Date: Wednesday, January 17, 1996 Time: 4:15 PM ­ Refreshments at 4:00 Location: ERL 126 Optical Observations of Storm Induced Optical Phenomena in the Upper Atmosphere: Sprites and ELV-s S.B. Mende Lockheed Martin Palo Alto Research Laboratory, Palo Alto, CA 94304 Abstract Recent video camera observations of atmospheric regions above thunderstorms show several optical features. In the past few years since the discovery of these features, considerable advances have been made towards understanding some of the key mechanisms responsible for their production. These and related phenomena provide evidence for electrical coupling between the lower atmosphere and the ionosphere. The frequently occurring vertically oriented "Sprites" (spanning the 50-90 km region) are thought to be caused by the quasi-static electric fields which are set up after a large lightning flash discharges the thunder cloud, leaving a high potential between the cloud and the ionosphere. The horizontally elongated faint ELV-s are driven by the large electromagnetic field pulses which are emitted from intense lightning discharges. In the summer of 1995 the Lockheed Martin Palo Alto Research Laboratories participated in the "Sprites 95" campaign and have taken low light level video images of Sprites and ELV-s. These images reveal many interesting morphological features of the phenomena, including measurement of their spatial extents. The Lockheed low light level imaging spectrograph documented some of the first spectra of Sprite-emitted light. These spectra showed that most of the electrons causing the excitation of the light in Sprites have only a few eV of energy. Light detected in the scanning register of one of the CCD cameras used in the 1995 field campaign showed that brighter features such as Sprites produced streak images which could be measured and that the time structure of Sprites could be obtained with a resolution of 60 microseconds. This allowed the studying of the temporal behavior pattern of Sprites. Many of the images show that ELV-s often accompany Sprites, but they sometimes occur by themselves. Several key questions still remain unanswered concerning the Sprites and ELV-s: What are their spectral and altitude profiles, and how do they show the changing of processes with altitude? Are there any other spectral features besides N21PG and (if so) what are the relative intensities of these other emissions compared to the N21PG? What is the direction of development or decay of the Sprite in the vertical direction? Does it start at the ionosphere? What governs the spatial form of Sprites? Is there a credible mechanism for the generation of gamma rays by Sprites, ELV-s or related phenomena?