Status of the PAIPS project and selected results

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Resumo

The PAIPS experiment was created for studying UV luminescence in the auroral region. This experiment represents a system of two imaging photometers with high temporal resolution, located 153 km apart in space and directed into the same region of the atmosphere. This experiment configuration allows stereometric spatial and temporal structure measurements of luminosity. We presented some results from the pulsating auroras (PA) and UV microbursts analysis, as well as examples of the track event reconstruction using probabilistic models based on Bayesian inference. Operation of luminescence altitude calculation algorithm is shown using a single PA event. A database of UV microbursts (series of short UV flashes) for two seasons of the experiment (2021/2022 and 2022/2023) was obtained and analysed.

Sobre autores

K. Sigaeva

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics; Lomonosov Moscow State University, Faculty of Physics

Email: sigaeva.kf15@physics.msu.ru
Moscow, Russia; Moscow, Russia

A. Belov

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics

Moscow, Russia

P. Klimov

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics

Moscow, Russia

B. Kozelov

Polar Geophysical Institute

Murmansk, Russia

A. Murashov

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics

Moscow, Russia

V. Nikolaeva

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics

Moscow, Russia

A. Roldugin

Polar Geophysical Institute

Murmansk, Russia

R. Saraev

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics; Lomonosov Moscow State University, Faculty of Physics

Moscow, Russia; Moscow, Russia

D. Trofimov

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics; Lomonosov Moscow State University, Faculty of Physics

Moscow, Russia; Moscow, Russia

S. Sharakin

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics

Moscow, Russia

K. Shchelkanov

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics; Lomonosov Moscow State University, Faculty of Physics

Moscow, Russia; Moscow, Russia

S. Blin

Universite Paris Cite, CNRS, Astroparticule et Cosmologie

Paris, France

M. Casolino

Istituto Nazionale di Fisica Nucleare, Section of Rome Tor Vergata; RIKEN; University of Rome Tor Vergata

Department of Physics Rome, Italy; Wako, Japan; Rome, Italy

W. Marszal

National Centre for Nuclear Research

Otwock, Poland

E. Parizot

Universite Paris Cite, CNRS, Astroparticule et Cosmologie

Paris, France

G. Prevôt

Universite Paris Cite, CNRS, Astroparticule et Cosmologie

Paris, France

Y. Takizawa

RIKEN

Wako, Japan

J. Szabelski

Stefan Batory Academy of Applied Sciences

Skierniewice, Poland

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