Difference between revisions of "NOvA pictures of the month"

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(Created page with "<gallery widths=500px heights=300px> Image:NOvA Picture of September 2018.png | '''Sept-2018''' NOvA Event Display for a part in the beginning of the Near Detector. 6 MeV kine...")
 
 
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Image:NOvA Picture of September 2018.png | '''Sept-2018''' NOvA Event Display for a part in the beginning of the Near Detector. 6 MeV kinetic energy proton in a scintillator filled cell, once proton with such low energy is produced, it stops, loosing all his energy in the same cell.
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Image:NOvA_Picture_of_August_2019.png | '''August-2019''' First proceedings at AYSS-2019 conference by [[Anastasia Kalitkina at NOvA|Anastasia Kalitkina]]
Image:NOvA Picture of August 2018.jpg | '''Aug-2018''' "Новый автор" на одном научно-популярном ресурсе.
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Image: NOvA_Picture_of_July_2019.png | '''July-2019''' SN Betelgeuse neutrino signal simulation based on SND data . The picture by [[Maria Petropavlova at NOvA|Maria Petropavlova]]
Image:NOvA Picture of July 2018.jpg | '''July-2018''' Scintillation output measurements at JINR with Gamma-Neutron coincidence.
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Image: NOvA_Picture_of_June_2019.png | '''June-2019''' Efficiency vs. SN distance for various methods of detectors combination. Percents show the fraction of SN candidates in our galaxy, covered by the combined trigger.
Image:NOvA Picture of June 2018.jpg | '''June-2018''' Tesla test machine for NOvA at JINR.
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Last combination method - "Comb" is the best way to do it, where we set a weight to each detector, proportional to their sensitivity to SN signal. The picture by [[Andrey Sheshukov at NOvA|Andrey Sheshukov]]
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Image: NOvA_Picture_of_May2_2019.png | '''May-2019''' Results presented at AYSS-2019 conference by [[Anastasia Kalitkina at NOvA|Anastasia Kalitkina]]
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Image: NOvA_Picture_of_May1_2019.png | '''May-2019''' ROC-Dubna excursion by [[Alexander Antoshkin at NOvA|Alexander Antoshkin]]
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Image: NOvA_Picture_of_April_2019.png | '''Apr-2019''' GENIE comparison workshop at Liverpool, 8-12 April 2019. The picture by [[Igor Kakorin at NOvA|Igor Kakorin]]
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Image: NOvA_Picture_of_March_2019.png | '''Mar-2019''' A toy example of server, combining supernova observation significances from various "experiments". Currently they are just fake clients, sending the gaussian random values to the server. The black curve is the combined significance. This is the way we expect the experiments to collaborate in the supernova hunt in future! The picture by [[Andrey Sheshukov at NOvA|Andrey Sheshukov]]
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Image: NOvA_Picture_of_February_2019.png | '''Feb-2019''' Validation of GenieSNova simulation: number of candidates, which passed the reconstruction and selection in SuperNovaDDT (blue line), incomparison with the expected rate (black line: product of analytical signal shape, reconstruction efficiency etc.). Our simulation is correct!. The picture by [[Andrey Sheshukov at NOvA|Andrey Sheshukov]]
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Image:NOvA_Picture_of_January_2019.png | '''Jan-2019''' West (blue) and East (orange) fluxes of cosmric ray muons stopping in the Far Detector of NOvA (reweighted to corrected reconstruction efficiency effects) in separated energy intervals. The picture by [[Olga Petrova at NOvA|Olga Petrova]]
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Image:NOvA_Picture_of_December_2018.png | '''Dec-2018''' Christmas tree in light and dark. Would you see a CP-violation here?. The picture by [[Oleg Samoylov at NOvA|Oleg Samoylov]]
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Image:NOvA_Picture_of_November_2018.png | '''Nov-2018''' Пример работы триггера регистрации нейтринного сигнала от взрыва Сверхновых звезд. Как различные формы ожидаемых сигналов будут определять время пришедшего сигнала. The picture by [[Andrey Sheshukov at NOvA|Andrey Sheshukov]]
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Image:NOvA Picture of October 2018.png | '''Oct-2018''' Бывает, идешь по Москве, очень холодно, заходишь погреться и выпить чаю в первое попавшееся кафе, садишься около телевизора и краем глаза видишь там родной event display дальнего детектора. Photo by [[Lyudmila Kolupaeva at NOvA|Lyudmila Kolupaeva]]
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Забавно, что из всех кафе я выбрала случайно именно то место, где показывали канал Дискавери, на котором именно в этот день с 14:00 до 15:00 шла передача Техногеника, эпизод "Телескоп без телескопа", где были вставки из Дубны и нашего ROC-Dubna.
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Там было еще много кадров, связанных с NOvA и нейтрино, но я прикрепляю первый, который удивил меня очень сильно. Photo by [[Lyudmila Kolupaeva at NOvA|Lyudmila Kolupaeva]]
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Image:NOvA Picture of September 2018.png | '''Sept-2018''' NOvA Event Display for a part in the beginning of the Near Detector. 6 MeV kinetic energy proton in a scintillator filled cell, once proton with such low energy is produced, it stops, loosing all his energy in the same cell. Picture by [[Oleg Samoylov at NOvA|Oleg Samoylov]]
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Image:NOvA Picture of August 2018.jpg | '''Aug-2018''' "Новый автор" на одном научно-популярном ресурсе. Screenshot by [[Lyudmila Kolupaeva at NOvA|Lyudmila Kolupaeva]]
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Image:NOvA Picture of July 2018.jpg | '''July-2018''' Scintillation output measurements at JINR with Gamma-Neutron coincidence. Figure by [[Albert Sotnikov at NOvA|Albert Sotnikov]]
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Image:NOvA Picture of June 2018.jpg | '''June-2018''' Tesla test machine for NOvA at JINR. Photo by [[Chris Kullenberg at NOvA|Chris Kullenberg]]
 
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[[User:OlegSamoylov|OlegSamoylov]] ([[User talk:OlegSamoylov|talk]]) 01:17, 1 October 2018 (MSK)
 
[[User:OlegSamoylov|OlegSamoylov]] ([[User talk:OlegSamoylov|talk]]) 01:17, 1 October 2018 (MSK)

Latest revision as of 12:10, 18 September 2019

OlegSamoylov (talk) 01:17, 1 October 2018 (MSK)