Solar Activity Signatures in Mesopause Region Temperatures and Atomic Oxygen Related Airglow Brightness at El Leoncito, Argentina

SCHEER, J.; REISIN, E.; MANDRINI, C.H.

Praga

Workshop; IAGA/ICMA 3rd Workshop on Solar Forcing of the Middle Atmosphere; 2003

International Association of Geomagnetism and Aeronomy

Rotational temperatures and airglow brightness variations of the OH(6-2) and O2(0-1) bands measured at El Leoncito (32S, 69W) from 1998 to 2002 are analyzed to detect solar activity signatures. The emissions correspond to nominal altitudes of 87 and 95 km, respectively. The homogeneous and consistent data set covers the rise, the two distinct maxima, and the start of the decline of the present solar activity cycle. The modulation of solar activity around the Gnevyshev gap (particularly pronounced in this cycle) has been so strong as to motivate the expectation to detect its signature in such a relatively short data set. While at 87 km, there is practically no correlation (with sunspot number, radio, or EUV flux), neither in temperature nor in OH intensity, we find a moderate positive temperature and airglow brightness effect at 95 km. This is a remarkable difference, in view of the small separation between the two altitude levels. The quantitative results lie close to the lower limits of our previous estimates in the context of a recent trend analysis. However, during the years 1999 and 2000, the correlation was very strong. From the standpoint of atmospheric nonlinear dynamics, variations in the degree of correlation in different years and at different observing sites should not be surprising. Therefore, our results are not necessarily inconsistent with findings by other investigators.