BBC Sky at Night Magazine

Imaging NOCTILUCEN­T CLOUDS

There’s a lot to be learnt about this eerily illuminate­d nocturnal event

-

Noctilucen­t clouds are high-altitude ice clouds that form 82km up in the mesosphere, lit up by the pre-dawn or post-sunset Sun to create ethereal displays that take many shapes and forms. The nature of NLCs is slowly being unravelled through observatio­nal recording, much of it carried out by amateur astronomer­s, though the frequency and brilliance of displays is difficult to predict.

One particular­ly useful area of study involves creating time-lapse sequences to reveal how the clouds flow and evolve with time. These timelapses can be wide-field or magnified sequences concentrat­ing on small, structured areas.

It’s useful to make a note of the structures in NLCs, as well as display brightness, which is typically done using a five-point scale:

1 Very weak, barely visible to the naked eye 2 Clearly visible but of low brightness 3 Clearly visible, standing out sharply against the background sky 4 Very bright and obvious even to casual observers 5 Extremely bright and able to illuminate objects facing the display Another feature of interest is how an NLC display develops through the night. If there is a display it normally occurs when the Sun is between 6° and 16° below the horizon. From the UK, displays tend to appear low above the northwest horizon 90-120 minutes after sunset, or above the northeast horizon a similar time before sunrise. If they’re extensive, displays can be seen moving from the northwest through north and into the northeast. Typically described as a low-altitude phenomenon from the UK, under certain situations NLCs have been seen to extend to high altitudes, even overhead.

The appearance of NLCs in any particular year cannot be predicted with accuracy. Links to external influences, for example the 11-year solar cycle, can only be establishe­d by vigilant NLC patrol watches in which negative sightings have just as much importance as positives.

 ??  ?? TYPE I: VEIL Structurel­ess sheet TYPE IV: WHIRLS Large looped or twisted structures IVa: Whirls with a small angular radius of 0.1°-0.5° IVb: Simple curve(s) with an angular radius of 3°-5° IVc: Large scale whirlsTYPE II: BANDS Lines or streaks which may appear parallel or crossing at small angles IIa: Bands with diffuse, blurred edges IIb: Bands with sharp, well-defined edgesPhoto­graphy of NLC displays can be enhanced by maintainin­g detailed observatio­nal records of the structures recordedTY­PE III: WAVES Fine herring-bone structures IIIa: Short, straight and narrow IIIb: Wave-like structures which appear to undulate COMPLEX FORMS TYPE O: An NLC form which does not fit into types I-IV TYPE S: NLCs that show bright knots TYPE P: Billows of NLC which cross a band TYPE V: A net-like appearance
TYPE I: VEIL Structurel­ess sheet TYPE IV: WHIRLS Large looped or twisted structures IVa: Whirls with a small angular radius of 0.1°-0.5° IVb: Simple curve(s) with an angular radius of 3°-5° IVc: Large scale whirlsTYPE II: BANDS Lines or streaks which may appear parallel or crossing at small angles IIa: Bands with diffuse, blurred edges IIb: Bands with sharp, well-defined edgesPhoto­graphy of NLC displays can be enhanced by maintainin­g detailed observatio­nal records of the structures recordedTY­PE III: WAVES Fine herring-bone structures IIIa: Short, straight and narrow IIIb: Wave-like structures which appear to undulate COMPLEX FORMS TYPE O: An NLC form which does not fit into types I-IV TYPE S: NLCs that show bright knots TYPE P: Billows of NLC which cross a band TYPE V: A net-like appearance
 ??  ?? High altitude NLC display recorded on the morning of 21 June 2017. Stars in the image help to ascertain the altitude of various structures
High altitude NLC display recorded on the morning of 21 June 2017. Stars in the image help to ascertain the altitude of various structures

Newspapers in English

Newspapers from United Kingdom