The new world atlas of artificial night sky brightness
by Fabio Falchi, Pierantonio Cinzano, Dan Duriscoe, Christopher C. M. Kyba, Christopher D. Elvidge,
Kimberly Baugh, Boris A. Portnov, Nataliya A. Rybnikova, Riccardo Furgoni
New Brunswick, Canada: Grade 8 students Holly Ayles and Emily Baxter are national winners in the recent
International Statistical Literacy Poster Competition.
Their poster will go to international level in Dublin Ireland later in August.
SQM user Henk Spoelstra of Lumineux Consult
has set up a network of SQM-LE units to monitor sky brightness in the Netherlands. You can view his nomograph of light pollution factor
and readings plot here.
Clear Sky Detection experiment
Here is an experiment to try to identify a clear sky using the SQM-LE/LU by observing the fluctuations in light level caused by clouds.
A Survey of Light Pollution in Hong Kong.
Researchers at the Department of Physics of The University of Hong Kong completed their light pollution survey and collected near 2,000
night sky brightness data sets from SQMs at more than 220 observation sites
around Hong Kong during the past 15 months.
Full report here.
GLOBE at Night: Shed Light on Light Pollution!
Connie Walker of the NOAO discusses the Globe at Night project as part of the 365 days of astronomy during the Year of Astronomy.
Knightware, makers of "Deep-Sky Planner", have released
SQM Reader Pro
for Windows and the SQM-LE. This low-cost package adds graphing, statistical
calculations, extended data storage and transmission capabilities to the
basic feature set of existing "SQM Reader" software.
A survey of light pollution in Hong Kong
using various tools including the Sky Quality Meter
Sky Quality Meter - LU-DL-V
"You've got to kick at the brightness 'til it bleeds starlight."
- with apologies to Bruce Cockburn
A USB enabled vector data-logging light meter for night-time sky brightness monitoring!
An affordable meter for continual, connected or autonomous data-logging to measure sky brightness for astronomers and light pollution investigators.
The "Sky Quality Meter - LU-DL-V" (SQM-LU-DL-V) measures the brightness of the night sky in magnitudes per square arcsecond.
Designed by Dr. Doug Welch and Anthony Tekatch
- Measuring the night sky brightness during remote biological field experiments.
- Find out how good the night or site REALLY is.
- Compare the sky brightness at different sites quantitatively.
- Document the evolution of light pollution in your area.
- Set planetarium dome illumination to mimic the skies people are likely to experience elsewhere in the city.
- Monitor sky brightness through the night, night-to-night, and year-to-year.
- Determine which nights show the greatest promise for finding the 'faintest fuzzies'!
- Calibrate the effect of sky brightness on qualitative measures such as the Bortle Scale.
- Investigate how sky brightness correlates with the solar cycle and month-to-month sunspot activity.
- Help provide local ground truth for future sky brightness prediction with the Clear Sky Clock.
- CCD users can make a correlation between the SQM reading and when the background reaches some ADC level.
SQM-LU-DL-V UDM contour plot
- Sky brightness reported in visual magnitudes per square arcsecond.
- Infrared blocking filter restricts measurement to visual bandpass.
- Sensor temperature, model number, and serial number are provided.
- Precision readings at even the darkest sites.
- Field-upgradeable firmware.
- All the features of our SQM-LU (USB model) plus Data logging capabilities and vector measurements.
- Open protocol document.
- USB connectivity.
- Data-logging capabilities while operated from external battery.
- Vector measurements of Altitude and Azimuth (built-in accelerometer/compass module).
- Included applications for reading data in Perl.
- The Half Width Half Maximum (HWHM) of the angular sensitivity is ~10°. The Full Width Half Maximum (FWHM) is then ~20°. The sensitivity to a point source ~19° off-axis is a factor of 10 lower than on-axis. A point source ~20° and ~40° off-axis would register 3.0 and 5.0 magnitudes fainter, respectively.
The "V" model comes with an improved lens/filter arrangement, see the comparison to the standard "L" model here.
- Size 5.5 x 2.6 x 1.1 in.
- Maximum light sampling time: 80 seconds.
- Minimum light sampling time: 1 seconds.
Battery adaptor fashioned like a handle for easy use in field during all sky surveys.
3D part view.
Specifications are subject to change without notice.
- The compass readings are very sensitive to any nearby hard and soft iron. The unit works well by hand operation as shown above.
- There is a slight magnetic offset (pinched and stretched at ≈±5° in some directions) due to internal components which have yet to be compensated
for in the UDM software, but the compensation is planned for a future release of UDM.
- The lens/filter arrangement has been improved over our standard "L" models. A comparison with the new UVIR650 IR Filter and half-ball lens can be found here. spectral response.
What you get:
- SQM-LU-DL-V unit
- SQM-LU-DL-V users manual
- CD with PDF manual and example software
- 15ft USB cable
- Battery-to-USB adapter with 4 AA cells and battery holder
- Calibration sheet indicates unit USB serial number, and calibration values
Ready to buy?
