SELECTED PUBLICATIONS

***** Journal Articles *****

• The Structure of the Coronal Soft X-ray Source Associated with the Dark Filament Dissappearence of September 28, 1992 using the Yohkoh Soft X-ray Telescope. McAllister, Uchida, Tsuneta, Strong, Acton, Hiei, Bruner, Watanabe, and Shibata, PASJ, 1992.
• The Continual Expansion of Active Region Corona Observed by the Yohkoh Soft X-ray Telescope. Uchida, McAllister, Strong, Ogawara, Shimizu, Matsumoto, and Hudson, PASJ 44(5), 1992.
• A Filament Eruption on November 5, 1992: Comparison of SXT and Ha. McAllister, Kurokawa, Shibata, and Nitta, Solar Phys. 169, 1996.
• A Large Polar Crown CME and a "Problem" Geomagnetic Storm: April 14-23, 1994. McAllister, Dryer, McIntosh, Singer, and Weiss, JGR, 101, 1996.
• Coronal Mass Ejections, Co-rotating Interactive Regions, and Geomagnetic Storms. McAllister and Crooker, in Coronal Mass Ejections: Causes and Consequences, 1997.
• Predicting the Sign of Helicity in Erupting Filaments and CMEs. Martin and McAllister, in Coronal Mass Ejections: Causes and Consequences, 1997.
• Identification of the Solar Drivers of the 3-4 November 1993 Geomagnetic Storm. McAllister, Knipp, Crooker, Mukai, and Kokubun, JGR, 1998.
• An Overview of the Early November 1993 Geomagnetic Storm. Knipp, Emery, Engebretson, Li, McAllister, Mukai, Kokubun, Reeves, Evans, Obara, Pi1, Weatherwax, McHarg, Chun, Codrescu, Lanzerotti, Rich, Wilkinson, Lazarus, Lepping. JGR, 1998.

***** Proceedings Papers *****

• Quiet Region Magnetic Inversion Line Restructurings. McAllister, Uchida, Khan, Hirayama, Shibata, Hiei, Watanabe, and Harvey, Yohkoh 1st Year Symposium, 1992.
• Long Time-Scale Coronal Dynamics Revealed by Yohkoh. Uchida, McAllister, and Khan, Yohkoh 1st Year Symposium, 1992.
• Coronal Magnetic Fields Parallel to Magnetic Polarity Inversion Lines. McAllister, Uchida, Khan, and Shibata, Intern. Yohkoh Seminar, 1994.
• Quadrapole Magnetic Field in Arcade-type Flares. Uchida, McAllister, Khan, Sakurai, and Jockers, Intern. Yohkoh Seminar, 1994.
• A Large Polar Crown CME and A Severe Geomagnetic Storm: April 14-17, 1994. McAllister, Dryer, McIntosh, Singer, and Weiss, SOHO III, and SOLTIP II, 1994.
• The Large Scale Coronal Eruptive Event of April 14, 1994. Alexander, Slater, Hudson, McAllister, and Harvey, SOHO III,1994.
• Declining Phase Coronal Evolution: The Statistics of X-ray Arcades. McAllister, Hundhausen, Burkepile, McIntosh, and Hiei, IAU 153,1996.
• The Skew of X-ray Coronal Loops Overlying Ha Filaments. Martin and McAllister, IAU 153, 1996.
• The Relation of Yohkoh Coronal Arcades to Coronal Streamers and CMEs. McAllister and Hundhausen, ASP Conf. Ser. Vol 95, 1996.
• The Skew of Polar Crown X-ray Arcades. McAllister, Hundhausen, MacKay, and Priest, IAU 167, 1998.
• Axial Soft X-ray Brightening Associated with Ha Filaments. Solberg and McAllister, IAU 167, and SOHO V, 1998.
• The Essential Role of Magnetic Reconnection in the Release of Erupting Prominences, McAllister and Martin, COSPAR, Adv. Space Res., 2000.

Last updated February 26, 2001. © Alan McAllister.