CONTENTS OF THE FILE phemu91.data.txt Contents: planet 5 - Jupiter satellites: J1 J2 J3 J4 total number: 375 observations of 111 events type: photometric observations dates: observed from november 1990 until march 1991, observatories: these events are observed from 55 sites, References: These observations are described in, . for the observations from the PHEMU91 campaign: Arlot, J.-E., Barroso J. Jr, Berthier, J., Blanco, C., Bouchet, P., Bourgeois, J., Bulder, H.J.J., Burchi, R., Casas, R., Chis, D., Colas, F., Colin, J., D'Ambrosio, V., De Angelis, De Benedetto, G., Denzau, H., Descamps, P., Di Paolantonio, A., Federspiel, M., Froeschle, M., Gomez-Forellad, J.M., Hainaut, O., Helmer, G., Hube, D., Kidger, M., Lecacheux, J., Lefloch, J.C., Mallama, A., Martin, B.E.,Mellilo, J.F., Meyer, C.,Molau, S., Morando, B., Nicolet, B., Oprescu, G., Protitch- Benishek, V., Rapaport, M., Riou, A., Ruatti, Ch., Sevre, F., Shkodrov, V, Souchay, J., Takami, T., Tholen, Thuillot, W., Vasundhara, R., Vu, D.T., White, G., Wilds, R.P., Yoshiharu, I.:1996, "A catalogue of the observations of the Jovian mutual phenomena of made in 1991 during the PHEMU91 Campaign", 1997, Astron. Astrophys. Suppl. Ser. 125, 399. . for the observation made at Kavalur Observatory (India) on September 3, 1991: Vasundhara, R., 1997, private communication. The lightcurve of this event is in the file: dvbo0752o1.093 . Format: This is a sequential file with a recordsize of 93 bytes wih a following format, - the date of the minimum of the light curve in UTC (year,month,day,hour,minute,second) I4,5I2, - the code of event A4, - the error on the date of the minimum in seconds A6, - the magnitude drop in magnitude unit F7.3, - the error on the magnitude in magnitude unit F5.3, - the C-O in seconds from the ephemerides G-5 I5, - the observational site A5, - the code of the observers A3, - the code of the instrument L, T ou X A1, - the aperture in centimeter I3, - the code of receptor A6, - the filter used A5, - the integration time in seconds A5, - the size of the diagragm when used A5, - the number of satellites in the diaphragm A5, - the distance to Jupiter in jovian radii F5.1, - the elevation of Jupiter in degrees I3, - the elevation of the Sun in degrees I3, - the codes for the observational conditions I2, Code of event: in the format, xMyC, as, - x, occulting or eclipsing satellite - M, type of event O, for Occult E, for Eclipses - y, occulted or eclipsed satellite - C, Category of event, P, Partial event T, Total event A, Annular event B, eclipse by penumBra G, Grazing occultation Code of the observers: cf. reference paper Code of the instrument: L, refractor T, reflector X, unknown Code of receptor: cf. reference paper Code for the observational conditions 0 = unknown conditions 1 = very good observational conditions 2 = acceptable observational conditions 3 = difficult observational conditions Comments: The photometric lightcurves are at the address: ftp://ftp.imcce.fr/pub/NSDC/jupiter/raw_data/phenomena/mutual/1991/ Contents: - 375 observations of 111 events observed from 55 sites from november 1990 until march 1991 - each light curve corresponding to each observation, - the light curves are provided in the files dXXXXaammjj.dat where XXXX is the coded name of the site of observation on 4 characters, aammjj, la date. Format: The lightcurves are provided in the files d.... with the following format, - first line: event, date, site of observation, number of points, - third line: longitude and latitude de of the observatory, the longitude is counted in hours and decimal fraction counted positively towards WEST (format F10.6), the latitude is counted in RADIANS counted positively towards north (format F9.7), - line 5 and next: hour minute second in UTC, magnitude drop ==============================================================================