAX'91 ............... 355 _,/_ K. R. Lang Status Report for the MAX'91 Campaign from the Ottawa River Solar Observatory ................ 361 " V. Gaizaukas Mees Solar Observatory, University of Hawaii ........ 363 R. C. Canfield Radio Observatory BLEIEN of ETH Zurich, Switzerland . 364 _ M. J. Aschwanden and A. O. Benz Research at C.U. related to MAX'91: Observational ..... 365 _ G. A. Dulk vi PREFACE More than 100 scientists attended the second workshop of the Max '91 program held at the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, on June 8 and 9, 1989, in conjunction with the meeting of the Solar Physics Division of the American Astronomical Society. The success of the workshop was due in large part to the excellent facilities at the Kossiakoff Center of the Johns Hopkins Applied Physics Laboratory and the support of the local organizing committee chaired by David Rust. The purpose of the Max '91 program is to gather coordinated sets of solar flare and active region data and to perform interpretive and theoretical research aimed at un- derstanding flare energy storage and release, particle acceleration, flare energy transport, and the propagation of the flare effects to Earth. Instruments for long-duration balloon flights are being funded by NASA and ground-based instruments are being funded by NSF. Coordination of Max '91 observations is being carried out by Alan Kiplinger at the Space Environment Laboratory in Boulder, CO. The Max '91 program is part of the SCOSTEP sponsored international FLARES 22 program led by Marcos Machado (Argentina) and Ernest Hildner (USA). Four discussion groups were organized during the workshop on the following sub- jects: high-ener_ flare physics, coordinated magnetograph observations, flare theory and modelling, and Max '91 communications and coordination. A special session also took place on observations of Active Region 5395 and the associated flares during March 1989. These proceedings of the workshop contain the group leaders' summaries of the discussions that took place in the different group meetings, papers resulting from the contributed oral and poster presentations, and outlines of talks that were presented by invited speakers on topics such as the scientific objectives of solar gamma ray observations, the solar capabil- ities of each of the four instruments on the Gamma Ray Observatory, and access to Max '91 information. Discussions focussed on developments in observations and theory, particularly in relations to plans for future space, rocket, balloon, and ground-based observations and their coordination, and theoretical questions relevant to the Max '91 program. The mag- netograph group discussed observations made during the International Solar Month on September 16 and 17, 1988, when observatories around the world participated in com- parative magnetograph observations of active regions AR 5148, 5105, and 5106. Clear difficulties were identified in calibrating measurements from the different observatories. Recent observations of the March '89 Active Region 5395 were presented. This active region was one of the largest flare producing active regions on record with 11 class vii X flares and 48 class M flares. Four great geomagnetic storms were produced by flares associated with the active region; one of these storms caused the Hydro-Quebec power sys- tem to fail. Preliminary results detailing these and other terrestrial effects were presented. Ground-based and satellite observations were also presented showing some of the unique characteristics of the active region and its associated flares. Capabilities of future observations from several new satellite and balloon instru- ments and their impact on solar physics were discussed in the high energy flare physics group. The satellites include the Gamma Ray Observatory, SOLAR-A, and Ulysses; the balloon instruments include GRID and SOUP. Scientists from many of the ground-based observatories also gave presentations of new facilities.
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