In particular, it is essential to connect the magnetohydrodynamic (MHD) wave processes with the small and large-scale solar phenomena vis-a-vis transport of energy and mass. The understanding of solar atmospheric dynamics requires hi-resolution modern observations which, in turn, further advances theoretical models of physical processes in the solar interior and atmosphere. ![]() These phenomena strongly influence interplanetary plasma dynamics and contribute to space-weather. The Sun is our nearest star and this star produces various plasma wave processes and energetic events. ![]() Preface: MHD wave phenomena in the solar interior and atmosphere We propose that stable, long-term funding, and thorough investigation of poorly understood and/or unexplored luminous phenomena occurring in the low atmosphere could lead to the creation of new inter-disciplinary research programs in multiple universities, and ultimately, to important fundamental discoveries in the field of atmospheric science, photonics and beyond. Here, we present the results of a survey indicating a significant support from a subset of the academic community to investigate rare, unusual and unexplained atmospheric light phenomena that have historically been unexplored by scientists — the transient luminous phenomena in the valley of Hessdalen in Norway in particular. To investigate or not to investigate? Researchers' views on unexplored atmospheric light phenomenaįor hundreds of years, scientists have been studying light, which is used nowadays to explore the universe and cure diseases. The state of knowledge of long-lived light phenomena in the atmosphere is reviewed in the light of contributions to the International Interdisciplinary Congress on Unsolved Problems of Atmospheric Electricity, September 1993, Salzburg, Austria and the First International Workshop on Unidentified Atmospheric Light Phenomena, March 1994, Hessdalen, Norway. ![]() CONFERENCES AND SYMPOSIA: Long-lived light phenomena in the atmosphere
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