sebastijan mozetič, jože rakovec, nedjeljka Žagar ... · conclusions • behind any observations...

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Conclusions Behind any observaons there are errors involved in making it. Clouds sing on the mountain top can tell the story of winds behind and above the mountains. Satellites are able to observe clouds with good resoluons. Bora speeds in the valley are 2 mes greater than on the slopes. Current weather models forecast average speeds of bora but can not forecast its gusts. Bora variaon along the valley basin are not significant. Impressions Bora simulaons SPACE-SI in collaboraon with Chair of Meteorology FMF UL has its own operaonal weather forecast on 3.7 km spaal resoluon with WRF-ARW model (hp://vreme.space.si). A special model setup was prepared for this project, fo- cusing on the Vipava valley region and using higher resoluon (1.2 km). Model forecasts have been com- pared with bora observaons. New observaons Nika: “Bora is a part of my life since the birth and I have always taken it as a self-evident fact of our lifes. The project enabled me to understand how bora develops and how we can use physics and mathemacs to understand and fore- cast its occurrence.Mirjam: “As a child, I though bora is everywhere and I was not aware it is a specialty of our valley. The project has tought me how different factors work together to make the unique climate of the Vipava valley.Andraž: “I am glad that I could parcipate in the project. To- gether we came up with interesng findings. In addion, I also improved my knowledge of Excell.Model verificaon Comparison of model outputs and DARS staons shows that the model predicts bora occurrence, evoluon and average speeds well. However, the model is not capable to represent bora gusts. 0 5 10 15 20 25 0:00 1:00 2:00 3:00 4:00 5:00 6:00 7:00 8:00 9:00 10:00 11:00 12:00 13:00 14:00 15:00 16:00 17:00 18:00 19:00 20:00 21:00 22:00 23:00 Wind speed [m/s] Hour Zemono, 10.2.2012 Model Measurements 0 5 10 15 20 25 0:00 1:00 2:00 3:00 4:00 5:00 6:00 7:00 8:00 9:00 10:00 11:00 12:00 13:00 14:00 15:00 16:00 17:00 18:00 19:00 20:00 21:00 22:00 23:00 Wind speed [m/s] Hour Ribnik, 10.2.2012 Model Measurements Model representaon of the Vipava valley and surrounding orography. We analyzed new observaons from 5 instruments along two measurement lines. Horizontal distance between the instruments is about 1.5 km. Bora measurements from 10 February 2012 illustrate the main findings: all observaons contain high-frequency variability, typical for bora (bora gusts), along A line bora strength doubles from A01 towards A02 over 1.5 km horizontal and 100 m vercal distance, in the valley average bora speed does not vary from one side to another. Other staons Locaons of the DARS (Slovenian motorway company) measurement sites along the highway H4 through the Vipava valley. 0 5 10 15 20 25 0:00 1:00 2:00 3:00 4:00 5:00 6:00 7:00 8:00 9:00 10:00 11:00 12:00 13:00 14:00 15:00 16:00 17:00 18:00 19:00 20:00 21:00 22:00 23:00 Wind speed [m/s] Hour Line A, 10.2.2012 A1 A2 A3 0 5 10 15 20 25 0:00 1:00 2:00 3:00 4:00 5:00 6:00 7:00 8:00 9:00 10:00 11:00 12:00 13:00 14:00 15:00 16:00 17:00 18:00 19:00 20:00 21:00 22:00 23:00 Wind speed [m/s] Hour Line B, 10.2.2012 B1 B2 SLOVENIA AUSTRIA CROATIA H ITALY N 0 25 50 km The most important bora property is its gusness. We studied bora gusts by using new observa- ons collected during the four-month period in 2012. On less than 2 km distance, bora velocity more than doubles. We compared bora forecasts of the SPACE-SI prognosc model with the ob- servaons to show that current forecast models lack the ability to describe the bora gusness. Example of the Adriac bora forecast by SPACE-SI model valid for 10.2. 2012 at 19.00. Bora in Vipava Valley Analysis of Observaonal and Forecast Data SECONDARY SCHOOL Diocesan Gymnasium Vipava Small Satellites Systems and Services - The 4S Symposium 2012 Portorož, Slovenia, 4-8 June 2012 AUTHORS: Nejc Povšič, Andraž Jurinčič, Rok Žorž, Ana Čufer, Nika Obed, Mirjam Mileč, Krisjan Zorn, Domen Rabak, Rok Miklavčič, Benjamin Smrdel, Dominik Vrčon SUPERVISORS: Nadja Pregeljc, Vladimir Anžel, Sebasjan Mozeč, Jože Rakovec, Nedjeljka Žagar, Rahela Žabkar, Gregor Skok, Luka Honzak, Vanja Blažica

