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- W2015016372 abstract "The STIP Project was instrumental in the coordination of multi-disciplinary ground- and space-based synoptic observations and analyses of solar/interplanetary events during the period covered by the Solar Maximum Year and Solar Maximum Analysis. Eight STIP Intervals for coordinated studies were conducted during the SMY/SMA period starting with STIP Interval VII (August 1979) and ending with Interval XIV (20 May – 20 July 1982). We present a summary of the significant scientific results achieved by scientists participating in these coordinated STIP studies. These results increased our understanding and knowledge of a variety of phenomena including coronal mass ejections (CMEs) and their in situ shock wave detections within 1 AU; shock physics; acceleration of particles at variously classified shocks by V × B drift and Fermi mechanisms; “magnetic clouds”; interplanetary disturbances; X-ray imaging of preflare and flare-generated CMEs, and white light imaging of CMEs during SMY by both spacecraft and ground-based instruments. In addition, scientific progress was made on the tracking of disturbances (initiated by flares, eruptive prominences, and coronal holes) into interplanetary space as well as some of their consequences as observed at 1 AU and throughout the heliosphere." @default.
- W2015016372 created "2016-06-24" @default.
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- W2015016372 date "1986-01-01" @default.
- W2015016372 modified "2023-10-16" @default.
- W2015016372 title "Scientific highlights of the Study of Travelling Interplanetary Phenomena (STIP) intervals during the SMY/SMA" @default.
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- W2015016372 doi "https://doi.org/10.1016/0273-1177(86)90174-2" @default.
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