Jupiter’s atmosphere is generally organized in dark belts and bright zones the presence, latitudinal limits, color and intensities of which are changeable [1]. The study of these changes may reveal…
Results (15/04/2015): Announcement (13/12/2015): The structure and variability of the upper atmospheres of the giant planets may be investigated by occultation techniques [1]. Ground-based photometric monitoring of stellar occultations measure…
Polar caps: Both caps look bright, the south cap is brighter, and the north cap more extended than the south cap. SSTB: The white Ovals look bright. The…
During the European Planetary Science Congress 2013 (Sep 8-13, 2013, London, UK) we presented the following work: Digital daylight observations of the planets with small telescopes Emmanuel (Manos) I. Kardasis…