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Page 1: Sebastijan Mozetič, Jože Rakovec, Nedjeljka Žagar ... · Conclusions • Behind any observations there are errors involved in making it. • Clouds sitting on the mountain top

Conclusions• Behind any observations there are errors involved in making it.• Clouds sitting on the mountain top can tell the story of winds behind and above the mountains.• Satellites are able to observe clouds with good resolutions.• Bora speeds in the valley are 2 times greater than on the slopes.• Current weather models forecast average speeds of bora but can not forecast its gusts.• Bora variation along the valley basin are not significant.

Impressions

Bora simulationsSPACE-SI in collaboration with Chair of Meteorology FMF UL has its own operational weather forecast on 3.7 km spatial resolution with WRF-ARW model (http://vreme.space.si).

A special model setup was prepared for this project, fo-cusing on the Vipava valley region and using higher resolution (1.2 km). Model forecasts have been com-pared with bora observations.

New observations

Nika: “Bora is a part of my life since the birth and I have always taken it as a self-evident fact of our lifes. The project enabled me to understand how bora develops and how we can use physics and mathematics to understand and fore-cast its occurrence.”

Mirjam: “As a child, I though bora is everywhere and I was not aware it is a specialty of our valley. The project has tought me how different factors work together to make the unique climate of the Vipava valley.”

Andraž: “I am glad that I could participate in the project. To-gether we came up with interesting findings. In addition, I also improved my knowledge of Excell.“

Model verificationComparison of model outputs and DARS stations shows that the model predicts bora occurrence, evolution and average speeds well. However, the model is not capable to represent bora gusts.

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Model representation of the Vipava valley and surrounding orography.

We analyzed new observations from 5 instruments along two measurement lines. Horizontal distance between theinstruments is about 1.5 km. Bora measurements from 10 February 2012 illustrate the main findings:• all observations contain high-frequency variability, typical for bora (bora gusts),• along A line bora strength doubles from A01 towards A02 over 1.5 km horizontal and 100 m vertical distance,• in the valley average bora speed does not vary from one side to another.

Other stations

Locations of the DARS (Slovenian motorway company) measurement sites along the highway H4 through the Vipava valley.

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The most important bora property is its gustiness. We studied bora gusts by using new observa-tions collected during the four-month period in 2012. On less than 2 km distance, bora velocity more than doubles. We compared bora forecasts of the SPACE-SI prognostic model with the ob-servations to show that current forecast models lack the ability to describe the bora gustiness.

Example of the Adriatic bora forecast by SPACE-SI model valid for 10.2. 2012 at 19.00.

Bora in Vipava ValleyAnalysis of Observational and Forecast Data

SECONDARY SCHOOLDiocesan Gymnasium Vipava

Small Satellites Systems and Services - The 4S Symposium 2012Portorož, Slovenia, 4-8 June 2012

AUTHORS: Nejc Povšič, Andraž Jurinčič, Rok Žorž,Ana Čufer, Nika Obed, Mirjam Miletič, Kristijan Zorn,

Domen Rabak, Rok Miklavčič, Benjamin Smrdel, Dominik Vrčon

SUPERVISORS: Nadja Pregeljc, Vladimir Anžel,Sebastijan Mozetič, Jože Rakovec, Nedjeljka Žagar,

Rahela Žabkar, Gregor Skok, Luka Honzak, Vanja Blažica