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--- en:vmds [2017/01/06 22:25] – [Visual observer] fluktuacia
+++ en:vmds [Unknown date] (current) – external edit (Unknown date) 127.0.0.1
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-FIXME **This page is not fully translated, yet. Please help completing the translation.**\\ //(remove this paragraph once the translation is finished)//
 ====== Visual Meteor Detection Station VMDS01A ======
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 ==== A use of KPF 131HR camera ====
-[[http://www.elnika.cz/elnika.php?p=cze/specifikace-produktu/12316|KPF 131HR cammera]] is originally designed for building surveillance and thus requires several technical changes in order to make is suitable for usage.
+[[http://www.elnika.cz/elnika.php?p=cze/specifikace-produktu/12316|KPF 131HR camera]] is originally designed for building surveillance and thus requires several technical changes in order to make is suitable for usage.
 === IR filter removal from CCD chip ===
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 Now it is possible to see the camera in /dev/video0
-. Further it is necessary to instal ucview [[http://rsbotics.wordpress.com/2012/05/18/how-to-get-a-working-version-of-unicap-and-ucview/|exactly according to instructions]] and then to install libunicapgtk2 from
+. Further it is necessary to install ucview [[http://rsbotics.wordpress.com/2012/05/18/how-to-get-a-working-version-of-unicap-and-ucview/|exactly according to instructions]] and then to install libunicapgtk2 from
 Ubuntu repository.
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 Note: On some system you may need root privileges while running ucview to get your camera working.
-=== Issus with currently used cameras ===
+=== Issues with the currently used cameras ===
-  * Signal transmission is not possible over longer distances (in orders of meters). This means, that computer has to be very close to the cameras usually under often problematic weather conditions.
+  * Signal transmission is not possible over longer distances (in orders of meters). This means that computer has to be very close to the cameras usually under often problematic weather conditions.
   * Small angular resolution of camera
   * Small dynamic range
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 ==== Protection of camera ====
-Camera placed in a way that it has direct view to the ecliptic has to be protected against direct sunshine that may damage the CCD chip.
+Camera placed in a way that it has a direct view to the ecliptic has to be protected against direct sunshine that may damage the CCD chip.
 It is customary to use a timer, that would close a camera shutter during a day by means of cutting off the power source.
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 A final version of detection software should use an [[en:opsa|OPSA01A]] based camera as an visual data input.
-=== Syntéza celooblohového obrazu ===
-Celohoblohovy kamerovy system  (celooblohova kamera slozena z vice kamer) do snimaneho obrazu rovnou kreslit souradnicovou sit. Podle aktualniho casu. (Vyuzit mozna automaticke identifikace vyznamnych objektu v obrazu)
+=== The synthesis of all-sky image ===
+All-sky camera system (composed of more cameras) directly plots a coordinate system to the captured image depending on the current time. At the same time it is possible to use an automatic detection of key objects found in the image.
-===== Využití dat =====
+===== Data usage =====
 ==== Bolidozor ====
-[[http://wiki.bolidozor.cz|Síť Bolidozor]] se jistě bude snažit o využití pozorovaných dat pro detekci bolidů a jejich následné vyhledávání.
+[[http://wiki.bolidozor.cz|Bolidozor network]] can make use of the observed data to detect and further search for the bolides.
-==== Meteorologie ====
+==== Meteorology ====
-Protože kamery této stanice by měly být směrovány tak, aby zabíraly oblohu, tak pozorovaná data lze také teoreticky využít pro meteorologické aplikace. Neboť oblačnost sledovaná zespodu z menší vzdálenosti může poskytovat cenné informace o výskytu stoupavých proudů, parametrech bouřek, nebo o postupu front.
+Because station's cameras should be directed in a way that they cover the whole sky, the data can be theoretically used for meteorological applications. Cloud cover observed at small distances from below can provide useful information concerning the occurrence of updrafts, storm parameters or moving of fronts.
-Fotometricky může být také měřena výška základny oblačnosti, nebo její tloušťka, úroveň pokrytí.
+Using photometry we can measure the height of cloud base, its thickness or the extent of the cloud cover.
-Dalším užitečným výstupem může být koncentrace prachu a aerosolů v atmosféře.
+Other useful output may be the measure of the concentration of dust and aerosols in the atmosphere.
-==== 3D rekonstrukce obrazu ====
+==== 3D image reconstruction ====
   * [[http://openmvg.readthedocs.org/en/latest/software/MVS/MVS/|OpenMVG]]
   * [[https://github.com/albertcheng/bundler_sfm|Bundler]]
   * [[https://github.com/kml27/insight3d/tree/master/insight3d|insight3d]]
-===== Reference =====
-  * Síť [[http://cement.fireball.sk/|CEMeNt]]
+===== References =====
-  * Ukázka [[http://www.astrozor.cz/index.php?udalost=56|Realizace stanice na Hvězdárně Svákov]]
+  * [[http://cement.fireball.sk/|CEMeNt]] network
+  * An illustration of [[http://www.astrozor.cz/index.php?udalost=56|station realisation on Svákov observatory]]