This is data for MFRSR inst #222 at table mountain for 1995 UV intercomp. (note: inst. 221 shadowband was not shading properly so dont use 221 data). Data format: Data was processed using SUNI's callang software. Midnight to midnight binary files (ext=".mtm") are input to callang. The data are cosine corrected and written to ascii output files (ext=".ccc"). Data is cosine corrected using SUNI supplied cos correction file solar222.sol. The data in output ascci files (ext=.ccc) are ordered as follows... time stamp, cos(zenith), aux ch, global1, global2, ...global7, diffuse1, diffuse2, ...diffuse7, direct1, direct2, ...direct7. (ie 24 cols of data) notes: a) there is an extra channel of data logged on #222 (aux ch). b) time stamp is in decimal day since 1900 (GMT). c) data are in raw datalogger counts (1 count=1mV) and no absolute calibrations are given. Langley analysis on direct beam data (using callang software) produces .lang files (note: the channel number in the .lang files is labled one unit higher than the actual ch number (labled 3 --> really is ch 2; this is because of the extra ch of data being logged (aux ch)). The .lang files are in the following format: Example: date* ch pts used op. dep. Io err R R^2*Io ---------------------------------------------------------------------------- 33882.25 2 143 113 0.378201 3727.94 0.00404078 0.99943 3723.69 33882.25 3 143 107 0.238373 2895.06 0.00418622 0.99943 2891.76 33882.25 4 143 109 0.203194 2553.38 0.00354154 0.99943 2550.47 33882.25 5 143 101 0.16874 3495.77 0.00386324 0.99943 3491.79 33882.25 6 143 78 0.114075 3421.36 0.00308531 0.99943 3417.46 * date is decimal day since 1900, .25 for am langley, .75 for pm langley. The op.dep. are total optical depth numbers. The channels correspond to wavelengths as follows: Channel wavelength(nm) 2 415 3 500 4 610 5 665 6 860 7 940 Tony.