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Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 1

Investigation of Light Pollution in

the Republic of Croatia

Željko Andreić1, Doroteja Andreić, Ana Bonaca, Korado Korlević, Petra Korlević, Mirna Kramar

Višnjan Education Center, Istarska 5, 51463 Višnjan, Croatia

1speaker, permanent address: Faculty of Mining, Geology and Petroleum Eng., University of Zagreb, Pierottijeva 6,

10 000 Zagreb, Croatia, E-mail: zandreic@rgn.hr

Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 2

Overview

1. Introduction

2. A short history of our efforts in Croatia

3. LP monitoring methods

4. Modeling

5. Results and conclusions

Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 3

Croatia

Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 4

A short history of our activities

1992: first popular articles about LP

1998: Višnjan obs. starts to discover

new asteroids

2001: LP blocks Visnjan obs.

asteroid program after approx 1350

discoveries

2002-3: first attempts to measure LP

in Istria

2006--: systematic measurements

and modelling

2002.

2003.

Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 5

A short history of our activities 2 (2006-7)

10%

40%30%

20%

fireflies live only here

Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 6

Monitoring methods: Sky quality meter

Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 7

Monitoring methods: all-sky cameras

Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 8

Satellite imaging (Cinzano at al.)

Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 9

Satellite imaging + modelling (Cinzano at al.)

Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 10

Statistical model (M. Walker 1966.-1977.)

Population cenzus + Walker's law:

D N

Ad_Bright=const×N×D-2,5

Ad_Bright??

Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 11

Shadowing correction (Albers et al. 2001)

corr = exp-(h/A)

typically, A = 4000 m

h

A

Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 12

Statistical model versus satelite imaging model

Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 13

LP map of Croatia

Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 14

LP map of

Croatia

Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 15

Results: "top 10" in Croatia

20,520,420,810. Japetić vrh

20,519,520,89. Kanfanar

19,520,420,98. Novigrad podravski

21,020,921,07. rt Kamenjak

21,020,921,06. Savičenta

20,520,921,15. Tičan

20,520,421,14. Japetić kamenolom

21,520,921,33. Vela Luka suburb

21,520,921,32. Korenica

21,521,721,81. Lastovo

Cinzano et al. prediction

model prediction

SQM measurement

location

Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 16

Results: "top 10" in Croatia

1

2

3

4,10

567

8

9

Vienna 2008: Investigation of Light Pollution in the Republic of Croatia 17

Conclusions

1. Walker's model and satelite imaging model are in agreement,

but Walker's model provides better resolution and is easier to

construct.

2. SQM is unusable near open lights, SQM-L is much beter in this

aspect. Measurements in rural areas in agreement with models,

SQM is very simple to use.

3. Places with minimum LP limited to southern Adriatic islands,

Llika and Gorski kotar and a few small spots far from cities in

other areas.

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