Price $339.99US plus Shipping & Handling.
Reports including the SQM:
Light pollution maps / databases:
Useful Light pollution links:
- Night Sky Photometry with Sky Quality Meter
by Pierantonio Cinzano.
- "Contributions of artificial lighting sources on light pollution in Hong Kong measured through a night sky brightness monitoring" article by
Chun Shing Jason Pun, Chu Wing So, Wai Yan Leung, Chung Fai Wong.
- Human Contrast Threshold and Astronomical Visibility paper by Andrew Crumey.
- Report on sky colour: Red is the new black; Chris Kyba and colleagues
- Documenting Local Night Sky Brightness report, Jennifer Birriel of MSU.
Measure Night Sky Brightness at Various Zenith Angles report, Jennifer Birriel of MSU.
- "Night sky photometry and spectroscopy performed at the Vienna University Observatory" published in the "Journal of Quantitative Spectroscopy and Radiative Transfer"
- "The night sky brightness at Potsdam-Babelsberg including overcast and moonlit conditions" published in the
"Journal of Quantitative Spectroscopy and Radiative Transfer"
- "Worldwide variations in artificial skyglow" by Christopher C. M. Kyba, Kai Pong Tong, and more.
Published in Nature.com : Scientific Reports.
- "Intercomparisons of Nine Sky Brightness Detector"
by Peter den Outer, Dorien Lolkema, Marty Haaima, Rene van der Hoff, Henk Spoelstra, and Wim Schmidt.
Published in 2014 The National Center for Biotechnology Information.
- Calibration of SQM-L photometers for the NixNox project,
Zamorano Calvo, Jaime and Munoz Marín, Victor Manuel (2010),
Zamorano, Jaime y Munoz Marin, Victor Manuel (2010),
Calibration of SQM-L photometers for the NixNox project. [ LICA report; no. #01],
- Zamorano, Jaime & Ruiz Carmona, Roque (2013),
Sky Quality Meter cross-calibration for the NixNox project. [ LICA report; no. #03],
- Nievas Rosillo, Miguel & Zamorano, Jaime (2014),
*PySQM the UCM open source software to read, plot and store data from SQM photometers*,
- Zamorano, Jaime, Sanchez de Miguel, Alejandro, Martinez Delgado, David & Alfaro Navarro,
Emilio (2011) Proyecto NixNox disfrutando de los cielos estrellados de Espana. Astronomia (142). pp. 36-42. ISSN 1699-7751,
- Zamorano, Jaime, Sanchez de Miguel, Alejandro, Nievas Rosillo, Miguel & Tapia Ayuga,
Carlos (2014) NixNox procedure to build Night Sky Brightness maps from SQM photometers observations.,
- A night sky brightness network with data obtained with fixed SQM photometers of the Spanish Light Pollution Research Network.
- "Initial Irish light pollution measurements and a new Sky Quality Meter-based data logger"
by B Espey, PhDa,b, and J McCauley, MSca.
Published on February 2014 vol. 46 no. 1 67-77.
Lighting Research and Technology.
- Excursion to Dark Sky Preserves in Canada 2015
by Andreas Hänel.
- SQM cross-calibration procedure by the BuioMetria Partecipativa team, 2011
Poster on the BuioMetria Partecipativa project presented at the IAU 2012 General Assembly in Beijing.
- Dark box for low-light-level measurements of a camera using an SQM-LU PDF
by Peter Hiscocks.
- Integrating Sphere for Luminance Calibration PDF
by Peter Hiscocks.
- Birds advance their dawn chorus near airports
Report uses SQM to assist in determining bird chorus timing due to other effects. By Diego Gil et al.
- Comprehensive list of SQM related reports found on 2017-02-17.
Quantifying and Monitoring Darkness over the RAO (Rothney Astrophysical Observatory)
By Phil Langill and Benjamin George.
Temperature Stability of the Sky Quality Meter
By by Sabrina Schnitt, Thomas Ruhtz, Jürgen Fischer, Franz Hölker, Christopher Kyba.
SQM-LU-DL tripod adaptor option
This adaptor kit was designed specifically for the SQM-LU-DL meter which is longer than our other meters.
The adaptor screws into the back of the SQM-LU-DL and allows the meter to be mounted on a tripod with a 1/4-20 thread.
The kit includes one tripod adaptor, 3D-printed plastic,
and two longer screws (to replace two short screws already in the meter) 3D part view.
Note: The built in compass on the SQM-LU-DL-V (Vector meter) is very sensitive to hard and soft iron.
You may notice variations in the Azimuth (compass reading) while mounted to a metal tripod.
Also, brass screws (that come with the SQM-LU-DL-V-battery holder) must be used to secure the adaptor to the SQM-LU-DL-V.
You may also be interested in; the SQM-LE/LU housing, or our low-cost handheld sky meter (SQM),
or our narrow-field handheld sky meter (SQM-L),
or our Ethernet conected sky meter (SQM-LE).