Homepage of NLC time-lapse movies

The following .avi-files contain NLC time-lapse movies and are fairly large (10-15 MB)

The movies are free to download and use for non-commercial purposes, obviously, with a reference to the source

Right-click to download rather then playing on-line

Stenudden, June 9-10, 2013, weak NLCs appear around 22:40

Stockholm, June 7-8, 2013, single band

Stenudden, May 24-25, 2013, weak, transient

Stockholm, Aurora March 17, 2013

Stockholm, Aurora September 19, 2012

Stockholm, July 17-18, 2012, early and strong

Stockholm, July 16-17, 2012

Stockholm, July 4-5, 2012

Stockholm, July 3-4, 2012, strong persistent

Stockholm, August 6-7, 2011, strong contrast

Stockholm, July 20-21, 2011

Stockholm, July 9-10, 2011

Stockholm, July 5-6, 2011

Stockholm, July 4-5, 2010, void

Stockholm, July 14-15, 2009, seen also from Paris

Stockholm, June 24-25, 2009, distinct

Stockholm, June 18-19, 2009

Stockholm, July 20-21, 2008

Stockholm, July 16-17, 2008, strong, first hidden

Stockholm, July 29-30, 2007, plane wave

Stockholm, July 26-27, 2007

Stockholm, June 29-30, 2007

Stockholm, July 15-16, 2006, rolling

Stockholm, July 14-15, 2006, flipped!!!

Stockholm, July 14-15, 2006

Stockholm, July 10-11, 2006

Stockholm, August 7-8, 2005

Stockholm, August 1-2, 2005

Stockholm, July 16-17, 2005, well-known

Mälarhöjden, July 16-17, 2005

Stockholm, July 10-11, 2005

Stockholm, July 19-20, 2004

Stockholm, July 15-16, 2004

Stockholm, July 14-15, 2004

To transfer




Since the summer 2004 we run a digital photo camera (Canon PowerShot G5) from the top floor window of the Arrhenius Laboratory at the University Campus in Frescati, Stockholm. The camera operates in the interval time shooting mode, taking every night hundreds of pictures of the twilight sky at the rate of 1 to 2 pictures per minute. Time-lapse movies made of these picture series for selected nights may be downloaded as .avi-files further below.

NLC occurance and brightness results obtained from these photographic observations for the last NLC-season (summer 2009) are summarised in the plot below.

The brightness and the extent of NLCs are represented here on the scale from 0 to 4 according to the following (obviously subjective) criteria: 0 = no NLC, 1 = local and weak, 2 = weak but extensive, 3 = strong but local, and 4 = strong and extensive.

To account for the visibility, tropospheric cloudiness and the presence/absence of data we use a scale from 0 to 1 in the following steps: 0 = clear skies, 0.25 = cloud patches, 0.5 = cloudy but with some openings, 0.75 = complete cloud cover, and 1 = no data. With this kind of scaling we hope it should be fairly obvious from the plot above that we are missing the data for a number of nights around day no 168 or so (June 16-18) and the reason that we do not detect NLCs around the days no 210-220 is not necessarily that they were not there, but the weather was bad and we simply cannot tell!

Contact Jacek Stegman for any further details.