Discussion Overview
The discussion revolves around the observation of small lunar haloes, specifically those within a 4-6 degree radius from the Moon. Participants explore the causes of these haloes, distinguishing them from the well-understood 22-degree halo, and consider various atmospheric conditions that may contribute to their formation.
Discussion Character
- Exploratory
- Technical explanation
- Conceptual clarification
- Debate/contested
Main Points Raised
- One participant describes observing multiple small haloes around the Moon, noting their bright central disc and darker gaps between outer circular haloes.
- Another participant suggests that the multiple haloes could result from Moonlight passing through water droplets and ice crystals at different altitudes.
- A different participant proposes that the size of the haloes may vary based on the thickness and density of cold air and moisture particles, emphasizing the roles of refraction and diffraction.
- One participant raises the possibility that the observed phenomenon could be a corona, providing links to external resources for further exploration.
- A later reply questions the relationship between droplet size and the angular size of the corona, suggesting it may relate to diffraction and comparing it to powder diffraction or scattering by colloids.
- Another participant notes that non-spherical aerosols, such as pollen, can produce non-circular rings, indicating a complexity in the atmospheric conditions affecting the observed haloes.
Areas of Agreement / Disagreement
Participants express various hypotheses regarding the causes of the small lunar haloes, with no consensus reached on a singular explanation. Multiple competing views remain regarding the mechanisms involved in their formation.
Contextual Notes
Participants mention different atmospheric conditions and the potential influence of droplet size on halo appearance, but these factors remain unresolved and depend on specific environmental conditions.