diff --git a/public/uploads/MontpellierRamanLidar-1600x1069.jpg b/public/uploads/MontpellierRamanLidar-1600x1069.jpg new file mode 100644 index 0000000..5b14593 Binary files /dev/null and b/public/uploads/MontpellierRamanLidar-1600x1069.jpg differ diff --git a/public/uploads/UAE_Event.jpg b/public/uploads/UAE_Event.jpg new file mode 100644 index 0000000..71930b3 Binary files /dev/null and b/public/uploads/UAE_Event.jpg differ diff --git a/src/content/news/testowy-artykuł-tytuł.md b/src/content/news/testowy-artykuł-tytuł.md index 3287686..c5b4216 100644 --- a/src/content/news/testowy-artykuł-tytuł.md +++ b/src/content/news/testowy-artykuł-tytuł.md @@ -4,13 +4,13 @@ description: Testowy artykuł - opis date: 2026-07-24 category: news author: CTAO -cover: /uploads/Zrzut ekranu 2026-07-24 o 20.28.05.jpg +cover: /uploads/UAE_Event.jpg draft: false --- -*Artykuł testowy — treść skopiowana z newsa CTAO: [Preparing the Montpellier Raman LIDAR Calibration System for CTAO-South](https://www.ctao.org/news/preparing-the-montpellier-raman-lidar-calibration-system-for-ctao-south/).* +_Artykuł testowy — treść skopiowana z newsa CTAO:_ [_Preparing the Montpellier Raman LIDAR Calibration System for CTAO-South_](https://www.ctao.org/news/preparing-the-montpellier-raman-lidar-calibration-system-for-ctao-south/)_._ ---- +*** **An essential part of the CTAO telescopes' detectors is situated well above their actual mechanical structure: the Earth's atmosphere.** It is there that high-energy gamma rays interact with atmospheric molecules, giving rise to a [cascade of particles that produce faint flashes of Cherenkov light](https://www.ctao.org/emission-to-discovery/science/how-ctao-works/). Because atmospheric conditions dictate how this light reaches the ground, it is fundamental to characterise our skies continuously — a task performed by devices known as **Raman LIDARs**. @@ -19,12 +19,13 @@ draft: false 1. The instrument fires powerful laser pulses into the atmosphere — two beams of different wavelengths at once, covering the spectrum of Cherenkov light seen by the telescopes. 2. A telescope collects the light that bounces back. 3. By measuring the exact time it takes for this light to return, it calculates the amount of aerosols present at different altitudes. -4. The backscattered signal is separated into four channels — one dedicated to *Raman-scattered* light, produced when photons interact with atmospheric nitrogen and shift slightly in wavelength. +4. The backscattered signal is separated into four channels — one dedicated to _Raman-scattered_ light, produced when photons interact with atmospheric nitrogen and shift slightly in wavelength. This configuration provides scientists with highly detailed atmospheric profiles, allowing them to pinpoint various aerosols. -[![Widok placu budowy CTAO-South na pustyni Atakama](/uploads/Zrzut%20ekranu%202026-07-24%20o%2020.29.07.jpg "Tytuł zdjęcia")](https://www.ctao.org/news/italian-minister-of-university-and-research-visits-the-ctao-south-site-in-chile/) -*Zdjęcie testowe — kliknięcie prowadzi do powiązanego newsa CTAO.* +[![Widok placu budowy CTAO-South na pustyni Atakama](/uploads/MontpellierRamanLidar-1600x1069.jpg "Tytuł zdjęcia")](https://www.ctao.org/news/italian-minister-of-university-and-research-visits-the-ctao-south-site-in-chile/) + +_Zdjęcie testowe — kliknięcie prowadzi do powiązanego newsa CTAO._ ## Two instruments, two sites